Mon, 14 Nov 2016 23:42:20 +0100
input file name changed
ulalume3@0 | 1 | # -*- coding: utf-8 -*- |
ulalume3@0 | 2 | """ |
ulalume3@0 | 3 | Copyright 2016 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 |
ulalume3@0 | 20 | Python 3.4.2 |
ulalume3@0 | 21 | """ |
ulalume3@0 | 22 | #!/usr/bin/env python3 |
ulalume3@0 | 23 | from __future__ import print_function |
ulalume3@0 | 24 | #import math |
ulalume3@0 | 25 | import numpy as np |
ulalume3@0 | 26 | import sys |
ulalume3@0 | 27 | import os |
ulalume3@0 | 28 | #import seaborn as sns |
ulalume3@0 | 29 | import matplotlib.pyplot as plt |
ulalume3@0 | 30 | from time import clock |
ulalume3@0 | 31 | |
ulalume3@0 | 32 | #from matplotlib.backends.backend_pdf import PdfPages |
ulalume3@0 | 33 | #pdffile = '{}.pdf'.format('path') |
ulalume3@0 | 34 | #pp = PdfPages(pdffile) |
ulalume3@0 | 35 | ## pp.savefig can be called multiple times to save to multiple pages |
ulalume3@0 | 36 | #pp.savefig() |
ulalume3@0 | 37 | #pp.close() |
ulalume3@0 | 38 | |
ulalume3@0 | 39 | from contextlib import contextmanager |
ulalume3@0 | 40 | @contextmanager |
ulalume3@0 | 41 | def redirect_stdout(new_target): |
ulalume3@0 | 42 | old_target, sys.stdout = sys.stdout, new_target # replace sys.stdout |
ulalume3@0 | 43 | try: |
ulalume3@0 | 44 | yield new_target # run some code with the replaced stdout |
ulalume3@0 | 45 | finally: |
ulalume3@0 | 46 | sys.stdout.flush() |
ulalume3@0 | 47 | sys.stdout = old_target # restore to the previous value |
ulalume3@0 | 48 | ''' |
ulalume3@0 | 49 | real_raw_input = vars(__builtins__).get('raw_input',input) |
ulalume3@0 | 50 | ''' |
ulalume3@0 | 51 | try: |
ulalume3@0 | 52 | import __builtin__ |
ulalume3@0 | 53 | input = getattr(__builtin__, 'raw_input') |
ulalume3@0 | 54 | except (ImportError, AttributeError): |
ulalume3@0 | 55 | pass |
ulalume3@0 | 56 | |
ulalume3@0 | 57 | from distutils.util import strtobool |
ulalume3@0 | 58 | def user_yes_no_query(question): |
ulalume3@0 | 59 | sys.stdout.write('%s [y/n]\n' % question) |
ulalume3@0 | 60 | while True: |
ulalume3@0 | 61 | try: |
ulalume3@0 | 62 | return strtobool(input().lower()) |
ulalume3@0 | 63 | except ValueError: |
ulalume3@0 | 64 | sys.stdout.write('Please respond with \'y\' or \'n\'.\n') |
ulalume3@0 | 65 | |
ulalume3@0 | 66 | #if user_yes_no_query('want to exit?') == 1: sys.exit() |
ulalume3@0 | 67 | |
ulalume3@0 | 68 | abspath = os.path.abspath(__file__) |
ulalume3@0 | 69 | dname = os.path.dirname(abspath) |
ulalume3@0 | 70 | fname = os.path.basename(abspath) |
ulalume3@0 | 71 | os.chdir(dname) |
ulalume3@0 | 72 | |
ulalume3@0 | 73 | #PrintToOutputFile = True |
ulalume3@0 | 74 | |
ulalume3@0 | 75 | sqr05 = 0.5**0.5 |
ulalume3@0 | 76 | |
ulalume3@0 | 77 | # ---- Initial definition of variables; the actual values will be read in with exec(open('./optic_input.py').read()) below |
ulalume3@0 | 78 | LID = "internal" |
ulalume3@0 | 79 | EID = "internal" |
ulalume3@0 | 80 | # --- IL Laser IL and +-Uncertainty |
ulalume3@0 | 81 | bL = 1. #degree of linear polarization; default 1 |
ulalume3@0 | 82 | RotL, dRotL, nRotL = 0.0, 0.0, 1 #alpha; rotation of laser polarization in degrees; default 0 |
ulalume3@0 | 83 | # --- ME Emitter and +-Uncertainty |
ulalume3@0 | 84 | DiE, dDiE, nDiE = 0., 0.00, 1 # Diattenuation |
ulalume3@0 | 85 | TiE = 1. # Unpolarized transmittance |
ulalume3@0 | 86 | RetE, dRetE, nRetE = 0., 180.0, 0 # Retardance in degrees |
ulalume3@0 | 87 | RotE, dRotE, nRotE = 0., 0.0, 0 # beta: Rotation of optical element in degrees |
ulalume3@0 | 88 | # --- MO Receiver Optics including telescope |
ulalume3@0 | 89 | DiO, dDiO, nDiO = -0.055, 0.003, 1 |
ulalume3@0 | 90 | TiO = 0.9 |
ulalume3@0 | 91 | RetO, dRetO, nRetO = 0., 180.0, 2 |
ulalume3@0 | 92 | RotO, dRotO, nRotO = 0., 0.1, 1 #gamma |
ulalume3@0 | 93 | # --- PBS MT transmitting path defined with (TS,TP); and +-Uncertainty |
ulalume3@0 | 94 | TP, dTP, nTP = 0.98, 0.02, 1 |
ulalume3@0 | 95 | TS, dTS, nTS = 0.001, 0.001, 1 |
ulalume3@0 | 96 | TiT = 0.5 * (TP + TS) |
ulalume3@0 | 97 | DiT = (TP-TS)/(TP+TS) |
ulalume3@0 | 98 | # PolFilter |
ulalume3@0 | 99 | RetT, dRetT, nRetT = 0., 180., 0 |
ulalume3@0 | 100 | ERaT, dERaT, nERaT = 0.001, 0.001, 1 |
ulalume3@0 | 101 | RotaT, dRotaT, nRotaT = 0., 3., 1 |
ulalume3@0 | 102 | DaT = (1-ERaT)/(1+ERaT) |
ulalume3@0 | 103 | TaT = 0.5*(1+ERaT) |
ulalume3@0 | 104 | # --- PBS MR reflecting path defined with (RS,RP); and +-Uncertainty |
ulalume3@0 | 105 | RS, dRS, nRS = 1 - TS, 0., 0 |
ulalume3@0 | 106 | RP, dRP, nRP = 1 - TP, 0., 0 |
ulalume3@0 | 107 | TiR = 0.5 * (RP + RS) |
ulalume3@0 | 108 | DiR = (RP-RS)/(RP+RS) |
ulalume3@0 | 109 | # PolFilter |
ulalume3@0 | 110 | RetR, dRetR, nRetR = 0., 180., 0 |
ulalume3@0 | 111 | ERaR, dERaR, nERaR = 0.001, 0.001, 1 |
ulalume3@0 | 112 | RotaR,dRotaR,nRotaR = 90., 3., 1 |
ulalume3@0 | 113 | DaR = (1-ERaR)/(1+ERaR) |
ulalume3@0 | 114 | TaR = 0.5*(1+ERaR) |
ulalume3@0 | 115 | |
ulalume3@0 | 116 | # Parellel signal detected in the transmitted channel => Y = 1, or in the reflected channel => Y = -1 |
ulalume3@0 | 117 | Y = -1. |
ulalume3@0 | 118 | |
ulalume3@0 | 119 | # Calibrator = type defined by matrix values |
ulalume3@0 | 120 | LocC = 4 # location of calibrator: behind laser = 1; behind emitter = 2; before receiver = 3; before PBS = 4 |
ulalume3@0 | 121 | |
ulalume3@0 | 122 | TypeC = 3 # linear polarizer calibrator |
ulalume3@0 | 123 | # example with extinction ratio 0.001 |
ulalume3@0 | 124 | DiC, dDiC, nDiC = 1.0, 0., 0 # ideal 1.0 |
ulalume3@0 | 125 | TiC = 0.5 # ideal 0.5 |
ulalume3@0 | 126 | RetC, dRetC, nRetC = 0., 0., 0 |
ulalume3@0 | 127 | RotC, dRotC, nRotC = 0.0, 0.1, 0 #constant calibrator offset epsilon |
ulalume3@0 | 128 | RotationErrorEpsilonForNormalMeasurements = False # is in general False for TypeC == 3 calibrator |
ulalume3@0 | 129 | |
ulalume3@0 | 130 | # Rotation error without calibrator: if False, then epsilon = 0 for normal measurements |
ulalume3@0 | 131 | RotationErrorEpsilonForNormalMeasurements = True |
ulalume3@0 | 132 | |
ulalume3@0 | 133 | # LDRCal assumed atmospheric linear depolarization ratio during the calibration measurements (first guess) |
ulalume3@0 | 134 | LDRCal0,dLDRCal,nLDRCal= 0.25, 0.04, 1 |
ulalume3@0 | 135 | LDRCal = LDRCal0 |
ulalume3@0 | 136 | # measured LDRm will be corrected with calculated parameters |
ulalume3@0 | 137 | LDRmeas = 0.015 |
ulalume3@0 | 138 | # LDRtrue for simulation of measurement => LDRsim |
ulalume3@0 | 139 | LDRtrue = 0.5 |
ulalume3@0 | 140 | LDRtrue2 = 0.004 |
ulalume3@0 | 141 | |
ulalume3@0 | 142 | # Initialize other values to 0 |
ulalume3@0 | 143 | ER, nER, dER = 0.001, 0, 0.001 |
ulalume3@0 | 144 | K = 0. |
ulalume3@0 | 145 | Km = 0. |
ulalume3@0 | 146 | Kp = 0. |
ulalume3@0 | 147 | LDRcorr = 0. |
ulalume3@0 | 148 | Eta = 0. |
ulalume3@0 | 149 | Ir = 0. |
ulalume3@0 | 150 | It = 0. |
ulalume3@0 | 151 | h = 1. |
ulalume3@0 | 152 | |
ulalume3@0 | 153 | Loc = ['', 'behind laser', 'behind emitter', 'before receiver', 'before PBS'] |
ulalume3@0 | 154 | Type = ['', 'mechanical rotator', 'hwp rotator', 'linear polarizer', 'qwp rotator', 'circular polarizer', 'real HWP +-22.5°'] |
ulalume3@0 | 155 | dY = ['reflected channel', '', 'transmitted channel'] |
ulalume3@0 | 156 | |
ulalume3@0 | 157 | # end of initial definition of variables |
ulalume3@0 | 158 | # ******************************************************************************************************************************* |
ulalume3@0 | 159 | |
ulalume3@0 | 160 | # --- Read actual lidar system parameters from ./optic_input.py (must be in the same directory) |
ulalume3@0 | 161 | |
ulalume3@0 | 162 | #InputFile = 'optic_input_ver6e_PollyXTSea.py' |
ulalume3@0 | 163 | #InputFile = 'optic_input_ver6e_PollyXTSea_JA.py' |
ulalume3@0 | 164 | #InputFile = 'optic_input_ver6e_PollyXT_RALPH.py' |
ulalume3@0 | 165 | #InputFile = 'optic_input_ver8c_PollyXT_RALPH.py' |
ulalume3@0 | 166 | #InputFile = 'optic_input_ver8c_PollyXT_RALPH_2.py' |
ulalume3@0 | 167 | #InputFile = 'optic_input_ver8c_PollyXT_RALPH_3.py' |
ulalume3@0 | 168 | #InputFile = 'optic_input_ver8c_PollyXT_RALPH_4.py' |
ulalume3@0 | 169 | #InputFile = 'optic_input_ver8c_PollyXT_RALPH_5.py' |
ulalume3@0 | 170 | #InputFile = 'optic_input_ver8c_PollyXT_RALPH_6.py' |
volker@11 | 171 | InputFile = 'system_settings/optic_input_ver8c_PollyXT_RALPH_7.py' |
ulalume3@0 | 172 | #InputFile = 'optic_input_ver6e_Bertha_b_355.py' |
ulalume3@0 | 173 | #InputFile = 'optic_input_ver6e_Bertha_b_532.py' |
ulalume3@0 | 174 | #InputFile = 'optic_input_ver6e_Bertha_b_1064.py' |
ulalume3@0 | 175 | |
ulalume3@0 | 176 | ''' |
ulalume3@0 | 177 | print("From ", dname) |
ulalume3@0 | 178 | print("Running ", fname) |
ulalume3@0 | 179 | print("Reading input file ", InputFile, " for") |
ulalume3@0 | 180 | ''' |
ulalume3@0 | 181 | # this works with Python 2 - and 3? |
ulalume3@0 | 182 | exec(open('./'+InputFile).read(), globals()) |
ulalume3@0 | 183 | # end of read actual system parameters |
ulalume3@0 | 184 | |
ulalume3@0 | 185 | # --- Manual Parameter Change --- |
ulalume3@0 | 186 | # (use for quick parameter changes without changing the input file ) |
ulalume3@0 | 187 | #DiO = 0. |
ulalume3@0 | 188 | #LDRtrue = 0.45 |
ulalume3@0 | 189 | #LDRtrue2 = 0.004 |
ulalume3@0 | 190 | #Y = -1 |
ulalume3@0 | 191 | #LocC = 4 #location of calibrator: 1 = behind laser; 2 = behind emitter; 3 = before receiver; 4 = before PBS |
ulalume3@0 | 192 | ##TypeC = 6 Don't change the TypeC here |
ulalume3@0 | 193 | #RotationErrorEpsilonForNormalMeasurements = True |
ulalume3@0 | 194 | #LDRCal = 0.25 |
ulalume3@0 | 195 | #bL = 0.8 |
ulalume3@0 | 196 | ## --- Errors |
ulalume3@0 | 197 | RotL0, dRotL, nRotL = RotL, dRotL, nRotL |
ulalume3@0 | 198 | |
ulalume3@0 | 199 | DiE0, dDiE, nDiE = DiE, dDiE, nDiE |
ulalume3@0 | 200 | RetE0, dRetE, nRetE = RetE, dRetE, nRetE |
ulalume3@0 | 201 | RotE0, dRotE, nRotE = RotE, dRotE, nRotE |
ulalume3@0 | 202 | |
ulalume3@0 | 203 | DiO0, dDiO, nDiO = DiO, dDiO, nDiO |
ulalume3@0 | 204 | RetO0, dRetO, nRetO = RetO, dRetO, nRetO |
ulalume3@0 | 205 | RotO0, dRotO, nRotO = RotO, dRotO, nRotO |
ulalume3@0 | 206 | |
ulalume3@0 | 207 | DiC0, dDiC, nDiC = DiC, dDiC, nDiC |
ulalume3@0 | 208 | RetC0, dRetC, nRetC = RetC, dRetC, nRetC |
ulalume3@0 | 209 | RotC0, dRotC, nRotC = RotC, dRotC, nRotC |
ulalume3@0 | 210 | |
ulalume3@0 | 211 | TP0, dTP, nTP = TP, dTP, nTP |
ulalume3@0 | 212 | TS0, dTS, nTS = TS, dTS, nTS |
ulalume3@0 | 213 | RetT0, dRetT, nRetT = RetT, dRetT, nRetT |
ulalume3@0 | 214 | |
ulalume3@0 | 215 | ERaT0, dERaT, nERaT = ERaT, dERaT, nERaT |
ulalume3@0 | 216 | RotaT0,dRotaT,nRotaT= RotaT,dRotaT,nRotaT |
ulalume3@0 | 217 | |
ulalume3@0 | 218 | RP0, dRP, nRP = RP, dRP, nRP |
ulalume3@0 | 219 | RS0, dRS, nRS = RS, dRS, nRS |
ulalume3@0 | 220 | RetR0, dRetR, nRetR = RetR, dRetR, nRetR |
ulalume3@0 | 221 | |
ulalume3@0 | 222 | ERaR0, dERaR, nERaR = ERaR, dERaR, nERaR |
ulalume3@0 | 223 | RotaR0,dRotaR,nRotaR= RotaR,dRotaR,nRotaR |
ulalume3@0 | 224 | |
ulalume3@0 | 225 | LDRCal0,dLDRCal,nLDRCal=LDRCal,dLDRCal,nLDRCal |
ulalume3@0 | 226 | #LDRCal0,dLDRCal,nLDRCal=LDRCal,dLDRCal,0 |
ulalume3@0 | 227 | # ---------- End of manual parameter change |
ulalume3@0 | 228 | |
ulalume3@0 | 229 | RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC = RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0 |
ulalume3@0 | 230 | TP, TS, RP, RS, ERaT, RotaT, RetT, ERaR, RotaR, RetR = TP0, TS0, RP0, RS0 , ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0 |
ulalume3@0 | 231 | LDRCal = LDRCal0 |
ulalume3@0 | 232 | DTa0, TTa0, DRa0, TRa0, LDRsimx, LDRCorr = 0,0,0,0,0,0 |
ulalume3@0 | 233 | |
ulalume3@0 | 234 | TiT = 0.5 * (TP + TS) |
ulalume3@0 | 235 | DiT = (TP-TS)/(TP+TS) |
ulalume3@0 | 236 | ZiT = (1. - DiT**2)**0.5 |
ulalume3@0 | 237 | TiR = 0.5 * (RP + RS) |
ulalume3@0 | 238 | DiR = (RP-RS)/(RP+RS) |
ulalume3@0 | 239 | ZiR = (1. - DiR**2)**0.5 |
ulalume3@0 | 240 | |
ulalume3@0 | 241 | # -------------------------------------------------------- |
ulalume3@0 | 242 | def Calc(RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC, TP, TS, RP, RS, ERaT, RotaT, RetT, ERaR, RotaR, RetR, LDRCal): |
ulalume3@0 | 243 | # ---- Do the calculations of bra-ket vectors |
ulalume3@0 | 244 | h = -1. if TypeC == 2 else 1 |
ulalume3@0 | 245 | # from input file: assumed LDRCal for calibration measurements |
ulalume3@0 | 246 | aCal = (1.-LDRCal)/(1+LDRCal) |
ulalume3@0 | 247 | # from input file: measured LDRm and true LDRtrue, LDRtrue2 => |
ulalume3@0 | 248 | #ameas = (1.-LDRmeas)/(1+LDRmeas) |
ulalume3@0 | 249 | atrue = (1.-LDRtrue)/(1+LDRtrue) |
ulalume3@0 | 250 | #atrue2 = (1.-LDRtrue2)/(1+LDRtrue2) |
ulalume3@0 | 251 | |
ulalume3@0 | 252 | # angles of emitter and laser and calibrator and receiver optics |
ulalume3@0 | 253 | # RotL = alpha, RotE = beta, RotO = gamma, RotC = epsilon |
ulalume3@0 | 254 | S2a = np.sin(2*np.deg2rad(RotL)) |
ulalume3@0 | 255 | C2a = np.cos(2*np.deg2rad(RotL)) |
ulalume3@0 | 256 | S2b = np.sin(2*np.deg2rad(RotE)) |
ulalume3@0 | 257 | C2b = np.cos(2*np.deg2rad(RotE)) |
ulalume3@0 | 258 | S2ab = np.sin(np.deg2rad(2*RotL-2*RotE)) |
ulalume3@0 | 259 | C2ab = np.cos(np.deg2rad(2*RotL-2*RotE)) |
ulalume3@0 | 260 | S2g = np.sin(np.deg2rad(2*RotO)) |
ulalume3@0 | 261 | C2g = np.cos(np.deg2rad(2*RotO)) |
ulalume3@0 | 262 | |
ulalume3@0 | 263 | # Laser with Degree of linear polarization DOLP = bL |
ulalume3@0 | 264 | IinL = 1. |
ulalume3@0 | 265 | QinL = bL |
ulalume3@0 | 266 | UinL = 0. |
ulalume3@0 | 267 | VinL = (1. - bL**2)**0.5 |
ulalume3@0 | 268 | |
ulalume3@0 | 269 | # Stokes Input Vector rotation Eq. E.4 |
ulalume3@0 | 270 | A = C2a*QinL - S2a*UinL |
ulalume3@0 | 271 | B = S2a*QinL + C2a*UinL |
ulalume3@0 | 272 | # Stokes Input Vector rotation Eq. E.9 |
ulalume3@0 | 273 | C = C2ab*QinL - S2ab*UinL |
ulalume3@0 | 274 | D = S2ab*QinL + C2ab*UinL |
ulalume3@0 | 275 | |
ulalume3@0 | 276 | # emitter optics |
ulalume3@0 | 277 | CosE = np.cos(np.deg2rad(RetE)) |
ulalume3@0 | 278 | SinE = np.sin(np.deg2rad(RetE)) |
ulalume3@0 | 279 | ZiE = (1. - DiE**2)**0.5 |
ulalume3@0 | 280 | WiE = (1. - ZiE*CosE) |
ulalume3@0 | 281 | |
ulalume3@0 | 282 | # Stokes Input Vector after emitter optics equivalent to Eq. E.9 with already rotated input vector from Eq. E.4 |
ulalume3@0 | 283 | # b = beta |
ulalume3@0 | 284 | IinE = (IinL + DiE*C) |
ulalume3@0 | 285 | QinE = (C2b*DiE*IinL + A + S2b*(WiE*D - ZiE*SinE*VinL)) |
ulalume3@0 | 286 | UinE = (S2b*DiE*IinL + B - C2b*(WiE*D - ZiE*SinE*VinL)) |
ulalume3@0 | 287 | VinE = (-ZiE*SinE*D + ZiE*CosE*VinL) |
ulalume3@0 | 288 | |
ulalume3@0 | 289 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 290 | IinF = IinE |
ulalume3@0 | 291 | QinF = aCal*QinE |
ulalume3@0 | 292 | UinF = -aCal*UinE |
ulalume3@0 | 293 | VinF = (1.-2.*aCal)*VinE |
ulalume3@0 | 294 | |
ulalume3@0 | 295 | # receiver optics |
ulalume3@0 | 296 | CosO = np.cos(np.deg2rad(RetO)) |
ulalume3@0 | 297 | SinO = np.sin(np.deg2rad(RetO)) |
ulalume3@0 | 298 | ZiO = (1. - DiO**2)**0.5 |
ulalume3@0 | 299 | WiO = (1. - ZiO*CosO) |
ulalume3@0 | 300 | |
ulalume3@0 | 301 | # calibrator |
ulalume3@0 | 302 | CosC = np.cos(np.deg2rad(RetC)) |
ulalume3@0 | 303 | SinC = np.sin(np.deg2rad(RetC)) |
ulalume3@0 | 304 | ZiC = (1. - DiC**2)**0.5 |
ulalume3@0 | 305 | WiC = (1. - ZiC*CosC) |
ulalume3@0 | 306 | |
ulalume3@0 | 307 | # Stokes Input Vector before the polarising beam splitter Eq. E.31 |
ulalume3@0 | 308 | A = C2g*QinE - S2g*UinE |
ulalume3@0 | 309 | B = S2g*QinE + C2g*UinE |
ulalume3@0 | 310 | |
ulalume3@0 | 311 | IinP = (IinE + DiO*aCal*A) |
ulalume3@0 | 312 | QinP = (C2g*DiO*IinE + aCal*QinE - S2g*(WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE)) |
ulalume3@0 | 313 | UinP = (S2g*DiO*IinE - aCal*UinE + C2g*(WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE)) |
ulalume3@0 | 314 | VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE) |
ulalume3@0 | 315 | |
ulalume3@0 | 316 | #------------------------- |
ulalume3@0 | 317 | # F11 assuemd to be = 1 => measured: F11m = IinP / IinE with atrue |
ulalume3@0 | 318 | #F11sim = TiO*(IinE + DiO*atrue*A)/IinE |
ulalume3@0 | 319 | #------------------------- |
ulalume3@0 | 320 | |
ulalume3@0 | 321 | # For PollyXT |
ulalume3@0 | 322 | # analyser |
ulalume3@0 | 323 | RS = 1 - TS |
ulalume3@0 | 324 | RP = 1 - TP |
ulalume3@0 | 325 | |
ulalume3@0 | 326 | TiT = 0.5 * (TP + TS) |
ulalume3@0 | 327 | DiT = (TP-TS)/(TP+TS) |
ulalume3@0 | 328 | ZiT = (1. - DiT**2)**0.5 |
ulalume3@0 | 329 | TiR = 0.5 * (RP + RS) |
ulalume3@0 | 330 | DiR = (RP-RS)/(RP+RS) |
ulalume3@0 | 331 | ZiR = (1. - DiR**2)**0.5 |
ulalume3@0 | 332 | CosT = np.cos(np.deg2rad(RetT)) |
ulalume3@0 | 333 | SinT = np.sin(np.deg2rad(RetT)) |
ulalume3@0 | 334 | CosR = np.cos(np.deg2rad(RetR)) |
ulalume3@0 | 335 | SinR = np.sin(np.deg2rad(RetR)) |
ulalume3@0 | 336 | |
ulalume3@0 | 337 | DaT = (1-ERaT)/(1+ERaT) |
ulalume3@0 | 338 | DaR = (1-ERaR)/(1+ERaR) |
ulalume3@0 | 339 | TaT = 0.5*(1+ERaT) |
ulalume3@0 | 340 | TaR = 0.5*(1+ERaR) |
ulalume3@0 | 341 | |
ulalume3@0 | 342 | S2aT = np.sin(np.deg2rad(h*2*RotaT)) |
ulalume3@0 | 343 | C2aT = np.cos(np.deg2rad(2*RotaT)) |
ulalume3@0 | 344 | S2aR = np.sin(np.deg2rad(h*2*RotaR)) |
ulalume3@0 | 345 | C2aR = np.cos(np.deg2rad(2*RotaR)) |
ulalume3@0 | 346 | |
ulalume3@0 | 347 | # Aanalyzer As before the PBS Eq. D.5 |
ulalume3@0 | 348 | ATP1 = (1+C2aT*DaT*DiT) |
ulalume3@0 | 349 | ATP2 = Y*(DiT+C2aT*DaT) |
ulalume3@0 | 350 | ATP3 = Y*S2aT*DaT*ZiT*CosT |
ulalume3@0 | 351 | ATP4 = S2aT*DaT*ZiT*SinT |
ulalume3@0 | 352 | ATP = np.array([ATP1,ATP2,ATP3,ATP4]) |
ulalume3@0 | 353 | |
ulalume3@0 | 354 | ARP1 = (1+C2aR*DaR*DiR) |
ulalume3@0 | 355 | ARP2 = Y*(DiR+C2aR*DaR) |
ulalume3@0 | 356 | ARP3 = Y*S2aR*DaR*ZiR*CosR |
ulalume3@0 | 357 | ARP4 = S2aR*DaR*ZiR*SinR |
ulalume3@0 | 358 | ARP = np.array([ARP1,ARP2,ARP3,ARP4]) |
ulalume3@0 | 359 | |
ulalume3@0 | 360 | DTa = ATP2*Y/ATP1 |
ulalume3@0 | 361 | DRa = ARP2*Y/ARP1 |
ulalume3@0 | 362 | |
ulalume3@0 | 363 | # ---- Calculate signals and correction parameters for diffeent locations and calibrators |
ulalume3@0 | 364 | if LocC == 4: # Calibrator before the PBS |
ulalume3@0 | 365 | #print("Calibrator location not implemented yet") |
ulalume3@0 | 366 | |
ulalume3@0 | 367 | #S2ge = np.sin(np.deg2rad(2*RotO + h*2*RotC)) |
ulalume3@0 | 368 | #C2ge = np.cos(np.deg2rad(2*RotO + h*2*RotC)) |
ulalume3@0 | 369 | S2e = np.sin(np.deg2rad(h*2*RotC)) |
ulalume3@0 | 370 | C2e = np.cos(np.deg2rad(2*RotC)) |
ulalume3@0 | 371 | # rotated AinP by epsilon Eq. C.3 |
ulalume3@0 | 372 | ATP2e = C2e*ATP2 + S2e*ATP3 |
ulalume3@0 | 373 | ATP3e = C2e*ATP3 - S2e*ATP2 |
ulalume3@0 | 374 | ARP2e = C2e*ARP2 + S2e*ARP3 |
ulalume3@0 | 375 | ARP3e = C2e*ARP3 - S2e*ARP2 |
ulalume3@0 | 376 | ATPe = np.array([ATP1,ATP2e,ATP3e,ATP4]) |
ulalume3@0 | 377 | ARPe = np.array([ARP1,ARP2e,ARP3e,ARP4]) |
ulalume3@0 | 378 | # Stokes Input Vector before the polarising beam splitter Eq. E.31 |
ulalume3@0 | 379 | A = C2g*QinE - S2g*UinE |
ulalume3@0 | 380 | B = S2g*QinE + C2g*UinE |
ulalume3@0 | 381 | #C = (WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE) |
ulalume3@0 | 382 | Co = ZiO*SinO*VinE |
ulalume3@0 | 383 | Ca = (WiO*B - 2*ZiO*SinO*VinE) |
ulalume3@0 | 384 | #C = Co + aCal*Ca |
ulalume3@0 | 385 | #IinP = (IinE + DiO*aCal*A) |
ulalume3@0 | 386 | #QinP = (C2g*DiO*IinE + aCal*QinE - S2g*C) |
ulalume3@0 | 387 | #UinP = (S2g*DiO*IinE - aCal*UinE + C2g*C) |
ulalume3@0 | 388 | #VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE) |
ulalume3@0 | 389 | IinPo = IinE |
ulalume3@0 | 390 | QinPo = (C2g*DiO*IinE - S2g*Co) |
ulalume3@0 | 391 | UinPo = (S2g*DiO*IinE + C2g*Co) |
ulalume3@0 | 392 | VinPo = ZiO*CosO*VinE |
ulalume3@0 | 393 | |
ulalume3@0 | 394 | IinPa = DiO*A |
ulalume3@0 | 395 | QinPa = QinE - S2g*Ca |
ulalume3@0 | 396 | UinPa = -UinE + C2g*Ca |
ulalume3@0 | 397 | VinPa = ZiO*(SinO*B - 2*CosO*VinE) |
ulalume3@0 | 398 | |
ulalume3@0 | 399 | IinP = IinPo + aCal*IinPa |
ulalume3@0 | 400 | QinP = QinPo + aCal*QinPa |
ulalume3@0 | 401 | UinP = UinPo + aCal*UinPa |
ulalume3@0 | 402 | VinP = VinPo + aCal*VinPa |
ulalume3@0 | 403 | # Stokes Input Vector before the polarising beam splitter rotated by epsilon Eq. C.3 |
ulalume3@0 | 404 | #QinPe = C2e*QinP + S2e*UinP |
ulalume3@0 | 405 | #UinPe = C2e*UinP - S2e*QinP |
ulalume3@0 | 406 | QinPoe = C2e*QinPo + S2e*UinPo |
ulalume3@0 | 407 | UinPoe = C2e*UinPo - S2e*QinPo |
ulalume3@0 | 408 | QinPae = C2e*QinPa + S2e*UinPa |
ulalume3@0 | 409 | UinPae = C2e*UinPa - S2e*QinPa |
ulalume3@0 | 410 | QinPe = C2e*QinP + S2e*UinP |
ulalume3@0 | 411 | UinPe = C2e*UinP - S2e*QinP |
ulalume3@0 | 412 | |
ulalume3@0 | 413 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 414 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
ulalume3@0 | 415 | # parameters for calibration with aCal |
ulalume3@0 | 416 | AT = ATP1*IinP + h*ATP4*VinP |
ulalume3@0 | 417 | BT = ATP3e*QinP - h*ATP2e*UinP |
ulalume3@0 | 418 | AR = ARP1*IinP + h*ARP4*VinP |
ulalume3@0 | 419 | BR = ARP3e*QinP - h*ARP2e*UinP |
ulalume3@0 | 420 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 421 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 422 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 423 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 424 | GT = np.dot(ATP,IS1) |
ulalume3@0 | 425 | GR = np.dot(ARP,IS1) |
ulalume3@0 | 426 | HT = np.dot(ATP,IS2) |
ulalume3@0 | 427 | HR = np.dot(ARP,IS2) |
ulalume3@0 | 428 | else: |
ulalume3@0 | 429 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 430 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 431 | GT = np.dot(ATPe,IS1) |
ulalume3@0 | 432 | GR = np.dot(ARPe,IS1) |
ulalume3@0 | 433 | HT = np.dot(ATPe,IS2) |
ulalume3@0 | 434 | HR = np.dot(ARPe,IS2) |
ulalume3@0 | 435 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
ulalume3@0 | 436 | # parameters for calibration with aCal |
ulalume3@0 | 437 | AT = ATP1*IinP + ATP3e*UinPe + ZiC*CosC*(ATP2e*QinPe + ATP4*VinP) |
ulalume3@0 | 438 | BT = DiC*(ATP1*UinPe + ATP3e*IinP) - ZiC*SinC*(ATP2e*VinP - ATP4*QinPe) |
ulalume3@0 | 439 | AR = ARP1*IinP + ARP3e*UinPe + ZiC*CosC*(ARP2e*QinPe + ARP4*VinP) |
ulalume3@0 | 440 | BR = DiC*(ARP1*UinPe + ARP3e*IinP) - ZiC*SinC*(ARP2e*VinP - ARP4*QinPe) |
ulalume3@0 | 441 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 442 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 443 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 444 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 445 | GT = np.dot(ATP,IS1) |
ulalume3@0 | 446 | GR = np.dot(ARP,IS1) |
ulalume3@0 | 447 | HT = np.dot(ATP,IS2) |
ulalume3@0 | 448 | HR = np.dot(ARP,IS2) |
ulalume3@0 | 449 | else: |
ulalume3@0 | 450 | IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)]) |
ulalume3@0 | 451 | IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)]) |
ulalume3@0 | 452 | GT = np.dot(ATPe,IS1e) |
ulalume3@0 | 453 | GR = np.dot(ARPe,IS1e) |
ulalume3@0 | 454 | HT = np.dot(ATPe,IS2e) |
ulalume3@0 | 455 | HR = np.dot(ARPe,IS2e) |
ulalume3@0 | 456 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 457 | # parameters for calibration with aCal |
ulalume3@0 | 458 | AT = ATP1*IinP + sqr05*DiC*(ATP1*QinPe + ATP2e*IinP) + (1-0.5*WiC)*(ATP2e*QinPe + ATP3e*UinPe) + ZiC*(sqr05*SinC*(ATP3e*VinP-ATP4*UinPe) + ATP4*CosC*VinP) |
ulalume3@0 | 459 | BT = sqr05*DiC*(ATP1*UinPe + ATP3e*IinP) + 0.5*WiC*(ATP2e*UinPe + ATP3e*QinPe) - sqr05*ZiC*SinC*(ATP2e*VinP - ATP4*QinPe) |
ulalume3@0 | 460 | AR = ARP1*IinP + sqr05*DiC*(ARP1*QinPe + ARP2e*IinP) + (1-0.5*WiC)*(ARP2e*QinPe + ARP3e*UinPe) + ZiC*(sqr05*SinC*(ARP3e*VinP-ARP4*UinPe) + ARP4*CosC*VinP) |
ulalume3@0 | 461 | BR = sqr05*DiC*(ARP1*UinPe + ARP3e*IinP) + 0.5*WiC*(ARP2e*UinPe + ARP3e*QinPe) - sqr05*ZiC*SinC*(ARP2e*VinP - ARP4*QinPe) |
ulalume3@0 | 462 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 463 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 464 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 465 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 466 | GT = np.dot(ATP,IS1) |
ulalume3@0 | 467 | GR = np.dot(ARP,IS1) |
ulalume3@0 | 468 | HT = np.dot(ATP,IS2) |
ulalume3@0 | 469 | HR = np.dot(ARP,IS2) |
ulalume3@0 | 470 | else: |
ulalume3@0 | 471 | IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)]) |
ulalume3@0 | 472 | IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)]) |
ulalume3@0 | 473 | GT = np.dot(ATPe,IS1e) |
ulalume3@0 | 474 | GR = np.dot(ARPe,IS1e) |
ulalume3@0 | 475 | HT = np.dot(ATPe,IS2e) |
ulalume3@0 | 476 | HR = np.dot(ARPe,IS2e) |
ulalume3@0 | 477 | else: |
ulalume3@0 | 478 | print("Calibrator not implemented yet") |
ulalume3@0 | 479 | sys.exit() |
ulalume3@0 | 480 | |
ulalume3@0 | 481 | elif LocC == 3: # C before receiver optics Eq.57 |
ulalume3@0 | 482 | |
ulalume3@0 | 483 | #S2ge = np.sin(np.deg2rad(2*RotO - 2*RotC)) |
ulalume3@0 | 484 | #C2ge = np.cos(np.deg2rad(2*RotO - 2*RotC)) |
ulalume3@0 | 485 | S2e = np.sin(np.deg2rad(2*RotC)) |
ulalume3@0 | 486 | C2e = np.cos(np.deg2rad(2*RotC)) |
ulalume3@0 | 487 | |
ulalume3@0 | 488 | # As with C before the receiver optics (rotated_diattenuator_X22x5deg.odt) |
ulalume3@0 | 489 | AF1 = np.array([1,C2g*DiO,S2g*DiO,0]) |
ulalume3@0 | 490 | AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO]) |
ulalume3@0 | 491 | AF3 = np.array([S2g*DiO,S2g*C2g*WiO,1-C2g**2*WiO,C2g*ZiO*SinO]) |
ulalume3@0 | 492 | AF4 = np.array([0,S2g*SinO,-C2g*SinO,CosO]) |
ulalume3@0 | 493 | |
ulalume3@0 | 494 | ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4) |
ulalume3@0 | 495 | ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4) |
ulalume3@0 | 496 | ATF2 = ATF[1] |
ulalume3@0 | 497 | ATF3 = ATF[2] |
ulalume3@0 | 498 | ARF2 = ARF[1] |
ulalume3@0 | 499 | ARF3 = ARF[2] |
ulalume3@0 | 500 | |
ulalume3@0 | 501 | # rotated AinF by epsilon |
ulalume3@0 | 502 | ATF1 = ATF[0] |
ulalume3@0 | 503 | ATF4 = ATF[3] |
ulalume3@0 | 504 | ATF2e = C2e*ATF[1] + S2e*ATF[2] |
ulalume3@0 | 505 | ATF3e = C2e*ATF[2] - S2e*ATF[1] |
ulalume3@0 | 506 | ARF1 = ARF[0] |
ulalume3@0 | 507 | ARF4 = ARF[3] |
ulalume3@0 | 508 | ARF2e = C2e*ARF[1] + S2e*ARF[2] |
ulalume3@0 | 509 | ARF3e = C2e*ARF[2] - S2e*ARF[1] |
ulalume3@0 | 510 | |
ulalume3@0 | 511 | ATFe = np.array([ATF1,ATF2e,ATF3e,ATF4]) |
ulalume3@0 | 512 | ARFe = np.array([ARF1,ARF2e,ARF3e,ARF4]) |
ulalume3@0 | 513 | |
ulalume3@0 | 514 | QinEe = C2e*QinE + S2e*UinE |
ulalume3@0 | 515 | UinEe = C2e*UinE - S2e*QinE |
ulalume3@0 | 516 | |
ulalume3@0 | 517 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 518 | IinF = IinE |
ulalume3@0 | 519 | QinF = aCal*QinE |
ulalume3@0 | 520 | UinF = -aCal*UinE |
ulalume3@0 | 521 | VinF = (1.-2.*aCal)*VinE |
ulalume3@0 | 522 | |
ulalume3@0 | 523 | IinFo = IinE |
ulalume3@0 | 524 | QinFo = 0. |
ulalume3@0 | 525 | UinFo = 0. |
ulalume3@0 | 526 | VinFo = VinE |
ulalume3@0 | 527 | |
ulalume3@0 | 528 | IinFa = 0. |
ulalume3@0 | 529 | QinFa = QinE |
ulalume3@0 | 530 | UinFa = -UinE |
ulalume3@0 | 531 | VinFa = -2.*VinE |
ulalume3@0 | 532 | |
ulalume3@0 | 533 | # Stokes Input Vector before receiver optics rotated by epsilon Eq. C.3 |
ulalume3@0 | 534 | QinFe = C2e*QinF + S2e*UinF |
ulalume3@0 | 535 | UinFe = C2e*UinF - S2e*QinF |
ulalume3@0 | 536 | QinFoe = C2e*QinFo + S2e*UinFo |
ulalume3@0 | 537 | UinFoe = C2e*UinFo - S2e*QinFo |
ulalume3@0 | 538 | QinFae = C2e*QinFa + S2e*UinFa |
ulalume3@0 | 539 | UinFae = C2e*UinFa - S2e*QinFa |
ulalume3@0 | 540 | |
ulalume3@0 | 541 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 542 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
ulalume3@0 | 543 | # parameters for calibration with aCal |
ulalume3@0 | 544 | AT = ATF1*IinF + ATF4*h*VinF |
ulalume3@0 | 545 | BT = ATF3e*QinF - ATF2e*h*UinF |
ulalume3@0 | 546 | AR = ARF1*IinF + ARF4*h*VinF |
ulalume3@0 | 547 | BR = ARF3e*QinF - ARF2e*h*UinF |
ulalume3@0 | 548 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 549 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 550 | GT = ATF1*IinE + ATF4*VinE |
ulalume3@0 | 551 | GR = ARF1*IinE + ARF4*VinE |
ulalume3@0 | 552 | HT = ATF2*QinE - ATF3*UinE - ATF4*2*VinE |
ulalume3@0 | 553 | HR = ARF2*QinE - ARF3*UinE - ARF4*2*VinE |
ulalume3@0 | 554 | else: |
ulalume3@0 | 555 | GT = ATF1*IinE + ATF4*h*VinE |
ulalume3@0 | 556 | GR = ARF1*IinE + ARF4*h*VinE |
ulalume3@0 | 557 | HT = ATF2e*QinE - ATF3e*h*UinE - ATF4*h*2*VinE |
ulalume3@0 | 558 | HR = ARF2e*QinE - ARF3e*h*UinE - ARF4*h*2*VinE |
ulalume3@0 | 559 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
ulalume3@0 | 560 | # p = +45°, m = -45° |
ulalume3@0 | 561 | IF1e = np.array([IinF, ZiC*CosC*QinFe, UinFe, ZiC*CosC*VinF]) |
ulalume3@0 | 562 | IF2e = np.array([DiC*UinFe, -ZiC*SinC*VinF, DiC*IinF, ZiC*SinC*QinFe]) |
ulalume3@0 | 563 | AT = np.dot(ATFe,IF1e) |
ulalume3@0 | 564 | AR = np.dot(ARFe,IF1e) |
ulalume3@0 | 565 | BT = np.dot(ATFe,IF2e) |
ulalume3@0 | 566 | BR = np.dot(ARFe,IF2e) |
ulalume3@0 | 567 | |
ulalume3@0 | 568 | # Correction paremeters for normal measurements; they are independent of LDR --- the same as for TypeC = 6 |
ulalume3@0 | 569 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 570 | IS1 = np.array([IinE,0,0,VinE]) |
ulalume3@0 | 571 | IS2 = np.array([0,QinE,-UinE,-2*VinE]) |
ulalume3@0 | 572 | GT = np.dot(ATF,IS1) |
ulalume3@0 | 573 | GR = np.dot(ARF,IS1) |
ulalume3@0 | 574 | HT = np.dot(ATF,IS2) |
ulalume3@0 | 575 | HR = np.dot(ARF,IS2) |
ulalume3@0 | 576 | else: |
ulalume3@0 | 577 | IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)]) |
ulalume3@0 | 578 | IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)]) |
ulalume3@0 | 579 | GT = np.dot(ATFe,IS1e) |
ulalume3@0 | 580 | GR = np.dot(ARFe,IS1e) |
ulalume3@0 | 581 | HT = np.dot(ATFe,IS2e) |
ulalume3@0 | 582 | HR = np.dot(ARFe,IS2e) |
ulalume3@0 | 583 | |
ulalume3@0 | 584 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 585 | # parameters for calibration with aCal |
ulalume3@0 | 586 | IF1e = np.array([IinF+sqr05*DiC*QinFe, sqr05*DiC*IinF+(1-0.5*WiC)*QinFe, (1-0.5*WiC)*UinFe+sqr05*ZiC*SinC*VinF, -sqr05*ZiC*SinC*UinFe+ZiC*CosC*VinF]) |
ulalume3@0 | 587 | IF2e = np.array([sqr05*DiC*UinFe, 0.5*WiC*UinFe-sqr05*ZiC*SinC*VinF, sqr05*DiC*IinF+0.5*WiC*QinFe, sqr05*ZiC*SinC*QinFe]) |
ulalume3@0 | 588 | AT = np.dot(ATFe,IF1e) |
ulalume3@0 | 589 | AR = np.dot(ARFe,IF1e) |
ulalume3@0 | 590 | BT = np.dot(ATFe,IF2e) |
ulalume3@0 | 591 | BR = np.dot(ARFe,IF2e) |
ulalume3@0 | 592 | |
ulalume3@0 | 593 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 594 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 595 | #IS1 = np.array([IinE,0,0,VinE]) |
ulalume3@0 | 596 | #IS2 = np.array([0,QinE,-UinE,-2*VinE]) |
ulalume3@0 | 597 | IS1 = np.array([IinFo,0,0,VinFo]) |
ulalume3@0 | 598 | IS2 = np.array([0,QinFa,UinFa,VinFa]) |
ulalume3@0 | 599 | GT = np.dot(ATF,IS1) |
ulalume3@0 | 600 | GR = np.dot(ARF,IS1) |
ulalume3@0 | 601 | HT = np.dot(ATF,IS2) |
ulalume3@0 | 602 | HR = np.dot(ARF,IS2) |
ulalume3@0 | 603 | else: |
ulalume3@0 | 604 | IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)]) |
ulalume3@0 | 605 | IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)]) |
ulalume3@0 | 606 | #IS1e = np.array([IinFo,0,0,VinFo]) |
ulalume3@0 | 607 | #IS2e = np.array([0,QinFae,UinFae,VinFa]) |
ulalume3@0 | 608 | GT = np.dot(ATFe,IS1e) |
ulalume3@0 | 609 | GR = np.dot(ARFe,IS1e) |
ulalume3@0 | 610 | HT = np.dot(ATFe,IS2e) |
ulalume3@0 | 611 | HR = np.dot(ARFe,IS2e) |
ulalume3@0 | 612 | |
ulalume3@0 | 613 | else: |
ulalume3@0 | 614 | print('Calibrator not implemented yet') |
ulalume3@0 | 615 | sys.exit() |
ulalume3@0 | 616 | |
ulalume3@0 | 617 | elif LocC == 2: # C behind emitter optics Eq.57 ------------------------------------------------------- |
ulalume3@0 | 618 | #print("Calibrator location not implemented yet") |
ulalume3@0 | 619 | S2e = np.sin(np.deg2rad(2*RotC)) |
ulalume3@0 | 620 | C2e = np.cos(np.deg2rad(2*RotC)) |
ulalume3@0 | 621 | |
ulalume3@0 | 622 | # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt) |
ulalume3@0 | 623 | AF1 = np.array([1,C2g*DiO,S2g*DiO,0]) |
ulalume3@0 | 624 | AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO]) |
ulalume3@0 | 625 | AF3 = np.array([S2g*DiO, S2g*C2g*WiO, 1-C2g**2*WiO, C2g*ZiO*SinO]) |
ulalume3@0 | 626 | AF4 = np.array([0, S2g*SinO, -C2g*SinO, CosO]) |
ulalume3@0 | 627 | |
ulalume3@0 | 628 | ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4) |
ulalume3@0 | 629 | ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4) |
ulalume3@0 | 630 | ATF1 = ATF[0] |
ulalume3@0 | 631 | ATF2 = ATF[1] |
ulalume3@0 | 632 | ATF3 = ATF[2] |
ulalume3@0 | 633 | ATF4 = ATF[3] |
ulalume3@0 | 634 | ARF1 = ARF[0] |
ulalume3@0 | 635 | ARF2 = ARF[1] |
ulalume3@0 | 636 | ARF3 = ARF[2] |
ulalume3@0 | 637 | ARF4 = ARF[3] |
ulalume3@0 | 638 | |
ulalume3@0 | 639 | # AS with C behind the emitter |
ulalume3@0 | 640 | # terms without aCal |
ulalume3@0 | 641 | ATE1o, ARE1o = ATF1, ARF1 |
ulalume3@0 | 642 | ATE2o, ARE2o = 0., 0. |
ulalume3@0 | 643 | ATE3o, ARE3o = 0., 0. |
ulalume3@0 | 644 | ATE4o, ARE4o = ATF4, ARF4 |
ulalume3@0 | 645 | # terms with aCal |
ulalume3@0 | 646 | ATE1a, ARE1a = 0. , 0. |
ulalume3@0 | 647 | ATE2a, ARE2a = ATF2, ARF2 |
ulalume3@0 | 648 | ATE3a, ARE3a = -ATF3, -ARF3 |
ulalume3@0 | 649 | ATE4a, ARE4a = -2*ATF4, -2*ARF4 |
ulalume3@0 | 650 | # rotated AinEa by epsilon |
ulalume3@0 | 651 | ATE2ae = C2e*ATF2 + S2e*ATF3 |
ulalume3@0 | 652 | ATE3ae = -S2e*ATF2 - C2e*ATF3 |
ulalume3@0 | 653 | ARE2ae = C2e*ARF2 + S2e*ARF3 |
ulalume3@0 | 654 | ARE3ae = -S2e*ARF2 - C2e*ARF3 |
ulalume3@0 | 655 | |
ulalume3@0 | 656 | ATE1 = ATE1o |
ulalume3@0 | 657 | ATE2e = aCal*ATE2ae |
ulalume3@0 | 658 | ATE3e = aCal*ATE3ae |
ulalume3@0 | 659 | ATE4 = (1-2*aCal)*ATF4 |
ulalume3@0 | 660 | ARE1 = ARE1o |
ulalume3@0 | 661 | ARE2e = aCal*ARE2ae |
ulalume3@0 | 662 | ARE3e = aCal*ARE3ae |
ulalume3@0 | 663 | ARE4 = (1-2*aCal)*ARF4 |
ulalume3@0 | 664 | |
ulalume3@0 | 665 | # rotated IinE |
ulalume3@0 | 666 | QinEe = C2e*QinE + S2e*UinE |
ulalume3@0 | 667 | UinEe = C2e*UinE - S2e*QinE |
ulalume3@0 | 668 | |
ulalume3@0 | 669 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 670 | if (TypeC == 2) or (TypeC == 1): # +++++++++ rotator calibration Eq. C.4 |
ulalume3@0 | 671 | AT = ATE1o*IinE + (ATE4o+aCal*ATE4a)*h*VinE |
ulalume3@0 | 672 | BT = aCal * (ATE3ae*QinEe - ATE2ae*h*UinEe) |
ulalume3@0 | 673 | AR = ARE1o*IinE + (ARE4o+aCal*ARE4a)*h*VinE |
ulalume3@0 | 674 | BR = aCal * (ARE3ae*QinEe - ARE2ae*h*UinEe) |
ulalume3@0 | 675 | |
ulalume3@0 | 676 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 677 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 678 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 679 | GT = ATE1o*IinE + ATE4o*h*VinE |
ulalume3@0 | 680 | GR = ARE1o*IinE + ARE4o*h*VinE |
ulalume3@0 | 681 | HT = ATE2a*QinE + ATE3a*h*UinEe + ATE4a*h*VinE |
ulalume3@0 | 682 | HR = ARE2a*QinE + ARE3a*h*UinEe + ARE4a*h*VinE |
ulalume3@0 | 683 | else: |
ulalume3@0 | 684 | GT = ATE1o*IinE + ATE4o*h*VinE |
ulalume3@0 | 685 | GR = ARE1o*IinE + ARE4o*h*VinE |
ulalume3@0 | 686 | HT = ATE2ae*QinE + ATE3ae*h*UinEe + ATE4a*h*VinE |
ulalume3@0 | 687 | HR = ARE2ae*QinE + ARE3ae*h*UinEe + ARE4a*h*VinE |
ulalume3@0 | 688 | |
ulalume3@0 | 689 | elif (TypeC == 3) or (TypeC == 4): # +++++++++ linear polariser calibration Eq. C.5 |
ulalume3@0 | 690 | # p = +45°, m = -45° |
ulalume3@0 | 691 | AT = ATE1*IinE + ZiC*CosC*(ATE2e*QinEe + ATE4*VinE) + ATE3e*UinEe |
ulalume3@0 | 692 | BT = DiC*(ATE1*UinEe + ATE3e*IinE) + ZiC*SinC*(ATE4*QinEe - ATE2e*VinE) |
ulalume3@0 | 693 | AR = ARE1*IinE + ZiC*CosC*(ARE2e*QinEe + ARE4*VinE) + ARE3e*UinEe |
ulalume3@0 | 694 | BR = DiC*(ARE1*UinEe + ARE3e*IinE) + ZiC*SinC*(ARE4*QinEe - ARE2e*VinE) |
ulalume3@0 | 695 | |
ulalume3@0 | 696 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 697 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 698 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 699 | GT = ATE1o*IinE + ATE4o*VinE |
ulalume3@0 | 700 | GR = ARE1o*IinE + ARE4o*VinE |
ulalume3@0 | 701 | HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE |
ulalume3@0 | 702 | HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE |
ulalume3@0 | 703 | else: |
ulalume3@0 | 704 | D = IinE + DiC*QinEe |
ulalume3@0 | 705 | A = DiC*IinE + QinEe |
ulalume3@0 | 706 | B = ZiC*(CosC*UinEe + SinC*VinE) |
ulalume3@0 | 707 | C = -ZiC*(SinC*UinEe - CosC*VinE) |
ulalume3@0 | 708 | GT = ATE1o*D + ATE4o*C |
ulalume3@0 | 709 | GR = ARE1o*D + ARE4o*C |
ulalume3@0 | 710 | HT = ATE2a*A + ATE3a*B + ATE4a*C |
ulalume3@0 | 711 | HR = ARE2a*A + ARE3a*B + ARE4a*C |
ulalume3@0 | 712 | |
ulalume3@0 | 713 | elif (TypeC == 6): # real HWP calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 714 | # p = +22.5°, m = -22.5° |
ulalume3@0 | 715 | IE1e = np.array([IinE+sqr05*DiC*QinEe, sqr05*DiC*IinE+(1-0.5*WiC)*QinEe, (1-0.5*WiC)*UinEe+sqr05*ZiC*SinC*VinE, -sqr05*ZiC*SinC*UinEe+ZiC*CosC*VinE]) |
ulalume3@0 | 716 | IE2e = np.array([sqr05*DiC*UinEe, 0.5*WiC*UinEe-sqr05*ZiC*SinC*VinE, sqr05*DiC*IinE+0.5*WiC*QinEe, sqr05*ZiC*SinC*QinEe]) |
ulalume3@0 | 717 | ATEe = np.array([ATE1,ATE2e,ATE3e,ATE4]) |
ulalume3@0 | 718 | AREe = np.array([ARE1,ARE2e,ARE3e,ARE4]) |
ulalume3@0 | 719 | AT = np.dot(ATEe,IE1e) |
ulalume3@0 | 720 | AR = np.dot(AREe,IE1e) |
ulalume3@0 | 721 | BT = np.dot(ATEe,IE2e) |
ulalume3@0 | 722 | BR = np.dot(AREe,IE2e) |
ulalume3@0 | 723 | |
ulalume3@0 | 724 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 725 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 726 | GT = ATE1o*IinE + ATE4o*VinE |
ulalume3@0 | 727 | GR = ARE1o*IinE + ARE4o*VinE |
ulalume3@0 | 728 | HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE |
ulalume3@0 | 729 | HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE |
ulalume3@0 | 730 | else: |
ulalume3@0 | 731 | D = IinE + DiC*QinEe |
ulalume3@0 | 732 | A = DiC*IinE + QinEe |
ulalume3@0 | 733 | B = ZiC*(CosC*UinEe + SinC*VinE) |
ulalume3@0 | 734 | C = -ZiC*(SinC*UinEe - CosC*VinE) |
ulalume3@0 | 735 | GT = ATE1o*D + ATE4o*C |
ulalume3@0 | 736 | GR = ARE1o*D + ARE4o*C |
ulalume3@0 | 737 | HT = ATE2a*A + ATE3a*B + ATE4a*C |
ulalume3@0 | 738 | HR = ARE2a*A + ARE3a*B + ARE4a*C |
ulalume3@0 | 739 | |
ulalume3@0 | 740 | else: |
ulalume3@0 | 741 | print('Calibrator not implemented yet') |
ulalume3@0 | 742 | sys.exit() |
ulalume3@0 | 743 | |
ulalume3@0 | 744 | else: |
ulalume3@0 | 745 | print("Calibrator location not implemented yet") |
ulalume3@0 | 746 | sys.exit() |
ulalume3@0 | 747 | |
ulalume3@0 | 748 | # Determination of the correction K of the calibration factor |
ulalume3@0 | 749 | IoutTp = TaT*TiT*TiO*TiE*(AT + BT) |
ulalume3@0 | 750 | IoutTm = TaT*TiT*TiO*TiE*(AT - BT) |
ulalume3@0 | 751 | IoutRp = TaR*TiR*TiO*TiE*(AR + BR) |
ulalume3@0 | 752 | IoutRm = TaR*TiR*TiO*TiE*(AR - BR) |
ulalume3@0 | 753 | |
ulalume3@0 | 754 | # --- Results and Corrections; electronic etaR and etaT are assumed to be 1 |
ulalume3@0 | 755 | Etapx = IoutRp/IoutTp |
ulalume3@0 | 756 | Etamx = IoutRm/IoutTm |
ulalume3@0 | 757 | Etax = (Etapx*Etamx)**0.5 |
ulalume3@0 | 758 | |
ulalume3@0 | 759 | Eta = (TaR*TiR)/(TaT*TiT) # Eta = Eta*/K Eq. 84 |
ulalume3@0 | 760 | K = Etax / Eta |
ulalume3@0 | 761 | |
ulalume3@0 | 762 | # For comparison with Volkers Libreoffice Müller Matrix spreadsheet |
ulalume3@0 | 763 | #Eta_test_p = (IoutRp/IoutTp) |
ulalume3@0 | 764 | #Eta_test_m = (IoutRm/IoutTm) |
ulalume3@0 | 765 | #Eta_test = (Eta_test_p*Eta_test_m)**0.5 |
ulalume3@0 | 766 | |
ulalume3@0 | 767 | # ----- Forward simulated signals and LDRsim with atrue; from input file |
ulalume3@0 | 768 | It = TaT*TiT*TiO*TiE*(GT+atrue*HT) |
ulalume3@0 | 769 | Ir = TaR*TiR*TiO*TiE*(GR+atrue*HR) |
ulalume3@0 | 770 | # LDRsim = 1/Eta*Ir/It # simulated LDR* with Y from input file |
ulalume3@0 | 771 | LDRsim = Ir/It # simulated uncorrected LDR with Y from input file |
ulalume3@0 | 772 | # Corrected LDRsimCorr from forward simulated LDRsim (atrue) |
ulalume3@0 | 773 | # LDRsimCorr = (1./Eta*LDRsim*(GT+HT)-(GR+HR))/((GR-HR)-1./Eta*LDRsim*(GT-HT)) |
ulalume3@0 | 774 | if Y == -1.: |
ulalume3@0 | 775 | LDRsimx = 1./LDRsim |
ulalume3@0 | 776 | else: |
ulalume3@0 | 777 | LDRsimx = LDRsim |
ulalume3@0 | 778 | |
ulalume3@0 | 779 | # The following is correct without doubt |
ulalume3@0 | 780 | #LDRCorr = (LDRsim*K/Etax*(GT+HT)-(GR+HR))/((GR-HR)-LDRsim*K/Etax*(GT-HT)) |
ulalume3@0 | 781 | |
ulalume3@0 | 782 | # The following is a test whether the equations for calibration Etax and normal signal (GHK, LDRsim) are consistent |
ulalume3@0 | 783 | LDRCorr = (LDRsim/Eta*(GT+HT)-(GR+HR))/((GR-HR)-LDRsim*K/Etax*(GT-HT)) |
ulalume3@0 | 784 | |
ulalume3@0 | 785 | TTa = TiT*TaT #*ATP1 |
ulalume3@0 | 786 | TRa = TiR*TaR #*ARP1 |
ulalume3@0 | 787 | |
ulalume3@0 | 788 | F11sim = 1/(TiO*TiE)*((HR*Etax/K*It/TTa-HT*Ir/TRa)/(HR*GT-HT*GR)) # IL = 1, Etat = Etar = 1 |
ulalume3@0 | 789 | |
ulalume3@0 | 790 | return (GT, HT, GR, HR, K, Eta, LDRsimx, LDRCorr, DTa, DRa, TTa, TRa, F11sim) |
ulalume3@0 | 791 | # ******************************************************************************************************************************* |
ulalume3@0 | 792 | |
ulalume3@0 | 793 | # --- CALC truth |
ulalume3@0 | 794 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
ulalume3@0 | 795 | |
ulalume3@0 | 796 | # -------------------------------------------------------- |
ulalume3@0 | 797 | with open('output_' + LID + '.dat', 'w') as f: |
ulalume3@0 | 798 | with redirect_stdout(f): |
ulalume3@0 | 799 | print("From ", dname) |
ulalume3@0 | 800 | print("Running ", fname) |
ulalume3@0 | 801 | print("Reading input file ", InputFile) #, " for Lidar system :", EID, ", ", LID) |
ulalume3@0 | 802 | print("for Lidar system: ", EID, ", ", LID) |
ulalume3@0 | 803 | # --- Print iput information********************************* |
ulalume3@0 | 804 | print(" --- Input parameters: value ±error / ±steps ----------------------") |
ulalume3@0 | 805 | print("{0:8} {1:8} {2:8.5f}; {3:8} {4:7.4f}±{5:7.4f}/{6:2d}".format("Laser: ", "DOLP = ", bL, " rotation alpha = ", RotL0, dRotL, nRotL)) |
ulalume3@0 | 806 | print(" Diatt., Tunpol, Retard., Rotation (deg)") |
ulalume3@0 | 807 | 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("Emitter ", DiE0, dDiE, TiE, RetE0, dRetE, RotE0, dRotE, nDiE, nRetE, nRotE)) |
ulalume3@0 | 808 | 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("Receiver ", DiO0, dDiO, TiO, RetO0, dRetO, RotO0, dRotO, nDiO, nRetO, nRotO)) |
ulalume3@0 | 809 | 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("Calibrator ", DiC0, dDiC, TiC, RetC0, dRetC, RotC0, dRotC, nDiC, nRetC, nRotC)) |
ulalume3@0 | 810 | print("{0:12}".format(" --- Pol.-filter ---")) |
ulalume3@0 | 811 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format("ERT, ERR :", ERaT0, dERaT, nERaT, ERaR0, dERaR, nERaR)) |
ulalume3@0 | 812 | print("{0:12}{1:7.4f}±{2:7.4f}/{3:2d}, {4:7.4f}±{5:7.4f}/{6:2d}".format("RotaT , RotaR :", RotaT0, dRotaT, nRotaT, RotaR0,dRotaR,nRotaR)) |
ulalume3@0 | 813 | print("{0:12}".format(" --- PBS ---")) |
ulalume3@0 | 814 | print("{0:12}{1:7.4f}±{2:7.4f}/{9:2d}, {3:7.4f}±{4:7.4f}/{10:2d}, {5:7.4f}±{6:7.4f}/{11:2d},{7:7.4f}±{8:7.4f}/{12:2d}".format("TP,TS,RP,RS :", TP0, dTP, TS0, dTS, RP0, dRP, RS0, dRS, nTP, nTS, nRP, nRS)) |
ulalume3@0 | 815 | print("{0:12}{1:7.4f},{2:7.4f}, {3:7.4f},{4:7.4f}, {5:1.0f}".format("DT,TT,DR,TR,Y :", DiT, TiT, DiR, TiR, Y)) |
ulalume3@0 | 816 | print("{0:12}".format(" --- Combined PBS + Pol.-filter ---")) |
ulalume3@0 | 817 | print("{0:12}{1:7.4f},{2:7.4f}, {3:7.4f},{4:7.4f}".format("DTa,TTa,DRa,TRa: ", DTa0, TTa0, DRa0, TRa0)) |
ulalume3@0 | 818 | print() |
ulalume3@0 | 819 | print("Rotation Error Epsilon For Normal Measurements = ", RotationErrorEpsilonForNormalMeasurements) |
ulalume3@0 | 820 | #print ('LocC = ', LocC, Loc[LocC], '; TypeC = ',TypeC, Type[TypeC]) |
ulalume3@0 | 821 | print(Type[TypeC], Loc[LocC], "; Parallel signal detected in", dY[int(Y+1)]) |
ulalume3@0 | 822 | # end of print actual system parameters |
ulalume3@0 | 823 | # ****************************************************************************** |
ulalume3@0 | 824 | |
ulalume3@0 | 825 | #print() |
ulalume3@0 | 826 | #print(" --- LDRCal during calibration | simulated and corrected LDRs -------------") |
ulalume3@0 | 827 | #print("{0:8} |{1:8}->{2:8},{3:9}->{4:9} |{5:8}->{6:8}".format(" LDRCal"," LDRtrue", " LDRsim"," LDRtrue2", " LDRsim2", " LDRmeas", " LDRcorr")) |
ulalume3@0 | 828 | #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)) |
ulalume3@0 | 829 | #print("{0:8} |{1:8}->{2:8}->{3:8}".format(" LDRCal"," LDRtrue", " LDRsimx", " LDRcorr")) |
ulalume3@0 | 830 | #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)) |
ulalume3@0 | 831 | #print("{0:8} |{1:8}->{2:8}->{3:8}".format(" LDRCal"," LDRtrue", " LDRsimx", " LDRcorr")) |
ulalume3@0 | 832 | #print(" --- LDRCal during calibration") |
ulalume3@0 | 833 | print("{0:26}: {1:6.3f}±{2:5.3f}/{3:2d}".format("LDRCal during calibration", LDRCal0, dLDRCal, nLDRCal)) |
ulalume3@0 | 834 | |
ulalume3@0 | 835 | #print("{0:8}={1:8.5f};{2:8}={3:8.5f}".format(" IinP",IinP," F11sim",F11sim)) |
ulalume3@0 | 836 | print() |
ulalume3@0 | 837 | |
ulalume3@0 | 838 | K0List = np.zeros(3) |
ulalume3@0 | 839 | LDRsimxList = np.zeros(3) |
ulalume3@0 | 840 | LDRCalList = 0.004, 0.2, 0.45 |
ulalume3@0 | 841 | for i,LDRCal in enumerate(LDRCalList): |
ulalume3@0 | 842 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal) |
ulalume3@0 | 843 | K0List[i] = K0 |
ulalume3@0 | 844 | LDRsimxList[i] = LDRsimx |
ulalume3@0 | 845 | |
ulalume3@0 | 846 | print("{0:8},{1:8},{2:8},{3:8},{4:9},{5:9},{6:9}".format(" GR", " GT", " HR", " HT", " K(0.004)", " K(0.2)", " K(0.45)")) |
ulalume3@0 | 847 | print("{0:8.5f},{1:8.5f},{2:8.5f},{3:8.5f},{4:9.5f},{5:9.5f},{6:9.5f}".format(GR0, GT0, HR0, HT0, K0List[0], K0List[1], K0List[2])) |
ulalume3@0 | 848 | print('========================================================================') |
ulalume3@0 | 849 | |
ulalume3@0 | 850 | print("{0:9},{1:9},{2:9}".format(" LDRtrue", " LDRsimx", " LDRCorr")) |
ulalume3@0 | 851 | LDRtrueList = 0.004, 0.02, 0.2, 0.45 |
ulalume3@0 | 852 | for i,LDRtrue in enumerate(LDRtrueList): |
ulalume3@0 | 853 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
ulalume3@0 | 854 | print("{0:9.5f},{1:9.5f},{2:9.5f}".format(LDRtrue, LDRsimx, LDRCorr)) |
ulalume3@0 | 855 | |
ulalume3@0 | 856 | |
ulalume3@0 | 857 | file = open('output_' + LID + '.dat', 'r') |
ulalume3@0 | 858 | print (file.read()) |
ulalume3@0 | 859 | file.close() |
ulalume3@0 | 860 | |
ulalume3@0 | 861 | ''' |
ulalume3@0 | 862 | if(PrintToOutputFile): |
ulalume3@0 | 863 | f = open('output_ver7.dat', 'w') |
ulalume3@0 | 864 | old_target = sys.stdout |
ulalume3@0 | 865 | sys.stdout = f |
ulalume3@0 | 866 | |
ulalume3@0 | 867 | print("something") |
ulalume3@0 | 868 | |
ulalume3@0 | 869 | if(PrintToOutputFile): |
ulalume3@0 | 870 | sys.stdout.flush() |
ulalume3@0 | 871 | f.close |
ulalume3@0 | 872 | sys.stdout = old_target |
ulalume3@0 | 873 | ''' |
ulalume3@0 | 874 | # --- CALC again truth with LDRCal0 to reset all 0-values |
ulalume3@0 | 875 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal0) |
ulalume3@0 | 876 | |
ulalume3@0 | 877 | # --- Start Errors calculation |
ulalume3@0 | 878 | |
ulalume3@0 | 879 | iN = -1 |
ulalume3@0 | 880 | N = ((nRotL*2+1)* |
ulalume3@0 | 881 | (nRotE*2+1)*(nRetE*2+1)*(nDiE*2+1)* |
ulalume3@0 | 882 | (nRotO*2+1)*(nRetO*2+1)*(nDiO*2+1)* |
ulalume3@0 | 883 | (nRotC*2+1)*(nRetC*2+1)*(nDiC*2+1)* |
ulalume3@0 | 884 | (nTP*2+1)*(nTS*2+1)*(nRP*2+1)*(nRS*2+1)*(nERaT*2+1)*(nERaR*2+1)* |
ulalume3@0 | 885 | (nRotaT*2+1)*(nRotaR*2+1)*(nRetT*2+1)*(nRetR*2+1)*(nLDRCal*2+1)) |
ulalume3@0 | 886 | print("N = ",N ," ", end="") |
ulalume3@0 | 887 | |
ulalume3@0 | 888 | if N > 1e6: |
ulalume3@0 | 889 | if user_yes_no_query('Warning: processing ' + str(N) + ' samples will take very long. Do you want to proceed?') == 0: sys.exit() |
ulalume3@0 | 890 | if N > 5e6: |
ulalume3@0 | 891 | if user_yes_no_query('Warning: the memory required for ' + str(N) + ' samples might be ' + '{0:5.1f}'.format(N/4e6) + ' GB. Do you anyway want to proceed?') == 0: sys.exit() |
ulalume3@0 | 892 | |
ulalume3@0 | 893 | #if user_yes_no_query('Warning: processing' + str(N) + ' samples will take very long. Do you want to proceed?') == 0: sys.exit() |
ulalume3@0 | 894 | |
ulalume3@0 | 895 | # --- Arrays for plotting ------ |
ulalume3@0 | 896 | LDRmin = np.zeros(5) |
ulalume3@0 | 897 | LDRmax = np.zeros(5) |
ulalume3@0 | 898 | F11min = np.zeros(5) |
ulalume3@0 | 899 | F11max = np.zeros(5) |
ulalume3@0 | 900 | |
ulalume3@0 | 901 | LDRrange = np.zeros(5) |
ulalume3@0 | 902 | LDRrange = 0.004, 0.02, 0.1, 0.3, 0.45 |
ulalume3@0 | 903 | #aLDRsimx = np.zeros(N) |
ulalume3@0 | 904 | #aLDRsimx2 = np.zeros(N) |
ulalume3@0 | 905 | #aLDRcorr = np.zeros(N) |
ulalume3@0 | 906 | #aLDRcorr2 = np.zeros(N) |
ulalume3@0 | 907 | aERaT = np.zeros(N) |
ulalume3@0 | 908 | aERaR = np.zeros(N) |
ulalume3@0 | 909 | aRotaT = np.zeros(N) |
ulalume3@0 | 910 | aRotaR = np.zeros(N) |
ulalume3@0 | 911 | aRetT = np.zeros(N) |
ulalume3@0 | 912 | aRetR = np.zeros(N) |
ulalume3@0 | 913 | aTP = np.zeros(N) |
ulalume3@0 | 914 | aTS = np.zeros(N) |
ulalume3@0 | 915 | aRP = np.zeros(N) |
ulalume3@0 | 916 | aRS = np.zeros(N) |
ulalume3@0 | 917 | aDiE = np.zeros(N) |
ulalume3@0 | 918 | aDiO = np.zeros(N) |
ulalume3@0 | 919 | aDiC = np.zeros(N) |
ulalume3@0 | 920 | aRotC = np.zeros(N) |
ulalume3@0 | 921 | aRetC = np.zeros(N) |
ulalume3@0 | 922 | aRotL = np.zeros(N) |
ulalume3@0 | 923 | aRetE = np.zeros(N) |
ulalume3@0 | 924 | aRotE = np.zeros(N) |
ulalume3@0 | 925 | aRetO = np.zeros(N) |
ulalume3@0 | 926 | aRotO = np.zeros(N) |
ulalume3@0 | 927 | aLDRCal = np.zeros(N) |
ulalume3@0 | 928 | aA = np.zeros((5,N)) |
ulalume3@0 | 929 | aX = np.zeros((5,N)) |
ulalume3@0 | 930 | aF11corr = np.zeros((5,N)) |
ulalume3@0 | 931 | |
ulalume3@0 | 932 | atime = clock() |
ulalume3@0 | 933 | dtime = clock() |
ulalume3@0 | 934 | |
ulalume3@0 | 935 | # --- Calc Error signals |
ulalume3@0 | 936 | #GT, HT, GR, HR, K, Eta, LDRsim = Calc(RotL, RotE, RetE, DiE, RotO, RetO, DiO, RotC, RetC, DiC, TP, TS) |
ulalume3@0 | 937 | # ---- Do the calculations of bra-ket vectors |
ulalume3@0 | 938 | h = -1. if TypeC == 2 else 1 |
ulalume3@0 | 939 | |
ulalume3@0 | 940 | # from input file: measured LDRm and true LDRtrue, LDRtrue2 => |
ulalume3@0 | 941 | ameas = (1.-LDRmeas)/(1+LDRmeas) |
ulalume3@0 | 942 | atrue = (1.-LDRtrue)/(1+LDRtrue) |
ulalume3@0 | 943 | atrue2 = (1.-LDRtrue2)/(1+LDRtrue2) |
ulalume3@0 | 944 | |
ulalume3@0 | 945 | for iLDRCal in range(-nLDRCal,nLDRCal+1): |
ulalume3@0 | 946 | # from input file: assumed LDRCal for calibration measurements |
ulalume3@0 | 947 | LDRCal = LDRCal0 |
ulalume3@0 | 948 | if nLDRCal > 0: LDRCal = LDRCal0 + iLDRCal*dLDRCal/nLDRCal |
ulalume3@0 | 949 | |
ulalume3@0 | 950 | GT0, HT0, GR0, HR0, K0, Eta0, LDRsimx, LDRCorr, DTa0, DRa0, TTa0, TRa0, F11sim0 = Calc(RotL0, RotE0, RetE0, DiE0, RotO0, RetO0, DiO0, RotC0, RetC0, DiC0, TP0, TS0, RP0, RS0, ERaT0, RotaT0, RetT0, ERaR0, RotaR0, RetR0, LDRCal) |
ulalume3@0 | 951 | aCal = (1.-LDRCal)/(1+LDRCal) |
ulalume3@0 | 952 | for iRotL, iRotE, iRetE, iDiE \ |
ulalume3@0 | 953 | in [(iRotL,iRotE,iRetE,iDiE) |
ulalume3@0 | 954 | for iRotL in range(-nRotL,nRotL+1) |
ulalume3@0 | 955 | for iRotE in range(-nRotE,nRotE+1) |
ulalume3@0 | 956 | for iRetE in range(-nRetE,nRetE+1) |
ulalume3@0 | 957 | for iDiE in range(-nDiE,nDiE+1)]: |
ulalume3@0 | 958 | |
ulalume3@0 | 959 | if nRotL > 0: RotL = RotL0 + iRotL*dRotL/nRotL |
ulalume3@0 | 960 | if nRotE > 0: RotE = RotE0 + iRotE*dRotE/nRotE |
ulalume3@0 | 961 | if nRetE > 0: RetE = RetE0 + iRetE*dRetE/nRetE |
ulalume3@0 | 962 | if nDiE > 0: DiE = DiE0 + iDiE*dDiE/nDiE |
ulalume3@0 | 963 | |
ulalume3@0 | 964 | # angles of emitter and laser and calibrator and receiver optics |
ulalume3@0 | 965 | # RotL = alpha, RotE = beta, RotO = gamma, RotC = epsilon |
ulalume3@0 | 966 | S2a = np.sin(2*np.deg2rad(RotL)) |
ulalume3@0 | 967 | C2a = np.cos(2*np.deg2rad(RotL)) |
ulalume3@0 | 968 | S2b = np.sin(2*np.deg2rad(RotE)) |
ulalume3@0 | 969 | C2b = np.cos(2*np.deg2rad(RotE)) |
ulalume3@0 | 970 | S2ab = np.sin(np.deg2rad(2*RotL-2*RotE)) |
ulalume3@0 | 971 | C2ab = np.cos(np.deg2rad(2*RotL-2*RotE)) |
ulalume3@0 | 972 | |
ulalume3@0 | 973 | # Laser with Degree of linear polarization DOLP = bL |
ulalume3@0 | 974 | IinL = 1. |
ulalume3@0 | 975 | QinL = bL |
ulalume3@0 | 976 | UinL = 0. |
ulalume3@0 | 977 | VinL = (1. - bL**2)**0.5 |
ulalume3@0 | 978 | |
ulalume3@0 | 979 | # Stokes Input Vector rotation Eq. E.4 |
ulalume3@0 | 980 | A = C2a*QinL - S2a*UinL |
ulalume3@0 | 981 | B = S2a*QinL + C2a*UinL |
ulalume3@0 | 982 | # Stokes Input Vector rotation Eq. E.9 |
ulalume3@0 | 983 | C = C2ab*QinL - S2ab*UinL |
ulalume3@0 | 984 | D = S2ab*QinL + C2ab*UinL |
ulalume3@0 | 985 | |
ulalume3@0 | 986 | # emitter optics |
ulalume3@0 | 987 | CosE = np.cos(np.deg2rad(RetE)) |
ulalume3@0 | 988 | SinE = np.sin(np.deg2rad(RetE)) |
ulalume3@0 | 989 | ZiE = (1. - DiE**2)**0.5 |
ulalume3@0 | 990 | WiE = (1. - ZiE*CosE) |
ulalume3@0 | 991 | |
ulalume3@0 | 992 | # Stokes Input Vector after emitter optics equivalent to Eq. E.9 with already rotated input vector from Eq. E.4 |
ulalume3@0 | 993 | # b = beta |
ulalume3@0 | 994 | IinE = (IinL + DiE*C) |
ulalume3@0 | 995 | QinE = (C2b*DiE*IinL + A + S2b*(WiE*D - ZiE*SinE*VinL)) |
ulalume3@0 | 996 | UinE = (S2b*DiE*IinL + B - C2b*(WiE*D - ZiE*SinE*VinL)) |
ulalume3@0 | 997 | VinE = (-ZiE*SinE*D + ZiE*CosE*VinL) |
ulalume3@0 | 998 | |
ulalume3@0 | 999 | #------------------------- |
ulalume3@0 | 1000 | # F11 assuemd to be = 1 => measured: F11m = IinP / IinE with atrue |
ulalume3@0 | 1001 | #F11sim = (IinE + DiO*atrue*(C2g*QinE - S2g*UinE))/IinE |
ulalume3@0 | 1002 | #------------------------- |
ulalume3@0 | 1003 | |
ulalume3@0 | 1004 | for iRotO, iRetO, iDiO, iRotC, iRetC, iDiC, iTP, iTS, iRP, iRS, iERaT, iRotaT, iRetT, iERaR, iRotaR, iRetR \ |
ulalume3@0 | 1005 | in [(iRotO,iRetO,iDiO,iRotC,iRetC,iDiC,iTP,iTS,iRP,iRS,iERaT,iRotaT,iRetT,iERaR,iRotaR,iRetR ) |
ulalume3@0 | 1006 | for iRotO in range(-nRotO,nRotO+1) |
ulalume3@0 | 1007 | for iRetO in range(-nRetO,nRetO+1) |
ulalume3@0 | 1008 | for iDiO in range(-nDiO,nDiO+1) |
ulalume3@0 | 1009 | for iRotC in range(-nRotC,nRotC+1) |
ulalume3@0 | 1010 | for iRetC in range(-nRetC,nRetC+1) |
ulalume3@0 | 1011 | for iDiC in range(-nDiC,nDiC+1) |
ulalume3@0 | 1012 | for iTP in range(-nTP,nTP+1) |
ulalume3@0 | 1013 | for iTS in range(-nTS,nTS+1) |
ulalume3@0 | 1014 | for iRP in range(-nRP,nRP+1) |
ulalume3@0 | 1015 | for iRS in range(-nRS,nRS+1) |
ulalume3@0 | 1016 | for iERaT in range(-nERaT,nERaT+1) |
ulalume3@0 | 1017 | for iRotaT in range(-nRotaT,nRotaT+1) |
ulalume3@0 | 1018 | for iRetT in range(-nRetT,nRetT+1) |
ulalume3@0 | 1019 | for iERaR in range(-nERaR,nERaR+1) |
ulalume3@0 | 1020 | for iRotaR in range(-nRotaR,nRotaR+1) |
ulalume3@0 | 1021 | for iRetR in range(-nRetR,nRetR+1)]: |
ulalume3@0 | 1022 | |
ulalume3@0 | 1023 | iN = iN + 1 |
ulalume3@0 | 1024 | if (iN == 10001): |
ulalume3@0 | 1025 | ctime = clock() |
ulalume3@0 | 1026 | print(" estimated time ", "{0:4.2f}".format(N/10000 * (ctime-atime)), "sec ") #, end="") |
ulalume3@0 | 1027 | print("\r elapsed time ", "{0:5.0f}".format((ctime-atime)), "sec ", end="\r") |
ulalume3@0 | 1028 | ctime = clock() |
ulalume3@0 | 1029 | if ((ctime - dtime) > 10): |
ulalume3@0 | 1030 | print("\r elapsed time ", "{0:5.0f}".format((ctime-atime)), "sec ", end="\r") |
ulalume3@0 | 1031 | dtime = ctime |
ulalume3@0 | 1032 | |
ulalume3@0 | 1033 | if nRotO > 0: RotO = RotO0 + iRotO*dRotO/nRotO |
ulalume3@0 | 1034 | if nRetO > 0: RetO = RetO0 + iRetO*dRetO/nRetO |
ulalume3@0 | 1035 | if nDiO > 0: DiO = DiO0 + iDiO*dDiO/nDiO |
ulalume3@0 | 1036 | if nRotC > 0: RotC = RotC0 + iRotC*dRotC/nRotC |
ulalume3@0 | 1037 | if nRetC > 0: RetC = RetC0 + iRetC*dRetC/nRetC |
ulalume3@0 | 1038 | if nDiC > 0: DiC = DiC0 + iDiC*dDiC/nDiC |
ulalume3@0 | 1039 | if nTP > 0: TP = TP0 + iTP*dTP/nTP |
ulalume3@0 | 1040 | if nTS > 0: TS = TS0 + iTS*dTS/nTS |
ulalume3@0 | 1041 | if nRP > 0: RP = RP0 + iRP*dRP/nRP |
ulalume3@0 | 1042 | if nRS > 0: RS = RS0 + iRS*dRS/nRS |
ulalume3@0 | 1043 | if nERaT > 0: ERaT = ERaT0 + iERaT*dERaT/nERaT |
ulalume3@0 | 1044 | if nRotaT > 0:RotaT= RotaT0+ iRotaT*dRotaT/nRotaT |
ulalume3@0 | 1045 | if nRetT > 0: RetT = RetT0 + iRetT*dRetT/nRetT |
ulalume3@0 | 1046 | if nERaR > 0: ERaR = ERaR0 + iERaR*dERaR/nERaR |
ulalume3@0 | 1047 | if nRotaR > 0:RotaR= RotaR0+ iRotaR*dRotaR/nRotaR |
ulalume3@0 | 1048 | if nRetR > 0: RetR = RetR0 + iRetR*dRetR/nRetR |
ulalume3@0 | 1049 | |
ulalume3@0 | 1050 | #print("{0:5.2f}, {1:5.2f}, {2:5.2f}, {3:10d}".format(RotL, RotE, RotO, iN)) |
ulalume3@0 | 1051 | |
ulalume3@0 | 1052 | # receiver optics |
ulalume3@0 | 1053 | CosO = np.cos(np.deg2rad(RetO)) |
ulalume3@0 | 1054 | SinO = np.sin(np.deg2rad(RetO)) |
ulalume3@0 | 1055 | ZiO = (1. - DiO**2)**0.5 |
ulalume3@0 | 1056 | WiO = (1. - ZiO*CosO) |
ulalume3@0 | 1057 | S2g = np.sin(np.deg2rad(2*RotO)) |
ulalume3@0 | 1058 | C2g = np.cos(np.deg2rad(2*RotO)) |
ulalume3@0 | 1059 | # calibrator |
ulalume3@0 | 1060 | CosC = np.cos(np.deg2rad(RetC)) |
ulalume3@0 | 1061 | SinC = np.sin(np.deg2rad(RetC)) |
ulalume3@0 | 1062 | ZiC = (1. - DiC**2)**0.5 |
ulalume3@0 | 1063 | WiC = (1. - ZiC*CosC) |
ulalume3@0 | 1064 | |
ulalume3@0 | 1065 | #For POLLY_XT |
ulalume3@0 | 1066 | # analyser |
ulalume3@0 | 1067 | RS = 1 - TS |
ulalume3@0 | 1068 | RP = 1 - TP |
ulalume3@0 | 1069 | TiT = 0.5 * (TP + TS) |
ulalume3@0 | 1070 | DiT = (TP-TS)/(TP+TS) |
ulalume3@0 | 1071 | ZiT = (1. - DiT**2)**0.5 |
ulalume3@0 | 1072 | TiR = 0.5 * (RP + RS) |
ulalume3@0 | 1073 | DiR = (RP-RS)/(RP+RS) |
ulalume3@0 | 1074 | ZiR = (1. - DiR**2)**0.5 |
ulalume3@0 | 1075 | CosT = np.cos(np.deg2rad(RetT)) |
ulalume3@0 | 1076 | SinT = np.sin(np.deg2rad(RetT)) |
ulalume3@0 | 1077 | CosR = np.cos(np.deg2rad(RetR)) |
ulalume3@0 | 1078 | SinR = np.sin(np.deg2rad(RetR)) |
ulalume3@0 | 1079 | |
ulalume3@0 | 1080 | DaT = (1-ERaT)/(1+ERaT) |
ulalume3@0 | 1081 | DaR = (1-ERaR)/(1+ERaR) |
ulalume3@0 | 1082 | TaT = 0.5*(1+ERaT) |
ulalume3@0 | 1083 | TaR = 0.5*(1+ERaR) |
ulalume3@0 | 1084 | |
ulalume3@0 | 1085 | S2aT = np.sin(np.deg2rad(h*2*RotaT)) |
ulalume3@0 | 1086 | C2aT = np.cos(np.deg2rad(2*RotaT)) |
ulalume3@0 | 1087 | S2aR = np.sin(np.deg2rad(h*2*RotaR)) |
ulalume3@0 | 1088 | C2aR = np.cos(np.deg2rad(2*RotaR)) |
ulalume3@0 | 1089 | |
ulalume3@0 | 1090 | # Aanalyzer As before the PBS Eq. D.5 |
ulalume3@0 | 1091 | ATP1 = (1+C2aT*DaT*DiT) |
ulalume3@0 | 1092 | ATP2 = Y*(DiT+C2aT*DaT) |
ulalume3@0 | 1093 | ATP3 = Y*S2aT*DaT*ZiT*CosT |
ulalume3@0 | 1094 | ATP4 = S2aT*DaT*ZiT*SinT |
ulalume3@0 | 1095 | ATP = np.array([ATP1,ATP2,ATP3,ATP4]) |
ulalume3@0 | 1096 | |
ulalume3@0 | 1097 | ARP1 = (1+C2aR*DaR*DiR) |
ulalume3@0 | 1098 | ARP2 = Y*(DiR+C2aR*DaR) |
ulalume3@0 | 1099 | ARP3 = Y*S2aR*DaR*ZiR*CosR |
ulalume3@0 | 1100 | ARP4 = S2aR*DaR*ZiR*SinR |
ulalume3@0 | 1101 | ARP = np.array([ARP1,ARP2,ARP3,ARP4]) |
ulalume3@0 | 1102 | |
ulalume3@0 | 1103 | TTa = TiT*TaT #*ATP1 |
ulalume3@0 | 1104 | TRa = TiR*TaR #*ARP1 |
ulalume3@0 | 1105 | |
ulalume3@0 | 1106 | # ---- Calculate signals and correction parameters for diffeent locations and calibrators |
ulalume3@0 | 1107 | if LocC == 4: # Calibrator before the PBS |
ulalume3@0 | 1108 | #print("Calibrator location not implemented yet") |
ulalume3@0 | 1109 | |
ulalume3@0 | 1110 | #S2ge = np.sin(np.deg2rad(2*RotO + h*2*RotC)) |
ulalume3@0 | 1111 | #C2ge = np.cos(np.deg2rad(2*RotO + h*2*RotC)) |
ulalume3@0 | 1112 | S2e = np.sin(np.deg2rad(h*2*RotC)) |
ulalume3@0 | 1113 | C2e = np.cos(np.deg2rad(2*RotC)) |
ulalume3@0 | 1114 | # rotated AinP by epsilon Eq. C.3 |
ulalume3@0 | 1115 | ATP2e = C2e*ATP2 + S2e*ATP3 |
ulalume3@0 | 1116 | ATP3e = C2e*ATP3 - S2e*ATP2 |
ulalume3@0 | 1117 | ARP2e = C2e*ARP2 + S2e*ARP3 |
ulalume3@0 | 1118 | ARP3e = C2e*ARP3 - S2e*ARP2 |
ulalume3@0 | 1119 | ATPe = np.array([ATP1,ATP2e,ATP3e,ATP4]) |
ulalume3@0 | 1120 | ARPe = np.array([ARP1,ARP2e,ARP3e,ARP4]) |
ulalume3@0 | 1121 | # Stokes Input Vector before the polarising beam splitter Eq. E.31 |
ulalume3@0 | 1122 | A = C2g*QinE - S2g*UinE |
ulalume3@0 | 1123 | B = S2g*QinE + C2g*UinE |
ulalume3@0 | 1124 | #C = (WiO*aCal*B + ZiO*SinO*(1-2*aCal)*VinE) |
ulalume3@0 | 1125 | Co = ZiO*SinO*VinE |
ulalume3@0 | 1126 | Ca = (WiO*B - 2*ZiO*SinO*VinE) |
ulalume3@0 | 1127 | #C = Co + aCal*Ca |
ulalume3@0 | 1128 | #IinP = (IinE + DiO*aCal*A) |
ulalume3@0 | 1129 | #QinP = (C2g*DiO*IinE + aCal*QinE - S2g*C) |
ulalume3@0 | 1130 | #UinP = (S2g*DiO*IinE - aCal*UinE + C2g*C) |
ulalume3@0 | 1131 | #VinP = (ZiO*SinO*aCal*B + ZiO*CosO*(1-2*aCal)*VinE) |
ulalume3@0 | 1132 | IinPo = IinE |
ulalume3@0 | 1133 | QinPo = (C2g*DiO*IinE - S2g*Co) |
ulalume3@0 | 1134 | UinPo = (S2g*DiO*IinE + C2g*Co) |
ulalume3@0 | 1135 | VinPo = ZiO*CosO*VinE |
ulalume3@0 | 1136 | |
ulalume3@0 | 1137 | IinPa = DiO*A |
ulalume3@0 | 1138 | QinPa = QinE - S2g*Ca |
ulalume3@0 | 1139 | UinPa = -UinE + C2g*Ca |
ulalume3@0 | 1140 | VinPa = ZiO*(SinO*B - 2*CosO*VinE) |
ulalume3@0 | 1141 | |
ulalume3@0 | 1142 | IinP = IinPo + aCal*IinPa |
ulalume3@0 | 1143 | QinP = QinPo + aCal*QinPa |
ulalume3@0 | 1144 | UinP = UinPo + aCal*UinPa |
ulalume3@0 | 1145 | VinP = VinPo + aCal*VinPa |
ulalume3@0 | 1146 | # Stokes Input Vector before the polarising beam splitter rotated by epsilon Eq. C.3 |
ulalume3@0 | 1147 | #QinPe = C2e*QinP + S2e*UinP |
ulalume3@0 | 1148 | #UinPe = C2e*UinP - S2e*QinP |
ulalume3@0 | 1149 | QinPoe = C2e*QinPo + S2e*UinPo |
ulalume3@0 | 1150 | UinPoe = C2e*UinPo - S2e*QinPo |
ulalume3@0 | 1151 | QinPae = C2e*QinPa + S2e*UinPa |
ulalume3@0 | 1152 | UinPae = C2e*UinPa - S2e*QinPa |
ulalume3@0 | 1153 | QinPe = C2e*QinP + S2e*UinP |
ulalume3@0 | 1154 | UinPe = C2e*UinP - S2e*QinP |
ulalume3@0 | 1155 | |
ulalume3@0 | 1156 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 1157 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
ulalume3@0 | 1158 | # parameters for calibration with aCal |
ulalume3@0 | 1159 | AT = ATP1*IinP + h*ATP4*VinP |
ulalume3@0 | 1160 | BT = ATP3e*QinP - h*ATP2e*UinP |
ulalume3@0 | 1161 | AR = ARP1*IinP + h*ARP4*VinP |
ulalume3@0 | 1162 | BR = ARP3e*QinP - h*ARP2e*UinP |
ulalume3@0 | 1163 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1164 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 1165 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 1166 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 1167 | GT = np.dot(ATP,IS1) |
ulalume3@0 | 1168 | GR = np.dot(ARP,IS1) |
ulalume3@0 | 1169 | HT = np.dot(ATP,IS2) |
ulalume3@0 | 1170 | HR = np.dot(ARP,IS2) |
ulalume3@0 | 1171 | else: |
ulalume3@0 | 1172 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 1173 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 1174 | GT = np.dot(ATPe,IS1) |
ulalume3@0 | 1175 | GR = np.dot(ARPe,IS1) |
ulalume3@0 | 1176 | HT = np.dot(ATPe,IS2) |
ulalume3@0 | 1177 | HR = np.dot(ARPe,IS2) |
ulalume3@0 | 1178 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
ulalume3@0 | 1179 | # parameters for calibration with aCal |
ulalume3@0 | 1180 | AT = ATP1*IinP + ATP3e*UinPe + ZiC*CosC*(ATP2e*QinPe + ATP4*VinP) |
ulalume3@0 | 1181 | BT = DiC*(ATP1*UinPe + ATP3e*IinP) - ZiC*SinC*(ATP2e*VinP - ATP4*QinPe) |
ulalume3@0 | 1182 | AR = ARP1*IinP + ARP3e*UinPe + ZiC*CosC*(ARP2e*QinPe + ARP4*VinP) |
ulalume3@0 | 1183 | BR = DiC*(ARP1*UinPe + ARP3e*IinP) - ZiC*SinC*(ARP2e*VinP - ARP4*QinPe) |
ulalume3@0 | 1184 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1185 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 1186 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 1187 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 1188 | GT = np.dot(ATP,IS1) |
ulalume3@0 | 1189 | GR = np.dot(ARP,IS1) |
ulalume3@0 | 1190 | HT = np.dot(ATP,IS2) |
ulalume3@0 | 1191 | HR = np.dot(ARP,IS2) |
ulalume3@0 | 1192 | else: |
ulalume3@0 | 1193 | IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)]) |
ulalume3@0 | 1194 | IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)]) |
ulalume3@0 | 1195 | GT = np.dot(ATPe,IS1e) |
ulalume3@0 | 1196 | GR = np.dot(ARPe,IS1e) |
ulalume3@0 | 1197 | HT = np.dot(ATPe,IS2e) |
ulalume3@0 | 1198 | HR = np.dot(ARPe,IS2e) |
ulalume3@0 | 1199 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 1200 | # parameters for calibration with aCal |
ulalume3@0 | 1201 | AT = ATP1*IinP + sqr05*DiC*(ATP1*QinPe + ATP2e*IinP) + (1-0.5*WiC)*(ATP2e*QinPe + ATP3e*UinPe) + ZiC*(sqr05*SinC*(ATP3e*VinP-ATP4*UinPe) + ATP4*CosC*VinP) |
ulalume3@0 | 1202 | BT = sqr05*DiC*(ATP1*UinPe + ATP3e*IinP) + 0.5*WiC*(ATP2e*UinPe + ATP3e*QinPe) - sqr05*ZiC*SinC*(ATP2e*VinP - ATP4*QinPe) |
ulalume3@0 | 1203 | AR = ARP1*IinP + sqr05*DiC*(ARP1*QinPe + ARP2e*IinP) + (1-0.5*WiC)*(ARP2e*QinPe + ARP3e*UinPe) + ZiC*(sqr05*SinC*(ARP3e*VinP-ARP4*UinPe) + ARP4*CosC*VinP) |
ulalume3@0 | 1204 | BR = sqr05*DiC*(ARP1*UinPe + ARP3e*IinP) + 0.5*WiC*(ARP2e*UinPe + ARP3e*QinPe) - sqr05*ZiC*SinC*(ARP2e*VinP - ARP4*QinPe) |
ulalume3@0 | 1205 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1206 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 1207 | IS1 = np.array([IinPo,QinPo,UinPo,VinPo]) |
ulalume3@0 | 1208 | IS2 = np.array([IinPa,QinPa,UinPa,VinPa]) |
ulalume3@0 | 1209 | GT = np.dot(ATP,IS1) |
ulalume3@0 | 1210 | GR = np.dot(ARP,IS1) |
ulalume3@0 | 1211 | HT = np.dot(ATP,IS2) |
ulalume3@0 | 1212 | HR = np.dot(ARP,IS2) |
ulalume3@0 | 1213 | else: |
ulalume3@0 | 1214 | IS1e = np.array([IinPo+DiC*QinPoe,DiC*IinPo+QinPoe,ZiC*(CosC*UinPoe+SinC*VinPo),-ZiC*(SinC*UinPoe-CosC*VinPo)]) |
ulalume3@0 | 1215 | IS2e = np.array([IinPa+DiC*QinPae,DiC*IinPa+QinPae,ZiC*(CosC*UinPae+SinC*VinPa),-ZiC*(SinC*UinPae-CosC*VinPa)]) |
ulalume3@0 | 1216 | GT = np.dot(ATPe,IS1e) |
ulalume3@0 | 1217 | GR = np.dot(ARPe,IS1e) |
ulalume3@0 | 1218 | HT = np.dot(ATPe,IS2e) |
ulalume3@0 | 1219 | HR = np.dot(ARPe,IS2e) |
ulalume3@0 | 1220 | else: |
ulalume3@0 | 1221 | print("Calibrator not implemented yet") |
ulalume3@0 | 1222 | sys.exit() |
ulalume3@0 | 1223 | |
ulalume3@0 | 1224 | elif LocC == 3: # C before receiver optics Eq.57 |
ulalume3@0 | 1225 | |
ulalume3@0 | 1226 | #S2ge = np.sin(np.deg2rad(2*RotO - 2*RotC)) |
ulalume3@0 | 1227 | #C2ge = np.cos(np.deg2rad(2*RotO - 2*RotC)) |
ulalume3@0 | 1228 | S2e = np.sin(np.deg2rad(2*RotC)) |
ulalume3@0 | 1229 | C2e = np.cos(np.deg2rad(2*RotC)) |
ulalume3@0 | 1230 | |
ulalume3@0 | 1231 | # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt) |
ulalume3@0 | 1232 | AF1 = np.array([1,C2g*DiO,S2g*DiO,0]) |
ulalume3@0 | 1233 | AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO]) |
ulalume3@0 | 1234 | AF3 = np.array([S2g*DiO, S2g*C2g*WiO, 1-C2g**2*WiO, C2g*ZiO*SinO]) |
ulalume3@0 | 1235 | AF4 = np.array([0, S2g*SinO, -C2g*SinO, CosO]) |
ulalume3@0 | 1236 | |
ulalume3@0 | 1237 | ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4) |
ulalume3@0 | 1238 | ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4) |
ulalume3@0 | 1239 | ATF1 = ATF[0] |
ulalume3@0 | 1240 | ATF2 = ATF[1] |
ulalume3@0 | 1241 | ATF3 = ATF[2] |
ulalume3@0 | 1242 | ATF4 = ATF[3] |
ulalume3@0 | 1243 | ARF1 = ARF[0] |
ulalume3@0 | 1244 | ARF2 = ARF[1] |
ulalume3@0 | 1245 | ARF3 = ARF[2] |
ulalume3@0 | 1246 | ARF4 = ARF[3] |
ulalume3@0 | 1247 | |
ulalume3@0 | 1248 | # rotated AinF by epsilon |
ulalume3@0 | 1249 | ATF2e = C2e*ATF[1] + S2e*ATF[2] |
ulalume3@0 | 1250 | ATF3e = C2e*ATF[2] - S2e*ATF[1] |
ulalume3@0 | 1251 | ARF2e = C2e*ARF[1] + S2e*ARF[2] |
ulalume3@0 | 1252 | ARF3e = C2e*ARF[2] - S2e*ARF[1] |
ulalume3@0 | 1253 | |
ulalume3@0 | 1254 | ATFe = np.array([ATF1,ATF2e,ATF3e,ATF4]) |
ulalume3@0 | 1255 | ARFe = np.array([ARF1,ARF2e,ARF3e,ARF4]) |
ulalume3@0 | 1256 | |
ulalume3@0 | 1257 | QinEe = C2e*QinE + S2e*UinE |
ulalume3@0 | 1258 | UinEe = C2e*UinE - S2e*QinE |
ulalume3@0 | 1259 | |
ulalume3@0 | 1260 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 1261 | IinF = IinE |
ulalume3@0 | 1262 | QinF = aCal*QinE |
ulalume3@0 | 1263 | UinF = -aCal*UinE |
ulalume3@0 | 1264 | VinF = (1.-2.*aCal)*VinE |
ulalume3@0 | 1265 | |
ulalume3@0 | 1266 | IinFo = IinE |
ulalume3@0 | 1267 | QinFo = 0. |
ulalume3@0 | 1268 | UinFo = 0. |
ulalume3@0 | 1269 | VinFo = VinE |
ulalume3@0 | 1270 | |
ulalume3@0 | 1271 | IinFa = 0. |
ulalume3@0 | 1272 | QinFa = QinE |
ulalume3@0 | 1273 | UinFa = -UinE |
ulalume3@0 | 1274 | VinFa = -2.*VinE |
ulalume3@0 | 1275 | |
ulalume3@0 | 1276 | # Stokes Input Vector before receiver optics rotated by epsilon Eq. C.3 |
ulalume3@0 | 1277 | QinFe = C2e*QinF + S2e*UinF |
ulalume3@0 | 1278 | UinFe = C2e*UinF - S2e*QinF |
ulalume3@0 | 1279 | QinFoe = C2e*QinFo + S2e*UinFo |
ulalume3@0 | 1280 | UinFoe = C2e*UinFo - S2e*QinFo |
ulalume3@0 | 1281 | QinFae = C2e*QinFa + S2e*UinFa |
ulalume3@0 | 1282 | UinFae = C2e*UinFa - S2e*QinFa |
ulalume3@0 | 1283 | |
ulalume3@0 | 1284 | # Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 1285 | if (TypeC == 2) or (TypeC == 1): # rotator calibration Eq. C.4 |
ulalume3@0 | 1286 | AT = ATF1*IinF + ATF4*h*VinF |
ulalume3@0 | 1287 | BT = ATF3e*QinF - ATF2e*h*UinF |
ulalume3@0 | 1288 | AR = ARF1*IinF + ARF4*h*VinF |
ulalume3@0 | 1289 | BR = ARF3e*QinF - ARF2e*h*UinF |
ulalume3@0 | 1290 | |
ulalume3@0 | 1291 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1292 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 1293 | GT = ATF1*IinE + ATF4*VinE |
ulalume3@0 | 1294 | GR = ARF1*IinE + ARF4*VinE |
ulalume3@0 | 1295 | HT = ATF2*QinE - ATF3*UinE - ATF4*2*VinE |
ulalume3@0 | 1296 | HR = ARF2*QinE - ARF3*UinE - ARF4*2*VinE |
ulalume3@0 | 1297 | else: |
ulalume3@0 | 1298 | GT = ATF1*IinE + ATF4*h*VinE |
ulalume3@0 | 1299 | GR = ARF1*IinE + ARF4*h*VinE |
ulalume3@0 | 1300 | HT = ATF2e*QinE - ATF3e*h*UinE - ATF4*h*2*VinE |
ulalume3@0 | 1301 | HR = ARF2e*QinE - ARF3e*h*UinE - ARF4*h*2*VinE |
ulalume3@0 | 1302 | |
ulalume3@0 | 1303 | elif (TypeC == 3) or (TypeC == 4): # linear polariser calibration Eq. C.5 |
ulalume3@0 | 1304 | # p = +45°, m = -45° |
ulalume3@0 | 1305 | IF1e = np.array([IinF, ZiC*CosC*QinFe, UinFe, ZiC*CosC*VinF]) |
ulalume3@0 | 1306 | IF2e = np.array([DiC*UinFe, -ZiC*SinC*VinF, DiC*IinF, ZiC*SinC*QinFe]) |
ulalume3@0 | 1307 | |
ulalume3@0 | 1308 | AT = np.dot(ATFe,IF1e) |
ulalume3@0 | 1309 | AR = np.dot(ARFe,IF1e) |
ulalume3@0 | 1310 | BT = np.dot(ATFe,IF2e) |
ulalume3@0 | 1311 | BR = np.dot(ARFe,IF2e) |
ulalume3@0 | 1312 | |
ulalume3@0 | 1313 | # Correction paremeters for normal measurements; they are independent of LDR --- the same as for TypeC = 6 |
ulalume3@0 | 1314 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 1315 | IS1 = np.array([IinE,0,0,VinE]) |
ulalume3@0 | 1316 | IS2 = np.array([0,QinE,-UinE,-2*VinE]) |
ulalume3@0 | 1317 | |
ulalume3@0 | 1318 | GT = np.dot(ATF,IS1) |
ulalume3@0 | 1319 | GR = np.dot(ARF,IS1) |
ulalume3@0 | 1320 | HT = np.dot(ATF,IS2) |
ulalume3@0 | 1321 | HR = np.dot(ARF,IS2) |
ulalume3@0 | 1322 | else: |
ulalume3@0 | 1323 | IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)]) |
ulalume3@0 | 1324 | IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)]) |
ulalume3@0 | 1325 | GT = np.dot(ATFe,IS1e) |
ulalume3@0 | 1326 | GR = np.dot(ARFe,IS1e) |
ulalume3@0 | 1327 | HT = np.dot(ATFe,IS2e) |
ulalume3@0 | 1328 | HR = np.dot(ARFe,IS2e) |
ulalume3@0 | 1329 | |
ulalume3@0 | 1330 | elif (TypeC == 6): # diattenuator calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 1331 | # p = +22.5°, m = -22.5° |
ulalume3@0 | 1332 | IF1e = np.array([IinF+sqr05*DiC*QinFe, sqr05*DiC*IinF+(1-0.5*WiC)*QinFe, (1-0.5*WiC)*UinFe+sqr05*ZiC*SinC*VinF, -sqr05*ZiC*SinC*UinFe+ZiC*CosC*VinF]) |
ulalume3@0 | 1333 | IF2e = np.array([sqr05*DiC*UinFe, 0.5*WiC*UinFe-sqr05*ZiC*SinC*VinF, sqr05*DiC*IinF+0.5*WiC*QinFe, sqr05*ZiC*SinC*QinFe]) |
ulalume3@0 | 1334 | |
ulalume3@0 | 1335 | AT = np.dot(ATFe,IF1e) |
ulalume3@0 | 1336 | AR = np.dot(ARFe,IF1e) |
ulalume3@0 | 1337 | BT = np.dot(ATFe,IF2e) |
ulalume3@0 | 1338 | BR = np.dot(ARFe,IF2e) |
ulalume3@0 | 1339 | |
ulalume3@0 | 1340 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1341 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 1342 | #IS1 = np.array([IinE,0,0,VinE]) |
ulalume3@0 | 1343 | #IS2 = np.array([0,QinE,-UinE,-2*VinE]) |
ulalume3@0 | 1344 | IS1 = np.array([IinFo,0,0,VinFo]) |
ulalume3@0 | 1345 | IS2 = np.array([0,QinFa,UinFa,VinFa]) |
ulalume3@0 | 1346 | GT = np.dot(ATF,IS1) |
ulalume3@0 | 1347 | GR = np.dot(ARF,IS1) |
ulalume3@0 | 1348 | HT = np.dot(ATF,IS2) |
ulalume3@0 | 1349 | HR = np.dot(ARF,IS2) |
ulalume3@0 | 1350 | else: |
ulalume3@0 | 1351 | #IS1e = np.array([IinE,DiC*IinE,ZiC*SinC*VinE,ZiC*CosC*VinE]) |
ulalume3@0 | 1352 | #IS2e = np.array([DiC*QinEe,QinEe,-ZiC*(CosC*UinEe+2*SinC*VinE),ZiC*(SinC*UinEe-2*CosC*VinE)]) |
ulalume3@0 | 1353 | IS1e = np.array([IinFo+DiC*QinFoe,DiC*IinFo+QinFoe,ZiC*(CosC*UinFoe+SinC*VinFo),-ZiC*(SinC*UinFoe-CosC*VinFo)]) |
ulalume3@0 | 1354 | IS2e = np.array([IinFa+DiC*QinFae,DiC*IinFa+QinFae,ZiC*(CosC*UinFae+SinC*VinFa),-ZiC*(SinC*UinFae-CosC*VinFa)]) |
ulalume3@0 | 1355 | GT = np.dot(ATFe,IS1e) |
ulalume3@0 | 1356 | GR = np.dot(ARFe,IS1e) |
ulalume3@0 | 1357 | HT = np.dot(ATFe,IS2e) |
ulalume3@0 | 1358 | HR = np.dot(ARFe,IS2e) |
ulalume3@0 | 1359 | |
ulalume3@0 | 1360 | |
ulalume3@0 | 1361 | else: |
ulalume3@0 | 1362 | print('Calibrator not implemented yet') |
ulalume3@0 | 1363 | sys.exit() |
ulalume3@0 | 1364 | |
ulalume3@0 | 1365 | elif LocC == 2: # C behind emitter optics Eq.57 |
ulalume3@0 | 1366 | #print("Calibrator location not implemented yet") |
ulalume3@0 | 1367 | S2e = np.sin(np.deg2rad(2*RotC)) |
ulalume3@0 | 1368 | C2e = np.cos(np.deg2rad(2*RotC)) |
ulalume3@0 | 1369 | |
ulalume3@0 | 1370 | # AS with C before the receiver optics (see document rotated_diattenuator_X22x5deg.odt) |
ulalume3@0 | 1371 | AF1 = np.array([1,C2g*DiO,S2g*DiO,0]) |
ulalume3@0 | 1372 | AF2 = np.array([C2g*DiO,1-S2g**2*WiO,S2g*C2g*WiO,-S2g*ZiO*SinO]) |
ulalume3@0 | 1373 | AF3 = np.array([S2g*DiO, S2g*C2g*WiO, 1-C2g**2*WiO, C2g*ZiO*SinO]) |
ulalume3@0 | 1374 | AF4 = np.array([0, S2g*SinO, -C2g*SinO, CosO]) |
ulalume3@0 | 1375 | |
ulalume3@0 | 1376 | ATF = (ATP1*AF1+ATP2*AF2+ATP3*AF3+ATP4*AF4) |
ulalume3@0 | 1377 | ARF = (ARP1*AF1+ARP2*AF2+ARP3*AF3+ARP4*AF4) |
ulalume3@0 | 1378 | ATF1 = ATF[0] |
ulalume3@0 | 1379 | ATF2 = ATF[1] |
ulalume3@0 | 1380 | ATF3 = ATF[2] |
ulalume3@0 | 1381 | ATF4 = ATF[3] |
ulalume3@0 | 1382 | ARF1 = ARF[0] |
ulalume3@0 | 1383 | ARF2 = ARF[1] |
ulalume3@0 | 1384 | ARF3 = ARF[2] |
ulalume3@0 | 1385 | ARF4 = ARF[3] |
ulalume3@0 | 1386 | |
ulalume3@0 | 1387 | # AS with C behind the emitter -------------------------------------------- |
ulalume3@0 | 1388 | # terms without aCal |
ulalume3@0 | 1389 | ATE1o, ARE1o = ATF1, ARF1 |
ulalume3@0 | 1390 | ATE2o, ARE2o = 0., 0. |
ulalume3@0 | 1391 | ATE3o, ARE3o = 0., 0. |
ulalume3@0 | 1392 | ATE4o, ARE4o = ATF4, ARF4 |
ulalume3@0 | 1393 | # terms with aCal |
ulalume3@0 | 1394 | ATE1a, ARE1a = 0. , 0. |
ulalume3@0 | 1395 | ATE2a, ARE2a = ATF2, ARF2 |
ulalume3@0 | 1396 | ATE3a, ARE3a = -ATF3, -ARF3 |
ulalume3@0 | 1397 | ATE4a, ARE4a = -2*ATF4, -2*ARF4 |
ulalume3@0 | 1398 | # rotated AinEa by epsilon |
ulalume3@0 | 1399 | ATE2ae = C2e*ATF2 + S2e*ATF3 |
ulalume3@0 | 1400 | ATE3ae = -S2e*ATF2 - C2e*ATF3 |
ulalume3@0 | 1401 | ARE2ae = C2e*ARF2 + S2e*ARF3 |
ulalume3@0 | 1402 | ARE3ae = -S2e*ARF2 - C2e*ARF3 |
ulalume3@0 | 1403 | |
ulalume3@0 | 1404 | ATE1 = ATE1o |
ulalume3@0 | 1405 | ATE2e = aCal*ATE2ae |
ulalume3@0 | 1406 | ATE3e = aCal*ATE3ae |
ulalume3@0 | 1407 | ATE4 = (1-2*aCal)*ATF4 |
ulalume3@0 | 1408 | ARE1 = ARE1o |
ulalume3@0 | 1409 | ARE2e = aCal*ARE2ae |
ulalume3@0 | 1410 | ARE3e = aCal*ARE3ae |
ulalume3@0 | 1411 | ARE4 = (1-2*aCal)*ARF4 |
ulalume3@0 | 1412 | |
ulalume3@0 | 1413 | # rotated IinE |
ulalume3@0 | 1414 | QinEe = C2e*QinE + S2e*UinE |
ulalume3@0 | 1415 | UinEe = C2e*UinE - S2e*QinE |
ulalume3@0 | 1416 | |
ulalume3@0 | 1417 | # --- Calibration signals and Calibration correction K from measurements with LDRCal / aCal |
ulalume3@0 | 1418 | if (TypeC == 2) or (TypeC == 1): # +++++++++ rotator calibration Eq. C.4 |
ulalume3@0 | 1419 | AT = ATE1o*IinE + (ATE4o+aCal*ATE4a)*h*VinE |
ulalume3@0 | 1420 | BT = aCal * (ATE3ae*QinEe - ATE2ae*h*UinEe) |
ulalume3@0 | 1421 | AR = ARE1o*IinE + (ARE4o+aCal*ARE4a)*h*VinE |
ulalume3@0 | 1422 | BR = aCal * (ARE3ae*QinEe - ARE2ae*h*UinEe) |
ulalume3@0 | 1423 | |
ulalume3@0 | 1424 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1425 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 1426 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 1427 | GT = ATE1o*IinE + ATE4o*h*VinE |
ulalume3@0 | 1428 | GR = ARE1o*IinE + ARE4o*h*VinE |
ulalume3@0 | 1429 | HT = ATE2a*QinE + ATE3a*h*UinEe + ATE4a*h*VinE |
ulalume3@0 | 1430 | HR = ARE2a*QinE + ARE3a*h*UinEe + ARE4a*h*VinE |
ulalume3@0 | 1431 | else: |
ulalume3@0 | 1432 | GT = ATE1o*IinE + ATE4o*h*VinE |
ulalume3@0 | 1433 | GR = ARE1o*IinE + ARE4o*h*VinE |
ulalume3@0 | 1434 | HT = ATE2ae*QinE + ATE3ae*h*UinEe + ATE4a*h*VinE |
ulalume3@0 | 1435 | HR = ARE2ae*QinE + ARE3ae*h*UinEe + ARE4a*h*VinE |
ulalume3@0 | 1436 | |
ulalume3@0 | 1437 | elif (TypeC == 3) or (TypeC == 4): # +++++++++ linear polariser calibration Eq. C.5 |
ulalume3@0 | 1438 | # p = +45°, m = -45° |
ulalume3@0 | 1439 | AT = ATE1*IinE + ZiC*CosC*(ATE2e*QinEe + ATE4*VinE) + ATE3e*UinEe |
ulalume3@0 | 1440 | BT = DiC*(ATE1*UinEe + ATE3e*IinE) + ZiC*SinC*(ATE4*QinEe - ATE2e*VinE) |
ulalume3@0 | 1441 | AR = ARE1*IinE + ZiC*CosC*(ARE2e*QinEe + ARE4*VinE) + ARE3e*UinEe |
ulalume3@0 | 1442 | BR = DiC*(ARE1*UinEe + ARE3e*IinE) + ZiC*SinC*(ARE4*QinEe - ARE2e*VinE) |
ulalume3@0 | 1443 | |
ulalume3@0 | 1444 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1445 | if (not RotationErrorEpsilonForNormalMeasurements): |
ulalume3@0 | 1446 | # Stokes Input Vector before receiver optics Eq. E.19 (after atmosphere F) |
ulalume3@0 | 1447 | GT = ATE1o*IinE + ATE4o*VinE |
ulalume3@0 | 1448 | GR = ARE1o*IinE + ARE4o*VinE |
ulalume3@0 | 1449 | HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE |
ulalume3@0 | 1450 | HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE |
ulalume3@0 | 1451 | else: |
ulalume3@0 | 1452 | D = IinE + DiC*QinEe |
ulalume3@0 | 1453 | A = DiC*IinE + QinEe |
ulalume3@0 | 1454 | B = ZiC*(CosC*UinEe + SinC*VinE) |
ulalume3@0 | 1455 | C = -ZiC*(SinC*UinEe - CosC*VinE) |
ulalume3@0 | 1456 | GT = ATE1o*D + ATE4o*C |
ulalume3@0 | 1457 | GR = ARE1o*D + ARE4o*C |
ulalume3@0 | 1458 | HT = ATE2a*A + ATE3a*B + ATE4a*C |
ulalume3@0 | 1459 | HR = ARE2a*A + ARE3a*B + ARE4a*C |
ulalume3@0 | 1460 | |
ulalume3@0 | 1461 | elif (TypeC == 6): # real HWP calibration +-22.5° rotated_diattenuator_X22x5deg.odt |
ulalume3@0 | 1462 | # p = +22.5°, m = -22.5° |
ulalume3@0 | 1463 | IE1e = np.array([IinE+sqr05*DiC*QinEe, sqr05*DiC*IinE+(1-0.5*WiC)*QinEe, (1-0.5*WiC)*UinEe+sqr05*ZiC*SinC*VinE, -sqr05*ZiC*SinC*UinEe+ZiC*CosC*VinE]) |
ulalume3@0 | 1464 | IE2e = np.array([sqr05*DiC*UinEe, 0.5*WiC*UinEe-sqr05*ZiC*SinC*VinE, sqr05*DiC*IinE+0.5*WiC*QinEe, sqr05*ZiC*SinC*QinEe]) |
ulalume3@0 | 1465 | ATEe = np.array([ATE1,ATE2e,ATE3e,ATE4]) |
ulalume3@0 | 1466 | AREe = np.array([ARE1,ARE2e,ARE3e,ARE4]) |
ulalume3@0 | 1467 | AT = np.dot(ATEe,IE1e) |
ulalume3@0 | 1468 | AR = np.dot(AREe,IE1e) |
ulalume3@0 | 1469 | BT = np.dot(ATEe,IE2e) |
ulalume3@0 | 1470 | BR = np.dot(AREe,IE2e) |
ulalume3@0 | 1471 | |
ulalume3@0 | 1472 | # Correction paremeters for normal measurements; they are independent of LDR |
ulalume3@0 | 1473 | if (not RotationErrorEpsilonForNormalMeasurements): # calibrator taken out |
ulalume3@0 | 1474 | GT = ATE1o*IinE + ATE4o*VinE |
ulalume3@0 | 1475 | GR = ARE1o*IinE + ARE4o*VinE |
ulalume3@0 | 1476 | HT = ATE2a*QinE + ATE3a*UinE + ATE4a*VinE |
ulalume3@0 | 1477 | HR = ARE2a*QinE + ARE3a*UinE + ARE4a*VinE |
ulalume3@0 | 1478 | else: |
ulalume3@0 | 1479 | D = IinE + DiC*QinEe |
ulalume3@0 | 1480 | A = DiC*IinE + QinEe |
ulalume3@0 | 1481 | B = ZiC*(CosC*UinEe + SinC*VinE) |
ulalume3@0 | 1482 | C = -ZiC*(SinC*UinEe - CosC*VinE) |
ulalume3@0 | 1483 | GT = ATE1o*D + ATE4o*C |
ulalume3@0 | 1484 | GR = ARE1o*D + ARE4o*C |
ulalume3@0 | 1485 | HT = ATE2a*A + ATE3a*B + ATE4a*C |
ulalume3@0 | 1486 | HR = ARE2a*A + ARE3a*B + ARE4a*C |
ulalume3@0 | 1487 | |
ulalume3@0 | 1488 | else: |
ulalume3@0 | 1489 | print('Calibrator not implemented yet') |
ulalume3@0 | 1490 | sys.exit() |
ulalume3@0 | 1491 | |
ulalume3@0 | 1492 | # Calibration signals with aCal => Determination of the correction K of the real calibration factor |
ulalume3@0 | 1493 | IoutTp = TaT*TiT*TiO*TiE*(AT + BT) |
ulalume3@0 | 1494 | IoutTm = TaT*TiT*TiO*TiE*(AT - BT) |
ulalume3@0 | 1495 | IoutRp = TaR*TiR*TiO*TiE*(AR + BR) |
ulalume3@0 | 1496 | IoutRm = TaR*TiR*TiO*TiE*(AR - BR) |
ulalume3@0 | 1497 | # --- Results and Corrections; electronic etaR and etaT are assumed to be 1 |
ulalume3@0 | 1498 | #Eta = TiR/TiT # Eta = Eta*/K Eq. 84 |
ulalume3@0 | 1499 | Etapx = IoutRp/IoutTp |
ulalume3@0 | 1500 | Etamx = IoutRm/IoutTm |
ulalume3@0 | 1501 | Etax = (Etapx*Etamx)**0.5 |
ulalume3@0 | 1502 | K = Etax / Eta0 |
ulalume3@0 | 1503 | #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)) |
ulalume3@0 | 1504 | #print("{0:6.3f},{1:6.3f},{2:6.3f},{3:6.3f}".format(DiC, ZiC, Kp, Km)) |
ulalume3@0 | 1505 | |
ulalume3@0 | 1506 | # For comparison with Volkers Libreoffice Müller Matrix spreadsheet |
ulalume3@0 | 1507 | #Eta_test_p = (IoutRp/IoutTp) |
ulalume3@0 | 1508 | #Eta_test_m = (IoutRm/IoutTm) |
ulalume3@0 | 1509 | #Eta_test = (Eta_test_p*Eta_test_m)**0.5 |
ulalume3@0 | 1510 | |
ulalume3@0 | 1511 | # ************************************************************************* |
ulalume3@0 | 1512 | iLDR = -1 |
ulalume3@0 | 1513 | for LDRTrue in LDRrange: |
ulalume3@0 | 1514 | iLDR = iLDR + 1 |
ulalume3@0 | 1515 | atrue = (1-LDRTrue)/(1+LDRTrue) |
ulalume3@0 | 1516 | # ----- Forward simulated signals and LDRsim with atrue; from input file |
ulalume3@0 | 1517 | It = TaT*TiT*TiO*TiE*(GT+atrue*HT) # TaT*TiT*TiC*TiO*IinL*(GT+atrue*HT) |
ulalume3@0 | 1518 | Ir = TaR*TiR*TiO*TiE*(GR+atrue*HR) # TaR*TiR*TiC*TiO*IinL*(GR+atrue*HR) |
ulalume3@0 | 1519 | |
ulalume3@0 | 1520 | # LDRsim = 1/Eta*Ir/It # simulated LDR* with Y from input file |
ulalume3@0 | 1521 | LDRsim = Ir/It # simulated uncorrected LDR with Y from input file |
ulalume3@0 | 1522 | ''' |
ulalume3@0 | 1523 | if Y == 1.: |
ulalume3@0 | 1524 | LDRsimx = LDRsim |
ulalume3@0 | 1525 | LDRsimx2 = LDRsim2 |
ulalume3@0 | 1526 | else: |
ulalume3@0 | 1527 | LDRsimx = 1./LDRsim |
ulalume3@0 | 1528 | LDRsimx2 = 1./LDRsim2 |
ulalume3@0 | 1529 | ''' |
ulalume3@0 | 1530 | # ----- Backward correction |
ulalume3@0 | 1531 | # Corrected LDRCorr from forward simulated LDRsim (atrue) with assumed true G0,H0,K0 |
ulalume3@0 | 1532 | LDRCorr = (LDRsim*K0/Etax*(GT0+HT0)-(GR0+HR0))/((GR0-HR0)-LDRsim*K0/Etax*(GT0-HT0)) |
ulalume3@0 | 1533 | |
ulalume3@0 | 1534 | # -- F11corr from It and Ir and calibration EtaX |
ulalume3@0 | 1535 | Text1 = "F11corr from It and Ir with calibration EtaX: x-axis: F11corr(LDRtrue) / F11corr(LDRtrue = 0.004) - 1" |
ulalume3@0 | 1536 | F11corr = 1/(TiO*TiE)*((HR0*Etax/K0*It/TTa-HT0*Ir/TRa)/(HR0*GT0-HT0*GR0)) # IL = 1 Eq.(64) |
ulalume3@0 | 1537 | |
ulalume3@0 | 1538 | #Text1 = "F11corr from It and Ir without corrections but with calibration EtaX: x-axis: F11corr(LDRtrue) devided by F11corr(LDRtrue = 0.004)" |
ulalume3@0 | 1539 | #F11corr = 0.5/(TiO*TiE)*(Etax*It/TTa+Ir/TRa) # IL = 1 Eq.(64) |
ulalume3@0 | 1540 | |
ulalume3@0 | 1541 | # -- It from It only with atrue without corrections - for BERTHA (and PollyXTs) |
ulalume3@0 | 1542 | #Text1 = " x-axis: IT(LDRtrue) / IT(LDRtrue = 0.004) - 1" |
ulalume3@0 | 1543 | #F11corr = It/(TaT*TiT*TiO*TiE) #/(TaT*TiT*TiO*TiE*(GT0+atrue*HT0)) |
ulalume3@0 | 1544 | # !!! see below line 1673ff |
ulalume3@0 | 1545 | |
ulalume3@0 | 1546 | aF11corr[iLDR,iN] = F11corr |
ulalume3@0 | 1547 | aA[iLDR,iN] = LDRCorr |
ulalume3@0 | 1548 | |
ulalume3@0 | 1549 | aX[0,iN] = GR |
ulalume3@0 | 1550 | aX[1,iN] = GT |
ulalume3@0 | 1551 | aX[2,iN] = HR |
ulalume3@0 | 1552 | aX[3,iN] = HT |
ulalume3@0 | 1553 | aX[4,iN] = K |
ulalume3@0 | 1554 | |
ulalume3@0 | 1555 | aLDRCal[iN] = iLDRCal |
ulalume3@0 | 1556 | aERaT[iN] = iERaT |
ulalume3@0 | 1557 | aERaR[iN] = iERaR |
ulalume3@0 | 1558 | aRotaT[iN] = iRotaT |
ulalume3@0 | 1559 | aRotaR[iN] = iRotaR |
ulalume3@0 | 1560 | aRetT[iN] = iRetT |
ulalume3@0 | 1561 | aRetR[iN] = iRetR |
ulalume3@0 | 1562 | |
ulalume3@0 | 1563 | aRotL[iN] = iRotL |
ulalume3@0 | 1564 | aRotE[iN] = iRotE |
ulalume3@0 | 1565 | aRetE[iN] = iRetE |
ulalume3@0 | 1566 | aRotO[iN] = iRotO |
ulalume3@0 | 1567 | aRetO[iN] = iRetO |
ulalume3@0 | 1568 | aRotC[iN] = iRotC |
ulalume3@0 | 1569 | aRetC[iN] = iRetC |
ulalume3@0 | 1570 | aDiO[iN] = iDiO |
ulalume3@0 | 1571 | aDiE[iN] = iDiE |
ulalume3@0 | 1572 | aDiC[iN] = iDiC |
ulalume3@0 | 1573 | aTP[iN] = iTP |
ulalume3@0 | 1574 | aTS[iN] = iTS |
ulalume3@0 | 1575 | aRP[iN] = iRP |
ulalume3@0 | 1576 | aRS[iN] = iRS |
ulalume3@0 | 1577 | |
ulalume3@0 | 1578 | # --- END loop |
ulalume3@0 | 1579 | btime = clock() |
ulalume3@0 | 1580 | print("\r done in ", "{0:5.0f}".format(btime-atime), "sec") #, end="\r") |
ulalume3@0 | 1581 | |
ulalume3@0 | 1582 | # --- Plot ----------------------------------------------------------------- |
ulalume3@0 | 1583 | #sns.set_style("whitegrid") |
ulalume3@0 | 1584 | #sns.set_palette("bright", 6) |
ulalume3@0 | 1585 | |
ulalume3@0 | 1586 | ''' |
ulalume3@0 | 1587 | fig2 = plt.figure() |
ulalume3@0 | 1588 | plt.plot(aA[2,:],'b.') |
ulalume3@0 | 1589 | plt.plot(aA[3,:],'r.') |
ulalume3@0 | 1590 | plt.plot(aA[4,:],'g.') |
ulalume3@0 | 1591 | #plt.plot(aA[6,:],'c.') |
ulalume3@0 | 1592 | plt.show |
ulalume3@0 | 1593 | ''' |
ulalume3@0 | 1594 | |
ulalume3@0 | 1595 | |
ulalume3@0 | 1596 | # Plot LDR |
ulalume3@0 | 1597 | def PlotSubHist(aVar, aX, X0, daX, iaX, naX): |
ulalume3@0 | 1598 | |
ulalume3@0 | 1599 | fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2)) |
ulalume3@0 | 1600 | iLDR = -1 |
ulalume3@0 | 1601 | for LDRTrue in LDRrange: |
ulalume3@0 | 1602 | iLDR = iLDR + 1 |
ulalume3@0 | 1603 | |
ulalume3@0 | 1604 | LDRmin[iLDR] = np.min(aA[iLDR,:]) |
ulalume3@0 | 1605 | LDRmax[iLDR] = np.max(aA[iLDR,:]) |
ulalume3@0 | 1606 | Rmin = LDRmin[iLDR] * 0.995 # np.min(aA[iLDR,:]) * 0.995 |
ulalume3@0 | 1607 | Rmax = LDRmax[iLDR] * 1.005 # np.max(aA[iLDR,:]) * 1.005 |
ulalume3@0 | 1608 | |
ulalume3@0 | 1609 | #plt.subplot(5,2,iLDR+1) |
ulalume3@0 | 1610 | plt.subplot(1,5,iLDR+1) |
ulalume3@0 | 1611 | (n, bins, patches) = plt.hist(aA[iLDR,:], |
ulalume3@0 | 1612 | bins=100, log=False, |
ulalume3@0 | 1613 | range=[Rmin, Rmax], |
ulalume3@0 | 1614 | alpha=0.5, normed=False, color = '0.5', histtype='stepfilled') |
ulalume3@0 | 1615 | |
ulalume3@0 | 1616 | for iaX in range(-naX,naX+1): |
ulalume3@0 | 1617 | plt.hist(aA[iLDR,aX == iaX], |
ulalume3@0 | 1618 | range=[Rmin, Rmax], |
ulalume3@0 | 1619 | bins=100, log=False, alpha=0.3, normed=False, histtype='stepfilled', label = str(round(X0 + iaX*daX/naX,5))) |
ulalume3@0 | 1620 | |
ulalume3@0 | 1621 | if (iLDR == 2): plt.legend() |
ulalume3@0 | 1622 | |
ulalume3@0 | 1623 | plt.tick_params(axis='both', labelsize=9) |
ulalume3@0 | 1624 | plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2) |
ulalume3@0 | 1625 | |
ulalume3@0 | 1626 | #plt.title(LID + ' ' + aVar, fontsize=18) |
ulalume3@0 | 1627 | #plt.ylabel('frequency', fontsize=10) |
ulalume3@0 | 1628 | #plt.xlabel('LDRcorr', fontsize=10) |
ulalume3@0 | 1629 | #fig.tight_layout() |
ulalume3@0 | 1630 | fig.suptitle(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05) |
ulalume3@0 | 1631 | #plt.show() |
ulalume3@0 | 1632 | #fig.savefig(LID + '_' + aVar + '.png', dpi=150, bbox_inches='tight', pad_inches=0) |
ulalume3@0 | 1633 | #plt.close |
ulalume3@0 | 1634 | return |
ulalume3@0 | 1635 | |
ulalume3@0 | 1636 | if (nRotL > 0): PlotSubHist("RotL", aRotL, RotL0, dRotL, iRotL, nRotL) |
ulalume3@0 | 1637 | if (nRetE > 0): PlotSubHist("RetE", aRetE, RetE0, dRetE, iRetE, nRetE) |
ulalume3@0 | 1638 | if (nRotE > 0): PlotSubHist("RotE", aRotE, RotE0, dRotE, iRotE, nRotE) |
ulalume3@0 | 1639 | if (nDiE > 0): PlotSubHist("DiE", aDiE, DiE0, dDiE, iDiE, nDiE) |
ulalume3@0 | 1640 | if (nRetO > 0): PlotSubHist("RetO", aRetO, RetO0, dRetO, iRetO, nRetO) |
ulalume3@0 | 1641 | if (nRotO > 0): PlotSubHist("RotO", aRotO, RotO0, dRotO, iRotO, nRotO) |
ulalume3@0 | 1642 | if (nDiO > 0): PlotSubHist("DiO", aDiO, DiO0, dDiO, iDiO, nDiO) |
ulalume3@0 | 1643 | if (nDiC > 0): PlotSubHist("DiC", aDiC, DiC0, dDiC, iDiC, nDiC) |
ulalume3@0 | 1644 | if (nRotC > 0): PlotSubHist("RotC", aRotC, RotC0, dRotC, iRotC, nRotC) |
ulalume3@0 | 1645 | if (nRetC > 0): PlotSubHist("RetC", aRetC, RetC0, dRetC, iRetC, nRetC) |
ulalume3@0 | 1646 | if (nTP > 0): PlotSubHist("TP", aTP, TP0, dTP, iTP, nTP) |
ulalume3@0 | 1647 | if (nTS > 0): PlotSubHist("TS", aTS, TS0, dTS, iTS, nTS) |
ulalume3@0 | 1648 | if (nRP > 0): PlotSubHist("RP", aRP, RP0, dRP, iRP, nRP) |
ulalume3@0 | 1649 | if (nRS > 0): PlotSubHist("RS", aRS, RS0, dRS, iRS, nRS) |
ulalume3@0 | 1650 | if (nRetT > 0): PlotSubHist("RetT", aRetT, RetT0, dRetT, iRetT, nRetT) |
ulalume3@0 | 1651 | if (nRetR > 0): PlotSubHist("RetR", aRetR, RetR0, dRetR, iRetR, nRetR) |
ulalume3@0 | 1652 | if (nERaT > 0): PlotSubHist("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT) |
ulalume3@0 | 1653 | if (nERaR > 0): PlotSubHist("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR) |
ulalume3@0 | 1654 | if (nRotaT > 0): PlotSubHist("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT) |
ulalume3@0 | 1655 | if (nRotaR > 0): PlotSubHist("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR) |
ulalume3@0 | 1656 | if (nLDRCal > 0): PlotSubHist("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal) |
ulalume3@0 | 1657 | |
ulalume3@0 | 1658 | plt.show() |
ulalume3@0 | 1659 | plt.close |
ulalume3@0 | 1660 | |
ulalume3@0 | 1661 | print() |
ulalume3@0 | 1662 | #print("IT(LDRtrue) devided by IT(LDRtrue = 0.004)") |
ulalume3@0 | 1663 | print(Text1) |
ulalume3@0 | 1664 | print() |
ulalume3@0 | 1665 | |
ulalume3@0 | 1666 | iLDR = 5 |
ulalume3@0 | 1667 | for LDRTrue in LDRrange: |
ulalume3@0 | 1668 | iLDR = iLDR - 1 |
ulalume3@0 | 1669 | aF11corr[iLDR,:] = aF11corr[iLDR,:] / aF11corr[0,:] - 1.0 |
ulalume3@0 | 1670 | |
ulalume3@0 | 1671 | # Plot F11 |
ulalume3@0 | 1672 | def PlotSubHistF11(aVar, aX, X0, daX, iaX, naX): |
ulalume3@0 | 1673 | |
ulalume3@0 | 1674 | fig, ax = plt.subplots(nrows=1, ncols=5, sharex=True, sharey=True, figsize=(25, 2)) |
ulalume3@0 | 1675 | iLDR = -1 |
ulalume3@0 | 1676 | for LDRTrue in LDRrange: |
ulalume3@0 | 1677 | iLDR = iLDR + 1 |
ulalume3@0 | 1678 | |
ulalume3@0 | 1679 | ''' |
ulalume3@0 | 1680 | F11min[iLDR] = np.min(aF11corr[iLDR,:]) |
ulalume3@0 | 1681 | F11max[iLDR] = np.max(aF11corr[iLDR,:]) |
ulalume3@0 | 1682 | Rmin = F11min[iLDR] * 0.995 # np.min(aA[iLDR,:]) * 0.995 |
ulalume3@0 | 1683 | Rmax = F11max[iLDR] * 1.005 # np.max(aA[iLDR,:]) * 1.005 |
ulalume3@0 | 1684 | ''' |
ulalume3@0 | 1685 | #Rmin = 0.8 |
ulalume3@0 | 1686 | #Rmax = 1.2 |
ulalume3@0 | 1687 | |
ulalume3@0 | 1688 | #plt.subplot(5,2,iLDR+1) |
ulalume3@0 | 1689 | plt.subplot(1,5,iLDR+1) |
ulalume3@0 | 1690 | (n, bins, patches) = plt.hist(aF11corr[iLDR,:], |
ulalume3@0 | 1691 | bins=100, log=False, |
ulalume3@0 | 1692 | alpha=0.5, normed=False, color = '0.5', histtype='stepfilled') |
ulalume3@0 | 1693 | |
ulalume3@0 | 1694 | for iaX in range(-naX,naX+1): |
ulalume3@0 | 1695 | plt.hist(aF11corr[iLDR,aX == iaX], |
ulalume3@0 | 1696 | bins=100, log=False, alpha=0.3, normed=False, histtype='stepfilled', label = str(round(X0 + iaX*daX/naX,5))) |
ulalume3@0 | 1697 | |
ulalume3@0 | 1698 | if (iLDR == 2): plt.legend() |
ulalume3@0 | 1699 | |
ulalume3@0 | 1700 | plt.tick_params(axis='both', labelsize=9) |
ulalume3@0 | 1701 | #plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2) |
ulalume3@0 | 1702 | |
ulalume3@0 | 1703 | #plt.title(LID + ' ' + aVar, fontsize=18) |
ulalume3@0 | 1704 | #plt.ylabel('frequency', fontsize=10) |
ulalume3@0 | 1705 | #plt.xlabel('LDRcorr', fontsize=10) |
ulalume3@0 | 1706 | #fig.tight_layout() |
ulalume3@0 | 1707 | fig.suptitle(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]) + ' - ' + aVar, fontsize=14, y=1.05) |
ulalume3@0 | 1708 | #plt.show() |
ulalume3@0 | 1709 | #fig.savefig(LID + '_' + aVar + '.png', dpi=150, bbox_inches='tight', pad_inches=0) |
ulalume3@0 | 1710 | #plt.close |
ulalume3@0 | 1711 | return |
ulalume3@0 | 1712 | |
ulalume3@0 | 1713 | if (nRotL > 0): PlotSubHistF11("RotL", aRotL, RotL0, dRotL, iRotL, nRotL) |
ulalume3@0 | 1714 | if (nRetE > 0): PlotSubHistF11("RetE", aRetE, RetE0, dRetE, iRetE, nRetE) |
ulalume3@0 | 1715 | if (nRotE > 0): PlotSubHistF11("RotE", aRotE, RotE0, dRotE, iRotE, nRotE) |
ulalume3@0 | 1716 | if (nDiE > 0): PlotSubHistF11("DiE", aDiE, DiE0, dDiE, iDiE, nDiE) |
ulalume3@0 | 1717 | if (nRetO > 0): PlotSubHistF11("RetO", aRetO, RetO0, dRetO, iRetO, nRetO) |
ulalume3@0 | 1718 | if (nRotO > 0): PlotSubHistF11("RotO", aRotO, RotO0, dRotO, iRotO, nRotO) |
ulalume3@0 | 1719 | if (nDiO > 0): PlotSubHistF11("DiO", aDiO, DiO0, dDiO, iDiO, nDiO) |
ulalume3@0 | 1720 | if (nDiC > 0): PlotSubHistF11("DiC", aDiC, DiC0, dDiC, iDiC, nDiC) |
ulalume3@0 | 1721 | if (nRotC > 0): PlotSubHistF11("RotC", aRotC, RotC0, dRotC, iRotC, nRotC) |
ulalume3@0 | 1722 | if (nRetC > 0): PlotSubHistF11("RetC", aRetC, RetC0, dRetC, iRetC, nRetC) |
ulalume3@0 | 1723 | if (nTP > 0): PlotSubHistF11("TP", aTP, TP0, dTP, iTP, nTP) |
ulalume3@0 | 1724 | if (nTS > 0): PlotSubHistF11("TS", aTS, TS0, dTS, iTS, nTS) |
ulalume3@0 | 1725 | if (nRP > 0): PlotSubHistF11("RP", aRP, RP0, dRP, iRP, nRP) |
ulalume3@0 | 1726 | if (nRS > 0): PlotSubHistF11("RS", aRS, RS0, dRS, iRS, nRS) |
ulalume3@0 | 1727 | if (nRetT > 0): PlotSubHistF11("RetT", aRetT, RetT0, dRetT, iRetT, nRetT) |
ulalume3@0 | 1728 | if (nRetR > 0): PlotSubHistF11("RetR", aRetR, RetR0, dRetR, iRetR, nRetR) |
ulalume3@0 | 1729 | if (nERaT > 0): PlotSubHistF11("ERaT", aERaT, ERaT0, dERaT, iERaT, nERaT) |
ulalume3@0 | 1730 | if (nERaR > 0): PlotSubHistF11("ERaR", aERaR, ERaR0, dERaR, iERaR, nERaR) |
ulalume3@0 | 1731 | if (nRotaT > 0): PlotSubHistF11("RotaT", aRotaT, RotaT0, dRotaT, iRotaT, nRotaT) |
ulalume3@0 | 1732 | if (nRotaR > 0): PlotSubHistF11("RotaR", aRotaR, RotaR0, dRotaR, iRotaR, nRotaR) |
ulalume3@0 | 1733 | if (nLDRCal > 0): PlotSubHistF11("LDRCal", aLDRCal, LDRCal0, dLDRCal, iLDRCal, nLDRCal) |
ulalume3@0 | 1734 | |
ulalume3@0 | 1735 | plt.show() |
ulalume3@0 | 1736 | plt.close |
ulalume3@0 | 1737 | ''' |
ulalume3@0 | 1738 | # only histogram |
ulalume3@0 | 1739 | #print("******************* " + aVar + " *******************") |
ulalume3@0 | 1740 | fig, ax = plt.subplots(nrows=5, ncols=2, sharex=True, sharey=True, figsize=(10, 10)) |
ulalume3@0 | 1741 | iLDR = -1 |
ulalume3@0 | 1742 | for LDRTrue in LDRrange: |
ulalume3@0 | 1743 | iLDR = iLDR + 1 |
ulalume3@0 | 1744 | LDRmin[iLDR] = np.min(aA[iLDR,:]) |
ulalume3@0 | 1745 | LDRmax[iLDR] = np.max(aA[iLDR,:]) |
ulalume3@0 | 1746 | Rmin = np.min(aA[iLDR,:]) * 0.999 |
ulalume3@0 | 1747 | Rmax = np.max(aA[iLDR,:]) * 1.001 |
ulalume3@0 | 1748 | plt.subplot(5,2,iLDR+1) |
ulalume3@0 | 1749 | (n, bins, patches) = plt.hist(aA[iLDR,:], |
ulalume3@0 | 1750 | range=[Rmin, Rmax], |
ulalume3@0 | 1751 | bins=200, log=False, alpha=0.2, normed=False, color = '0.5', histtype='stepfilled') |
ulalume3@0 | 1752 | plt.tick_params(axis='both', labelsize=9) |
ulalume3@0 | 1753 | plt.plot([LDRTrue, LDRTrue], [0, np.max(n)], 'r-', lw=2) |
ulalume3@0 | 1754 | plt.show() |
ulalume3@0 | 1755 | plt.close |
ulalume3@0 | 1756 | ''' |
ulalume3@0 | 1757 | |
ulalume3@0 | 1758 | # --- Plot LDRmin, LDRmax |
ulalume3@0 | 1759 | fig2 = plt.figure() |
ulalume3@0 | 1760 | plt.plot(LDRrange,LDRmax-LDRrange, linewidth=2.0, color='b') |
ulalume3@0 | 1761 | plt.plot(LDRrange,LDRmin-LDRrange, linewidth=2.0, color='g') |
ulalume3@0 | 1762 | |
ulalume3@0 | 1763 | plt.xlabel('LDRtrue', fontsize=18) |
ulalume3@0 | 1764 | plt.ylabel('LDRTrue-LDRmin, LDRTrue-LDRmax', fontsize=14) |
ulalume3@0 | 1765 | plt.title(LID + ' ' + str(Type[TypeC]) + ' ' + str(Loc[LocC]), fontsize=18) |
ulalume3@0 | 1766 | #plt.ylimit(-0.07, 0.07) |
ulalume3@0 | 1767 | plt.show() |
ulalume3@0 | 1768 | plt.close |
ulalume3@0 | 1769 | |
ulalume3@0 | 1770 | # --- Save LDRmin, LDRmax to file |
ulalume3@0 | 1771 | # http://stackoverflow.com/questions/4675728/redirect-stdout-to-a-file-in-python |
ulalume3@0 | 1772 | with open('LDR_min_max_ver7_' + LID + '.dat', 'w') as f: |
ulalume3@0 | 1773 | with redirect_stdout(f): |
ulalume3@0 | 1774 | print(LID) |
ulalume3@0 | 1775 | print("LDRtrue, LDRmin, LDRmax") |
ulalume3@0 | 1776 | for i in range(len(LDRrange)): |
ulalume3@0 | 1777 | print("{0:7.4f},{1:7.4f},{2:7.4f}".format(LDRrange[i], LDRmin[i], LDRmax[i])) |
ulalume3@0 | 1778 | |
ulalume3@0 | 1779 | ''' |
ulalume3@0 | 1780 | # --- Plot K over LDRCal |
ulalume3@0 | 1781 | fig3 = plt.figure() |
ulalume3@0 | 1782 | plt.plot(LDRCal0+aLDRCal*dLDRCal/nLDRCal,aX[4,:], linewidth=2.0, color='b') |
ulalume3@0 | 1783 | |
ulalume3@0 | 1784 | plt.xlabel('LDRCal', fontsize=18) |
ulalume3@0 | 1785 | plt.ylabel('K', fontsize=14) |
ulalume3@0 | 1786 | plt.title(LID, fontsize=18) |
ulalume3@0 | 1787 | plt.show() |
ulalume3@0 | 1788 | plt.close |
ulalume3@0 | 1789 | ''' |
ulalume3@0 | 1790 | |
ulalume3@0 | 1791 | # Additional plot routines ======> |
ulalume3@0 | 1792 | ''' |
ulalume3@0 | 1793 | #****************************************************************************** |
ulalume3@0 | 1794 | # 1. Plot LDRcorrected - LDR(measured Icross/Iparallel) |
ulalume3@0 | 1795 | LDRa = np.arange(1.,100.)*0.005 |
ulalume3@0 | 1796 | LDRCorra = np.arange(1.,100.) |
ulalume3@0 | 1797 | if Y == - 1.: LDRa = 1./LDRa |
ulalume3@0 | 1798 | LDRCorra = (1./Eta*LDRa*(GT+HT)-(GR+HR))/((GR-HR)-1./Eta*LDRa*(GT-HT)) |
ulalume3@0 | 1799 | if Y == - 1.: LDRa = 1./LDRa |
ulalume3@0 | 1800 | # |
ulalume3@0 | 1801 | #fig = plt.figure() |
ulalume3@0 | 1802 | plt.plot(LDRa,LDRCorra-LDRa) |
ulalume3@0 | 1803 | plt.plot([0.,0.5],[0.,0.5]) |
ulalume3@0 | 1804 | plt.suptitle('LDRcorrected - LDR(measured Icross/Iparallel)', fontsize=16) |
ulalume3@0 | 1805 | plt.xlabel('LDR', fontsize=18) |
ulalume3@0 | 1806 | plt.ylabel('LDRCorr - LDR', fontsize=16) |
ulalume3@0 | 1807 | #plt.savefig('test.png') |
ulalume3@0 | 1808 | # |
ulalume3@0 | 1809 | ''' |
ulalume3@0 | 1810 | ''' |
ulalume3@0 | 1811 | #****************************************************************************** |
ulalume3@0 | 1812 | # 2. Plot LDRsim (simulated measurements without corrections = Icross/Iparallel) over LDRtrue |
ulalume3@0 | 1813 | LDRa = np.arange(1.,100.)*0.005 |
ulalume3@0 | 1814 | LDRsima = np.arange(1.,100.) |
ulalume3@0 | 1815 | |
ulalume3@0 | 1816 | atruea = (1.-LDRa)/(1+LDRa) |
ulalume3@0 | 1817 | Ita = TiT*TiO*IinL*(GT+atruea*HT) |
ulalume3@0 | 1818 | Ira = TiR*TiO*IinL*(GR+atruea*HR) |
ulalume3@0 | 1819 | LDRsima = Ira/Ita # simulated uncorrected LDR with Y from input file |
ulalume3@0 | 1820 | if Y == -1.: LDRsima = 1./LDRsima |
ulalume3@0 | 1821 | # |
ulalume3@0 | 1822 | #fig = plt.figure() |
ulalume3@0 | 1823 | plt.plot(LDRa,LDRsima) |
ulalume3@0 | 1824 | plt.plot([0.,0.5],[0.,0.5]) |
ulalume3@0 | 1825 | plt.suptitle('LDRsim (simulated measurements without corrections = Icross/Iparallel) over LDRtrue', fontsize=10) |
ulalume3@0 | 1826 | plt.xlabel('LDRtrue', fontsize=18) |
ulalume3@0 | 1827 | plt.ylabel('LDRsim', fontsize=16) |
ulalume3@0 | 1828 | #plt.savefig('test.png') |
ulalume3@0 | 1829 | # |
ulalume3@0 | 1830 | ''' |