Thu, 24 Jan 2019 21:24:25 +0100
Bug fixes and further options. Read Improvements_of_lidar_correction_ghk_ver.0.9.8_190124.pdf
ulalume3@0 | 1 | # -*- coding: utf-8 -*- |
ulalume3@0 | 2 | """ |
volker@28 | 3 | Copyright 2016, 2019 Volker Freudenthaler |
ulalume3@0 | 4 | |
ulalume3@0 | 5 | Licensed under the EUPL, Version 1.1 only (the "Licence"). |
ulalume3@0 | 6 | |
ulalume3@0 | 7 | You may not use this work except in compliance with the Licence. |
ulalume3@0 | 8 | A copy of the licence is distributed with the code. Alternatively, you may obtain |
ulalume3@0 | 9 | a copy of the Licence at: |
ulalume3@0 | 10 | |
ulalume3@0 | 11 | https://joinup.ec.europa.eu/community/eupl/og_page/eupl |
ulalume3@0 | 12 | |
ulalume3@0 | 13 | Unless required by applicable law or agreed to in writing, software distributed |
ulalume3@0 | 14 | under the Licence is distributed on an "AS IS" basis, WITHOUT WARRANTIES OR CONDITIONS |
ulalume3@0 | 15 | OF ANY KIND, either express or implied. See the Licence for the specific language governing |
ulalume3@0 | 16 | permissions and limitations under the Licence. |
ulalume3@0 | 17 | |
ulalume3@0 | 18 | Equation reference: http://www.atmos-meas-tech-discuss.net/amt-2015-338/amt-2015-338.pdf |
ulalume3@0 | 19 | With equations code from Appendix C |
volker@28 | 20 | Python 3.7, seaborn 0.9.0 |
volker@21 | 21 | |
volker@21 | 22 | Code description: |
volker@21 | 23 | |
volker@21 | 24 | From measured lidar signals we cannot directly determine the desired backscatter coefficient (F11) and the linear depolarization ratio (LDR) |
volker@21 | 25 | because of the cross talk between the channles and systematic errors of a lidar system. |
volker@21 | 26 | http://www.atmos-meas-tech-discuss.net/amt-2015-338/amt-2015-338.pdf provides an analytical model for the description of these errors, |
volker@21 | 27 | with which the measured signals can be corrected. |
volker@21 | 28 | This code simulates the lidar measurements with "assumed true" model parameters from an input file, and calculates the correction parameters (G,H, and K). |
volker@21 | 29 | The "assumed true" system parameters are the ones we think are the right ones, but in reality these parameters probably deviate from the assumed truth due to |
volker@21 | 30 | uncertainties. The uncertainties of the "assumed true" parameters can be described in the input file. Then this code calculates the lidar signals and the |
volker@21 | 31 | gain ratio eta* with all possible combinations of "errors", which represents the distribution of "possibly real" signals, and "corrects" them with the "assumed true" |
volker@21 | 32 | GHK parameters (GT0, GR0, HT0, HR0, and K0) to derive finally the distributions of "possibly real" linear depolarization ratios (LDRcorr), |
volker@21 | 33 | which are plotted for five different input linear depolarization ratios (LDRtrue). The red bars in the plots represent the input values of LDRtrue. |
volker@21 | 34 | A complication arises from the fact that the correction parameter K = eta*/eta (Eq. 83) can depend on the LDR during the calibration measurement, i.e. LDRcal or aCal |
volker@21 | 35 | in the code (see e.g. Eqs. (103), (115), and (141); mind the mistake in Eq. (116)). Therefor values of K for LDRcal = 0.004, 0.2, and 0.45 are calculated for |
volker@21 | 36 | "assumed true" system parameters and printed in the output file behind the GH parameters. The full impact of the LDRcal dependent K can be considered in the error |
volker@21 | 37 | calculation by specifying a range of possible LDRcal values in the input file. For the real calibration measurements a calibration range with low or no aerosol |
volker@21 | 38 | content should be chosen, and the default in the input file is a range of LDRcal between 0.004 and 0.014 (i.e. 0.009 +-0.005). |
volker@21 | 39 | |
volker@21 | 40 | Tip: In case you run the code with Spyder, all output text and plots can be displayed together in an IPython console, which can be saved as an html file. |
volker@28 | 41 | |
volker@28 | 42 | Ver. 0.9.8: - for details, see "Improvements_of_lidar_correction_ghk_ver.0.9.8_190124.pdf" |
volker@28 | 43 | - correct calculation of Eta for cleaned anaylsers considering the combined transmission Eta = (TaT* TiT)(1 + cos2RotaT * DaT * DiT) and (TaR * TiR)(1 + cos2RotaR * DaR * DiR) according to the papers supplement Eqs. (S.10.10.1) ff |
volker@28 | 44 | - ND-filters can be added for the calibration measurements in the transmitted (TCalT) and the reflected path (TCalR) in order to include their uncertainties in the error calculation. |
volker@28 | 45 | - includes the simulation of signal noise |
ulalume3@0 | 46 | """ |
volker@28 | 47 | # Comment: The code might works with Python 2.7 with the help of following line, which enables Python2 to correctly interpret the Python 3 print statements. |
ulalume3@0 | 48 | from __future__ import print_function |
volker@21 | 49 | # !/usr/bin/env python3 |
binietoglou@19 | 50 | |
binietoglou@19 | 51 | import os |
binietoglou@19 | 52 | import sys |
binietoglou@19 | 53 | |
ulalume3@0 | 54 | import numpy as np |
ulalume3@0 | 55 | |
volker@11 | 56 | # Comment: the seaborn library makes nicer plots, but the code works also without it. |
volker@11 | 57 | try: |
volker@11 | 58 | import seaborn as sns |
binietoglou@19 | 59 | |
volker@11 | 60 | sns_loaded = True |
volker@11 | 61 | except ImportError: |
volker@11 | 62 | sns_loaded = False |
volker@11 | 63 | |
ulalume3@0 | 64 | import matplotlib.pyplot as plt |
volker@28 | 65 | # from time import clock # python 2 |
volker@28 | 66 | from timeit import default_timer as clock |
ulalume3@0 | 67 | |
binietoglou@19 | 68 | # from matplotlib.backends.backend_pdf import PdfPages |
binietoglou@19 | 69 | # pdffile = '{}.pdf'.format('path') |
binietoglou@19 | 70 | # pp = PdfPages(pdffile) |
ulalume3@0 | 71 | ## pp.savefig can be called multiple times to save to multiple pages |
binietoglou@19 | 72 | # pp.savefig() |
binietoglou@19 | 73 | # pp.close() |
ulalume3@0 | 74 | |
ulalume3@0 | 75 | from contextlib import contextmanager |
binietoglou@19 | 76 | |
ulalume3@0 | 77 | @contextmanager |
ulalume3@0 | 78 | def redirect_stdout(new_target): |
binietoglou@19 | 79 | old_target, sys.stdout = sys.stdout, new_target # replace sys.stdout |
ulalume3@0 | 80 | try: |
binietoglou@19 | 81 | yield new_target # run some code with the replaced stdout |
ulalume3@0 | 82 | finally: |
ulalume3@0 | 83 | sys.stdout.flush() |
binietoglou@19 | 84 | sys.stdout = old_target # restore to the previous value |
binietoglou@19 | 85 | |
ulalume3@0 | 86 | ''' |
ulalume3@0 | 87 | real_raw_input = vars(__builtins__).get('raw_input',input) |
ulalume3@0 | 88 | ''' |
ulalume3@0 | 89 | try: |
ulalume3@0 | 90 | import __builtin__ |
binietoglou@19 | 91 | |
ulalume3@0 | 92 | input = getattr(__builtin__, 'raw_input') |
ulalume3@0 | 93 | except (ImportError, AttributeError): |
ulalume3@0 | 94 | pass |
ulalume3@0 | 95 | |
ulalume3@0 | 96 | from distutils.util import strtobool |
binietoglou@19 | 97 | |
binietoglou@19 | 98 | |
ulalume3@0 | 99 | def user_yes_no_query(question): |
ulalume3@0 | 100 | sys.stdout.write('%s [y/n]\n' % question) |
ulalume3@0 | 101 | while True: |
ulalume3@0 | 102 | try: |
ulalume3@0 | 103 | return strtobool(input().lower()) |
ulalume3@0 | 104 | except ValueError: |
ulalume3@0 | 105 | sys.stdout.write('Please respond with \'y\' or \'n\'.\n') |
ulalume3@0 | 106 | |
binietoglou@19 | 107 | |
binietoglou@19 | 108 | # if user_yes_no_query('want to exit?') == 1: sys.exit() |
ulalume3@0 | 109 | |
ulalume3@0 | 110 | abspath = os.path.abspath(__file__) |
ulalume3@0 | 111 | dname = os.path.dirname(abspath) |
ulalume3@0 | 112 | fname = os.path.basename(abspath) |
ulalume3@0 | 113 | os.chdir(dname) |
ulalume3@0 | 114 | |
binietoglou@19 | 115 | # PrintToOutputFile = True |
ulalume3@0 | 116 | |
binietoglou@19 | 117 | sqr05 = 0.5 ** 0.5 |
ulalume3@0 | 118 | |
volker@21 | 119 | # ---- Initial definition of variables; the actual values will be read in with exec(open('./optic_input.py').read()) below |
volker@16 | 120 | # Do you want to calculate the errors? If not, just the GHK-parameters are determined. |
volker@28 | 121 | ScriptVersion = "0.9.8d" |
volker@16 | 122 | Error_Calc = True |
ulalume3@0 | 123 | LID = "internal" |
ulalume3@0 | 124 | EID = "internal" |
ulalume3@0 | 125 | # --- IL Laser IL and +-Uncertainty |
volker@23 | 126 | DOLP, dDOLP, nDOLP = 0.995, 0.005, 1 # degree of linear polarization; default 1 |
binietoglou@19 | 127 | RotL, dRotL, nRotL = 0.0, 0.0, 1 # alpha; rotation of laser polarization in degrees; default 0 |
volker@28 | 128 | # IL = 1e5 #photons in the laser beam, including detection efficiency of the telescope, atmodspheric and r^2 attenuation |
ulalume3@0 | 129 | # --- ME Emitter and +-Uncertainty |
binietoglou@19 | 130 | DiE, dDiE, nDiE = 0., 0.00, 1 # Diattenuation |
binietoglou@19 | 131 | TiE = 1. # Unpolarized transmittance |
binietoglou@19 | 132 | RetE, dRetE, nRetE = 0., 180.0, 0 # Retardance in degrees |
binietoglou@19 | 133 | RotE, dRotE, nRotE = 0., 0.0, 0 # beta: Rotation of optical element in degrees |
ulalume3@0 | 134 | # --- MO Receiver Optics including telescope |
binietoglou@19 | 135 | DiO, dDiO, nDiO = -0.055, 0.003, 1 |
binietoglou@19 | 136 | TiO = 0.9 |
binietoglou@19 | 137 | RetO, dRetO, nRetO = 0., 180.0, 2 |
binietoglou@19 | 138 | RotO, dRotO, nRotO = 0., 0.1, 1 # gamma |
ulalume3@0 | 139 | # --- PBS MT transmitting path defined with (TS,TP); and +-Uncertainty |
binietoglou@19 | 140 | TP, dTP, nTP = 0.98, 0.02, 1 |
binietoglou@19 | 141 | TS, dTS, nTS = 0.001, 0.001, 1 |
ulalume3@0 | 142 | TiT = 0.5 * (TP + TS) |
binietoglou@19 | 143 | DiT = (TP - TS) / (TP + TS) |
ulalume3@0 | 144 | # PolFilter |
binietoglou@19 | 145 | RetT, dRetT, nRetT = 0., 180., 0 |
binietoglou@19 | 146 | ERaT, dERaT, nERaT = 0.001, 0.001, 1 |
binietoglou@19 | 147 | RotaT, dRotaT, nRotaT = 0., 3., 1 |
binietoglou@19 | 148 | DaT = (1 - ERaT) / (1 + ERaT) |
binietoglou@19 | 149 | TaT = 0.5 * (1 + ERaT) |
ulalume3@0 | 150 | # --- PBS MR reflecting path defined with (RS,RP); and +-Uncertainty |
volker@13 | 151 | RS_RP_depend_on_TS_TP = False |
binietoglou@19 | 152 | if (RS_RP_depend_on_TS_TP): |
binietoglou@19 | 153 | RP, dRP, nRP = 1 - TP, 0.00, 0 |
binietoglou@19 | 154 | RS, dRS, nRS = 1 - TS, 0.00, 0 |
volker@13 | 155 | else: |
binietoglou@19 | 156 | RP, dRP, nRP = 0.05, 0.01, 1 |
binietoglou@19 | 157 | RS, dRS, nRS = 0.98, 0.01, 1 |
ulalume3@0 | 158 | TiR = 0.5 * (RP + RS) |
binietoglou@19 | 159 | DiR = (RP - RS) / (RP + RS) |
ulalume3@0 | 160 | # PolFilter |
binietoglou@19 | 161 | RetR, dRetR, nRetR = 0., 180., 0 |
binietoglou@19 | 162 | ERaR, dERaR, nERaR = 0.001, 0.001, 1 |
binietoglou@19 | 163 | RotaR, dRotaR, nRotaR = 90., 3., 1 |
binietoglou@19 | 164 | DaR = (1 - ERaR) / (1 + ERaR) |
binietoglou@19 | 165 | TaR = 0.5 * (1 + ERaR) |
ulalume3@0 | 166 | |
volker@28 | 167 | # +++ Orientation of the PBS with respect to the reference plane (see Polarisation-orientation.png and Polarisation-orientation-2.png in /system_settings) |
volker@28 | 168 | # Y = +1: polarisation in reference plane is finally transmitted, |
volker@28 | 169 | # Y = -1: polarisation in reference plane is finally reflected. |
volker@28 | 170 | Y = 1. |
ulalume3@0 | 171 | |
ulalume3@0 | 172 | # Calibrator = type defined by matrix values |
binietoglou@19 | 173 | LocC = 4 # location of calibrator: behind laser = 1; behind emitter = 2; before receiver = 3; before PBS = 4 |
ulalume3@0 | 174 | |
volker@28 | 175 | # --- Additional attenuation (transmission of the ND-filter) during the calibration |
volker@28 | 176 | TCalT, dTCalT, nTCalT = 1, 0, 0 # transmitting path; error calc not working yet |
volker@28 | 177 | TCalR, dTCalR, nTCalR = 1, 0, 0 # reflecting path; error calc not working yet |
volker@28 | 178 | |
volker@28 | 179 | # *** signal noise error calculation |
volker@28 | 180 | # --- number of photon counts in the signal summed up in the calibration range during the calibration measurements |
volker@28 | 181 | NCalT = 1e6 # default 1e6, assumed the same in +45° and -45° signals |
volker@28 | 182 | NCalR = 1e6 # default 1e6, assumed the same in +45° and -45° signals |
volker@28 | 183 | NILfac = 200 # duration of standard (0°) measurement relative to calibration measurements |
volker@28 | 184 | nNCal = 0 # error nNCal: one-sigma in steps to left and right for calibration signals |
volker@28 | 185 | nNI = 0 # error nNI: one-sigma in steps to left and right for 0° signals |
volker@28 | 186 | IoutTp0, IoutTp, dIoutTp0 = 0.5, 0.5, 0 |
volker@28 | 187 | IoutTm0, IoutTm, dIoutTm0 = 0.5, 0.5, 0 |
volker@28 | 188 | IoutRp0, IoutRp, dIoutRp0 = 0.5, 0.5, 0 |
volker@28 | 189 | IoutRm0, IoutRm, dIoutRm0 = 0.5, 0.5, 0 |
volker@28 | 190 | It0, It, dIt0 = 1 , 1, 0 |
volker@28 | 191 | Ir0, Ir, dTr0 = 1 , 1, 0 |
volker@28 | 192 | CalcFrom0deg = True |
volker@28 | 193 | |
binietoglou@19 | 194 | TypeC = 3 # linear polarizer calibrator |
ulalume3@0 | 195 | # example with extinction ratio 0.001 |
binietoglou@19 | 196 | DiC, dDiC, nDiC = 1.0, 0., 0 # ideal 1.0 |
binietoglou@19 | 197 | TiC = 0.5 # ideal 0.5 |
binietoglou@19 | 198 | RetC, dRetC, nRetC = 0., 0., 0 |
binietoglou@19 | 199 | RotC, dRotC, nRotC = 0.0, 0.1, 0 # constant calibrator offset epsilon |
binietoglou@19 | 200 | RotationErrorEpsilonForNormalMeasurements = False # is in general False for TypeC == 3 calibrator |
ulalume3@0 | 201 | |
ulalume3@0 | 202 | # Rotation error without calibrator: if False, then epsilon = 0 for normal measurements |
ulalume3@0 | 203 | RotationErrorEpsilonForNormalMeasurements = True |
volker@28 | 204 | # BSR backscatter ratio |
volker@28 | 205 | # BSR, dBSR, nBSR = 10, 0.05, 1 |
volker@28 | 206 | BSR = np.zeros(5) |
volker@28 | 207 | BSR = [1.1, 2, 5, 10, 50] |
volker@28 | 208 | # theoretical molecular LDR LDRm |
volker@28 | 209 | LDRm, dLDRm, nLDRm = 0.004, 0.001, 1 |
ulalume3@0 | 210 | # LDRCal assumed atmospheric linear depolarization ratio during the calibration measurements (first guess) |
binietoglou@19 | 211 | LDRCal0, dLDRCal, nLDRCal = 0.25, 0.04, 1 |
ulalume3@0 | 212 | LDRCal = LDRCal0 |
ulalume3@0 | 213 | # measured LDRm will be corrected with calculated parameters |
ulalume3@0 | 214 | LDRmeas = 0.015 |
ulalume3@0 | 215 | # LDRtrue for simulation of measurement => LDRsim |
ulalume3@0 | 216 | LDRtrue = 0.5 |
ulalume3@0 | 217 | LDRtrue2 = 0.004 |
volker@28 | 218 | LDRunCorr = 1 |
ulalume3@0 | 219 | # Initialize other values to 0 |
ulalume3@0 | 220 | ER, nER, dER = 0.001, 0, 0.001 |
ulalume3@0 | 221 | K = 0. |
ulalume3@0 | 222 | Km = 0. |
ulalume3@0 | 223 | Kp = 0. |
ulalume3@0 | 224 | LDRcorr = 0. |
ulalume3@0 | 225 | Eta = 0. |
ulalume3@0 | 226 | Ir = 0. |
ulalume3@0 | 227 | It = 0. |
ulalume3@0 | 228 | h = 1. |
ulalume3@0 | 229 | |
ulalume3@0 | 230 | Loc = ['', 'behind laser', 'behind emitter', 'before receiver', 'before PBS'] |
binietoglou@19 | 231 | Type = ['', 'mechanical rotator', 'hwp rotator', 'linear polarizer', 'qwp rotator', 'circular polarizer', |
binietoglou@19 | 232 | 'real HWP +-22.5°'] |
ulalume3@0 | 233 | dY = ['reflected channel', '', 'transmitted channel'] |
volker@28 | 234 | bPlotEtax = False |
ulalume3@0 | 235 | |
ulalume3@0 | 236 | # end of initial definition of variables |
ulalume3@0 | 237 | # ******************************************************************************************************************************* |
ulalume3@0 | 238 | |
volker@28 | 239 | # --- Read actual lidar system parameters from optic_input.py (must be in the programs sub-directory 'system_settings') |
volker@28 | 240 | #InputFile = 'optic_input_example_lidar_2.py' |
volker@28 | 241 | #InputFile = 'optic_input_example_lidar_3.py' |
volker@28 | 242 | #InputFile = 'optic_input_example_lidar_4.py' |
volker@28 | 243 | #InputFile = 'optic_input_example_lidar_5.py' |
volker@28 | 244 | InputFile = 'optic_input_example_lidar.py' |
volker@28 | 245 | |
ulalume3@0 | 246 | ''' |
ulalume3@0 | 247 | print("From ", dname) |
ulalume3@0 | 248 | print("Running ", fname) |
ulalume3@0 | 249 | print("Reading input file ", InputFile, " for") |
ulalume3@0 | 250 | ''' |
ulalume3@0 | 251 | input_path = os.path.join('.', 'system_settings', InputFile) |
volker@21 | 252 | # this works with Python 2 and 3! |
binietoglou@19 | 253 | exec (open(input_path).read(), globals()) |
ulalume3@0 | 254 | # end of read actual system parameters |
ulalume3@0 | 255 | |
volker@21 | 256 | |
ulalume3@0 | 257 | # --- Manual Parameter Change --- |
ulalume3@0 | 258 | # (use for quick parameter changes without changing the input file ) |
binietoglou@19 | 259 | # DiO = 0. |
binietoglou@19 | 260 | # LDRtrue = 0.45 |
binietoglou@19 | 261 | # LDRtrue2 = 0.004 |
binietoglou@19 | 262 | # Y = -1 |
binietoglou@19 | 263 | # LocC = 4 #location of calibrator: 1 = behind laser; 2 = behind emitter; 3 = before receiver; 4 = before PBS |
ulalume3@0 | 264 | ##TypeC = 6 Don't change the TypeC here |
binietoglou@19 | 265 | # RotationErrorEpsilonForNormalMeasurements = True |
binietoglou@19 | 266 | # LDRCal = 0.25 |
ulalume3@0 | 267 | ## --- Errors |
volker@23 | 268 | DOLP0, dDOLP, nDOLP = DOLP, dDOLP, nDOLP |
ulalume3@0 | 269 | RotL0, dRotL, nRotL = RotL, dRotL, nRotL |
ulalume3@0 | 270 | |
binietoglou@19 | 271 | DiE0, dDiE, nDiE = DiE, dDiE, nDiE |
ulalume3@0 | 272 | RetE0, dRetE, nRetE = RetE, dRetE, nRetE |
ulalume3@0 | 273 | RotE0, dRotE, nRotE = RotE, dRotE, nRotE |
ulalume3@0 | 274 | |
binietoglou@19 | 275 | DiO0, dDiO, nDiO = DiO, dDiO, nDiO |
ulalume3@0 | 276 | RetO0, dRetO, nRetO = RetO, dRetO, nRetO |
ulalume3@0 | 277 | RotO0, dRotO, nRotO = RotO, dRotO, nRotO |
ulalume3@0 | 278 | |
binietoglou@19 | 279 | DiC0, dDiC, nDiC = DiC, dDiC, nDiC |
ulalume3@0 | 280 | RetC0, dRetC, nRetC = RetC, dRetC, nRetC |
ulalume3@0 | 281 | RotC0, dRotC, nRotC = RotC, dRotC, nRotC |
ulalume3@0 | 282 | |
binietoglou@19 | 283 | TP0, dTP, nTP = TP, dTP, nTP |
binietoglou@19 | 284 | TS0, dTS, nTS = TS, dTS, nTS |
ulalume3@0 | 285 | RetT0, dRetT, nRetT = RetT, dRetT, nRetT |
ulalume3@0 | 286 | |
ulalume3@0 | 287 | ERaT0, dERaT, nERaT = ERaT, dERaT, nERaT |
binietoglou@19 | 288 | RotaT0, dRotaT, nRotaT = RotaT, dRotaT, nRotaT |
ulalume3@0 | 289 | |
binietoglou@19 | 290 | RP0, dRP, nRP = RP, dRP, nRP |
binietoglou@19 | 291 | RS0, dRS, nRS = RS, dRS, nRS |
ulalume3@0 | 292 | RetR0, dRetR, nRetR = RetR, dRetR, nRetR |
ulalume3@0 | 293 | |
ulalume3@0 | 294 | ERaR0, dERaR, nERaR = ERaR, dERaR, nERaR |
binietoglou@19 | 295 | RotaR0, dRotaR, nRotaR = RotaR, dRotaR, nRotaR |
ulalume3@0 | 296 | |
binietoglou@19 | 297 | LDRCal0, dLDRCal, nLDRCal = LDRCal, dLDRCal, nLDRCal |
volker@28 | 298 | |
volker@28 | 299 | # BSR0, dBSR, nBSR = BSR, dBSR, nBSR |
volker@28 | 300 | LDRm0, dLDRm, nLDRm = LDRm, dLDRm, nLDRm |
ulalume3@0 | 301 | # ---------- End of manual parameter change |
ulalume3@0 | 302 | |
ulalume3@0 | 303 | RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC = RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0 |
binietoglou@19 | 304 | TP, TS, RP, RS, ERaT, RotaT, RetT, ERaR, RotaR, RetR = TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0 |
ulalume3@0 | 305 | LDRCal = LDRCal0 |
binietoglou@19 | 306 | DTa0, TTa0, DRa0, TRa0, LDRsimx, LDRCorr = 0, 0, 0, 0, 0, 0 |
volker@28 | 307 | TCalT0, TCalR0 = TCalT, TCalR |
ulalume3@0 | 308 | |
ulalume3@0 | 309 | TiT = 0.5 * (TP + TS) |
binietoglou@19 | 310 | DiT = (TP - TS) / (TP + TS) |
binietoglou@19 | 311 | ZiT = (1. - DiT ** 2) ** 0.5 |
ulalume3@0 | 312 | TiR = 0.5 * (RP + RS) |
binietoglou@19 | 313 | DiR = (RP - RS) / (RP + RS) |
binietoglou@19 | 314 | ZiR = (1. - DiR ** 2) ** 0.5 |
binietoglou@19 | 315 | |
volker@28 | 316 | C2aT = np.cos(np.deg2rad(2 * RotaT)) |
volker@28 | 317 | C2aR = np.cos(np.deg2rad(2 * RotaR)) |
volker@28 | 318 | ATPT = (1 + C2aT * DaT * DiT) |
volker@28 | 319 | ARPT = (1 + C2aR * DaR * DiR) |
volker@28 | 320 | TTa = TiT * TaT * ATPT # unpolarized transmission |
volker@28 | 321 | TRa = TiR * TaR * ARPT # unpolarized transmission |
volker@28 | 322 | Eta0 = TRa / TTa |
volker@28 | 323 | # --- this subroutine is for the calculation of the PLDR from LDR, BSR, and LDRm ----------------------------------------------------- |
volker@28 | 324 | def CalcPLDR(LDR, BSR, LDRm): |
volker@28 | 325 | PLDR = (BSR * (1. + LDRm) * LDR - LDRm * (1. + LDR)) / (BSR * (1. + LDRm) - (1. + LDR)) |
volker@28 | 326 | return (PLDR) |
volker@13 | 327 | # --- this subroutine is for the calculation with certain fixed parameters ----------------------------------------------------- |
volker@28 | 328 | def Calc(TCalT, TCalR, NCalT, NCalR, DOLP, RotL, RotE, RetE, DiE, RotO, RetO, DiO, |
volker@28 | 329 | RotC, RetC, DiC, TP, TS, RP, RS, |
volker@28 | 330 | ERaT, RotaT, RetT, ERaR, RotaR, RetR, LDRCal): |
ulalume3@0 | 331 | # ---- Do the calculations of bra-ket vectors |
ulalume3@0 | 332 | h = -1. if TypeC == 2 else 1 |
ulalume3@0 | 333 | # from input file: assumed LDRCal for calibration measurements |
binietoglou@19 | 334 | aCal = (1. - LDRCal) / (1 + LDRCal) |
ulalume3@0 | 335 | # from input file: measured LDRm and true LDRtrue, LDRtrue2 => |
binietoglou@19 | 336 | # ameas = (1.-LDRmeas)/(1+LDRmeas) |
binietoglou@19 | 337 | atrue = (1. - LDRtrue) / (1 + LDRtrue) |
binietoglou@19 | 338 | # atrue2 = (1.-LDRtrue2)/(1+LDRtrue2) |
ulalume3@0 | 339 | |
ulalume3@0 | 340 | # angles of emitter and laser and calibrator and receiver optics |
ulalume3@0 | 341 | # RotL = alpha, RotE = beta, RotO = gamma, RotC = epsilon |
binietoglou@19 | 342 | S2a = np.sin(2 * np.deg2rad(RotL)) |
binietoglou@19 | 343 | C2a = np.cos(2 * np.deg2rad(RotL)) |
binietoglou@19 | 344 | S2b = np.sin(2 * np.deg2rad(RotE)) |
binietoglou@19 | 345 | C2b = np.cos(2 * np.deg2rad(RotE)) |
binietoglou@19 | 346 | S2ab = np.sin(np.deg2rad(2 * RotL - 2 * RotE)) |
binietoglou@19 | 347 | C2ab = np.cos(np.deg2rad(2 * RotL - 2 * RotE)) |
binietoglou@19 | 348 | S2g = np.sin(np.deg2rad(2 * RotO)) |
binietoglou@19 | 349 | C2g = np.cos(np.deg2rad(2 * RotO)) |
ulalume3@0 | 350 | |
volker@23 | 351 | # Laser with Degree of linear polarization DOLP |
ulalume3@0 | 352 | IinL = 1. |
volker@23 | 353 | QinL = DOLP |
ulalume3@0 | 354 | UinL = 0. |
volker@23 | 355 | VinL = (1. - DOLP ** 2) ** 0.5 |
ulalume3@0 | 356 | |
ulalume3@0 | 357 | # Stokes Input Vector rotation Eq. E.4 |
binietoglou@19 | 358 | A = C2a * QinL - S2a * UinL |
binietoglou@19 | 359 | B = S2a * QinL + C2a * UinL |
ulalume3@0 | 360 | # Stokes Input Vector rotation Eq. E.9 |
binietoglou@19 | 361 | C = C2ab * QinL - S2ab * UinL |
binietoglou@19 | 362 | D = S2ab * QinL + C2ab * UinL |
ulalume3@0 | 363 | |
ulalume3@0 | 364 | # emitter optics |
ulalume3@0 | 365 | CosE = np.cos(np.deg2rad(RetE)) |
ulalume3@0 | 366 | SinE = np.sin(np.deg2rad(RetE)) |
binietoglou@19 | 367 | ZiE = (1. - DiE ** 2) ** 0.5 |
binietoglou@19 | 368 | WiE = (1. - ZiE * CosE) |
ulalume3@0 | 369 | |
ulalume3@0 | 370 | # Stokes Input Vector after emitter optics equivalent to Eq. E.9 with already rotated input vector from Eq. E.4 |
ulalume3@0 | 371 | # b = beta |
binietoglou@19 | 372 | IinE = (IinL + DiE * C) |
binietoglou@19 | 373 | QinE = (C2b * DiE * IinL + A + S2b * (WiE * D - ZiE * SinE * VinL)) |
binietoglou@19 | 374 | UinE = (S2b * DiE * IinL + B - C2b * (WiE * D - ZiE * SinE * VinL)) |
binietoglou@19 | 375 | VinE = (-ZiE * SinE * D + ZiE * CosE * VinL) |
ulalume3@0 | 376 | |
ulalume3@0 | 377 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 378 | IinF = IinE |
binietoglou@19 | 379 | QinF = aCal * QinE |
binietoglou@19 | 380 | UinF = -aCal * UinE |
binietoglou@19 | 381 | VinF = (1. - 2. * aCal) * VinE |
ulalume3@0 | 382 | |
ulalume3@0 | 383 | # receiver optics |
ulalume3@0 | 384 | CosO = np.cos(np.deg2rad(RetO)) |
ulalume3@0 | 385 | SinO = np.sin(np.deg2rad(RetO)) |
binietoglou@19 | 386 | ZiO = (1. - DiO ** 2) ** 0.5 |
binietoglou@19 | 387 | WiO = (1. - ZiO * CosO) |
ulalume3@0 | 388 | |
ulalume3@0 | 389 | # calibrator |
ulalume3@0 | 390 | CosC = np.cos(np.deg2rad(RetC)) |
ulalume3@0 | 391 | SinC = np.sin(np.deg2rad(RetC)) |
binietoglou@19 | 392 | ZiC = (1. - DiC ** 2) ** 0.5 |
binietoglou@19 | 393 | WiC = (1. - ZiC * CosC) |
ulalume3@0 | 394 | |
ulalume3@0 | 395 | # Stokes Input Vector before the polarising beam splitter Eq. E.31 |
binietoglou@19 | 396 | A = C2g * QinE - S2g * UinE |
binietoglou@19 | 397 | B = S2g * QinE + C2g * UinE |
ulalume3@0 | 398 | |
binietoglou@19 | 399 | IinP = (IinE + DiO * aCal * A) |
binietoglou@19 | 400 | QinP = (C2g * DiO * IinE + aCal * QinE - S2g * (WiO * aCal * B + ZiO * SinO * (1 - 2 * aCal) * VinE)) |
binietoglou@19 | 401 | UinP = (S2g * DiO * IinE - aCal * UinE + C2g * (WiO * aCal * B + ZiO * SinO * (1 - 2 * aCal) * VinE)) |
binietoglou@19 | 402 | VinP = (ZiO * SinO * aCal * B + ZiO * CosO * (1 - 2 * aCal) * VinE) |
ulalume3@0 | 403 | |
binietoglou@19 | 404 | # ------------------------- |
ulalume3@0 | 405 | # F11 assuemd to be = 1 => measured: F11m = IinP / IinE with atrue |
binietoglou@19 | 406 | # F11sim = TiO*(IinE + DiO*atrue*A)/IinE |
binietoglou@19 | 407 | # ------------------------- |
ulalume3@0 | 408 | |
ulalume3@0 | 409 | # analyser |
binietoglou@19 | 410 | if (RS_RP_depend_on_TS_TP): |
volker@13 | 411 | RS = 1 - TS |
volker@13 | 412 | RP = 1 - TP |
volker@21 | 413 | |
ulalume3@0 | 414 | TiT = 0.5 * (TP + TS) |
binietoglou@19 | 415 | DiT = (TP - TS) / (TP + TS) |
binietoglou@19 | 416 | ZiT = (1. - DiT ** 2) ** 0.5 |
ulalume3@0 | 417 | TiR = 0.5 * (RP + RS) |
binietoglou@19 | 418 | DiR = (RP - RS) / (RP + RS) |
binietoglou@19 | 419 | ZiR = (1. - DiR ** 2) ** 0.5 |
ulalume3@0 | 420 | CosT = np.cos(np.deg2rad(RetT)) |
ulalume3@0 | 421 | SinT = np.sin(np.deg2rad(RetT)) |
ulalume3@0 | 422 | CosR = np.cos(np.deg2rad(RetR)) |
ulalume3@0 | 423 | SinR = np.sin(np.deg2rad(RetR)) |
ulalume3@0 | 424 | |
binietoglou@19 | 425 | DaT = (1 - ERaT) / (1 + ERaT) |
binietoglou@19 | 426 | DaR = (1 - ERaR) / (1 + ERaR) |
binietoglou@19 | 427 | TaT = 0.5 * (1 + ERaT) |
binietoglou@19 | 428 | TaR = 0.5 * (1 + ERaR) |
ulalume3@0 | 429 | |
binietoglou@19 | 430 | S2aT = np.sin(np.deg2rad(h * 2 * RotaT)) |
binietoglou@19 | 431 | C2aT = np.cos(np.deg2rad(2 * RotaT)) |
binietoglou@19 | 432 | S2aR = np.sin(np.deg2rad(h * 2 * RotaR)) |
binietoglou@19 | 433 | C2aR = np.cos(np.deg2rad(2 * RotaR)) |
ulalume3@0 | 434 | |
volker@28 | 435 | # Analyzer As before the PBS Eq. D.5; combined PBS and cleaning pol-filter |
volker@28 | 436 | ATPT = (1 + C2aT * DaT * DiT) # unpolarized transmission correction |
volker@28 | 437 | TTa = TiT * TaT * ATPT # unpolarized transmission |
volker@28 | 438 | ATP1 = 1 |
volker@28 | 439 | ATP2 = Y * (DiT + C2aT * DaT) / ATPT |
volker@28 | 440 | ATP3 = Y * S2aT * DaT * ZiT * CosT / ATPT |
volker@28 | 441 | ATP4 = S2aT * DaT * ZiT * SinT / ATPT |
binietoglou@19 | 442 | ATP = np.array([ATP1, ATP2, ATP3, ATP4]) |
volker@28 | 443 | DTa = ATP2 * Y |
ulalume3@0 | 444 | |
volker@28 | 445 | ARPT = (1 + C2aR * DaR * DiR) # unpolarized transmission correction |
volker@28 | 446 | TRa = TiR * TaR * ARPT # unpolarized transmission |
volker@28 | 447 | ARP1 = 1 |
volker@28 | 448 | ARP2 = Y * (DiR + C2aR * DaR) / ARPT |
volker@28 | 449 | ARP3 = Y * S2aR * DaR * ZiR * CosR / ARPT |
volker@28 | 450 | ARP4 = S2aR * DaR * ZiR * SinR / ARPT |
binietoglou@19 | 451 | ARP = np.array([ARP1, ARP2, ARP3, ARP4]) |
volker@28 | 452 | DRa = ARP2 * Y |
ulalume3@0 | 453 | |
ulalume3@0 | 454 | |
ulalume3@0 | 455 | # ---- Calculate signals and correction parameters for diffeent locations and calibrators |
ulalume3@0 | 456 | if LocC == 4: # Calibrator before the PBS |
binietoglou@19 | 457 | # print("Calibrator location not implemented yet") |
ulalume3@0 | 458 | |
binietoglou@19 | 459 | # S2ge = np.sin(np.deg2rad(2*RotO + h*2*RotC)) |
binietoglou@19 | 460 | # C2ge = np.cos(np.deg2rad(2*RotO + h*2*RotC)) |
binietoglou@19 | 461 | S2e = np.sin(np.deg2rad(h * 2 * RotC)) |
binietoglou@19 | 462 | C2e = np.cos(np.deg2rad(2 * RotC)) |
ulalume3@0 | 463 | # rotated AinP by epsilon Eq. C.3 |
binietoglou@19 | 464 | ATP2e = C2e * ATP2 + S2e * ATP3 |
binietoglou@19 | 465 | ATP3e = C2e * ATP3 - S2e * ATP2 |
binietoglou@19 | 466 | ARP2e = C2e * ARP2 + S2e * ARP3 |
binietoglou@19 | 467 | ARP3e = C2e * ARP3 - S2e * ARP2 |
binietoglou@19 | 468 | ATPe = np.array([ATP1, ATP2e, ATP3e, ATP4]) |
binietoglou@19 | 469 | ARPe = np.array([ARP1, ARP2e, ARP3e, ARP4]) |
ulalume3@0 | 470 | # Stokes Input Vector before the polarising beam splitter Eq. E.31 |
binietoglou@19 | 471 | A = C2g * QinE - S2g * UinE |
binietoglou@19 | 472 | B = S2g * QinE + C2g * UinE |
binietoglou@19 | 473 | # C = (WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE) |
binietoglou@19 | 474 | Co = ZiO * SinO * VinE |
binietoglou@19 | 475 | Ca = (WiO * B - 2 * ZiO * SinO * VinE) |
binietoglou@19 | 476 | # C = Co + aCal*Ca |
binietoglou@19 | 477 | # IinP = (IinE + DiO*aCal*A) |
binietoglou@19 | 478 | # QinP = (C2g*DiO*IinE + aCal*QinE - S2g*C) |
binietoglou@19 | 479 | # UinP = (S2g*DiO*IinE - aCal*UinE + C2g*C) |
binietoglou@19 | 480 | # VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE) |
ulalume3@0 | 481 | IinPo = IinE |
binietoglou@19 | 482 | QinPo = (C2g * DiO * IinE - S2g * Co) |
binietoglou@19 | 483 | UinPo = (S2g * DiO * IinE + C2g * Co) |
binietoglou@19 | 484 | VinPo = ZiO * CosO * VinE |
ulalume3@0 | 485 | |
binietoglou@19 | 486 | IinPa = DiO * A |
binietoglou@19 | 487 | QinPa = QinE - S2g * Ca |
binietoglou@19 | 488 | UinPa = -UinE + C2g * Ca |
binietoglou@19 | 489 | VinPa = ZiO * (SinO * B - 2 * CosO * VinE) |
ulalume3@0 | 490 | |
binietoglou@19 | 491 | IinP = IinPo + aCal * IinPa |
binietoglou@19 | 492 | QinP = QinPo + aCal * QinPa |
binietoglou@19 | 493 | UinP = UinPo + aCal * UinPa |
binietoglou@19 | 494 | VinP = VinPo + aCal * VinPa |
ulalume3@0 | 495 | # Stokes Input Vector before the polarising beam splitter rotated by epsilon Eq. C.3 |
binietoglou@19 | 496 | # QinPe = C2e*QinP + S2e*UinP |
binietoglou@19 | 497 | # UinPe = C2e*UinP - S2e*QinP |
binietoglou@19 | 498 | QinPoe = C2e * QinPo + S2e * UinPo |
binietoglou@19 | 499 | UinPoe = C2e * UinPo - S2e * QinPo |
binietoglou@19 | 500 | QinPae = C2e * QinPa + S2e * UinPa |
binietoglou@19 | 501 | UinPae = C2e * UinPa - S2e * QinPa |
binietoglou@19 | 502 | QinPe = C2e * QinP + S2e * UinP |
binietoglou@19 | 503 | UinPe = C2e * UinP - S2e * QinP |
ulalume3@0 | 504 | |
ulalume3@0 | 505 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 506 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
ulalume3@0 | 507 | # parameters for calibration with aCal |
binietoglou@19 | 508 | AT = ATP1 * IinP + h * ATP4 * VinP |
binietoglou@19 | 509 | BT = ATP3e * QinP - h * ATP2e * UinP |
binietoglou@19 | 510 | AR = ARP1 * IinP + h * ARP4 * VinP |
binietoglou@19 | 511 | BR = ARP3e * QinP - h * ARP2e * UinP |
volker@23 | 512 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 513 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 514 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 515 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 516 | GT = np.dot(ATP, IS1) |
binietoglou@19 | 517 | GR = np.dot(ARP, IS1) |
binietoglou@19 | 518 | HT = np.dot(ATP, IS2) |
binietoglou@19 | 519 | HR = np.dot(ARP, IS2) |
ulalume3@0 | 520 | else: |
binietoglou@19 | 521 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 522 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 523 | GT = np.dot(ATPe, IS1) |
binietoglou@19 | 524 | GR = np.dot(ARPe, IS1) |
binietoglou@19 | 525 | HT = np.dot(ATPe, IS2) |
binietoglou@19 | 526 | HR = np.dot(ARPe, IS2) |
ulalume3@0 | 527 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
ulalume3@0 | 528 | # parameters for calibration with aCal |
binietoglou@19 | 529 | AT = ATP1 * IinP + ATP3e * UinPe + ZiC * CosC * (ATP2e * QinPe + ATP4 * VinP) |
binietoglou@19 | 530 | BT = DiC * (ATP1 * UinPe + ATP3e * IinP) - ZiC * SinC * (ATP2e * VinP - ATP4 * QinPe) |
binietoglou@19 | 531 | AR = ARP1 * IinP + ARP3e * UinPe + ZiC * CosC * (ARP2e * QinPe + ARP4 * VinP) |
binietoglou@19 | 532 | BR = DiC * (ARP1 * UinPe + ARP3e * IinP) - ZiC * SinC * (ARP2e * VinP - ARP4 * QinPe) |
volker@23 | 533 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 534 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 535 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 536 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 537 | GT = np.dot(ATP, IS1) |
binietoglou@19 | 538 | GR = np.dot(ARP, IS1) |
binietoglou@19 | 539 | HT = np.dot(ATP, IS2) |
binietoglou@19 | 540 | HR = np.dot(ARP, IS2) |
ulalume3@0 | 541 | else: |
binietoglou@19 | 542 | IS1e = np.array([IinPo + DiC * QinPoe, DiC * IinPo + QinPoe, ZiC * (CosC * UinPoe + SinC * VinPo), |
binietoglou@19 | 543 | -ZiC * (SinC * UinPoe - CosC * VinPo)]) |
binietoglou@19 | 544 | IS2e = np.array([IinPa + DiC * QinPae, DiC * IinPa + QinPae, ZiC * (CosC * UinPae + SinC * VinPa), |
binietoglou@19 | 545 | -ZiC * (SinC * UinPae - CosC * VinPa)]) |
binietoglou@19 | 546 | GT = np.dot(ATPe, IS1e) |
binietoglou@19 | 547 | GR = np.dot(ARPe, IS1e) |
binietoglou@19 | 548 | HT = np.dot(ATPe, IS2e) |
binietoglou@19 | 549 | HR = np.dot(ARPe, IS2e) |
ulalume3@0 | 550 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 551 | # parameters for calibration with aCal |
binietoglou@19 | 552 | AT = ATP1 * IinP + sqr05 * DiC * (ATP1 * QinPe + ATP2e * IinP) + (1 - 0.5 * WiC) * ( |
binietoglou@19 | 553 | ATP2e * QinPe + ATP3e * UinPe) + ZiC * (sqr05 * SinC * (ATP3e * VinP - ATP4 * UinPe) + ATP4 * CosC * VinP) |
binietoglou@19 | 554 | BT = sqr05 * DiC * (ATP1 * UinPe + ATP3e * IinP) + 0.5 * WiC * ( |
binietoglou@19 | 555 | ATP2e * UinPe + ATP3e * QinPe) - sqr05 * ZiC * SinC * (ATP2e * VinP - ATP4 * QinPe) |
binietoglou@19 | 556 | AR = ARP1 * IinP + sqr05 * DiC * (ARP1 * QinPe + ARP2e * IinP) + (1 - 0.5 * WiC) * ( |
binietoglou@19 | 557 | ARP2e * QinPe + ARP3e * UinPe) + ZiC * (sqr05 * SinC * (ARP3e * VinP - ARP4 * UinPe) + ARP4 * CosC * VinP) |
binietoglou@19 | 558 | BR = sqr05 * DiC * (ARP1 * UinPe + ARP3e * IinP) + 0.5 * WiC * ( |
binietoglou@19 | 559 | ARP2e * UinPe + ARP3e * QinPe) - sqr05 * ZiC * SinC * (ARP2e * VinP - ARP4 * QinPe) |
volker@23 | 560 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 561 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 562 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 563 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 564 | GT = np.dot(ATP, IS1) |
binietoglou@19 | 565 | GR = np.dot(ARP, IS1) |
binietoglou@19 | 566 | HT = np.dot(ATP, IS2) |
binietoglou@19 | 567 | HR = np.dot(ARP, IS2) |
ulalume3@0 | 568 | else: |
binietoglou@19 | 569 | IS1e = np.array([IinPo + DiC * QinPoe, DiC * IinPo + QinPoe, ZiC * (CosC * UinPoe + SinC * VinPo), |
binietoglou@19 | 570 | -ZiC * (SinC * UinPoe - CosC * VinPo)]) |
binietoglou@19 | 571 | IS2e = np.array([IinPa + DiC * QinPae, DiC * IinPa + QinPae, ZiC * (CosC * UinPae + SinC * VinPa), |
binietoglou@19 | 572 | -ZiC * (SinC * UinPae - CosC * VinPa)]) |
binietoglou@19 | 573 | GT = np.dot(ATPe, IS1e) |
binietoglou@19 | 574 | GR = np.dot(ARPe, IS1e) |
binietoglou@19 | 575 | HT = np.dot(ATPe, IS2e) |
binietoglou@19 | 576 | HR = np.dot(ARPe, IS2e) |
ulalume3@0 | 577 | else: |
ulalume3@0 | 578 | print("Calibrator not implemented yet") |
ulalume3@0 | 579 | sys.exit() |
ulalume3@0 | 580 | |
ulalume3@0 | 581 | elif LocC == 3: # C before receiver optics Eq.57 |
ulalume3@0 | 582 | |
binietoglou@19 | 583 | # S2ge = np.sin(np.deg2rad(2*RotO - 2*RotC)) |
binietoglou@19 | 584 | # C2ge = np.cos(np.deg2rad(2*RotO - 2*RotC)) |
binietoglou@19 | 585 | S2e = np.sin(np.deg2rad(2 * RotC)) |
binietoglou@19 | 586 | C2e = np.cos(np.deg2rad(2 * RotC)) |
ulalume3@0 | 587 | |
ulalume3@0 | 588 | # As with C before the receiver optics (rotated_diattenuator_X22x5deg.odt) |
binietoglou@19 | 589 | AF1 = np.array([1, C2g * DiO, S2g * DiO, 0]) |
binietoglou@19 | 590 | AF2 = np.array([C2g * DiO, 1 - S2g ** 2 * WiO, S2g * C2g * WiO, -S2g * ZiO * SinO]) |
binietoglou@19 | 591 | AF3 = np.array([S2g * DiO, S2g * C2g * WiO, 1 - C2g ** 2 * WiO, C2g * ZiO * SinO]) |
binietoglou@19 | 592 | AF4 = np.array([0, S2g * SinO, -C2g * SinO, CosO]) |
ulalume3@0 | 593 | |
binietoglou@19 | 594 | ATF = (ATP1 * AF1 + ATP2 * AF2 + ATP3 * AF3 + ATP4 * AF4) |
binietoglou@19 | 595 | ARF = (ARP1 * AF1 + ARP2 * AF2 + ARP3 * AF3 + ARP4 * AF4) |
ulalume3@0 | 596 | ATF2 = ATF[1] |
ulalume3@0 | 597 | ATF3 = ATF[2] |
ulalume3@0 | 598 | ARF2 = ARF[1] |
ulalume3@0 | 599 | ARF3 = ARF[2] |
ulalume3@0 | 600 | |
ulalume3@0 | 601 | # rotated AinF by epsilon |
ulalume3@0 | 602 | ATF1 = ATF[0] |
ulalume3@0 | 603 | ATF4 = ATF[3] |
binietoglou@19 | 604 | ATF2e = C2e * ATF[1] + S2e * ATF[2] |
binietoglou@19 | 605 | ATF3e = C2e * ATF[2] - S2e * ATF[1] |
ulalume3@0 | 606 | ARF1 = ARF[0] |
ulalume3@0 | 607 | ARF4 = ARF[3] |
binietoglou@19 | 608 | ARF2e = C2e * ARF[1] + S2e * ARF[2] |
binietoglou@19 | 609 | ARF3e = C2e * ARF[2] - S2e * ARF[1] |
ulalume3@0 | 610 | |
binietoglou@19 | 611 | ATFe = np.array([ATF1, ATF2e, ATF3e, ATF4]) |
binietoglou@19 | 612 | ARFe = np.array([ARF1, ARF2e, ARF3e, ARF4]) |
ulalume3@0 | 613 | |
binietoglou@19 | 614 | QinEe = C2e * QinE + S2e * UinE |
binietoglou@19 | 615 | UinEe = C2e * UinE - S2e * QinE |
ulalume3@0 | 616 | |
ulalume3@0 | 617 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 618 | IinF = IinE |
binietoglou@19 | 619 | QinF = aCal * QinE |
binietoglou@19 | 620 | UinF = -aCal * UinE |
binietoglou@19 | 621 | VinF = (1. - 2. * aCal) * VinE |
ulalume3@0 | 622 | |
ulalume3@0 | 623 | IinFo = IinE |
ulalume3@0 | 624 | QinFo = 0. |
ulalume3@0 | 625 | UinFo = 0. |
ulalume3@0 | 626 | VinFo = VinE |
ulalume3@0 | 627 | |
ulalume3@0 | 628 | IinFa = 0. |
ulalume3@0 | 629 | QinFa = QinE |
ulalume3@0 | 630 | UinFa = -UinE |
binietoglou@19 | 631 | VinFa = -2. * VinE |
ulalume3@0 | 632 | |
ulalume3@0 | 633 | # Stokes Input Vector before receiver optics rotated by epsilon Eq. C.3 |
binietoglou@19 | 634 | QinFe = C2e * QinF + S2e * UinF |
binietoglou@19 | 635 | UinFe = C2e * UinF - S2e * QinF |
binietoglou@19 | 636 | QinFoe = C2e * QinFo + S2e * UinFo |
binietoglou@19 | 637 | UinFoe = C2e * UinFo - S2e * QinFo |
binietoglou@19 | 638 | QinFae = C2e * QinFa + S2e * UinFa |
binietoglou@19 | 639 | UinFae = C2e * UinFa - S2e * QinFa |
ulalume3@0 | 640 | |
ulalume3@0 | 641 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
binietoglou@19 | 642 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
ulalume3@0 | 643 | # parameters for calibration with aCal |
binietoglou@19 | 644 | AT = ATF1 * IinF + ATF4 * h * VinF |
binietoglou@19 | 645 | BT = ATF3e * QinF - ATF2e * h * UinF |
binietoglou@19 | 646 | AR = ARF1 * IinF + ARF4 * h * VinF |
binietoglou@19 | 647 | BR = ARF3e * QinF - ARF2e * h * UinF |
volker@23 | 648 | # Correction parameters for normal measurements; they are independent of LDR |
ulalume3@0 | 649 | if (not RotationErrorEpsilonForNormalMeasurements): |
binietoglou@19 | 650 | GT = ATF1 * IinE + ATF4 * VinE |
binietoglou@19 | 651 | GR = ARF1 * IinE + ARF4 * VinE |
binietoglou@19 | 652 | HT = ATF2 * QinE - ATF3 * UinE - ATF4 * 2 * VinE |
binietoglou@19 | 653 | HR = ARF2 * QinE - ARF3 * UinE - ARF4 * 2 * VinE |
ulalume3@0 | 654 | else: |
binietoglou@19 | 655 | GT = ATF1 * IinE + ATF4 * h * VinE |
binietoglou@19 | 656 | GR = ARF1 * IinE + ARF4 * h * VinE |
binietoglou@19 | 657 | HT = ATF2e * QinE - ATF3e * h * UinE - ATF4 * h * 2 * VinE |
binietoglou@19 | 658 | HR = ARF2e * QinE - ARF3e * h * UinE - ARF4 * h * 2 * VinE |
ulalume3@0 | 659 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
ulalume3@0 | 660 | # p = +45°, m = -45° |
binietoglou@19 | 661 | IF1e = np.array([IinF, ZiC * CosC * QinFe, UinFe, ZiC * CosC * VinF]) |
binietoglou@19 | 662 | IF2e = np.array([DiC * UinFe, -ZiC * SinC * VinF, DiC * IinF, ZiC * SinC * QinFe]) |
binietoglou@19 | 663 | AT = np.dot(ATFe, IF1e) |
binietoglou@19 | 664 | AR = np.dot(ARFe, IF1e) |
binietoglou@19 | 665 | BT = np.dot(ATFe, IF2e) |
binietoglou@19 | 666 | BR = np.dot(ARFe, IF2e) |
ulalume3@0 | 667 | |
volker@23 | 668 | # Correction parameters for normal measurements; they are independent of LDR --- the same as for TypeC = 6 |
binietoglou@19 | 669 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 670 | IS1 = np.array([IinE, 0, 0, VinE]) |
binietoglou@19 | 671 | IS2 = np.array([0, QinE, -UinE, -2 * VinE]) |
binietoglou@19 | 672 | GT = np.dot(ATF, IS1) |
binietoglou@19 | 673 | GR = np.dot(ARF, IS1) |
binietoglou@19 | 674 | HT = np.dot(ATF, IS2) |
binietoglou@19 | 675 | HR = np.dot(ARF, IS2) |
ulalume3@0 | 676 | else: |
binietoglou@19 | 677 | IS1e = np.array([IinFo + DiC * QinFoe, DiC * IinFo + QinFoe, ZiC * (CosC * UinFoe + SinC * VinFo), |
binietoglou@19 | 678 | -ZiC * (SinC * UinFoe - CosC * VinFo)]) |
binietoglou@19 | 679 | IS2e = np.array([IinFa + DiC * QinFae, DiC * IinFa + QinFae, ZiC * (CosC * UinFae + SinC * VinFa), |
binietoglou@19 | 680 | -ZiC * (SinC * UinFae - CosC * VinFa)]) |
binietoglou@19 | 681 | GT = np.dot(ATFe, IS1e) |
binietoglou@19 | 682 | GR = np.dot(ARFe, IS1e) |
binietoglou@19 | 683 | HT = np.dot(ATFe, IS2e) |
binietoglou@19 | 684 | HR = np.dot(ARFe, IS2e) |
ulalume3@0 | 685 | |
ulalume3@0 | 686 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 687 | # parameters for calibration with aCal |
binietoglou@19 | 688 | IF1e = np.array([IinF + sqr05 * DiC * QinFe, sqr05 * DiC * IinF + (1 - 0.5 * WiC) * QinFe, |
binietoglou@19 | 689 | (1 - 0.5 * WiC) * UinFe + sqr05 * ZiC * SinC * VinF, |
binietoglou@19 | 690 | -sqr05 * ZiC * SinC * UinFe + ZiC * CosC * VinF]) |
binietoglou@19 | 691 | IF2e = np.array([sqr05 * DiC * UinFe, 0.5 * WiC * UinFe - sqr05 * ZiC * SinC * VinF, |
binietoglou@19 | 692 | sqr05 * DiC * IinF + 0.5 * WiC * QinFe, sqr05 * ZiC * SinC * QinFe]) |
binietoglou@19 | 693 | AT = np.dot(ATFe, IF1e) |
binietoglou@19 | 694 | AR = np.dot(ARFe, IF1e) |
binietoglou@19 | 695 | BT = np.dot(ATFe, IF2e) |
binietoglou@19 | 696 | BR = np.dot(ARFe, IF2e) |
ulalume3@0 | 697 | |
volker@23 | 698 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 699 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 700 | # IS1 = np.array([IinE,0,0,VinE]) |
binietoglou@19 | 701 | # IS2 = np.array([0,QinE,-UinE,-2*VinE]) |
binietoglou@19 | 702 | IS1 = np.array([IinFo, 0, 0, VinFo]) |
binietoglou@19 | 703 | IS2 = np.array([0, QinFa, UinFa, VinFa]) |
binietoglou@19 | 704 | GT = np.dot(ATF, IS1) |
binietoglou@19 | 705 | GR = np.dot(ARF, IS1) |
binietoglou@19 | 706 | HT = np.dot(ATF, IS2) |
binietoglou@19 | 707 | HR = np.dot(ARF, IS2) |
ulalume3@0 | 708 | else: |
binietoglou@19 | 709 | IS1e = np.array([IinFo + DiC * QinFoe, DiC * IinFo + QinFoe, ZiC * (CosC * UinFoe + SinC * VinFo), |
binietoglou@19 | 710 | -ZiC * (SinC * UinFoe - CosC * VinFo)]) |
binietoglou@19 | 711 | IS2e = np.array([IinFa + DiC * QinFae, DiC * IinFa + QinFae, ZiC * (CosC * UinFae + SinC * VinFa), |
binietoglou@19 | 712 | -ZiC * (SinC * UinFae - CosC * VinFa)]) |
binietoglou@19 | 713 | # IS1e = np.array([IinFo,0,0,VinFo]) |
binietoglou@19 | 714 | # IS2e = np.array([0,QinFae,UinFae,VinFa]) |
binietoglou@19 | 715 | GT = np.dot(ATFe, IS1e) |
binietoglou@19 | 716 | GR = np.dot(ARFe, IS1e) |
binietoglou@19 | 717 | HT = np.dot(ATFe, IS2e) |
binietoglou@19 | 718 | HR = np.dot(ARFe, IS2e) |
ulalume3@0 | 719 | |
ulalume3@0 | 720 | else: |
ulalume3@0 | 721 | print('Calibrator not implemented yet') |
ulalume3@0 | 722 | sys.exit() |
ulalume3@0 | 723 | |
ulalume3@0 | 724 | elif LocC == 2: # C behind emitter optics Eq.57 ------------------------------------------------------- |
binietoglou@19 | 725 | # print("Calibrator location not implemented yet") |
binietoglou@19 | 726 | S2e = np.sin(np.deg2rad(2 * RotC)) |
binietoglou@19 | 727 | C2e = np.cos(np.deg2rad(2 * RotC)) |
ulalume3@0 | 728 | |
ulalume3@0 | 729 | # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt) |
binietoglou@19 | 730 | AF1 = np.array([1, C2g * DiO, S2g * DiO, 0]) |
binietoglou@19 | 731 | AF2 = np.array([C2g * DiO, 1 - S2g ** 2 * WiO, S2g * C2g * WiO, -S2g * ZiO * SinO]) |
binietoglou@19 | 732 | AF3 = np.array([S2g * DiO, S2g * C2g * WiO, 1 - C2g ** 2 * WiO, C2g * ZiO * SinO]) |
binietoglou@19 | 733 | AF4 = np.array([0, S2g * SinO, -C2g * SinO, CosO]) |
ulalume3@0 | 734 | |
binietoglou@19 | 735 | ATF = (ATP1 * AF1 + ATP2 * AF2 + ATP3 * AF3 + ATP4 * AF4) |
binietoglou@19 | 736 | ARF = (ARP1 * AF1 + ARP2 * AF2 + ARP3 * AF3 + ARP4 * AF4) |
ulalume3@0 | 737 | ATF1 = ATF[0] |
ulalume3@0 | 738 | ATF2 = ATF[1] |
ulalume3@0 | 739 | ATF3 = ATF[2] |
ulalume3@0 | 740 | ATF4 = ATF[3] |
ulalume3@0 | 741 | ARF1 = ARF[0] |
ulalume3@0 | 742 | ARF2 = ARF[1] |
ulalume3@0 | 743 | ARF3 = ARF[2] |
ulalume3@0 | 744 | ARF4 = ARF[3] |
ulalume3@0 | 745 | |
ulalume3@0 | 746 | # AS with C behind the emitter |
ulalume3@0 | 747 | # terms without aCal |
ulalume3@0 | 748 | ATE1o, ARE1o = ATF1, ARF1 |
ulalume3@0 | 749 | ATE2o, ARE2o = 0., 0. |
ulalume3@0 | 750 | ATE3o, ARE3o = 0., 0. |
ulalume3@0 | 751 | ATE4o, ARE4o = ATF4, ARF4 |
ulalume3@0 | 752 | # terms with aCal |
binietoglou@19 | 753 | ATE1a, ARE1a = 0., 0. |
ulalume3@0 | 754 | ATE2a, ARE2a = ATF2, ARF2 |
ulalume3@0 | 755 | ATE3a, ARE3a = -ATF3, -ARF3 |
binietoglou@19 | 756 | ATE4a, ARE4a = -2 * ATF4, -2 * ARF4 |
ulalume3@0 | 757 | # rotated AinEa by epsilon |
binietoglou@19 | 758 | ATE2ae = C2e * ATF2 + S2e * ATF3 |
binietoglou@19 | 759 | ATE3ae = -S2e * ATF2 - C2e * ATF3 |
binietoglou@19 | 760 | ARE2ae = C2e * ARF2 + S2e * ARF3 |
binietoglou@19 | 761 | ARE3ae = -S2e * ARF2 - C2e * ARF3 |
ulalume3@0 | 762 | |
ulalume3@0 | 763 | ATE1 = ATE1o |
binietoglou@19 | 764 | ATE2e = aCal * ATE2ae |
binietoglou@19 | 765 | ATE3e = aCal * ATE3ae |
binietoglou@19 | 766 | ATE4 = (1 - 2 * aCal) * ATF4 |
ulalume3@0 | 767 | ARE1 = ARE1o |
binietoglou@19 | 768 | ARE2e = aCal * ARE2ae |
binietoglou@19 | 769 | ARE3e = aCal * ARE3ae |
binietoglou@19 | 770 | ARE4 = (1 - 2 * aCal) * ARF4 |
ulalume3@0 | 771 | |
ulalume3@0 | 772 | # rotated IinE |
binietoglou@19 | 773 | QinEe = C2e * QinE + S2e * UinE |
binietoglou@19 | 774 | UinEe = C2e * UinE - S2e * QinE |
ulalume3@0 | 775 | |
ulalume3@0 | 776 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
binietoglou@19 | 777 | if (TypeC == 2) or (TypeC == 1): # +++++++++ rotator calibration Eq. C.4 |
binietoglou@19 | 778 | AT = ATE1o * IinE + (ATE4o + aCal * ATE4a) * h * VinE |
binietoglou@19 | 779 | BT = aCal * (ATE3ae * QinEe - ATE2ae * h * UinEe) |
binietoglou@19 | 780 | AR = ARE1o * IinE + (ARE4o + aCal * ARE4a) * h * VinE |
binietoglou@19 | 781 | BR = aCal * (ARE3ae * QinEe - ARE2ae * h * UinEe) |
ulalume3@0 | 782 | |
volker@23 | 783 | # Correction parameters for normal measurements; they are independent of LDR |
ulalume3@0 | 784 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 785 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
binietoglou@19 | 786 | GT = ATE1o * IinE + ATE4o * h * VinE |
binietoglou@19 | 787 | GR = ARE1o * IinE + ARE4o * h * VinE |
binietoglou@19 | 788 | HT = ATE2a * QinE + ATE3a * h * UinEe + ATE4a * h * VinE |
binietoglou@19 | 789 | HR = ARE2a * QinE + ARE3a * h * UinEe + ARE4a * h * VinE |
ulalume3@0 | 790 | else: |
binietoglou@19 | 791 | GT = ATE1o * IinE + ATE4o * h * VinE |
binietoglou@19 | 792 | GR = ARE1o * IinE + ARE4o * h * VinE |
binietoglou@19 | 793 | HT = ATE2ae * QinE + ATE3ae * h * UinEe + ATE4a * h * VinE |
binietoglou@19 | 794 | HR = ARE2ae * QinE + ARE3ae * h * UinEe + ARE4a * h * VinE |
ulalume3@0 | 795 | |
ulalume3@0 | 796 | elif (TypeC == 3) or (TypeC == 4): # +++++++++ linear polariser calibration Eq. C.5 |
ulalume3@0 | 797 | # p = +45°, m = -45° |
binietoglou@19 | 798 | AT = ATE1 * IinE + ZiC * CosC * (ATE2e * QinEe + ATE4 * VinE) + ATE3e * UinEe |
binietoglou@19 | 799 | BT = DiC * (ATE1 * UinEe + ATE3e * IinE) + ZiC * SinC * (ATE4 * QinEe - ATE2e * VinE) |
binietoglou@19 | 800 | AR = ARE1 * IinE + ZiC * CosC * (ARE2e * QinEe + ARE4 * VinE) + ARE3e * UinEe |
binietoglou@19 | 801 | BR = DiC * (ARE1 * UinEe + ARE3e * IinE) + ZiC * SinC * (ARE4 * QinEe - ARE2e * VinE) |
ulalume3@0 | 802 | |
volker@23 | 803 | # Correction parameters for normal measurements; they are independent of LDR |
ulalume3@0 | 804 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 805 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
binietoglou@19 | 806 | GT = ATE1o * IinE + ATE4o * VinE |
binietoglou@19 | 807 | GR = ARE1o * IinE + ARE4o * VinE |
binietoglou@19 | 808 | HT = ATE2a * QinE + ATE3a * UinE + ATE4a * VinE |
binietoglou@19 | 809 | HR = ARE2a * QinE + ARE3a * UinE + ARE4a * VinE |
ulalume3@0 | 810 | else: |
binietoglou@19 | 811 | D = IinE + DiC * QinEe |
binietoglou@19 | 812 | A = DiC * IinE + QinEe |
binietoglou@19 | 813 | B = ZiC * (CosC * UinEe + SinC * VinE) |
binietoglou@19 | 814 | C = -ZiC * (SinC * UinEe - CosC * VinE) |
binietoglou@19 | 815 | GT = ATE1o * D + ATE4o * C |
binietoglou@19 | 816 | GR = ARE1o * D + ARE4o * C |
binietoglou@19 | 817 | HT = ATE2a * A + ATE3a * B + ATE4a * C |
binietoglou@19 | 818 | HR = ARE2a * A + ARE3a * B + ARE4a * C |
ulalume3@0 | 819 | |
ulalume3@0 | 820 | elif (TypeC == 6): # real HWP calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 821 | # p = +22.5°, m = -22.5° |
binietoglou@19 | 822 | IE1e = np.array([IinE + sqr05 * DiC * QinEe, sqr05 * DiC * IinE + (1 - 0.5 * WiC) * QinEe, |
binietoglou@19 | 823 | (1 - 0.5 * WiC) * UinEe + sqr05 * ZiC * SinC * VinE, |
binietoglou@19 | 824 | -sqr05 * ZiC * SinC * UinEe + ZiC * CosC * VinE]) |
binietoglou@19 | 825 | IE2e = np.array([sqr05 * DiC * UinEe, 0.5 * WiC * UinEe - sqr05 * ZiC * SinC * VinE, |
binietoglou@19 | 826 | sqr05 * DiC * IinE + 0.5 * WiC * QinEe, sqr05 * ZiC * SinC * QinEe]) |
binietoglou@19 | 827 | ATEe = np.array([ATE1, ATE2e, ATE3e, ATE4]) |
binietoglou@19 | 828 | AREe = np.array([ARE1, ARE2e, ARE3e, ARE4]) |
binietoglou@19 | 829 | AT = np.dot(ATEe, IE1e) |
binietoglou@19 | 830 | AR = np.dot(AREe, IE1e) |
binietoglou@19 | 831 | BT = np.dot(ATEe, IE2e) |
binietoglou@19 | 832 | BR = np.dot(AREe, IE2e) |
ulalume3@0 | 833 | |
volker@23 | 834 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 835 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 836 | GT = ATE1o * IinE + ATE4o * VinE |
binietoglou@19 | 837 | GR = ARE1o * IinE + ARE4o * VinE |
binietoglou@19 | 838 | HT = ATE2a * QinE + ATE3a * UinE + ATE4a * VinE |
binietoglou@19 | 839 | HR = ARE2a * QinE + ARE3a * UinE + ARE4a * VinE |
ulalume3@0 | 840 | else: |
binietoglou@19 | 841 | D = IinE + DiC * QinEe |
binietoglou@19 | 842 | A = DiC * IinE + QinEe |
binietoglou@19 | 843 | B = ZiC * (CosC * UinEe + SinC * VinE) |
binietoglou@19 | 844 | C = -ZiC * (SinC * UinEe - CosC * VinE) |
binietoglou@19 | 845 | GT = ATE1o * D + ATE4o * C |
binietoglou@19 | 846 | GR = ARE1o * D + ARE4o * C |
binietoglou@19 | 847 | HT = ATE2a * A + ATE3a * B + ATE4a * C |
binietoglou@19 | 848 | HR = ARE2a * A + ARE3a * B + ARE4a * C |
ulalume3@0 | 849 | |
ulalume3@0 | 850 | else: |
ulalume3@0 | 851 | print('Calibrator not implemented yet') |
ulalume3@0 | 852 | sys.exit() |
ulalume3@0 | 853 | |
ulalume3@0 | 854 | else: |
ulalume3@0 | 855 | print("Calibrator location not implemented yet") |
ulalume3@0 | 856 | sys.exit() |
ulalume3@0 | 857 | |
volker@28 | 858 | # Determination of the correction K of the calibration factor. |
volker@28 | 859 | IoutTp = TTa * TiC * TiO * TiE * (AT + BT) |
volker@28 | 860 | IoutTm = TTa * TiC * TiO * TiE * (AT - BT) |
volker@28 | 861 | IoutRp = TRa * TiC * TiO * TiE * (AR + BR) |
volker@28 | 862 | IoutRm = TRa * TiC * TiO * TiE * (AR - BR) |
ulalume3@0 | 863 | # --- Results and Corrections; electronic etaR and etaT are assumed to be 1 |
binietoglou@19 | 864 | Etapx = IoutRp / IoutTp |
binietoglou@19 | 865 | Etamx = IoutRm / IoutTm |
binietoglou@19 | 866 | Etax = (Etapx * Etamx) ** 0.5 |
ulalume3@0 | 867 | |
volker@28 | 868 | Eta = (TRa / TTa) # = TRa / TTa; Eta = Eta*/K Eq. 84 => K = Eta* / Eta; equation corrected according to the papers supplement Eqs. (S.10.10.1) ff |
ulalume3@0 | 869 | K = Etax / Eta |
ulalume3@0 | 870 | |
ulalume3@0 | 871 | # For comparison with Volkers Libreoffice Müller Matrix spreadsheet |
binietoglou@19 | 872 | # Eta_test_p = (IoutRp/IoutTp) |
binietoglou@19 | 873 | # Eta_test_m = (IoutRm/IoutTm) |
binietoglou@19 | 874 | # Eta_test = (Eta_test_p*Eta_test_m)**0.5 |
ulalume3@0 | 875 | |
volker@28 | 876 | # ----- random error calculation ---------- |
volker@28 | 877 | # noise must be calculated with the photon counts of measured signals; |
volker@28 | 878 | # relative standard deviation of calibration signals with LDRcal; assumed to be statisitcally independent |
volker@28 | 879 | # normalised noise errors |
volker@28 | 880 | if (CalcFrom0deg): |
volker@28 | 881 | dIoutTp = (NCalT * IoutTp) ** -0.5 |
volker@28 | 882 | dIoutTm = (NCalT * IoutTm) ** -0.5 |
volker@28 | 883 | dIoutRp = (NCalR * IoutRp) ** -0.5 |
volker@28 | 884 | dIoutRm = (NCalR * IoutRm) ** -0.5 |
volker@28 | 885 | else: |
volker@28 | 886 | dIoutTp = (NCalT ** -0.5) |
volker@28 | 887 | dIoutTm = (NCalT ** -0.5) |
volker@28 | 888 | dIoutRp = (NCalR ** -0.5) |
volker@28 | 889 | dIoutRm = (NCalR ** -0.5) |
volker@28 | 890 | # Forward simulated 0°-signals with LDRCal with atrue; from input file |
volker@28 | 891 | |
volker@28 | 892 | It = TTa * TiO * TiE * (GT + atrue * HT) |
volker@28 | 893 | Ir = TRa * TiO * TiE * (GR + atrue * HR) |
volker@28 | 894 | # relative standard deviation of standard signals with LDRmeas; assumed to be statisitcally independent |
volker@28 | 895 | if (CalcFrom0deg): |
volker@28 | 896 | dIt = ((NCalT * It / IoutTp * NILfac / TCalT) ** -0.5) |
volker@28 | 897 | dIr = ((NCalR * Ir / IoutRp * NILfac / TCalR) ** -0.5) |
volker@28 | 898 | else: |
volker@28 | 899 | dIt = ((NCalT * 2 * NILfac / TCalT ) ** -0.5) * It |
volker@28 | 900 | dIr = ((NCalR * 2 * NILfac / TCalR) ** -0.5) * Ir |
volker@28 | 901 | |
volker@28 | 902 | # ----- Forward simulated LDRsim = 1/Eta*Ir/It # simulated LDR* with Y from input file |
binietoglou@19 | 903 | LDRsim = Ir / It # simulated uncorrected LDR with Y from input file |
ulalume3@0 | 904 | # Corrected LDRsimCorr from forward simulated LDRsim (atrue) |
ulalume3@0 | 905 | # LDRsimCorr = (1./Eta*LDRsim*(GT+HT)-(GR+HR))/((GR-HR)-1./Eta*LDRsim*(GT-HT)) |
volker@26 | 906 | ''' |
volker@26 | 907 | if ((Y == -1.) and (abs(RotL0) < 45)) or ((Y == +1.) and (abs(RotL0) > 45)): |
volker@26 | 908 | LDRsimx = 1. / LDRsim / Etax |
ulalume3@0 | 909 | else: |
volker@26 | 910 | LDRsimx = LDRsim / Etax |
volker@28 | 911 | ''' |
volker@26 | 912 | LDRsimx = LDRsim |
ulalume3@0 | 913 | |
ulalume3@0 | 914 | # The following is correct without doubt |
volker@28 | 915 | # LDRCorr = (LDRsim/(Etax/K)*(GT+HT)-(GR+HR))/((GR-HR)-LDRsim/(Etax/K)*(GT-HT)) |
ulalume3@0 | 916 | |
ulalume3@0 | 917 | # The following is a test whether the equations for calibration Etax and normal signal (GHK, LDRsim) are consistent |
volker@28 | 918 | LDRCorr = (LDRsim / (Etax / K) * (GT + HT) - (GR + HR)) / ((GR - HR) - LDRsim / (Etax / K) * (GT - HT)) |
volker@28 | 919 | # here we could also use Eta instead of Etax / K => how to test whether Etax is correct? => comparison with MüllerMatrix simulation! |
volker@28 | 920 | # Without any correction: only measured It, Ir, EtaX are used |
volker@28 | 921 | LDRunCorr = (LDRsim / Etax * (GT / abs(GT) + HT / abs(HT)) - (GR / abs(GR) + HR / abs(HR))) / ((GR / abs(GR) - HR / abs(HR)) - LDRsim / Etax * (GT / abs(GT) - HT / abs(HT))) |
ulalume3@0 | 922 | |
volker@28 | 923 | #LDRCorr = LDRsimx # for test only |
volker@28 | 924 | |
volker@28 | 925 | F11sim = 1 / (TiO * TiE) * ((HR * Eta * It - HT * Ir) / (HR * GT - HT * GR)) # IL = 1, Etat = Etar = 1 ; AMT Eq.64; what is Etax/K? => see about 20 lines above: = Eta |
ulalume3@0 | 926 | |
volker@28 | 927 | return (IoutTp, IoutTm, IoutRp, IoutRm, It, Ir, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr, |
volker@28 | 928 | GT, HT, GR, HR, K, Eta, LDRsimx, LDRCorr, DTa, DRa, TTa, TRa, F11sim, LDRunCorr) |
volker@28 | 929 | |
binietoglou@19 | 930 | |
binietoglou@19 | 931 | |
ulalume3@0 | 932 | # ******************************************************************************************************************************* |
ulalume3@0 | 933 | |
volker@28 | 934 | # --- CALC with assumed true parameters from the input file |
volker@28 | 935 | IoutTp0, IoutTm0, IoutRp0, IoutRm0, It0, Ir0, dIoutTp0, dIoutTm0, dIoutRp0, dIoutRm0, dIt0, dIr0, \ |
volker@28 | 936 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0, LDRunCorr = \ |
volker@28 | 937 | Calc(TCalT, TCalR, NCalT, NCalR, DOLP0, RotL0, RotE0, RetE0, DiE0, |
volker@28 | 938 | RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, |
volker@28 | 939 | ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
volker@28 | 940 | Etax0 = K0 * Eta0 |
volker@13 | 941 | # --- Print parameters to console and output file |
volker@28 | 942 | with open('output_files\\' + LID + '-' + InputFile[0:-3] + '-GHK.dat', 'w') as f: |
ulalume3@0 | 943 | with redirect_stdout(f): |
volker@28 | 944 | print("From folder", dname) |
volker@28 | 945 | print("Running prog", fname) |
volker@28 | 946 | print("Version", ScriptVersion) |
binietoglou@19 | 947 | print("Reading input file ", InputFile) # , " for Lidar system :", EID, ", ", LID) |
ulalume3@0 | 948 | print("for Lidar system: ", EID, ", ", LID) |
ulalume3@0 | 949 | # --- Print iput information********************************* |
ulalume3@0 | 950 | print(" --- Input parameters: value ±error / ±steps ----------------------") |
volker@28 | 951 | print("{0:5}{1:5} {2:6.4f}±{3:7.4f}/{4:2d}; {5:8} {6:8.4f}±{7:7.4f}/{8:2d}".format( |
volker@28 | 952 | "Laser: ", "DOLP =", DOLP0, dDOLP, nDOLP," Rotation alpha = ", RotL0, dRotL, nRotL)) |
ulalume3@0 | 953 | print(" Diatt., Tunpol, Retard., Rotation (deg)") |
binietoglou@19 | 954 | print("{0:12} {1:7.4f}±{2:7.4f}/{8:2d}, {3:7.4f}, {4:3.0f}±{5:3.0f}/{9:2d}, {6:7.4f}±{7:7.4f}/{10:2d}".format( |
binietoglou@19 | 955 | "Emitter ", DiE0, dDiE, TiE, RetE0, dRetE, RotE0, dRotE, nDiE, nRetE, nRotE)) |
binietoglou@19 | 956 | print("{0:12} {1:7.4f}±{2:7.4f}/{8:2d}, {3:7.4f}, {4:3.0f}±{5:3.0f}/{9:2d}, {6:7.4f}±{7:7.4f}/{10:2d}".format( |
binietoglou@19 | 957 | "Receiver ", DiO0, dDiO, TiO, RetO0, dRetO, RotO0, dRotO, nDiO, nRetO, nRotO)) |
binietoglou@19 | 958 | print("{0:12} {1:7.4f}±{2:7.4f}/{8:2d}, {3:7.4f}, {4:3.0f}±{5:3.0f}/{9:2d}, {6:7.4f}±{7:7.4f}/{10:2d}".format( |
binietoglou@19 | 959 | "Calibrator ", DiC0, dDiC, TiC, RetC0, dRetC, RotC0, dRotC, nDiC, nRetC, nRotC)) |
ulalume3@0 | 960 | print("{0:12}".format(" --- Pol.-filter ---")) |
volker@28 | 961 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format( |
volker@28 | 962 | "ERT, RotT :", ERaT0, dERaT, nERaT, RotaT0, dRotaT, nRotaT)) |
volker@28 | 963 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format( |
volker@28 | 964 | "ERR, RotR :", ERaR0, dERaR, nERaR, RotaR0, dRotaR, nRotaR)) |
ulalume3@0 | 965 | print("{0:12}".format(" --- PBS ---")) |
volker@28 | 966 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format( |
volker@28 | 967 | "TP,TS :", TP0, dTP, nTP, TS0, dTS, nTS)) |
volker@28 | 968 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format( |
volker@28 | 969 | "RP,RS :", RP0, dRP, nRP, RS0, dRS, nRS)) |
volker@28 | 970 | print("{0:12}{1:7.4f},{2:7.4f}, {3:7.4f},{4:7.4f}, {5:1.0f}".format( |
volker@28 | 971 | "DT,TT,DR,TR,Y :", DiT, TiT, DiR, TiR, Y)) |
ulalume3@0 | 972 | print("{0:12}".format(" --- Combined PBS + Pol.-filter ---")) |
volker@28 | 973 | print("{0:12}{1:7.4f},{2:7.4f}, {3:7.4f},{4:7.4f}".format( |
volker@28 | 974 | "DT,TT,DR,TR :", DTa0, TTa0, DRa0, TRa0)) |
volker@28 | 975 | print("{0:26}: {1:6.3f}± {2:5.3f}/{3:2d}".format( |
volker@28 | 976 | "LDRCal during calibration in calibration range", LDRCal0, dLDRCal, nLDRCal)) |
volker@28 | 977 | print("{0:12}".format(" --- Additional ND filter attenuation (transmission) during the calibration ---")) |
volker@28 | 978 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format( |
volker@28 | 979 | "TCalT,TCalR :", TCalT0, dTCalT, nTCalT, TCalR0, dTCalR, nTCalR)) |
ulalume3@0 | 980 | print() |
ulalume3@0 | 981 | print("Rotation Error Epsilon For Normal Measurements = ", RotationErrorEpsilonForNormalMeasurements) |
volker@13 | 982 | print(Type[TypeC], Loc[LocC]) |
binietoglou@19 | 983 | print("Parallel signal detected in", dY[int(Y + 1)]) |
volker@13 | 984 | print("RS_RP_depend_on_TS_TP = ", RS_RP_depend_on_TS_TP) |
ulalume3@0 | 985 | # end of print actual system parameters |
ulalume3@0 | 986 | # ****************************************************************************** |
ulalume3@0 | 987 | |
binietoglou@19 | 988 | # print() |
binietoglou@19 | 989 | # print(" --- LDRCal during calibration | simulated and corrected LDRs -------------") |
binietoglou@19 | 990 | # print("{0:8} |{1:8}->{2:8},{3:9}->{4:9} |{5:8}->{6:8}".format(" LDRCal"," LDRtrue", " LDRsim"," LDRtrue2", " LDRsim2", " LDRmeas", " LDRcorr")) |
binietoglou@19 | 991 | # print("{0:8.5f} |{1:8.5f}->{2:8.5f},{3:9.5f}->{4:9.5f} |{5:8.5f}->{6:8.5f}".format(LDRCal, LDRtrue, LDRsim, LDRtrue2, LDRsim2, LDRmeas, LDRCorr)) |
binietoglou@19 | 992 | # print("{0:8} |{1:8}->{2:8}->{3:8}".format(" LDRCal"," LDRtrue", " LDRsimx", " LDRcorr")) |
binietoglou@19 | 993 | # print("{0:6.3f}±{1:5.3f}/{2:2d}|{3:8.5f}->{4:8.5f}->{5:8.5f}".format(LDRCal0, dLDRCal, nLDRCal, LDRtrue, LDRsimx, LDRCorr)) |
binietoglou@19 | 994 | # print("{0:8} |{1:8}->{2:8}->{3:8}".format(" LDRCal"," LDRtrue", " LDRsimx", " LDRcorr")) |
binietoglou@19 | 995 | # print(" --- LDRCal during calibration") |
ulalume3@0 | 996 | |
binietoglou@19 | 997 | # print("{0:8}={1:8.5f};{2:8}={3:8.5f}".format(" IinP",IinP," F11sim",F11sim)) |
ulalume3@0 | 998 | print() |
ulalume3@0 | 999 | |
volker@28 | 1000 | K0List = np.zeros(6) |
volker@28 | 1001 | LDRsimxList = np.zeros(6) |
volker@28 | 1002 | LDRCalList = 0.004, 0.02, 0.1, 0.2, 0.3, 0.45 |
volker@21 | 1003 | # The loop over LDRCalList is ony for checking whether and how much the LDR depends on the LDRCal during calibration and whether the corrections work. |
volker@21 | 1004 | # Still with assumed true parameters in input file |
volker@28 | 1005 | |
volker@28 | 1006 | facIt = NCalT / TCalT0 * NILfac |
volker@28 | 1007 | facIr = NCalR / TCalR0 * NILfac |
volker@28 | 1008 | print("IoutTp, IoutTm, IoutRp, IoutRm, It , Ir , dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr") |
volker@28 | 1009 | |
binietoglou@19 | 1010 | for i, LDRCal in enumerate(LDRCalList): |
volker@28 | 1011 | IoutTp, IoutTm, IoutRp, IoutRm, It, Ir, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr, \ |
volker@28 | 1012 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0, LDRunCorr = \ |
volker@28 | 1013 | Calc(TCalT0, TCalR0, NCalT, NCalR, DOLP0, RotL0, RotE0, RetE0, DiE0, |
volker@28 | 1014 | RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, |
volker@28 | 1015 | ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal) |
ulalume3@0 | 1016 | K0List[i] = K0 |
ulalume3@0 | 1017 | LDRsimxList[i] = LDRsimx |
ulalume3@0 | 1018 | |
volker@28 | 1019 | # check error signals |
volker@28 | 1020 | # print( "{:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}" |
volker@28 | 1021 | # .format(IoutTp * NCalT, IoutTm * NCalT, IoutRp * NCalR, IoutRm * NCalR, It * facIt, Ir * facIr, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr)) |
volker@28 | 1022 | #print( "{:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}".format(IoutTp, IoutTm, IoutRp, IoutRm, It, Ir, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr)) |
volker@28 | 1023 | # end check error signals |
volker@28 | 1024 | print('===========================================================================================================') |
volker@28 | 1025 | print("{0:8},{1:8},{2:8},{3:8},{4:9},{5:8},{6:9},{7:9},{8:9},{9:9}".format( |
volker@28 | 1026 | " GR", " GT", " HR", " HT", " K(0.004)", " K(0.02)", " K(0.1)", " K(0.2)", " K(0.3)", " K(0.45)")) |
volker@28 | 1027 | print("{0:8.5f},{1:8.5f},{2:8.5f},{3:8.5f},{4:9.5f},{5:9.5f},{6:9.5f},{7:9.5f},{8:9.5f},{9:9.5f}".format( |
volker@28 | 1028 | GR0, GT0, HR0, HT0, K0List[0], K0List[1], K0List[2], K0List[3], K0List[4], K0List[5])) |
volker@28 | 1029 | print('===========================================================================================================') |
volker@28 | 1030 | print() |
volker@28 | 1031 | print("Errors from neglecting GHK corrections and/or calibration:") |
volker@28 | 1032 | print("{0:>10},{1:>10},{2:>10},{3:>10},{4:>10},{5:>10}".format( |
volker@28 | 1033 | "LDRtrue", "LDRunCorr", "1/LDRunCorr", "LDRsimx", "1/LDRsimx", "LDRCorr")) |
ulalume3@0 | 1034 | |
volker@21 | 1035 | #LDRtrueList = 0.004, 0.02, 0.2, 0.45 |
volker@21 | 1036 | aF11sim0 = np.zeros(5) |
volker@21 | 1037 | LDRrange = np.zeros(5) |
volker@28 | 1038 | LDRrange = [0.004, 0.02, 0.1, 0.3, 0.45] # list |
volker@21 | 1039 | |
volker@28 | 1040 | # The loop over LDRtrueList is only for checking how much the uncorrected LDRsimx deviates from LDRtrue ... and whether the corrections work. |
volker@21 | 1041 | # LDRsimx = LDRsim = Ir / It or 1/LDRsim |
volker@21 | 1042 | # Still with assumed true parameters in input file |
volker@21 | 1043 | for i, LDRtrue in enumerate(LDRrange): |
volker@21 | 1044 | #for LDRtrue in LDRrange: |
volker@28 | 1045 | IoutTp, IoutTm, IoutRp, IoutRm, It, Ir, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr, \ |
volker@28 | 1046 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0, LDRunCorr = \ |
volker@28 | 1047 | Calc(TCalT0, TCalR0, NCalT, NCalR, DOLP0, RotL0, RotE0, RetE0, DiE0, |
volker@28 | 1048 | RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, |
volker@28 | 1049 | ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
volker@28 | 1050 | print("{0:10.5f},{1:10.5f},{2:10.5f},{3:10.5f},{4:10.5f},{5:10.5f}".format(LDRtrue, LDRunCorr, 1/LDRunCorr, LDRsimx, 1/LDRsimx, LDRCorr)) |
volker@21 | 1051 | aF11sim0[i] = F11sim0 |
volker@21 | 1052 | # the assumed true aF11sim0 results will be used below to calc the deviation from the real signals |
volker@28 | 1053 | print("LDRsimx = LDR of the nominal system directly from measured signals without calibration and GHK-corrections") |
volker@28 | 1054 | print("LDRunCorr = LDR of the nominal system directly from measured signals with calibration but without GHK-corrections; electronic amplifications = 1 assumed") |
volker@28 | 1055 | print("LDRCorr = LDR calibrated and GHK-corrected") |
volker@28 | 1056 | print() |
volker@28 | 1057 | print("Errors from signal noise:") |
volker@28 | 1058 | print("Signal counts: NCalT, NCalR, NILfac, nNCal, nNI = {0:10.0f},{1:10.0f},{2:3.0f},{3:2.0f},{4:2.0f}".format( |
volker@28 | 1059 | NCalT, NCalR, NILfac, nNCal, nNI)) |
ulalume3@0 | 1060 | |
volker@28 | 1061 | '''# das muß wieder weg |
volker@28 | 1062 | print("IoutTp, IoutTm, IoutRp, IoutRm, It , Ir , dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr") |
volker@28 | 1063 | LDRCal = 0.01 |
volker@28 | 1064 | for i, LDRtrue in enumerate(LDRrange): |
volker@28 | 1065 | IoutTp, IoutTm, IoutRp, IoutRm, It, Ir, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr, \ |
volker@28 | 1066 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0, LDRunCorr = \ |
volker@28 | 1067 | Calc(TCalT0, TCalR0, NCalT, NCalR, DOLP0, RotL0, RotE0, RetE0, DiE0, |
volker@28 | 1068 | RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, |
volker@28 | 1069 | ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
volker@28 | 1070 | print( "{:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}, {:0.4f}".format( |
volker@28 | 1071 | IoutTp * NCalT, IoutTm * NCalT, IoutRp * NCalR, IoutRm * NCalR, It * facIt, Ir * facIr, |
volker@28 | 1072 | dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr)) |
volker@28 | 1073 | aF11sim0[i] = F11sim0 |
volker@28 | 1074 | # the assumed true aF11sim0 results will be used below to calc the deviation from the real signals |
volker@28 | 1075 | # bis hierher weg |
volker@28 | 1076 | ''' |
volker@28 | 1077 | |
volker@28 | 1078 | file = open('output_files\\' + LID + '-' + InputFile[0:-3] + '-GHK.dat', 'r') |
binietoglou@19 | 1079 | print(file.read()) |
ulalume3@0 | 1080 | file.close() |
ulalume3@0 | 1081 | |
ulalume3@0 | 1082 | ''' |
ulalume3@0 | 1083 | if(PrintToOutputFile): |
ulalume3@0 | 1084 | f = open('output_ver7.dat', 'w') |
ulalume3@0 | 1085 | old_target = sys.stdout |
ulalume3@0 | 1086 | sys.stdout = f |
ulalume3@0 | 1087 | |
ulalume3@0 | 1088 | print("something") |
ulalume3@0 | 1089 | |
ulalume3@0 | 1090 | if(PrintToOutputFile): |
ulalume3@0 | 1091 | sys.stdout.flush() |
ulalume3@0 | 1092 | f.close |
ulalume3@0 | 1093 | sys.stdout = old_target |
ulalume3@0 | 1094 | ''' |
binietoglou@19 | 1095 | if (Error_Calc): |
volker@21 | 1096 | # --- CALC again assumed truth with LDRCal0 and with assumed true parameters in input file to reset all 0-values |
volker@28 | 1097 | IoutTp0, IoutTm0, IoutRp0, IoutRm0, It0, Ir0, dIoutTp0, dIoutTm0, dIoutRp0, dIoutRm0, dIt0, dIr0, \ |
volker@28 | 1098 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0, LDRunCorr = \ |
volker@28 | 1099 | Calc(TCalT0, TCalR0, NCalT, NCalR, DOLP0, RotL0, RotE0, RetE0, DiE0, |
volker@28 | 1100 | RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, |
volker@28 | 1101 | ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
volker@28 | 1102 | Etax0 = K0 * Eta0 |
volker@28 | 1103 | # --- Start Error calculation with variable parameters ------------------------------------------------------------------ |
volker@28 | 1104 | # error nNCal: one-sigma in steps to left and right for calibration signals |
volker@28 | 1105 | # error nNI: one-sigma in steps to left and right for 0° signals |
ulalume3@0 | 1106 | |
volker@16 | 1107 | iN = -1 |
volker@28 | 1108 | N = ((nTCalT * 2 + 1) * (nTCalR * 2 + 1) * |
volker@28 | 1109 | (nNCal * 2 + 1) ** 4 * (nNI * 2 + 1) ** 2 * |
volker@28 | 1110 | (nDOLP * 2 + 1) * (nRotL * 2 + 1) * |
binietoglou@19 | 1111 | (nRotE * 2 + 1) * (nRetE * 2 + 1) * (nDiE * 2 + 1) * |
binietoglou@19 | 1112 | (nRotO * 2 + 1) * (nRetO * 2 + 1) * (nDiO * 2 + 1) * |
binietoglou@19 | 1113 | (nRotC * 2 + 1) * (nRetC * 2 + 1) * (nDiC * 2 + 1) * |
binietoglou@19 | 1114 | (nTP * 2 + 1) * (nTS * 2 + 1) * (nRP * 2 + 1) * (nRS * 2 + 1) * (nERaT * 2 + 1) * (nERaR * 2 + 1) * |
binietoglou@19 | 1115 | (nRotaT * 2 + 1) * (nRotaR * 2 + 1) * (nRetT * 2 + 1) * (nRetR * 2 + 1) * (nLDRCal * 2 + 1)) |
volker@28 | 1116 | print("number of system variations N = ", N, " ", end="") |
ulalume3@0 | 1117 | |
volker@16 | 1118 | if N > 1e6: |
binietoglou@19 | 1119 | if user_yes_no_query('Warning: processing ' + str( |
binietoglou@19 | 1120 | N) + ' samples will take very long. Do you want to proceed?') == 0: sys.exit() |
volker@16 | 1121 | if N > 5e6: |
binietoglou@19 | 1122 | if user_yes_no_query('Warning: the memory required for ' + str(N) + ' samples might be ' + '{0:5.1f}'.format( |
binietoglou@19 | 1123 | N / 4e6) + ' GB. Do you anyway want to proceed?') == 0: sys.exit() |
ulalume3@0 | 1124 | |
binietoglou@19 | 1125 | # if user_yes_no_query('Warning: processing' + str(N) + ' samples will take very long. Do you want to proceed?') == 0: sys.exit() |
ulalume3@0 | 1126 | |
volker@16 | 1127 | # --- Arrays for plotting ------ |
volker@16 | 1128 | LDRmin = np.zeros(5) |
volker@16 | 1129 | LDRmax = np.zeros(5) |
volker@16 | 1130 | F11min = np.zeros(5) |
volker@16 | 1131 | F11max = np.zeros(5) |
volker@28 | 1132 | Etaxmin = np.zeros(5) |
volker@28 | 1133 | Etaxmax = np.zeros(5) |
ulalume3@0 | 1134 | |
volker@28 | 1135 | # LDRrange = np.zeros(5) |
volker@28 | 1136 | # LDRrange = 0.004, 0.02, 0.1, 0.3, 0.45 |
binietoglou@19 | 1137 | # aLDRsimx = np.zeros(N) |
binietoglou@19 | 1138 | # aLDRsimx2 = np.zeros(N) |
binietoglou@19 | 1139 | # aLDRcorr = np.zeros(N) |
binietoglou@19 | 1140 | # aLDRcorr2 = np.zeros(N) |
volker@23 | 1141 | aDOLP = np.zeros(N) |
volker@16 | 1142 | aERaT = np.zeros(N) |
volker@16 | 1143 | aERaR = np.zeros(N) |
volker@16 | 1144 | aRotaT = np.zeros(N) |
volker@16 | 1145 | aRotaR = np.zeros(N) |
volker@16 | 1146 | aRetT = np.zeros(N) |
volker@16 | 1147 | aRetR = np.zeros(N) |
volker@16 | 1148 | aTP = np.zeros(N) |
volker@16 | 1149 | aTS = np.zeros(N) |
volker@16 | 1150 | aRP = np.zeros(N) |
volker@16 | 1151 | aRS = np.zeros(N) |
volker@16 | 1152 | aDiE = np.zeros(N) |
volker@16 | 1153 | aDiO = np.zeros(N) |
volker@16 | 1154 | aDiC = np.zeros(N) |
volker@16 | 1155 | aRotC = np.zeros(N) |
volker@16 | 1156 | aRetC = np.zeros(N) |
volker@16 | 1157 | aRotL = np.zeros(N) |
volker@16 | 1158 | aRetE = np.zeros(N) |
volker@16 | 1159 | aRotE = np.zeros(N) |
volker@16 | 1160 | aRetO = np.zeros(N) |
volker@16 | 1161 | aRotO = np.zeros(N) |
volker@16 | 1162 | aLDRCal = np.zeros(N) |
volker@28 | 1163 | aNCalTp = np.zeros(N) |
volker@28 | 1164 | aNCalTm = np.zeros(N) |
volker@28 | 1165 | aNCalRp = np.zeros(N) |
volker@28 | 1166 | aNCalRm = np.zeros(N) |
volker@28 | 1167 | aNIt = np.zeros(N) |
volker@28 | 1168 | aNIr = np.zeros(N) |
volker@28 | 1169 | aTCalT = np.zeros(N) |
volker@28 | 1170 | aTCalR = np.zeros(N) |
volker@28 | 1171 | |
volker@28 | 1172 | # each np.zeros((LDRrange, N)) array has the same N-dependency |
volker@28 | 1173 | aLDRcorr = np.zeros((5, N)) |
binietoglou@19 | 1174 | aF11corr = np.zeros((5, N)) |
volker@28 | 1175 | aPLDR = np.zeros((5, N)) |
volker@28 | 1176 | aEtax = np.zeros((5, N)) |
volker@28 | 1177 | |
volker@28 | 1178 | # np.zeros((GHKs, N)) |
volker@28 | 1179 | aGHK = np.zeros((5, N)) |
ulalume3@0 | 1180 | |
volker@16 | 1181 | atime = clock() |
volker@16 | 1182 | dtime = clock() |
ulalume3@0 | 1183 | |
volker@16 | 1184 | # --- Calc Error signals |
volker@16 | 1185 | # ---- Do the calculations of bra-ket vectors |
volker@16 | 1186 | h = -1. if TypeC == 2 else 1 |
ulalume3@0 | 1187 | |
volker@21 | 1188 | ''' |
volker@16 | 1189 | # from input file: measured LDRm and true LDRtrue, LDRtrue2 => |
binietoglou@19 | 1190 | ameas = (1. - LDRmeas) / (1 + LDRmeas) |
binietoglou@19 | 1191 | atrue = (1. - LDRtrue) / (1 + LDRtrue) |
binietoglou@19 | 1192 | atrue2 = (1. - LDRtrue2) / (1 + LDRtrue2) |
volker@21 | 1193 | ''' |
ulalume3@0 | 1194 | |
binietoglou@19 | 1195 | for iLDRCal in range(-nLDRCal, nLDRCal + 1): |
volker@28 | 1196 | # from input file: LDRCal for calibration measurements |
volker@16 | 1197 | LDRCal = LDRCal0 |
volker@28 | 1198 | if nLDRCal > 0: |
volker@28 | 1199 | LDRCal = LDRCal0 + iLDRCal * dLDRCal / nLDRCal |
volker@28 | 1200 | # provides the intensities of the calibration measurements at various LDRCal for signal noise errors |
volker@28 | 1201 | # IoutTp, IoutTm, IoutRp, IoutRm, dIoutTp, dIoutTm, dIoutRp, dIoutRm |
volker@28 | 1202 | ''' |
volker@28 | 1203 | IoutTp, IoutTm, IoutRp, IoutRm, It, Ir, dIoutTp, dIoutTm, dIoutRp, dIoutRm, dIt, dIr, \ |
volker@28 | 1204 | GT, HT, GR, HR, K, Eta, LDRsimx, LDRCorr, DTa, DRa, TTa, TRa, F11sim, LDRunCorr = \ |
volker@28 | 1205 | Calc(TCalT, TCalR, NCalT, NCalR, DOLP0, RotL0, RotE0, RetE0, DiE0, |
volker@28 | 1206 | RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, |
volker@28 | 1207 | ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal) |
volker@28 | 1208 | ''' |
binietoglou@19 | 1209 | aCal = (1. - LDRCal) / (1 + LDRCal) |
volker@23 | 1210 | for iDOLP, iRotL, iRotE, iRetE, iDiE \ |
volker@23 | 1211 | in [(iDOLP, iRotL, iRotE, iRetE, iDiE) |
volker@23 | 1212 | for iDOLP in range(-nDOLP, nDOLP + 1) |
binietoglou@19 | 1213 | for iRotL in range(-nRotL, nRotL + 1) |
binietoglou@19 | 1214 | for iRotE in range(-nRotE, nRotE + 1) |
binietoglou@19 | 1215 | for iRetE in range(-nRetE, nRetE + 1) |
binietoglou@19 | 1216 | for iDiE in range(-nDiE, nDiE + 1)]: |
ulalume3@0 | 1217 | |
volker@23 | 1218 | if nDOLP > 0: DOLP = DOLP0 + iDOLP * dDOLP / nDOLP |
binietoglou@19 | 1219 | if nRotL > 0: RotL = RotL0 + iRotL * dRotL / nRotL |
binietoglou@19 | 1220 | if nRotE > 0: RotE = RotE0 + iRotE * dRotE / nRotE |
binietoglou@19 | 1221 | if nRetE > 0: RetE = RetE0 + iRetE * dRetE / nRetE |
binietoglou@19 | 1222 | if nDiE > 0: DiE = DiE0 + iDiE * dDiE / nDiE |
ulalume3@0 | 1223 | |
volker@16 | 1224 | # angles of emitter and laser and calibrator and receiver optics |
volker@16 | 1225 | # RotL = alpha, RotE = beta, RotO = gamma, RotC = epsilon |
binietoglou@19 | 1226 | S2a = np.sin(2 * np.deg2rad(RotL)) |
binietoglou@19 | 1227 | C2a = np.cos(2 * np.deg2rad(RotL)) |
binietoglou@19 | 1228 | S2b = np.sin(2 * np.deg2rad(RotE)) |
binietoglou@19 | 1229 | C2b = np.cos(2 * np.deg2rad(RotE)) |
binietoglou@19 | 1230 | S2ab = np.sin(np.deg2rad(2 * RotL - 2 * RotE)) |
binietoglou@19 | 1231 | C2ab = np.cos(np.deg2rad(2 * RotL - 2 * RotE)) |
ulalume3@0 | 1232 | |
volker@23 | 1233 | # Laser with Degree of linear polarization DOLP |
volker@16 | 1234 | IinL = 1. |
volker@23 | 1235 | QinL = DOLP |
volker@16 | 1236 | UinL = 0. |
volker@23 | 1237 | VinL = (1. - DOLP ** 2) ** 0.5 |
ulalume3@0 | 1238 | |
volker@16 | 1239 | # Stokes Input Vector rotation Eq. E.4 |
binietoglou@19 | 1240 | A = C2a * QinL - S2a * UinL |
binietoglou@19 | 1241 | B = S2a * QinL + C2a * UinL |
volker@16 | 1242 | # Stokes Input Vector rotation Eq. E.9 |
binietoglou@19 | 1243 | C = C2ab * QinL - S2ab * UinL |
binietoglou@19 | 1244 | D = S2ab * QinL + C2ab * UinL |
ulalume3@0 | 1245 | |
volker@16 | 1246 | # emitter optics |
volker@16 | 1247 | CosE = np.cos(np.deg2rad(RetE)) |
volker@16 | 1248 | SinE = np.sin(np.deg2rad(RetE)) |
binietoglou@19 | 1249 | ZiE = (1. - DiE ** 2) ** 0.5 |
binietoglou@19 | 1250 | WiE = (1. - ZiE * CosE) |
ulalume3@0 | 1251 | |
volker@16 | 1252 | # Stokes Input Vector after emitter optics equivalent to Eq. E.9 with already rotated input vector from Eq. E.4 |
volker@16 | 1253 | # b = beta |
binietoglou@19 | 1254 | IinE = (IinL + DiE * C) |
binietoglou@19 | 1255 | QinE = (C2b * DiE * IinL + A + S2b * (WiE * D - ZiE * SinE * VinL)) |
binietoglou@19 | 1256 | UinE = (S2b * DiE * IinL + B - C2b * (WiE * D - ZiE * SinE * VinL)) |
binietoglou@19 | 1257 | VinE = (-ZiE * SinE * D + ZiE * CosE * VinL) |
ulalume3@0 | 1258 | |
binietoglou@19 | 1259 | # ------------------------- |
volker@16 | 1260 | # F11 assuemd to be = 1 => measured: F11m = IinP / IinE with atrue |
binietoglou@19 | 1261 | # F11sim = (IinE + DiO*atrue*(C2g*QinE - S2g*UinE))/IinE |
binietoglou@19 | 1262 | # ------------------------- |
ulalume3@0 | 1263 | |
volker@16 | 1264 | for iRotO, iRetO, iDiO, iRotC, iRetC, iDiC, iTP, iTS, iRP, iRS, iERaT, iRotaT, iRetT, iERaR, iRotaR, iRetR \ |
binietoglou@19 | 1265 | in [ |
binietoglou@19 | 1266 | (iRotO, iRetO, iDiO, iRotC, iRetC, iDiC, iTP, iTS, iRP, iRS, iERaT, iRotaT, iRetT, iERaR, iRotaR, iRetR) |
binietoglou@19 | 1267 | for iRotO in range(-nRotO, nRotO + 1) |
binietoglou@19 | 1268 | for iRetO in range(-nRetO, nRetO + 1) |
binietoglou@19 | 1269 | for iDiO in range(-nDiO, nDiO + 1) |
binietoglou@19 | 1270 | for iRotC in range(-nRotC, nRotC + 1) |
binietoglou@19 | 1271 | for iRetC in range(-nRetC, nRetC + 1) |
binietoglou@19 | 1272 | for iDiC in range(-nDiC, nDiC + 1) |
binietoglou@19 | 1273 | for iTP in range(-nTP, nTP + 1) |
binietoglou@19 | 1274 | for iTS in range(-nTS, nTS + 1) |
binietoglou@19 | 1275 | for iRP in range(-nRP, nRP + 1) |
binietoglou@19 | 1276 | for iRS in range(-nRS, nRS + 1) |
binietoglou@19 | 1277 | for iERaT in range(-nERaT, nERaT + 1) |
binietoglou@19 | 1278 | for iRotaT in range(-nRotaT, nRotaT + 1) |
binietoglou@19 | 1279 | for iRetT in range(-nRetT, nRetT + 1) |
binietoglou@19 | 1280 | for iERaR in range(-nERaR, nERaR + 1) |
binietoglou@19 | 1281 | for iRotaR in range(-nRotaR, nRotaR + 1) |
binietoglou@19 | 1282 | for iRetR in range(-nRetR, nRetR + 1)]: |
ulalume3@0 | 1283 | |
binietoglou@19 | 1284 | if nRotO > 0: RotO = RotO0 + iRotO * dRotO / nRotO |
binietoglou@19 | 1285 | if nRetO > 0: RetO = RetO0 + iRetO * dRetO / nRetO |
binietoglou@19 | 1286 | if nDiO > 0: DiO = DiO0 + iDiO * dDiO / nDiO |
binietoglou@19 | 1287 | if nRotC > 0: RotC = RotC0 + iRotC * dRotC / nRotC |
binietoglou@19 | 1288 | if nRetC > 0: RetC = RetC0 + iRetC * dRetC / nRetC |
binietoglou@19 | 1289 | if nDiC > 0: DiC = DiC0 + iDiC * dDiC / nDiC |
binietoglou@19 | 1290 | if nTP > 0: TP = TP0 + iTP * dTP / nTP |
binietoglou@19 | 1291 | if nTS > 0: TS = TS0 + iTS * dTS / nTS |
binietoglou@19 | 1292 | if nRP > 0: RP = RP0 + iRP * dRP / nRP |
binietoglou@19 | 1293 | if nRS > 0: RS = RS0 + iRS * dRS / nRS |
binietoglou@19 | 1294 | if nERaT > 0: ERaT = ERaT0 + iERaT * dERaT / nERaT |
binietoglou@19 | 1295 | if nRotaT > 0: RotaT = RotaT0 + iRotaT * dRotaT / nRotaT |
binietoglou@19 | 1296 | if nRetT > 0: RetT = RetT0 + iRetT * dRetT / nRetT |
binietoglou@19 | 1297 | if nERaR > 0: ERaR = ERaR0 + iERaR * dERaR / nERaR |
binietoglou@19 | 1298 | if nRotaR > 0: RotaR = RotaR0 + iRotaR * dRotaR / nRotaR |
binietoglou@19 | 1299 | if nRetR > 0: RetR = RetR0 + iRetR * dRetR / nRetR |
ulalume3@0 | 1300 | |
binietoglou@19 | 1301 | # print("{0:5.2f}, {1:5.2f}, {2:5.2f}, {3:10d}".format(RotL, RotE, RotO, iN)) |
ulalume3@0 | 1302 | |
volker@16 | 1303 | # receiver optics |
volker@16 | 1304 | CosO = np.cos(np.deg2rad(RetO)) |
volker@16 | 1305 | SinO = np.sin(np.deg2rad(RetO)) |
binietoglou@19 | 1306 | ZiO = (1. - DiO ** 2) ** 0.5 |
binietoglou@19 | 1307 | WiO = (1. - ZiO * CosO) |
binietoglou@19 | 1308 | S2g = np.sin(np.deg2rad(2 * RotO)) |
binietoglou@19 | 1309 | C2g = np.cos(np.deg2rad(2 * RotO)) |
volker@16 | 1310 | # calibrator |
volker@16 | 1311 | CosC = np.cos(np.deg2rad(RetC)) |
volker@16 | 1312 | SinC = np.sin(np.deg2rad(RetC)) |
binietoglou@19 | 1313 | ZiC = (1. - DiC ** 2) ** 0.5 |
binietoglou@19 | 1314 | WiC = (1. - ZiC * CosC) |
ulalume3@0 | 1315 | |
volker@16 | 1316 | # analyser |
binietoglou@19 | 1317 | # For POLLY_XTs |
binietoglou@19 | 1318 | if (RS_RP_depend_on_TS_TP): |
volker@16 | 1319 | RS = 1 - TS |
volker@16 | 1320 | RP = 1 - TP |
volker@16 | 1321 | TiT = 0.5 * (TP + TS) |
binietoglou@19 | 1322 | DiT = (TP - TS) / (TP + TS) |
binietoglou@19 | 1323 | ZiT = (1. - DiT ** 2) ** 0.5 |
volker@16 | 1324 | TiR = 0.5 * (RP + RS) |
binietoglou@19 | 1325 | DiR = (RP - RS) / (RP + RS) |
binietoglou@19 | 1326 | ZiR = (1. - DiR ** 2) ** 0.5 |
volker@16 | 1327 | CosT = np.cos(np.deg2rad(RetT)) |
volker@16 | 1328 | SinT = np.sin(np.deg2rad(RetT)) |
volker@16 | 1329 | CosR = np.cos(np.deg2rad(RetR)) |
volker@16 | 1330 | SinR = np.sin(np.deg2rad(RetR)) |
ulalume3@0 | 1331 | |
volker@28 | 1332 | # cleaning pol-filter |
binietoglou@19 | 1333 | DaT = (1 - ERaT) / (1 + ERaT) |
binietoglou@19 | 1334 | DaR = (1 - ERaR) / (1 + ERaR) |
binietoglou@19 | 1335 | TaT = 0.5 * (1 + ERaT) |
binietoglou@19 | 1336 | TaR = 0.5 * (1 + ERaR) |
ulalume3@0 | 1337 | |
binietoglou@19 | 1338 | S2aT = np.sin(np.deg2rad(h * 2 * RotaT)) |
binietoglou@19 | 1339 | C2aT = np.cos(np.deg2rad(2 * RotaT)) |
binietoglou@19 | 1340 | S2aR = np.sin(np.deg2rad(h * 2 * RotaR)) |
binietoglou@19 | 1341 | C2aR = np.cos(np.deg2rad(2 * RotaR)) |
ulalume3@0 | 1342 | |
volker@28 | 1343 | # Analyzer As before the PBS Eq. D.5; combined PBS and cleaning pol-filter |
volker@28 | 1344 | ATPT = (1 + C2aT * DaT * DiT) # unpolarized transmission correction |
volker@28 | 1345 | TTa = TiT * TaT * ATPT # unpolarized transmission |
volker@28 | 1346 | ATP1 = 1 |
volker@28 | 1347 | ATP2 = Y * (DiT + C2aT * DaT) / ATPT |
volker@28 | 1348 | ATP3 = Y * S2aT * DaT * ZiT * CosT / ATPT |
volker@28 | 1349 | ATP4 = S2aT * DaT * ZiT * SinT / ATPT |
binietoglou@19 | 1350 | ATP = np.array([ATP1, ATP2, ATP3, ATP4]) |
volker@28 | 1351 | DTa = ATP2 * Y |
ulalume3@0 | 1352 | |
volker@28 | 1353 | ARPT = (1 + C2aR * DaR * DiR) # unpolarized transmission correction |
volker@28 | 1354 | TRa = TiR * TaR * ARPT # unpolarized transmission |
volker@28 | 1355 | ARP1 = 1 |
volker@28 | 1356 | ARP2 = Y * (DiR + C2aR * DaR) / ARPT |
volker@28 | 1357 | ARP3 = Y * S2aR * DaR * ZiR * CosR / ARPT |
volker@28 | 1358 | ARP4 = S2aR * DaR * ZiR * SinR / ARPT |
binietoglou@19 | 1359 | ARP = np.array([ARP1, ARP2, ARP3, ARP4]) |
volker@28 | 1360 | DRa = ARP2 * Y |
ulalume3@0 | 1361 | |
volker@16 | 1362 | # ---- Calculate signals and correction parameters for diffeent locations and calibrators |
volker@16 | 1363 | if LocC == 4: # Calibrator before the PBS |
binietoglou@19 | 1364 | # print("Calibrator location not implemented yet") |
ulalume3@0 | 1365 | |
binietoglou@19 | 1366 | # S2ge = np.sin(np.deg2rad(2*RotO + h*2*RotC)) |
binietoglou@19 | 1367 | # C2ge = np.cos(np.deg2rad(2*RotO + h*2*RotC)) |
binietoglou@19 | 1368 | S2e = np.sin(np.deg2rad(h * 2 * RotC)) |
binietoglou@19 | 1369 | C2e = np.cos(np.deg2rad(2 * RotC)) |
volker@16 | 1370 | # rotated AinP by epsilon Eq. C.3 |
binietoglou@19 | 1371 | ATP2e = C2e * ATP2 + S2e * ATP3 |
binietoglou@19 | 1372 | ATP3e = C2e * ATP3 - S2e * ATP2 |
binietoglou@19 | 1373 | ARP2e = C2e * ARP2 + S2e * ARP3 |
binietoglou@19 | 1374 | ARP3e = C2e * ARP3 - S2e * ARP2 |
binietoglou@19 | 1375 | ATPe = np.array([ATP1, ATP2e, ATP3e, ATP4]) |
binietoglou@19 | 1376 | ARPe = np.array([ARP1, ARP2e, ARP3e, ARP4]) |
volker@16 | 1377 | # Stokes Input Vector before the polarising beam splitter Eq. E.31 |
binietoglou@19 | 1378 | A = C2g * QinE - S2g * UinE |
binietoglou@19 | 1379 | B = S2g * QinE + C2g * UinE |
binietoglou@19 | 1380 | # C = (WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE) |
binietoglou@19 | 1381 | Co = ZiO * SinO * VinE |
binietoglou@19 | 1382 | Ca = (WiO * B - 2 * ZiO * SinO * VinE) |
binietoglou@19 | 1383 | # C = Co + aCal*Ca |
binietoglou@19 | 1384 | # IinP = (IinE + DiO*aCal*A) |
binietoglou@19 | 1385 | # QinP = (C2g*DiO*IinE + aCal*QinE - S2g*C) |
binietoglou@19 | 1386 | # UinP = (S2g*DiO*IinE - aCal*UinE + C2g*C) |
binietoglou@19 | 1387 | # VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE) |
volker@16 | 1388 | IinPo = IinE |
binietoglou@19 | 1389 | QinPo = (C2g * DiO * IinE - S2g * Co) |
binietoglou@19 | 1390 | UinPo = (S2g * DiO * IinE + C2g * Co) |
binietoglou@19 | 1391 | VinPo = ZiO * CosO * VinE |
ulalume3@0 | 1392 | |
binietoglou@19 | 1393 | IinPa = DiO * A |
binietoglou@19 | 1394 | QinPa = QinE - S2g * Ca |
binietoglou@19 | 1395 | UinPa = -UinE + C2g * Ca |
binietoglou@19 | 1396 | VinPa = ZiO * (SinO * B - 2 * CosO * VinE) |
ulalume3@0 | 1397 | |
binietoglou@19 | 1398 | IinP = IinPo + aCal * IinPa |
binietoglou@19 | 1399 | QinP = QinPo + aCal * QinPa |
binietoglou@19 | 1400 | UinP = UinPo + aCal * UinPa |
binietoglou@19 | 1401 | VinP = VinPo + aCal * VinPa |
volker@16 | 1402 | # Stokes Input Vector before the polarising beam splitter rotated by epsilon Eq. C.3 |
binietoglou@19 | 1403 | # QinPe = C2e*QinP + S2e*UinP |
binietoglou@19 | 1404 | # UinPe = C2e*UinP - S2e*QinP |
binietoglou@19 | 1405 | QinPoe = C2e * QinPo + S2e * UinPo |
binietoglou@19 | 1406 | UinPoe = C2e * UinPo - S2e * QinPo |
binietoglou@19 | 1407 | QinPae = C2e * QinPa + S2e * UinPa |
binietoglou@19 | 1408 | UinPae = C2e * UinPa - S2e * QinPa |
binietoglou@19 | 1409 | QinPe = C2e * QinP + S2e * UinP |
binietoglou@19 | 1410 | UinPe = C2e * UinP - S2e * QinP |
ulalume3@0 | 1411 | |
volker@16 | 1412 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
volker@16 | 1413 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
volker@16 | 1414 | # parameters for calibration with aCal |
binietoglou@19 | 1415 | AT = ATP1 * IinP + h * ATP4 * VinP |
binietoglou@19 | 1416 | BT = ATP3e * QinP - h * ATP2e * UinP |
binietoglou@19 | 1417 | AR = ARP1 * IinP + h * ARP4 * VinP |
binietoglou@19 | 1418 | BR = ARP3e * QinP - h * ARP2e * UinP |
volker@23 | 1419 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 1420 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 1421 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 1422 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 1423 | GT = np.dot(ATP, IS1) |
binietoglou@19 | 1424 | GR = np.dot(ARP, IS1) |
binietoglou@19 | 1425 | HT = np.dot(ATP, IS2) |
binietoglou@19 | 1426 | HR = np.dot(ARP, IS2) |
volker@16 | 1427 | else: |
binietoglou@19 | 1428 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 1429 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 1430 | GT = np.dot(ATPe, IS1) |
binietoglou@19 | 1431 | GR = np.dot(ARPe, IS1) |
binietoglou@19 | 1432 | HT = np.dot(ATPe, IS2) |
binietoglou@19 | 1433 | HR = np.dot(ARPe, IS2) |
volker@16 | 1434 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
volker@16 | 1435 | # parameters for calibration with aCal |
binietoglou@19 | 1436 | AT = ATP1 * IinP + ATP3e * UinPe + ZiC * CosC * (ATP2e * QinPe + ATP4 * VinP) |
binietoglou@19 | 1437 | BT = DiC * (ATP1 * UinPe + ATP3e * IinP) - ZiC * SinC * (ATP2e * VinP - ATP4 * QinPe) |
binietoglou@19 | 1438 | AR = ARP1 * IinP + ARP3e * UinPe + ZiC * CosC * (ARP2e * QinPe + ARP4 * VinP) |
binietoglou@19 | 1439 | BR = DiC * (ARP1 * UinPe + ARP3e * IinP) - ZiC * SinC * (ARP2e * VinP - ARP4 * QinPe) |
volker@23 | 1440 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 1441 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 1442 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 1443 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 1444 | GT = np.dot(ATP, IS1) |
binietoglou@19 | 1445 | GR = np.dot(ARP, IS1) |
binietoglou@19 | 1446 | HT = np.dot(ATP, IS2) |
binietoglou@19 | 1447 | HR = np.dot(ARP, IS2) |
volker@16 | 1448 | else: |
binietoglou@19 | 1449 | IS1e = np.array( |
binietoglou@19 | 1450 | [IinPo + DiC * QinPoe, DiC * IinPo + QinPoe, ZiC * (CosC * UinPoe + SinC * VinPo), |
binietoglou@19 | 1451 | -ZiC * (SinC * UinPoe - CosC * VinPo)]) |
binietoglou@19 | 1452 | IS2e = np.array( |
binietoglou@19 | 1453 | [IinPa + DiC * QinPae, DiC * IinPa + QinPae, ZiC * (CosC * UinPae + SinC * VinPa), |
binietoglou@19 | 1454 | -ZiC * (SinC * UinPae - CosC * VinPa)]) |
binietoglou@19 | 1455 | GT = np.dot(ATPe, IS1e) |
binietoglou@19 | 1456 | GR = np.dot(ARPe, IS1e) |
binietoglou@19 | 1457 | HT = np.dot(ATPe, IS2e) |
binietoglou@19 | 1458 | HR = np.dot(ARPe, IS2e) |
volker@16 | 1459 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
volker@16 | 1460 | # parameters for calibration with aCal |
binietoglou@19 | 1461 | AT = ATP1 * IinP + sqr05 * DiC * (ATP1 * QinPe + ATP2e * IinP) + (1 - 0.5 * WiC) * ( |
binietoglou@19 | 1462 | ATP2e * QinPe + ATP3e * UinPe) + ZiC * ( |
binietoglou@19 | 1463 | sqr05 * SinC * (ATP3e * VinP - ATP4 * UinPe) + ATP4 * CosC * VinP) |
binietoglou@19 | 1464 | BT = sqr05 * DiC * (ATP1 * UinPe + ATP3e * IinP) + 0.5 * WiC * ( |
binietoglou@19 | 1465 | ATP2e * UinPe + ATP3e * QinPe) - sqr05 * ZiC * SinC * (ATP2e * VinP - ATP4 * QinPe) |
binietoglou@19 | 1466 | AR = ARP1 * IinP + sqr05 * DiC * (ARP1 * QinPe + ARP2e * IinP) + (1 - 0.5 * WiC) * ( |
binietoglou@19 | 1467 | ARP2e * QinPe + ARP3e * UinPe) + ZiC * ( |
binietoglou@19 | 1468 | sqr05 * SinC * (ARP3e * VinP - ARP4 * UinPe) + ARP4 * CosC * VinP) |
binietoglou@19 | 1469 | BR = sqr05 * DiC * (ARP1 * UinPe + ARP3e * IinP) + 0.5 * WiC * ( |
binietoglou@19 | 1470 | ARP2e * UinPe + ARP3e * QinPe) - sqr05 * ZiC * SinC * (ARP2e * VinP - ARP4 * QinPe) |
volker@23 | 1471 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 1472 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 1473 | IS1 = np.array([IinPo, QinPo, UinPo, VinPo]) |
binietoglou@19 | 1474 | IS2 = np.array([IinPa, QinPa, UinPa, VinPa]) |
binietoglou@19 | 1475 | GT = np.dot(ATP, IS1) |
binietoglou@19 | 1476 | GR = np.dot(ARP, IS1) |
binietoglou@19 | 1477 | HT = np.dot(ATP, IS2) |
binietoglou@19 | 1478 | HR = np.dot(ARP, IS2) |
volker@16 | 1479 | else: |
binietoglou@19 | 1480 | IS1e = np.array( |
binietoglou@19 | 1481 | [IinPo + DiC * QinPoe, DiC * IinPo + QinPoe, ZiC * (CosC * UinPoe + SinC * VinPo), |
binietoglou@19 | 1482 | -ZiC * (SinC * UinPoe - CosC * VinPo)]) |
binietoglou@19 | 1483 | IS2e = np.array( |
binietoglou@19 | 1484 | [IinPa + DiC * QinPae, DiC * IinPa + QinPae, ZiC * (CosC * UinPae + SinC * VinPa), |
binietoglou@19 | 1485 | -ZiC * (SinC * UinPae - CosC * VinPa)]) |
binietoglou@19 | 1486 | GT = np.dot(ATPe, IS1e) |
binietoglou@19 | 1487 | GR = np.dot(ARPe, IS1e) |
binietoglou@19 | 1488 | HT = np.dot(ATPe, IS2e) |
binietoglou@19 | 1489 | HR = np.dot(ARPe, IS2e) |
ulalume3@0 | 1490 | else: |
volker@16 | 1491 | print("Calibrator not implemented yet") |
volker@16 | 1492 | sys.exit() |
volker@16 | 1493 | |
volker@16 | 1494 | elif LocC == 3: # C before receiver optics Eq.57 |
ulalume3@0 | 1495 | |
binietoglou@19 | 1496 | # S2ge = np.sin(np.deg2rad(2*RotO - 2*RotC)) |
binietoglou@19 | 1497 | # C2ge = np.cos(np.deg2rad(2*RotO - 2*RotC)) |
binietoglou@19 | 1498 | S2e = np.sin(np.deg2rad(2 * RotC)) |
binietoglou@19 | 1499 | C2e = np.cos(np.deg2rad(2 * RotC)) |
ulalume3@0 | 1500 | |
volker@16 | 1501 | # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt) |
binietoglou@19 | 1502 | AF1 = np.array([1, C2g * DiO, S2g * DiO, 0]) |
binietoglou@19 | 1503 | AF2 = np.array([C2g * DiO, 1 - S2g ** 2 * WiO, S2g * C2g * WiO, -S2g * ZiO * SinO]) |
binietoglou@19 | 1504 | AF3 = np.array([S2g * DiO, S2g * C2g * WiO, 1 - C2g ** 2 * WiO, C2g * ZiO * SinO]) |
binietoglou@19 | 1505 | AF4 = np.array([0, S2g * SinO, -C2g * SinO, CosO]) |
ulalume3@0 | 1506 | |
binietoglou@19 | 1507 | ATF = (ATP1 * AF1 + ATP2 * AF2 + ATP3 * AF3 + ATP4 * AF4) |
binietoglou@19 | 1508 | ARF = (ARP1 * AF1 + ARP2 * AF2 + ARP3 * AF3 + ARP4 * AF4) |
volker@16 | 1509 | ATF1 = ATF[0] |
volker@16 | 1510 | ATF2 = ATF[1] |
volker@16 | 1511 | ATF3 = ATF[2] |
volker@16 | 1512 | ATF4 = ATF[3] |
volker@16 | 1513 | ARF1 = ARF[0] |
volker@16 | 1514 | ARF2 = ARF[1] |
volker@16 | 1515 | ARF3 = ARF[2] |
volker@16 | 1516 | ARF4 = ARF[3] |
ulalume3@0 | 1517 | |
volker@16 | 1518 | # rotated AinF by epsilon |
binietoglou@19 | 1519 | ATF2e = C2e * ATF[1] + S2e * ATF[2] |
binietoglou@19 | 1520 | ATF3e = C2e * ATF[2] - S2e * ATF[1] |
binietoglou@19 | 1521 | ARF2e = C2e * ARF[1] + S2e * ARF[2] |
binietoglou@19 | 1522 | ARF3e = C2e * ARF[2] - S2e * ARF[1] |
ulalume3@0 | 1523 | |
binietoglou@19 | 1524 | ATFe = np.array([ATF1, ATF2e, ATF3e, ATF4]) |
binietoglou@19 | 1525 | ARFe = np.array([ARF1, ARF2e, ARF3e, ARF4]) |
ulalume3@0 | 1526 | |
binietoglou@19 | 1527 | QinEe = C2e * QinE + S2e * UinE |
binietoglou@19 | 1528 | UinEe = C2e * UinE - S2e * QinE |
ulalume3@0 | 1529 | |
volker@16 | 1530 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
volker@16 | 1531 | IinF = IinE |
binietoglou@19 | 1532 | QinF = aCal * QinE |
binietoglou@19 | 1533 | UinF = -aCal * UinE |
binietoglou@19 | 1534 | VinF = (1. - 2. * aCal) * VinE |
ulalume3@0 | 1535 | |
volker@16 | 1536 | IinFo = IinE |
volker@16 | 1537 | QinFo = 0. |
volker@16 | 1538 | UinFo = 0. |
volker@16 | 1539 | VinFo = VinE |
ulalume3@0 | 1540 | |
volker@16 | 1541 | IinFa = 0. |
volker@16 | 1542 | QinFa = QinE |
volker@16 | 1543 | UinFa = -UinE |
binietoglou@19 | 1544 | VinFa = -2. * VinE |
ulalume3@0 | 1545 | |
volker@16 | 1546 | # Stokes Input Vector before receiver optics rotated by epsilon Eq. C.3 |
binietoglou@19 | 1547 | QinFe = C2e * QinF + S2e * UinF |
binietoglou@19 | 1548 | UinFe = C2e * UinF - S2e * QinF |
binietoglou@19 | 1549 | QinFoe = C2e * QinFo + S2e * UinFo |
binietoglou@19 | 1550 | UinFoe = C2e * UinFo - S2e * QinFo |
binietoglou@19 | 1551 | QinFae = C2e * QinFa + S2e * UinFa |
binietoglou@19 | 1552 | UinFae = C2e * UinFa - S2e * QinFa |
ulalume3@0 | 1553 | |
volker@16 | 1554 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
binietoglou@19 | 1555 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
binietoglou@19 | 1556 | AT = ATF1 * IinF + ATF4 * h * VinF |
binietoglou@19 | 1557 | BT = ATF3e * QinF - ATF2e * h * UinF |
binietoglou@19 | 1558 | AR = ARF1 * IinF + ARF4 * h * VinF |
binietoglou@19 | 1559 | BR = ARF3e * QinF - ARF2e * h * UinF |
ulalume3@0 | 1560 | |
volker@23 | 1561 | # Correction parameters for normal measurements; they are independent of LDR |
volker@16 | 1562 | if (not RotationErrorEpsilonForNormalMeasurements): |
binietoglou@19 | 1563 | GT = ATF1 * IinE + ATF4 * VinE |
binietoglou@19 | 1564 | GR = ARF1 * IinE + ARF4 * VinE |
binietoglou@19 | 1565 | HT = ATF2 * QinE - ATF3 * UinE - ATF4 * 2 * VinE |
binietoglou@19 | 1566 | HR = ARF2 * QinE - ARF3 * UinE - ARF4 * 2 * VinE |
volker@16 | 1567 | else: |
binietoglou@19 | 1568 | GT = ATF1 * IinE + ATF4 * h * VinE |
binietoglou@19 | 1569 | GR = ARF1 * IinE + ARF4 * h * VinE |
binietoglou@19 | 1570 | HT = ATF2e * QinE - ATF3e * h * UinE - ATF4 * h * 2 * VinE |
binietoglou@19 | 1571 | HR = ARF2e * QinE - ARF3e * h * UinE - ARF4 * h * 2 * VinE |
ulalume3@0 | 1572 | |
volker@16 | 1573 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
volker@16 | 1574 | # p = +45°, m = -45° |
binietoglou@19 | 1575 | IF1e = np.array([IinF, ZiC * CosC * QinFe, UinFe, ZiC * CosC * VinF]) |
binietoglou@19 | 1576 | IF2e = np.array([DiC * UinFe, -ZiC * SinC * VinF, DiC * IinF, ZiC * SinC * QinFe]) |
ulalume3@0 | 1577 | |
binietoglou@19 | 1578 | AT = np.dot(ATFe, IF1e) |
binietoglou@19 | 1579 | AR = np.dot(ARFe, IF1e) |
binietoglou@19 | 1580 | BT = np.dot(ATFe, IF2e) |
binietoglou@19 | 1581 | BR = np.dot(ARFe, IF2e) |
ulalume3@0 | 1582 | |
volker@23 | 1583 | # Correction parameters for normal measurements; they are independent of LDR --- the same as for TypeC = 6 |
binietoglou@19 | 1584 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 1585 | IS1 = np.array([IinE, 0, 0, VinE]) |
binietoglou@19 | 1586 | IS2 = np.array([0, QinE, -UinE, -2 * VinE]) |
ulalume3@0 | 1587 | |
binietoglou@19 | 1588 | GT = np.dot(ATF, IS1) |
binietoglou@19 | 1589 | GR = np.dot(ARF, IS1) |
binietoglou@19 | 1590 | HT = np.dot(ATF, IS2) |
binietoglou@19 | 1591 | HR = np.dot(ARF, IS2) |
volker@16 | 1592 | else: |
binietoglou@19 | 1593 | IS1e = np.array( |
binietoglou@19 | 1594 | [IinFo + DiC * QinFoe, DiC * IinFo + QinFoe, ZiC * (CosC * UinFoe + SinC * VinFo), |
binietoglou@19 | 1595 | -ZiC * (SinC * UinFoe - CosC * VinFo)]) |
binietoglou@19 | 1596 | IS2e = np.array( |
binietoglou@19 | 1597 | [IinFa + DiC * QinFae, DiC * IinFa + QinFae, ZiC * (CosC * UinFae + SinC * VinFa), |
binietoglou@19 | 1598 | -ZiC * (SinC * UinFae - CosC * VinFa)]) |
binietoglou@19 | 1599 | GT = np.dot(ATFe, IS1e) |
binietoglou@19 | 1600 | GR = np.dot(ARFe, IS1e) |
binietoglou@19 | 1601 | HT = np.dot(ATFe, IS2e) |
binietoglou@19 | 1602 | HR = np.dot(ARFe, IS2e) |
ulalume3@0 | 1603 | |
volker@16 | 1604 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
volker@16 | 1605 | # p = +22.5°, m = -22.5° |
binietoglou@19 | 1606 | IF1e = np.array([IinF + sqr05 * DiC * QinFe, sqr05 * DiC * IinF + (1 - 0.5 * WiC) * QinFe, |
binietoglou@19 | 1607 | (1 - 0.5 * WiC) * UinFe + sqr05 * ZiC * SinC * VinF, |
binietoglou@19 | 1608 | -sqr05 * ZiC * SinC * UinFe + ZiC * CosC * VinF]) |
binietoglou@19 | 1609 | IF2e = np.array([sqr05 * DiC * UinFe, 0.5 * WiC * UinFe - sqr05 * ZiC * SinC * VinF, |
binietoglou@19 | 1610 | sqr05 * DiC * IinF + 0.5 * WiC * QinFe, sqr05 * ZiC * SinC * QinFe]) |
ulalume3@0 | 1611 | |
binietoglou@19 | 1612 | AT = np.dot(ATFe, IF1e) |
binietoglou@19 | 1613 | AR = np.dot(ARFe, IF1e) |
binietoglou@19 | 1614 | BT = np.dot(ATFe, IF2e) |
binietoglou@19 | 1615 | BR = np.dot(ARFe, IF2e) |
ulalume3@0 | 1616 | |
volker@23 | 1617 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 1618 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 1619 | # IS1 = np.array([IinE,0,0,VinE]) |
binietoglou@19 | 1620 | # IS2 = np.array([0,QinE,-UinE,-2*VinE]) |
binietoglou@19 | 1621 | IS1 = np.array([IinFo, 0, 0, VinFo]) |
binietoglou@19 | 1622 | IS2 = np.array([0, QinFa, UinFa, VinFa]) |
binietoglou@19 | 1623 | GT = np.dot(ATF, IS1) |
binietoglou@19 | 1624 | GR = np.dot(ARF, IS1) |
binietoglou@19 | 1625 | HT = np.dot(ATF, IS2) |
binietoglou@19 | 1626 | HR = np.dot(ARF, IS2) |
volker@16 | 1627 | else: |
binietoglou@19 | 1628 | # IS1e = np.array([IinE,DiC*IinE,ZiC*SinC*VinE,ZiC*CosC*VinE]) |
binietoglou@19 | 1629 | # IS2e = np.array([DiC*QinEe,QinEe,-ZiC*(CosC*UinEe+2*SinC*VinE),ZiC*(SinC*UinEe-2*CosC*VinE)]) |
binietoglou@19 | 1630 | IS1e = np.array( |
binietoglou@19 | 1631 | [IinFo + DiC * QinFoe, DiC * IinFo + QinFoe, ZiC * (CosC * UinFoe + SinC * VinFo), |
binietoglou@19 | 1632 | -ZiC * (SinC * UinFoe - CosC * VinFo)]) |
binietoglou@19 | 1633 | IS2e = np.array( |
binietoglou@19 | 1634 | [IinFa + DiC * QinFae, DiC * IinFa + QinFae, ZiC * (CosC * UinFae + SinC * VinFa), |
binietoglou@19 | 1635 | -ZiC * (SinC * UinFae - CosC * VinFa)]) |
binietoglou@19 | 1636 | GT = np.dot(ATFe, IS1e) |
binietoglou@19 | 1637 | GR = np.dot(ARFe, IS1e) |
binietoglou@19 | 1638 | HT = np.dot(ATFe, IS2e) |
binietoglou@19 | 1639 | HR = np.dot(ARFe, IS2e) |
ulalume3@0 | 1640 | |
ulalume3@0 | 1641 | |
volker@16 | 1642 | else: |
volker@16 | 1643 | print('Calibrator not implemented yet') |
volker@16 | 1644 | sys.exit() |
ulalume3@0 | 1645 | |
volker@16 | 1646 | elif LocC == 2: # C behind emitter optics Eq.57 |
binietoglou@19 | 1647 | # print("Calibrator location not implemented yet") |
binietoglou@19 | 1648 | S2e = np.sin(np.deg2rad(2 * RotC)) |
binietoglou@19 | 1649 | C2e = np.cos(np.deg2rad(2 * RotC)) |
ulalume3@0 | 1650 | |
volker@16 | 1651 | # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt) |
binietoglou@19 | 1652 | AF1 = np.array([1, C2g * DiO, S2g * DiO, 0]) |
binietoglou@19 | 1653 | AF2 = np.array([C2g * DiO, 1 - S2g ** 2 * WiO, S2g * C2g * WiO, -S2g * ZiO * SinO]) |
binietoglou@19 | 1654 | AF3 = np.array([S2g * DiO, S2g * C2g * WiO, 1 - C2g ** 2 * WiO, C2g * ZiO * SinO]) |
binietoglou@19 | 1655 | AF4 = np.array([0, S2g * SinO, -C2g * SinO, CosO]) |
ulalume3@0 | 1656 | |
binietoglou@19 | 1657 | ATF = (ATP1 * AF1 + ATP2 * AF2 + ATP3 * AF3 + ATP4 * AF4) |
binietoglou@19 | 1658 | ARF = (ARP1 * AF1 + ARP2 * AF2 + ARP3 * AF3 + ARP4 * AF4) |
volker@16 | 1659 | ATF1 = ATF[0] |
volker@16 | 1660 | ATF2 = ATF[1] |
volker@16 | 1661 | ATF3 = ATF[2] |
volker@16 | 1662 | ATF4 = ATF[3] |
volker@16 | 1663 | ARF1 = ARF[0] |
volker@16 | 1664 | ARF2 = ARF[1] |
volker@16 | 1665 | ARF3 = ARF[2] |
volker@16 | 1666 | ARF4 = ARF[3] |
ulalume3@0 | 1667 | |
volker@16 | 1668 | # AS with C behind the emitter -------------------------------------------- |
volker@16 | 1669 | # terms without aCal |
volker@16 | 1670 | ATE1o, ARE1o = ATF1, ARF1 |
volker@16 | 1671 | ATE2o, ARE2o = 0., 0. |
volker@16 | 1672 | ATE3o, ARE3o = 0., 0. |
volker@16 | 1673 | ATE4o, ARE4o = ATF4, ARF4 |
volker@16 | 1674 | # terms with aCal |
binietoglou@19 | 1675 | ATE1a, ARE1a = 0., 0. |
volker@16 | 1676 | ATE2a, ARE2a = ATF2, ARF2 |
volker@16 | 1677 | ATE3a, ARE3a = -ATF3, -ARF3 |
binietoglou@19 | 1678 | ATE4a, ARE4a = -2 * ATF4, -2 * ARF4 |
volker@16 | 1679 | # rotated AinEa by epsilon |
binietoglou@19 | 1680 | ATE2ae = C2e * ATF2 + S2e * ATF3 |
binietoglou@19 | 1681 | ATE3ae = -S2e * ATF2 - C2e * ATF3 |
binietoglou@19 | 1682 | ARE2ae = C2e * ARF2 + S2e * ARF3 |
binietoglou@19 | 1683 | ARE3ae = -S2e * ARF2 - C2e * ARF3 |
volker@16 | 1684 | |
volker@16 | 1685 | ATE1 = ATE1o |
binietoglou@19 | 1686 | ATE2e = aCal * ATE2ae |
binietoglou@19 | 1687 | ATE3e = aCal * ATE3ae |
binietoglou@19 | 1688 | ATE4 = (1 - 2 * aCal) * ATF4 |
volker@16 | 1689 | ARE1 = ARE1o |
binietoglou@19 | 1690 | ARE2e = aCal * ARE2ae |
binietoglou@19 | 1691 | ARE3e = aCal * ARE3ae |
binietoglou@19 | 1692 | ARE4 = (1 - 2 * aCal) * ARF4 |
ulalume3@0 | 1693 | |
volker@16 | 1694 | # rotated IinE |
binietoglou@19 | 1695 | QinEe = C2e * QinE + S2e * UinE |
binietoglou@19 | 1696 | UinEe = C2e * UinE - S2e * QinE |
volker@16 | 1697 | |
volker@16 | 1698 | # --- Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
binietoglou@19 | 1699 | if (TypeC == 2) or (TypeC == 1): # +++++++++ rotator calibration Eq. C.4 |
binietoglou@19 | 1700 | AT = ATE1o * IinE + (ATE4o + aCal * ATE4a) * h * VinE |
binietoglou@19 | 1701 | BT = aCal * (ATE3ae * QinEe - ATE2ae * h * UinEe) |
binietoglou@19 | 1702 | AR = ARE1o * IinE + (ARE4o + aCal * ARE4a) * h * VinE |
binietoglou@19 | 1703 | BR = aCal * (ARE3ae * QinEe - ARE2ae * h * UinEe) |
ulalume3@0 | 1704 | |
volker@23 | 1705 | # Correction parameters for normal measurements; they are independent of LDR |
volker@16 | 1706 | if (not RotationErrorEpsilonForNormalMeasurements): |
volker@16 | 1707 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
binietoglou@19 | 1708 | GT = ATE1o * IinE + ATE4o * h * VinE |
binietoglou@19 | 1709 | GR = ARE1o * IinE + ARE4o * h * VinE |
binietoglou@19 | 1710 | HT = ATE2a * QinE + ATE3a * h * UinEe + ATE4a * h * VinE |
binietoglou@19 | 1711 | HR = ARE2a * QinE + ARE3a * h * UinEe + ARE4a * h * VinE |
volker@16 | 1712 | else: |
binietoglou@19 | 1713 | GT = ATE1o * IinE + ATE4o * h * VinE |
binietoglou@19 | 1714 | GR = ARE1o * IinE + ARE4o * h * VinE |
binietoglou@19 | 1715 | HT = ATE2ae * QinE + ATE3ae * h * UinEe + ATE4a * h * VinE |
binietoglou@19 | 1716 | HR = ARE2ae * QinE + ARE3ae * h * UinEe + ARE4a * h * VinE |
volker@16 | 1717 | |
volker@16 | 1718 | elif (TypeC == 3) or (TypeC == 4): # +++++++++ linear polariser calibration Eq. C.5 |
volker@16 | 1719 | # p = +45°, m = -45° |
binietoglou@19 | 1720 | AT = ATE1 * IinE + ZiC * CosC * (ATE2e * QinEe + ATE4 * VinE) + ATE3e * UinEe |
binietoglou@19 | 1721 | BT = DiC * (ATE1 * UinEe + ATE3e * IinE) + ZiC * SinC * (ATE4 * QinEe - ATE2e * VinE) |
binietoglou@19 | 1722 | AR = ARE1 * IinE + ZiC * CosC * (ARE2e * QinEe + ARE4 * VinE) + ARE3e * UinEe |
binietoglou@19 | 1723 | BR = DiC * (ARE1 * UinEe + ARE3e * IinE) + ZiC * SinC * (ARE4 * QinEe - ARE2e * VinE) |
ulalume3@0 | 1724 | |
volker@23 | 1725 | # Correction parameters for normal measurements; they are independent of LDR |
volker@16 | 1726 | if (not RotationErrorEpsilonForNormalMeasurements): |
volker@16 | 1727 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
binietoglou@19 | 1728 | GT = ATE1o * IinE + ATE4o * VinE |
binietoglou@19 | 1729 | GR = ARE1o * IinE + ARE4o * VinE |
binietoglou@19 | 1730 | HT = ATE2a * QinE + ATE3a * UinE + ATE4a * VinE |
binietoglou@19 | 1731 | HR = ARE2a * QinE + ARE3a * UinE + ARE4a * VinE |
volker@16 | 1732 | else: |
binietoglou@19 | 1733 | D = IinE + DiC * QinEe |
binietoglou@19 | 1734 | A = DiC * IinE + QinEe |
binietoglou@19 | 1735 | B = ZiC * (CosC * UinEe + SinC * VinE) |
binietoglou@19 | 1736 | C = -ZiC * (SinC * UinEe - CosC * VinE) |
binietoglou@19 | 1737 | GT = ATE1o * D + ATE4o * C |
binietoglou@19 | 1738 | GR = ARE1o * D + ARE4o * C |
binietoglou@19 | 1739 | HT = ATE2a * A + ATE3a * B + ATE4a * C |
binietoglou@19 | 1740 | HR = ARE2a * A + ARE3a * B + ARE4a * C |
ulalume3@0 | 1741 | |
volker@16 | 1742 | elif (TypeC == 6): # real HWP calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
volker@16 | 1743 | # p = +22.5°, m = -22.5° |
binietoglou@19 | 1744 | IE1e = np.array([IinE + sqr05 * DiC * QinEe, sqr05 * DiC * IinE + (1 - 0.5 * WiC) * QinEe, |
binietoglou@19 | 1745 | (1 - 0.5 * WiC) * UinEe + sqr05 * ZiC * SinC * VinE, |
binietoglou@19 | 1746 | -sqr05 * ZiC * SinC * UinEe + ZiC * CosC * VinE]) |
binietoglou@19 | 1747 | IE2e = np.array([sqr05 * DiC * UinEe, 0.5 * WiC * UinEe - sqr05 * ZiC * SinC * VinE, |
binietoglou@19 | 1748 | sqr05 * DiC * IinE + 0.5 * WiC * QinEe, sqr05 * ZiC * SinC * QinEe]) |
binietoglou@19 | 1749 | ATEe = np.array([ATE1, ATE2e, ATE3e, ATE4]) |
binietoglou@19 | 1750 | AREe = np.array([ARE1, ARE2e, ARE3e, ARE4]) |
binietoglou@19 | 1751 | AT = np.dot(ATEe, IE1e) |
binietoglou@19 | 1752 | AR = np.dot(AREe, IE1e) |
binietoglou@19 | 1753 | BT = np.dot(ATEe, IE2e) |
binietoglou@19 | 1754 | BR = np.dot(AREe, IE2e) |
ulalume3@0 | 1755 | |
volker@23 | 1756 | # Correction parameters for normal measurements; they are independent of LDR |
binietoglou@19 | 1757 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
binietoglou@19 | 1758 | GT = ATE1o * IinE + ATE4o * VinE |
binietoglou@19 | 1759 | GR = ARE1o * IinE + ARE4o * VinE |
binietoglou@19 | 1760 | HT = ATE2a * QinE + ATE3a * UinE + ATE4a * VinE |
binietoglou@19 | 1761 | HR = ARE2a * QinE + ARE3a * UinE + ARE4a * VinE |
volker@16 | 1762 | else: |
binietoglou@19 | 1763 | D = IinE + DiC * QinEe |
binietoglou@19 | 1764 | A = DiC * IinE + QinEe |
binietoglou@19 | 1765 | B = ZiC * (CosC * UinEe + SinC * VinE) |
binietoglou@19 | 1766 | C = -ZiC * (SinC * UinEe - CosC * VinE) |
binietoglou@19 | 1767 | GT = ATE1o * D + ATE4o * C |
binietoglou@19 | 1768 | GR = ARE1o * D + ARE4o * C |
binietoglou@19 | 1769 | HT = ATE2a * A + ATE3a * B + ATE4a * C |
binietoglou@19 | 1770 | HR = ARE2a * A + ARE3a * B + ARE4a * C |
ulalume3@0 | 1771 | else: |
volker@16 | 1772 | print('Calibrator not implemented yet') |
volker@16 | 1773 | sys.exit() |
ulalume3@0 | 1774 | |
volker@28 | 1775 | for iTCalT, iTCalR, iNCalTp, iNCalTm, iNCalRp, iNCalRm, iNIt, iNIr \ |
volker@28 | 1776 | in [ |
volker@28 | 1777 | (iTCalT, iTCalR, iNCalTp, iNCalTm, iNCalRp, iNCalRm, iNIt, iNIr) |
volker@28 | 1778 | for iTCalT in range(-nTCalT, nTCalT + 1) # Etax |
volker@28 | 1779 | for iTCalR in range(-nTCalR, nTCalR + 1) # Etax |
volker@28 | 1780 | for iNCalTp in range(-nNCal, nNCal + 1) # noise error of calibration signals => Etax |
volker@28 | 1781 | for iNCalTm in range(-nNCal, nNCal + 1) # noise error of calibration signals => Etax |
volker@28 | 1782 | for iNCalRp in range(-nNCal, nNCal + 1) # noise error of calibration signals => Etax |
volker@28 | 1783 | for iNCalRm in range(-nNCal, nNCal + 1) # noise error of calibration signals => Etax |
volker@28 | 1784 | for iNIt in range(-nNI, nNI + 1) |
volker@28 | 1785 | for iNIr in range(-nNI, nNI + 1)]: |
ulalume3@0 | 1786 | |
volker@28 | 1787 | # Calibration signals with aCal => Determination of the correction K of the real calibration factor |
volker@28 | 1788 | IoutTp = TTa * TiC * TiO * TiE * (AT + BT) |
volker@28 | 1789 | IoutTm = TTa * TiC * TiO * TiE * (AT - BT) |
volker@28 | 1790 | IoutRp = TRa * TiC * TiO * TiE * (AR + BR) |
volker@28 | 1791 | IoutRm = TRa * TiC * TiO * TiE * (AR - BR) |
volker@16 | 1792 | |
volker@28 | 1793 | if nTCalT > 0: TCalT = TCalT0 + iTCalT * dTCalT / nTCalT |
volker@28 | 1794 | if nTCalR > 0: TCalR = TCalR0 + iTCalR * dTCalR / nTCalR |
volker@28 | 1795 | # signal noise errors |
volker@28 | 1796 | # ----- random error calculation ---------- |
volker@28 | 1797 | # noise must be calculated from/with the actually measured signals; influence of TCalT, TCalR errors on nouse are not considered ? |
volker@28 | 1798 | # actually measured signals are in input file and don't change |
volker@28 | 1799 | # relative standard deviation of calibration signals with LDRcal; assumed to be statisitcally independent |
volker@28 | 1800 | # error nNCal: one-sigma in steps to left and right for calibration signals |
volker@28 | 1801 | if nNCal > 0: |
volker@28 | 1802 | if (CalcFrom0deg): |
volker@28 | 1803 | dIoutTp = (NCalT * IoutTp) ** -0.5 |
volker@28 | 1804 | dIoutTm = (NCalT * IoutTm) ** -0.5 |
volker@28 | 1805 | dIoutRp = (NCalR * IoutRp) ** -0.5 |
volker@28 | 1806 | dIoutRm = (NCalR * IoutRm) ** -0.5 |
volker@28 | 1807 | else: |
volker@28 | 1808 | dIoutTp = dIoutTp0 * (IoutTp / IoutTp0) |
volker@28 | 1809 | dIoutTm = dIoutTm0 * (IoutTm / IoutTm0) |
volker@28 | 1810 | dIoutRp = dIoutRp0 * (IoutRp / IoutRp0) |
volker@28 | 1811 | dIoutRm = dIoutRm0 * (IoutRm / IoutRm0) |
volker@28 | 1812 | # print(iTCalT, iTCalR, iNCalTp, iNCalTm, iNCalRp, iNCalRm, iNIt, iNIr, IoutTp, dIoutTp) |
volker@28 | 1813 | IoutTp = IoutTp * (1 + iNCalTp * dIoutTp / nNCal) |
volker@28 | 1814 | IoutTm = IoutTm * (1 + iNCalTm * dIoutTm / nNCal) |
volker@28 | 1815 | IoutRp = IoutRp * (1 + iNCalRp * dIoutRp / nNCal) |
volker@28 | 1816 | IoutRm = IoutRm * (1 + iNCalRm * dIoutRm / nNCal) |
volker@16 | 1817 | |
volker@28 | 1818 | IoutTp = IoutTp * TCalT / TCalT0 |
volker@28 | 1819 | IoutTm = IoutTm * TCalT / TCalT0 |
volker@28 | 1820 | IoutRp = IoutRp * TCalR / TCalR0 |
volker@28 | 1821 | IoutRm = IoutRm * TCalR / TCalR0 |
volker@28 | 1822 | # --- Results and Corrections; electronic etaR and etaT are assumed to be 1 for true and assumed true systems |
volker@28 | 1823 | # calibration factor |
volker@28 | 1824 | Eta = (TRa / TTa) # = TRa / TTa; Eta = Eta*/K Eq. 84; corrected according to the papers supplement Eqs. (S.10.10.1) ff |
volker@28 | 1825 | # possibly real calibration factor |
volker@28 | 1826 | Etapx = IoutRp / IoutTp |
volker@28 | 1827 | Etamx = IoutRm / IoutTm |
volker@28 | 1828 | Etax = (Etapx * Etamx) ** 0.5 |
volker@28 | 1829 | K = Etax / Eta |
volker@28 | 1830 | # print("{0:6.3f},{1:6.3f},{2:6.3f},{3:6.3f},{4:6.3f},{5:6.3f},{6:6.3f},{7:6.3f},{8:6.3f},{9:6.3f},{10:6.3f}".format(AT, BT, AR, BR, DiC, ZiC, RetO, TP, TS, Kp, Km)) |
volker@28 | 1831 | # print("{0:6.3f},{1:6.3f},{2:6.3f},{3:6.3f}".format(DiC, ZiC, Kp, Km)) |
volker@28 | 1832 | |
volker@28 | 1833 | # For comparison with Volkers Libreoffice Müller Matrix spreadsheet |
volker@28 | 1834 | # Eta_test_p = (IoutRp/IoutTp) |
volker@28 | 1835 | # Eta_test_m = (IoutRm/IoutTm) |
volker@28 | 1836 | # Eta_test = (Eta_test_p*Eta_test_m)**0.5 |
volker@16 | 1837 | ''' |
volker@28 | 1838 | for iIt, iIr \ |
volker@28 | 1839 | in [(iIt, iIr) |
volker@28 | 1840 | for iIt in range(-nNI, nNI + 1) |
volker@28 | 1841 | for iIr in range(-nNI, nNI + 1)]: |
volker@21 | 1842 | ''' |
volker@28 | 1843 | |
volker@28 | 1844 | iN = iN + 1 |
volker@28 | 1845 | if (iN == 10001): |
volker@28 | 1846 | ctime = clock() |
volker@28 | 1847 | print(" estimated time ", "{0:4.2f}".format(N / 10000 * (ctime - atime)), "sec ") # , end="") |
volker@28 | 1848 | print("\r elapsed time ", "{0:5.0f}".format((ctime - atime)), "sec ", end="\r") |
volker@28 | 1849 | ctime = clock() |
volker@28 | 1850 | if ((ctime - dtime) > 10): |
volker@28 | 1851 | print("\r elapsed time ", "{0:5.0f}".format((ctime - atime)), "sec ", end="\r") |
volker@28 | 1852 | dtime = ctime |
ulalume3@0 | 1853 | |
volker@28 | 1854 | # *** loop for different real LDRs ********************************************************************** |
volker@28 | 1855 | iLDR = -1 |
volker@28 | 1856 | for LDRTrue in LDRrange: |
volker@28 | 1857 | iLDR = iLDR + 1 |
volker@28 | 1858 | atrue = (1 - LDRTrue) / (1 + LDRTrue) |
volker@28 | 1859 | # ----- Forward simulated signals and LDRsim with atrue; from input file; not considering TiC. |
volker@28 | 1860 | It = TTa * TiO * TiE * (GT + atrue * HT) # TaT*TiT*TiC*TiO*IinL*(GT+atrue*HT) |
volker@28 | 1861 | Ir = TRa * TiO * TiE * (GR + atrue * HR) # TaR*TiR*TiC*TiO*IinL*(GR+atrue*HR) |
volker@28 | 1862 | # # signal noise errors; standard deviation of signals; assumed to be statisitcally independent |
volker@28 | 1863 | # because the signals depend on LDRtrue, the errors dIt and dIr must be calculated for each LDRtrue |
volker@28 | 1864 | if (CalcFrom0deg): |
volker@28 | 1865 | dIt = ((NCalT * It / IoutTp * NILfac / TCalT) ** -0.5) |
volker@28 | 1866 | dIr = ((NCalR * Ir / IoutRp * NILfac / TCalR) ** -0.5) |
volker@28 | 1867 | else: |
volker@28 | 1868 | dIt = ((NCalT * 2 * NILfac / TCalT ) ** -0.5) * It |
volker@28 | 1869 | dIr = ((NCalR * 2 * NILfac / TCalR) ** -0.5) * Ir |
volker@28 | 1870 | # error nNI: one-sigma in steps to left and right for 0° signals |
volker@28 | 1871 | if nNI > 0: |
volker@28 | 1872 | It = It * (1 + iNIt * dIt / nNI) |
volker@28 | 1873 | Ir = Ir * (1 + iNIr * dIr / nNI) |
volker@16 | 1874 | |
volker@28 | 1875 | # LDRsim = 1/Eta*Ir/It # simulated LDR* with Y from input file |
volker@28 | 1876 | LDRsim = Ir / It # simulated uncorrected LDR with Y from input file |
volker@16 | 1877 | |
volker@28 | 1878 | # ----- Backward correction |
volker@28 | 1879 | # Corrected LDRCorr with assumed true G0,H0,K0,Eta0 from forward simulated (real) LDRsim(atrue) |
volker@28 | 1880 | LDRCorr = (LDRsim / (Etax / K0) * (GT0 + HT0) - (GR0 + HR0)) / ((GR0 - HR0) - LDRsim / (Etax / K0) * (GT0 - HT0)) |
volker@28 | 1881 | |
volker@28 | 1882 | # The following is a test whether the equations for calibration Etax and normal signal (GHK, LDRsim) are consistent |
volker@28 | 1883 | # LDRCorr = (LDRsim / Eta * (GT + HT) - (GR + HR)) / ((GR - HR) - LDRsim / Eta * (GT - HT)) |
volker@28 | 1884 | # Without any correction |
volker@28 | 1885 | LDRunCorr = (LDRsim / Etax * (GT / abs(GT) + HT / abs(HT)) - (GR / abs(GR) + HR / abs(HR))) / ((GR / abs(GR) - HR / abs(HR)) - LDRsim / Etax * (GT / abs(GT) - HT / abs(HT))) |
volker@28 | 1886 | |
ulalume3@0 | 1887 | |
volker@28 | 1888 | ''' |
volker@28 | 1889 | # -- F11corr from It and Ir and calibration EtaX |
volker@28 | 1890 | Text1 = "!!! EXPERIMENTAL !!! F11corr from It and Ir with calibration EtaX: x-axis: F11corr(LDRtrue) / F11corr(LDRtrue = 0.004) - 1" |
volker@28 | 1891 | F11corr = 1 / (TiO * TiE) * ( |
volker@28 | 1892 | (HR0 * Etax / K0 * It / TTa - HT0 * Ir / TRa) / (HR0 * GT0 - HT0 * GR0)) # IL = 1 Eq.(64); Etax/K0 = Eta0. |
volker@28 | 1893 | ''' |
volker@28 | 1894 | # Corrected F11corr with assumed true G0,H0,K0 from forward simulated (real) It and Ir (atrue) |
volker@28 | 1895 | Text1 = "!!! EXPERIMENTAL !!! F11corr from real It and Ir with real calibration EtaX: x-axis: F11corr(LDRtrue) / aF11sim0(LDRtrue) - 1" |
volker@28 | 1896 | F11corr = 1 / (TiO * TiE) * ( |
volker@28 | 1897 | (HR0 * Etax / K0 * It / TTa - HT0 * Ir / TRa) / (HR0 * GT0 - HT0 * GR0)) # IL = 1 Eq.(64); Etax/K0 = Eta0. |
volker@28 | 1898 | |
volker@28 | 1899 | # Text1 = "F11corr from It and Ir without corrections but with calibration EtaX: x-axis: F11corr(LDRtrue) devided by F11corr(LDRtrue = 0.004)" |
volker@28 | 1900 | # F11corr = 0.5/(TiO*TiE)*(Etax*It/TTa+Ir/TRa) # IL = 1 Eq.(64) |
volker@16 | 1901 | |
volker@28 | 1902 | # -- It from It only with atrue without corrections - for BERTHA (and PollyXTs) |
volker@28 | 1903 | # Text1 = " x-axis: IT(LDRtrue) / IT(LDRtrue = 0.004) - 1" |
volker@28 | 1904 | # F11corr = It/(TaT*TiT*TiO*TiE) #/(TaT*TiT*TiO*TiE*(GT0+atrue*HT0)) |
volker@28 | 1905 | # ! see below line 1673ff |
volker@28 | 1906 | |
volker@28 | 1907 | aF11corr[iLDR, iN] = F11corr |
volker@28 | 1908 | aLDRcorr[iLDR, iN] = LDRCorr # LDRCorr # LDRsim # for test only |
volker@28 | 1909 | # aPLDR[iLDR, iN] = CalcPLDR(LDRCorr, BSR[iLDR], LDRm0) |
volker@28 | 1910 | aEtax[iLDR, iN] = Etax |
volker@28 | 1911 | |
volker@28 | 1912 | aGHK[0, iN] = GR |
volker@28 | 1913 | aGHK[1, iN] = GT |
volker@28 | 1914 | aGHK[2, iN] = HR |
volker@28 | 1915 | aGHK[3, iN] = HT |
volker@28 | 1916 | aGHK[4, iN] = K |
volker@16 | 1917 | |
volker@28 | 1918 | aLDRCal[iN] = iLDRCal |
volker@28 | 1919 | aDOLP[iN] = iDOLP |
volker@28 | 1920 | aERaT[iN] = iERaT |
volker@28 | 1921 | aERaR[iN] = iERaR |
volker@28 | 1922 | aRotaT[iN] = iRotaT |
volker@28 | 1923 | aRotaR[iN] = iRotaR |
volker@28 | 1924 | aRetT[iN] = iRetT |
volker@28 | 1925 | aRetR[iN] = iRetR |
volker@28 | 1926 | |
volker@28 | 1927 | aRotL[iN] = iRotL |
volker@28 | 1928 | aRotE[iN] = iRotE |
volker@28 | 1929 | aRetE[iN] = iRetE |
volker@28 | 1930 | aRotO[iN] = iRotO |
volker@28 | 1931 | aRetO[iN] = iRetO |
volker@28 | 1932 | aRotC[iN] = iRotC |
volker@28 | 1933 | aRetC[iN] = iRetC |
volker@28 | 1934 | aDiO[iN] = iDiO |
volker@28 | 1935 | aDiE[iN] = iDiE |
volker@28 | 1936 | aDiC[iN] = iDiC |
volker@28 | 1937 | aTP[iN] = iTP |
volker@28 | 1938 | aTS[iN] = iTS |
volker@28 | 1939 | aRP[iN] = iRP |
volker@28 | 1940 | aRS[iN] = iRS |
volker@28 | 1941 | aTCalT[iN] = iTCalT |
volker@28 | 1942 | aTCalR[iN] = iTCalR |
volker@28 | 1943 | |
volker@28 | 1944 | aNCalTp[iN] = iNCalTp # IoutTp, IoutTm, IoutRp, IoutRm => Etax |
volker@28 | 1945 | aNCalTm[iN] = iNCalTm # IoutTp, IoutTm, IoutRp, IoutRm => Etax |
volker@28 | 1946 | aNCalRp[iN] = iNCalRp # IoutTp, IoutTm, IoutRp, IoutRm => Etax |
volker@28 | 1947 | aNCalRm[iN] = iNCalRm # IoutTp, IoutTm, IoutRp, IoutRm => Etax |
volker@28 | 1948 | aNIt[iN] = iNIt # It, Tr |
volker@28 | 1949 | aNIr[iN] = iNIr # It, Tr |
ulalume3@0 | 1950 | |
volker@16 | 1951 | # --- END loop |
volker@16 | 1952 | btime = clock() |
volker@28 | 1953 | # print("\r done in ", "{0:5.0f}".format(btime - atime), "sec. => producing plots now .... some more seconds ..."), # , end="\r"); |
volker@28 | 1954 | print(" done in ", "{0:5.0f}".format(btime - atime), "sec. => producing plots now .... some more seconds ...") |
volker@16 | 1955 | # --- Plot ----------------------------------------------------------------- |
volker@28 | 1956 | print("Errors from GHK correction uncertainties:") |
volker@16 | 1957 | if (sns_loaded): |
volker@16 | 1958 | sns.set_style("whitegrid") |
volker@28 | 1959 | sns.set_palette("bright6", 6) |
volker@28 | 1960 | # for older seaborn versions: |
volker@28 | 1961 | # sns.set_palette("bright", 6) |
ulalume3@0 | 1962 | |
volker@16 | 1963 | ''' |
volker@16 | 1964 | fig2 = plt.figure() |
volker@28 | 1965 | plt.plot(aLDRcorr[2,:],'b.') |
volker@28 | 1966 | plt.plot(aLDRcorr[3,:],'r.') |
volker@28 | 1967 | plt.plot(aLDRcorr[4,:],'g.') |
volker@28 | 1968 | #plt.plot(aLDRcorr[6,:],'c.') |
volker@16 | 1969 | plt.show |
volker@16 | 1970 | ''' |
binietoglou@19 | 1971 | |
volker@16 | 1972 | # Plot LDR |
volker@16 | 1973 | def PlotSubHist(aVar, aX, X0, daX, iaX, naX): |
volker@28 | 1974 | # aVar is the name of the parameter and aX is the subset of aLDRcorr which is coloured in the plot |
volker@28 | 1975 | # example: PlotSubHist("DOLP", aDOLP, DOLP0, dDOLP, iDOLP, nDOLP) |
volker@16 | 1976 | fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2)) |
volker@16 | 1977 | iLDR = -1 |
volker@16 | 1978 | for LDRTrue in LDRrange: |
volker@16 | 1979 | iLDR = iLDR + 1 |
volker@28 | 1980 | LDRmin[iLDR] = np.amin(aLDRcorr[iLDR, :]) |
volker@28 | 1981 | LDRmax[iLDR] = np.amax(aLDRcorr[iLDR, :]) |
volker@28 | 1982 | Rmin = LDRmin[iLDR] * 0.995 # np.min(aLDRcorr[iLDR,:]) * 0.995 |
volker@28 | 1983 | Rmax = LDRmax[iLDR] * 1.005 # np.max(aLDRcorr[iLDR,:]) * 1.005 |
volker@16 | 1984 | |
binietoglou@19 | 1985 | # plt.subplot(5,2,iLDR+1) |
binietoglou@19 | 1986 | plt.subplot(1, 5, iLDR + 1) |
volker@28 | 1987 | (n, bins, patches) = plt.hist(aLDRcorr[iLDR, :], |
binietoglou@19 | 1988 | bins=100, log=False, |
binietoglou@19 | 1989 | range=[Rmin, Rmax], |
volker@28 | 1990 | alpha=0.5, density=False, color='0.5', histtype='stepfilled') |
ulalume3@0 | 1991 | |
binietoglou@19 | 1992 | for iaX in range(-naX, naX + 1): |
volker@28 | 1993 | plt.hist(aLDRcorr[iLDR, aX == iaX], |
volker@16 | 1994 | range=[Rmin, Rmax], |
volker@28 | 1995 | bins=100, log=False, alpha=0.3, density=False, histtype='stepfilled', |
binietoglou@19 | 1996 | label=str(round(X0 + iaX * daX / naX, 5))) |
volker@16 | 1997 | |
volker@28 | 1998 | if (iLDR == 2): |
volker@28 | 1999 | leg = plt.legend() |
volker@28 | 2000 | leg.get_frame().set_alpha(0.1) |
volker@28 | 2001 | |
volker@16 | 2002 | |
volker@16 | 2003 | plt.tick_params(axis='both', labelsize=9) |
volker@16 | 2004 | plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2) |
volker@16 | 2005 | |
binietoglou@19 | 2006 | # plt.title(LID + ' ' + aVar, fontsize=18) |
binietoglou@19 | 2007 | # plt.ylabel('frequency', fontsize=10) |
binietoglou@19 | 2008 | # plt.xlabel('LDRcorr', fontsize=10) |
binietoglou@19 | 2009 | # fig.tight_layout() |
binietoglou@19 | 2010 | fig.suptitle(LID + ' with ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05) |
binietoglou@19 | 2011 | # plt.show() |
binietoglou@19 | 2012 | # fig.savefig(LID + '_' + aVar + '.png', dpi=150, bbox_inches='tight', pad_inches=0) |
binietoglou@19 | 2013 | # plt.close |
volker@16 | 2014 | return |
ulalume3@0 | 2015 | |
volker@28 | 2016 | # Plot Etax |
volker@28 | 2017 | def PlotEtax(aVar, aX, X0, daX, iaX, naX): |
volker@28 | 2018 | # aVar is the name of the parameter and aX is the subset of aLDRcorr which is coloured in the plot |
volker@28 | 2019 | # example: PlotSubHist("DOLP", aDOLP, DOLP0, dDOLP, iDOLP, nDOLP) |
volker@28 | 2020 | fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2)) |
volker@28 | 2021 | iLDR = -1 |
volker@28 | 2022 | for LDRTrue in LDRrange: |
volker@28 | 2023 | iLDR = iLDR + 1 |
volker@28 | 2024 | Etaxmin[iLDR] = np.amin(aEtax[iLDR, :]) |
volker@28 | 2025 | Etaxmax[iLDR] = np.amax(aEtax[iLDR, :]) |
volker@28 | 2026 | Rmin = Etaxmin[iLDR] * 0.995 # np.min(aLDRcorr[iLDR,:]) * 0.995 |
volker@28 | 2027 | Rmax = Etaxmax[iLDR] * 1.005 # np.max(aLDRcorr[iLDR,:]) * 1.005 |
volker@28 | 2028 | |
volker@28 | 2029 | # plt.subplot(5,2,iLDR+1) |
volker@28 | 2030 | plt.subplot(1, 5, iLDR + 1) |
volker@28 | 2031 | (n, bins, patches) = plt.hist(aEtax[iLDR, :], |
volker@28 | 2032 | bins=100, log=False, |
volker@28 | 2033 | range=[Rmin, Rmax], |
volker@28 | 2034 | alpha=0.5, density=False, color='0.5', histtype='stepfilled') |
volker@28 | 2035 | for iaX in range(-naX, naX + 1): |
volker@28 | 2036 | plt.hist(aEtax[iLDR, aX == iaX], |
volker@28 | 2037 | range=[Rmin, Rmax], |
volker@28 | 2038 | bins=100, log=False, alpha=0.3, density=False, histtype='stepfilled', |
volker@28 | 2039 | label=str(round(X0 + iaX * daX / naX, 5))) |
volker@28 | 2040 | if (iLDR == 2): |
volker@28 | 2041 | leg = plt.legend() |
volker@28 | 2042 | leg.get_frame().set_alpha(0.1) |
volker@28 | 2043 | plt.tick_params(axis='both', labelsize=9) |
volker@28 | 2044 | plt.plot([Etax0, Etax0], [0, np.max(n)], 'r-', lw=2) |
volker@28 | 2045 | fig.suptitle('Etax - ' + LID + ' with ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05) |
volker@28 | 2046 | return |
binietoglou@19 | 2047 | |
volker@23 | 2048 | if (nDOLP > 0): PlotSubHist("DOLP", aDOLP, DOLP0, dDOLP, iDOLP, nDOLP) |
volker@16 | 2049 | if (nRotL > 0): PlotSubHist("RotL", aRotL, RotL0, dRotL, iRotL, nRotL) |
volker@16 | 2050 | if (nRetE > 0): PlotSubHist("RetE", aRetE, RetE0, dRetE, iRetE, nRetE) |
volker@16 | 2051 | if (nRotE > 0): PlotSubHist("RotE", aRotE, RotE0, dRotE, iRotE, nRotE) |
volker@16 | 2052 | if (nDiE > 0): PlotSubHist("DiE", aDiE, DiE0, dDiE, iDiE, nDiE) |
volker@16 | 2053 | if (nRetO > 0): PlotSubHist("RetO", aRetO, RetO0, dRetO, iRetO, nRetO) |
volker@16 | 2054 | if (nRotO > 0): PlotSubHist("RotO", aRotO, RotO0, dRotO, iRotO, nRotO) |
volker@16 | 2055 | if (nDiO > 0): PlotSubHist("DiO", aDiO, DiO0, dDiO, iDiO, nDiO) |
volker@16 | 2056 | if (nDiC > 0): PlotSubHist("DiC", aDiC, DiC0, dDiC, iDiC, nDiC) |
volker@16 | 2057 | if (nRotC > 0): PlotSubHist("RotC", aRotC, RotC0, dRotC, iRotC, nRotC) |
volker@16 | 2058 | if (nRetC > 0): PlotSubHist("RetC", aRetC, RetC0, dRetC, iRetC, nRetC) |
volker@16 | 2059 | if (nTP > 0): PlotSubHist("TP", aTP, TP0, dTP, iTP, nTP) |
volker@16 | 2060 | if (nTS > 0): PlotSubHist("TS", aTS, TS0, dTS, iTS, nTS) |
volker@16 | 2061 | if (nRP > 0): PlotSubHist("RP", aRP, RP0, dRP, iRP, nRP) |
volker@16 | 2062 | if (nRS > 0): PlotSubHist("RS", aRS, RS0, dRS, iRS, nRS) |
volker@16 | 2063 | if (nRetT > 0): PlotSubHist("RetT", aRetT, RetT0, dRetT, iRetT, nRetT) |
volker@16 | 2064 | if (nRetR > 0): PlotSubHist("RetR", aRetR, RetR0, dRetR, iRetR, nRetR) |
volker@16 | 2065 | if (nERaT > 0): PlotSubHist("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT) |
volker@16 | 2066 | if (nERaR > 0): PlotSubHist("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR) |
volker@16 | 2067 | if (nRotaT > 0): PlotSubHist("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT) |
volker@16 | 2068 | if (nRotaR > 0): PlotSubHist("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR) |
volker@16 | 2069 | if (nLDRCal > 0): PlotSubHist("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal) |
volker@28 | 2070 | if (nTCalT > 0): PlotSubHist("TCalT", aTCalT, TCalT0, dTCalT, iTCalT, nTCalT) |
volker@28 | 2071 | if (nTCalR > 0): PlotSubHist("TCalR", aTCalR, TCalR0, dTCalR, iTCalR, nTCalR) |
volker@28 | 2072 | if (nNCal > 0): PlotSubHist("CalNoiseTp", aNCalTp, 0, 1, iNCalTp, nNCal) |
volker@28 | 2073 | if (nNCal > 0): PlotSubHist("CalNoiseTm", aNCalTm, 0, 1, iNCalTm, nNCal) |
volker@28 | 2074 | if (nNCal > 0): PlotSubHist("CalNoiseRp", aNCalRp, 0, 1, iNCalRp, nNCal) |
volker@28 | 2075 | if (nNCal > 0): PlotSubHist("CalNoiseRm", aNCalRm, 0, 1, iNCalRm, nNCal) |
volker@28 | 2076 | if (nNI > 0): PlotSubHist("SigNoiseIt", aNIt, 0, 1, iNIt, nNI) |
volker@28 | 2077 | if (nNI > 0): PlotSubHist("SigNoiseIr", aNIr, 0, 1, iNIr, nNI) |
volker@16 | 2078 | plt.show() |
volker@16 | 2079 | plt.close |
volker@21 | 2080 | |
volker@16 | 2081 | ''' |
volker@21 | 2082 | # --- Plot F11 histograms |
volker@16 | 2083 | print() |
volker@16 | 2084 | print(" ############################################################################## ") |
volker@16 | 2085 | print(Text1) |
volker@16 | 2086 | print() |
volker@16 | 2087 | |
volker@16 | 2088 | iLDR = 5 |
volker@16 | 2089 | for LDRTrue in LDRrange: |
volker@16 | 2090 | iLDR = iLDR - 1 |
volker@21 | 2091 | #aF11corr[iLDR,:] = aF11corr[iLDR,:] / aF11corr[0,:] - 1.0 |
volker@21 | 2092 | aF11corr[iLDR,:] = aF11corr[iLDR,:] / aF11sim0[iLDR] - 1.0 |
volker@16 | 2093 | # Plot F11 |
volker@16 | 2094 | def PlotSubHistF11(aVar, aX, X0, daX, iaX, naX): |
volker@16 | 2095 | fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2)) |
volker@16 | 2096 | iLDR = -1 |
volker@16 | 2097 | for LDRTrue in LDRrange: |
volker@16 | 2098 | iLDR = iLDR + 1 |
volker@16 | 2099 | |
volker@16 | 2100 | #F11min[iLDR] = np.min(aF11corr[iLDR,:]) |
volker@16 | 2101 | #F11max[iLDR] = np.max(aF11corr[iLDR,:]) |
volker@28 | 2102 | #Rmin = F11min[iLDR] * 0.995 # np.min(aLDRcorr[iLDR,:]) * 0.995 |
volker@28 | 2103 | #Rmax = F11max[iLDR] * 1.005 # np.max(aLDRcorr[iLDR,:]) * 1.005 |
volker@16 | 2104 | |
volker@16 | 2105 | #Rmin = 0.8 |
volker@16 | 2106 | #Rmax = 1.2 |
ulalume3@0 | 2107 | |
volker@16 | 2108 | #plt.subplot(5,2,iLDR+1) |
volker@16 | 2109 | plt.subplot(1,5,iLDR+1) |
volker@16 | 2110 | (n, bins, patches) = plt.hist(aF11corr[iLDR,:], |
volker@16 | 2111 | bins=100, log=False, |
volker@28 | 2112 | alpha=0.5, density=False, color = '0.5', histtype='stepfilled') |
volker@16 | 2113 | |
volker@16 | 2114 | for iaX in range(-naX,naX+1): |
volker@16 | 2115 | plt.hist(aF11corr[iLDR,aX == iaX], |
volker@28 | 2116 | bins=100, log=False, alpha=0.3, density=False, histtype='stepfilled', label = str(round(X0 + iaX*daX/naX,5))) |
volker@16 | 2117 | |
volker@16 | 2118 | if (iLDR == 2): plt.legend() |
volker@16 | 2119 | |
volker@16 | 2120 | plt.tick_params(axis='both', labelsize=9) |
volker@16 | 2121 | #plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2) |
volker@16 | 2122 | |
volker@16 | 2123 | #plt.title(LID + ' ' + aVar, fontsize=18) |
volker@16 | 2124 | #plt.ylabel('frequency', fontsize=10) |
volker@16 | 2125 | #plt.xlabel('LDRcorr', fontsize=10) |
volker@16 | 2126 | #fig.tight_layout() |
volker@16 | 2127 | fig.suptitle(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05) |
volker@16 | 2128 | #plt.show() |
volker@16 | 2129 | #fig.savefig(LID + '_' + aVar + '.png', dpi=150, bbox_inches='tight', pad_inches=0) |
volker@16 | 2130 | #plt.close |
volker@16 | 2131 | return |
ulalume3@0 | 2132 | |
volker@23 | 2133 | if (nDOLP > 0): PlotSubHistF11("DOLP", aDOLP, DOLP0, dDOLP, iDOLP, nDOLP) |
volker@16 | 2134 | if (nRotL > 0): PlotSubHistF11("RotL", aRotL, RotL0, dRotL, iRotL, nRotL) |
volker@16 | 2135 | if (nRetE > 0): PlotSubHistF11("RetE", aRetE, RetE0, dRetE, iRetE, nRetE) |
volker@16 | 2136 | if (nRotE > 0): PlotSubHistF11("RotE", aRotE, RotE0, dRotE, iRotE, nRotE) |
volker@16 | 2137 | if (nDiE > 0): PlotSubHistF11("DiE", aDiE, DiE0, dDiE, iDiE, nDiE) |
volker@16 | 2138 | if (nRetO > 0): PlotSubHistF11("RetO", aRetO, RetO0, dRetO, iRetO, nRetO) |
volker@16 | 2139 | if (nRotO > 0): PlotSubHistF11("RotO", aRotO, RotO0, dRotO, iRotO, nRotO) |
volker@16 | 2140 | if (nDiO > 0): PlotSubHistF11("DiO", aDiO, DiO0, dDiO, iDiO, nDiO) |
volker@16 | 2141 | if (nDiC > 0): PlotSubHistF11("DiC", aDiC, DiC0, dDiC, iDiC, nDiC) |
volker@16 | 2142 | if (nRotC > 0): PlotSubHistF11("RotC", aRotC, RotC0, dRotC, iRotC, nRotC) |
volker@16 | 2143 | if (nRetC > 0): PlotSubHistF11("RetC", aRetC, RetC0, dRetC, iRetC, nRetC) |
volker@16 | 2144 | if (nTP > 0): PlotSubHistF11("TP", aTP, TP0, dTP, iTP, nTP) |
volker@16 | 2145 | if (nTS > 0): PlotSubHistF11("TS", aTS, TS0, dTS, iTS, nTS) |
volker@16 | 2146 | if (nRP > 0): PlotSubHistF11("RP", aRP, RP0, dRP, iRP, nRP) |
volker@16 | 2147 | if (nRS > 0): PlotSubHistF11("RS", aRS, RS0, dRS, iRS, nRS) |
volker@16 | 2148 | if (nRetT > 0): PlotSubHistF11("RetT", aRetT, RetT0, dRetT, iRetT, nRetT) |
volker@16 | 2149 | if (nRetR > 0): PlotSubHistF11("RetR", aRetR, RetR0, dRetR, iRetR, nRetR) |
volker@16 | 2150 | if (nERaT > 0): PlotSubHistF11("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT) |
volker@16 | 2151 | if (nERaR > 0): PlotSubHistF11("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR) |
volker@16 | 2152 | if (nRotaT > 0): PlotSubHistF11("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT) |
volker@16 | 2153 | if (nRotaR > 0): PlotSubHistF11("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR) |
volker@16 | 2154 | if (nLDRCal > 0): PlotSubHistF11("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal) |
volker@28 | 2155 | if (nTCalT > 0): PlotSubHistF11("TCalT", aTCalT, TCalT0, dTCalT, iTCalT, nTCalT) |
volker@28 | 2156 | if (nTCalR > 0): PlotSubHistF11("TCalR", aTCalR, TCalR0, dTCalR, iTCalR, nTCalR) |
volker@28 | 2157 | if (nNCal > 0): PlotSubHistF11("CalNoise", aNCal, 0, 1/nNCal, iNCal, nNCal) |
volker@28 | 2158 | if (nNI > 0): PlotSubHistF11("SigNoise", aNI, 0, 1/nNI, iNI, nNI) |
volker@28 | 2159 | |
ulalume3@0 | 2160 | |
volker@16 | 2161 | plt.show() |
volker@16 | 2162 | plt.close |
volker@21 | 2163 | |
volker@16 | 2164 | ''' |
volker@16 | 2165 | ''' |
volker@16 | 2166 | # only histogram |
volker@16 | 2167 | #print("******************* " + aVar + " *******************") |
volker@16 | 2168 | fig, ax = plt.subplots(nrows=5, ncols=2, sharex=True, sharey=True, figsize=(10, 10)) |
ulalume3@0 | 2169 | iLDR = -1 |
ulalume3@0 | 2170 | for LDRTrue in LDRrange: |
ulalume3@0 | 2171 | iLDR = iLDR + 1 |
volker@28 | 2172 | LDRmin[iLDR] = np.min(aLDRcorr[iLDR,:]) |
volker@28 | 2173 | LDRmax[iLDR] = np.max(aLDRcorr[iLDR,:]) |
volker@28 | 2174 | Rmin = np.min(aLDRcorr[iLDR,:]) * 0.999 |
volker@28 | 2175 | Rmax = np.max(aLDRcorr[iLDR,:]) * 1.001 |
volker@16 | 2176 | plt.subplot(5,2,iLDR+1) |
volker@28 | 2177 | (n, bins, patches) = plt.hist(aLDRcorr[iLDR,:], |
ulalume3@0 | 2178 | range=[Rmin, Rmax], |
volker@28 | 2179 | bins=200, log=False, alpha=0.2, density=False, color = '0.5', histtype='stepfilled') |
ulalume3@0 | 2180 | plt.tick_params(axis='both', labelsize=9) |
ulalume3@0 | 2181 | plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2) |
volker@16 | 2182 | plt.show() |
volker@16 | 2183 | plt.close |
volker@21 | 2184 | # --- End of Plot F11 histograms |
volker@16 | 2185 | ''' |
ulalume3@0 | 2186 | |
volker@16 | 2187 | # --- Plot LDRmin, LDRmax |
volker@28 | 2188 | iLDR = -1 |
volker@28 | 2189 | for LDRTrue in LDRrange: |
volker@28 | 2190 | iLDR = iLDR + 1 |
volker@28 | 2191 | LDRmin[iLDR] = np.amin(aLDRcorr[iLDR, :]) |
volker@28 | 2192 | LDRmax[iLDR] = np.amax(aLDRcorr[iLDR, :]) |
volker@28 | 2193 | |
volker@16 | 2194 | fig2 = plt.figure() |
volker@28 | 2195 | LDRrangeA = np.array(LDRrange) |
volker@28 | 2196 | if((np.amax(LDRmax - LDRrangeA)-np.amin(LDRmin - LDRrangeA)) < 0.001): |
volker@28 | 2197 | plt.ylim(-0.001,0.001) |
volker@28 | 2198 | plt.plot(LDRrangeA, LDRmax - LDRrangeA, linewidth=2.0, color='b') |
volker@28 | 2199 | plt.plot(LDRrangeA, LDRmin - LDRrangeA, linewidth=2.0, color='g') |
ulalume3@0 | 2200 | |
volker@16 | 2201 | plt.xlabel('LDRtrue', fontsize=18) |
volker@16 | 2202 | plt.ylabel('LDRTrue-LDRmin, LDRTrue-LDRmax', fontsize=14) |
volker@16 | 2203 | plt.title(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]), fontsize=18) |
binietoglou@19 | 2204 | # plt.ylimit(-0.07, 0.07) |
volker@16 | 2205 | plt.show() |
volker@16 | 2206 | plt.close |
ulalume3@0 | 2207 | |
volker@16 | 2208 | # --- Save LDRmin, LDRmax to file |
volker@16 | 2209 | # http://stackoverflow.com/questions/4675728/redirect-stdout-to-a-file-in-python |
volker@28 | 2210 | with open('output_files\\' + LID + '-' + InputFile[0:-3] + '-LDR_min_max.dat', 'w') as f: |
volker@16 | 2211 | with redirect_stdout(f): |
volker@16 | 2212 | print(LID) |
volker@16 | 2213 | print("LDRtrue, LDRmin, LDRmax") |
volker@28 | 2214 | for i in range(len(LDRrangeA)): |
volker@28 | 2215 | print("{0:7.4f},{1:7.4f},{2:7.4f}".format(LDRrangeA[i], LDRmin[i], LDRmax[i])) |
volker@28 | 2216 | |
ulalume3@0 | 2217 | |
volker@28 | 2218 | if (bPlotEtax): |
volker@28 | 2219 | if (nDOLP > 0): PlotEtax("DOLP", aDOLP, DOLP0, dDOLP, iDOLP, nDOLP) |
volker@28 | 2220 | if (nRotL > 0): PlotEtax("RotL", aRotL, RotL0, dRotL, iRotL, nRotL) |
volker@28 | 2221 | if (nRetE > 0): PlotEtax("RetE", aRetE, RetE0, dRetE, iRetE, nRetE) |
volker@28 | 2222 | if (nRotE > 0): PlotEtax("RotE", aRotE, RotE0, dRotE, iRotE, nRotE) |
volker@28 | 2223 | if (nDiE > 0): PlotEtax("DiE", aDiE, DiE0, dDiE, iDiE, nDiE) |
volker@28 | 2224 | if (nRetO > 0): PlotEtax("RetO", aRetO, RetO0, dRetO, iRetO, nRetO) |
volker@28 | 2225 | if (nRotO > 0): PlotEtax("RotO", aRotO, RotO0, dRotO, iRotO, nRotO) |
volker@28 | 2226 | if (nDiO > 0): PlotEtax("DiO", aDiO, DiO0, dDiO, iDiO, nDiO) |
volker@28 | 2227 | if (nDiC > 0): PlotEtax("DiC", aDiC, DiC0, dDiC, iDiC, nDiC) |
volker@28 | 2228 | if (nRotC > 0): PlotEtax("RotC", aRotC, RotC0, dRotC, iRotC, nRotC) |
volker@28 | 2229 | if (nRetC > 0): PlotEtax("RetC", aRetC, RetC0, dRetC, iRetC, nRetC) |
volker@28 | 2230 | if (nTP > 0): PlotEtax("TP", aTP, TP0, dTP, iTP, nTP) |
volker@28 | 2231 | if (nTS > 0): PlotEtax("TS", aTS, TS0, dTS, iTS, nTS) |
volker@28 | 2232 | if (nRP > 0): PlotEtax("RP", aRP, RP0, dRP, iRP, nRP) |
volker@28 | 2233 | if (nRS > 0): PlotEtax("RS", aRS, RS0, dRS, iRS, nRS) |
volker@28 | 2234 | if (nRetT > 0): PlotEtax("RetT", aRetT, RetT0, dRetT, iRetT, nRetT) |
volker@28 | 2235 | if (nRetR > 0): PlotEtax("RetR", aRetR, RetR0, dRetR, iRetR, nRetR) |
volker@28 | 2236 | if (nERaT > 0): PlotEtax("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT) |
volker@28 | 2237 | if (nERaR > 0): PlotEtax("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR) |
volker@28 | 2238 | if (nRotaT > 0): PlotEtax("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT) |
volker@28 | 2239 | if (nRotaR > 0): PlotEtax("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR) |
volker@28 | 2240 | if (nLDRCal > 0): PlotEtax("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal) |
volker@28 | 2241 | if (nTCalT > 0): PlotEtax("TCalT", aTCalT, TCalT0, dTCalT, iTCalT, nTCalT) |
volker@28 | 2242 | if (nTCalR > 0): PlotEtax("TCalR", aTCalR, TCalR0, dTCalR, iTCalR, nTCalR) |
volker@28 | 2243 | if (nNCal > 0): PlotEtax("CalNoiseTp", aNCalTp, 0, 1, iNCalTp, nNCal) |
volker@28 | 2244 | if (nNCal > 0): PlotEtax("CalNoiseTm", aNCalTm, 0, 1, iNCalTm, nNCal) |
volker@28 | 2245 | if (nNCal > 0): PlotEtax("CalNoiseRp", aNCalRp, 0, 1, iNCalRp, nNCal) |
volker@28 | 2246 | if (nNCal > 0): PlotEtax("CalNoiseRm", aNCalRm, 0, 1, iNCalRm, nNCal) |
volker@28 | 2247 | if (nNI > 0): PlotEtax("SigNoiseIt", aNIt, 0, 1, iNIt, nNI) |
volker@28 | 2248 | if (nNI > 0): PlotEtax("SigNoiseIr", aNIr, 0, 1, iNIr, nNI) |
volker@28 | 2249 | plt.show() |
volker@28 | 2250 | plt.close |
volker@28 | 2251 | |
volker@28 | 2252 | #Etaxmin = np.amin(aEtax[1, :]) |
volker@28 | 2253 | Etaxmin = np.amin(aEtax[1, :]) |
volker@28 | 2254 | Etaxmax = np.amax(aEtax[1, :]) |
volker@28 | 2255 | Etaxstd = np.std(aEtax[1, :]) |
volker@28 | 2256 | Etaxmean = np.mean(aEtax[1, :]) |
volker@28 | 2257 | Etaxmedian = np.mean(aEtax[1, :]) |
volker@28 | 2258 | |
volker@28 | 2259 | print("Etax: mean±std, median, max-mean, mean-min") |
volker@28 | 2260 | print("{0:7.4f}±{1:7.4f},{2:7.4f},+{3:7.4f},-{4:7.4f}".format(Etaxmean, Etaxstd, Etaxmedian, Etaxmax-Etaxmean, Etaxmean-Etaxmin, )) |
volker@28 | 2261 | |
volker@16 | 2262 | ''' |
volker@16 | 2263 | # --- Plot K over LDRCal |
volker@16 | 2264 | fig3 = plt.figure() |
volker@28 | 2265 | plt.plot(LDRCal0+aLDRCal*dLDRCal/nLDRCal,aGHK[4,:], linewidth=2.0, color='b') |
ulalume3@0 | 2266 | |
volker@16 | 2267 | plt.xlabel('LDRCal', fontsize=18) |
volker@16 | 2268 | plt.ylabel('K', fontsize=14) |
volker@16 | 2269 | plt.title(LID, fontsize=18) |
volker@16 | 2270 | plt.show() |
volker@16 | 2271 | plt.close |
volker@16 | 2272 | ''' |
ulalume3@0 | 2273 | |
ulalume3@0 | 2274 | # Additional plot routines ======> |
ulalume3@0 | 2275 | ''' |
ulalume3@0 | 2276 | #****************************************************************************** |
ulalume3@0 | 2277 | # 1. Plot LDRcorrected - LDR(measured Icross/Iparallel) |
ulalume3@0 | 2278 | LDRa = np.arange(1.,100.)*0.005 |
ulalume3@0 | 2279 | LDRCorra = np.arange(1.,100.) |
ulalume3@0 | 2280 | if Y == - 1.: LDRa = 1./LDRa |
ulalume3@0 | 2281 | LDRCorra = (1./Eta*LDRa*(GT+HT)-(GR+HR))/((GR-HR)-1./Eta*LDRa*(GT-HT)) |
ulalume3@0 | 2282 | if Y == - 1.: LDRa = 1./LDRa |
ulalume3@0 | 2283 | # |
ulalume3@0 | 2284 | #fig = plt.figure() |
ulalume3@0 | 2285 | plt.plot(LDRa,LDRCorra-LDRa) |
ulalume3@0 | 2286 | plt.plot([0.,0.5],[0.,0.5]) |
ulalume3@0 | 2287 | plt.suptitle('LDRcorrected - LDR(measured Icross/Iparallel)', fontsize=16) |
ulalume3@0 | 2288 | plt.xlabel('LDR', fontsize=18) |
ulalume3@0 | 2289 | plt.ylabel('LDRCorr - LDR', fontsize=16) |
ulalume3@0 | 2290 | #plt.savefig('test.png') |
ulalume3@0 | 2291 | # |
ulalume3@0 | 2292 | ''' |
ulalume3@0 | 2293 | ''' |
ulalume3@0 | 2294 | #****************************************************************************** |
ulalume3@0 | 2295 | # 2. Plot LDRsim (simulated measurements without corrections = Icross/Iparallel) over LDRtrue |
ulalume3@0 | 2296 | LDRa = np.arange(1.,100.)*0.005 |
ulalume3@0 | 2297 | LDRsima = np.arange(1.,100.) |
ulalume3@0 | 2298 | |
ulalume3@0 | 2299 | atruea = (1.-LDRa)/(1+LDRa) |
ulalume3@0 | 2300 | Ita = TiT*TiO*IinL*(GT+atruea*HT) |
ulalume3@0 | 2301 | Ira = TiR*TiO*IinL*(GR+atruea*HR) |
ulalume3@0 | 2302 | LDRsima = Ira/Ita # simulated uncorrected LDR with Y from input file |
ulalume3@0 | 2303 | if Y == -1.: LDRsima = 1./LDRsima |
ulalume3@0 | 2304 | # |
ulalume3@0 | 2305 | #fig = plt.figure() |
ulalume3@0 | 2306 | plt.plot(LDRa,LDRsima) |
ulalume3@0 | 2307 | plt.plot([0.,0.5],[0.,0.5]) |
ulalume3@0 | 2308 | plt.suptitle('LDRsim (simulated measurements without corrections = Icross/Iparallel) over LDRtrue', fontsize=10) |
ulalume3@0 | 2309 | plt.xlabel('LDRtrue', fontsize=18) |
ulalume3@0 | 2310 | plt.ylabel('LDRsim', fontsize=16) |
ulalume3@0 | 2311 | #plt.savefig('test.png') |
ulalume3@0 | 2312 | # |
ulalume3@0 | 2313 | ''' |