docs/lidar_retrievals/lidar_retrievals.rst

Thu, 17 Jun 2021 14:09:17 +0200

author
Giuseppe D'Amico <giuseppe.damico@imaa.cnr.it>
date
Thu, 17 Jun 2021 14:09:17 +0200
changeset 128
6757f7d0af2a
parent 125
003aa42747f5
permissions
-rw-r--r--

Updated documetation: new options for Molecular_Calc have been described

giuseppe@125 1 1. Algorithm Theoretical Basis
giuseppe@125 2 ==============================
giuseppe@125 3
giuseppe@125 4
giuseppe@125 5 The European Aerosol Research Lidar Network, EARLINET, was founded in 2000 as a research
giuseppe@125 6 project for establishing a quantitative, comprehensive, and statistically significant database for the
giuseppe@125 7 horizontal, vertical, and temporal distribution of aerosols on a continental scale.
giuseppe@125 8
giuseppe@125 9 ACTRIS/EARLINET stations are typically able to retrieve aerosol optical properties, such as extinction and backscatter coefficients,
giuseppe@125 10 lidar ratio, optical depth, and the Angstrom exponent if Raman lidar signals are available. In cases when only elastic lidar signals are used,
giuseppe@125 11 backscatter and a backscatter-related Angstrom exponent are derived.
giuseppe@125 12
giuseppe@125 13 The calculation of all these quantities is done after the cloud masking procedure and it is therefore attributed exclusively to aerosol particles.
giuseppe@125 14
giuseppe@125 15
giuseppe@125 16 1.1 Physical meaning of the retrieved properties
giuseppe@125 17 ------------------------------------------------
giuseppe@125 18
giuseppe@125 19
giuseppe@125 20 When laser radiation with power :math:`P_L` at wavelength :math:`\lambda_L` is sent into the atmosphere, part of the radiation is backscattered.
giuseppe@125 21 The optical power :math:`P(\lambda,\lambda_L,z)` of the backscattered radiation received from the distance :math:`z` at wavelength :math:`\lambda` depends
giuseppe@125 22 on atmospheric composition through two parameters: the backscattering coefficient and the extinction coefficient, and is described by the lidar equation:
giuseppe@125 23
giuseppe@125 24 .. math::
giuseppe@125 25 P(\lambda,\lambda_L,z) \sim \frac{P_L}{z^2}\beta(\lambda,\lambda_L,z) \exp \left[-\int_0^z \alpha(\lambda,\xi) d\xi \right] \exp \left[ -\int_0^z \alpha(\lambda_L,\xi) d\xi \right]
giuseppe@125 26 :label: eq_lidar
giuseppe@125 27
giuseppe@125 28 The backscattering coefficient :math:`\beta` is the fraction of incident radiation backscattered for unitary solid angle and for unitary length [m-1sr-1].
giuseppe@125 29 It depends on the kind of scattering process and on both emission (:math:`\lambda_L`) and detection (:math:`\lambda`) wavelength.
giuseppe@125 30
giuseppe@125 31 It is due to contributions of both molecules (m) and particles (p) of atmosphere:
giuseppe@125 32
giuseppe@125 33 .. math::
giuseppe@125 34 \beta(\lambda,\lambda_L,z)= \beta_m(\lambda,\lambda_L,z)+\beta_p(\lambda,\lambda_L,z)
giuseppe@125 35 :label: eq_beta
giuseppe@125 36
giuseppe@125 37 The extinction coefficient is defined as the energy flux reduction per unitary path [m-1].
giuseppe@125 38
giuseppe@125 39 It gives a measurement of the energy loss of the laser beam in the atmosphere.
giuseppe@125 40
giuseppe@125 41 It is due to contributions of both molecules (m) and particles (p) of atmosphere deriving from both the scattering (s) and absorption (a) processes:
giuseppe@125 42
giuseppe@125 43 .. math::
giuseppe@125 44 \alpha(\lambda,z)=\alpha_{m,a}(\lambda,z)+\alpha_{m,s}(\lambda,z) + \alpha_{p,a}(\lambda,z)+\alpha_{p,s}(\lambda,z)
giuseppe@125 45 :label: eq_alpha
giuseppe@125 46
giuseppe@125 47 The extinction coefficient integrated over a spatial path provides the optical depth:
giuseppe@125 48
giuseppe@125 49 .. math::
giuseppe@125 50 \tau(\lambda,z)=\int_0^z \alpha(\lambda,\xi)d\xi
giuseppe@125 51 :label: eq_tau
giuseppe@125 52
giuseppe@125 53 The Raman configuration allows for the retrieval of the range-resolved particle lidar ratio. The lidar ratio is defined as the ration between the
giuseppe@125 54 particle extinction coefficient and the particle backscatter coefficient:
giuseppe@125 55
giuseppe@125 56 .. math::
giuseppe@125 57 S(\lambda,z)=\frac{\alpha(\lambda,z)}{\beta(\lambda,z)}
giuseppe@125 58 :label: eq_lr
giuseppe@125 59
giuseppe@125 60 It is a parameter strongly related to the microphysical properties of the aerosols: shape, size distribution, chemical composition,
giuseppe@125 61 relative humidity. Unlike :math:`\alpha` and :math:`\beta`, :math:`S` doesn’t depend on atmospheric aerosol load, but only on aerosol type.
giuseppe@125 62
giuseppe@125 63 The combination of the particle extinction at different wavelengths allows for the calculation of the Angstrom exponent:
giuseppe@125 64
giuseppe@125 65 .. math::
giuseppe@125 66 k_{\alpha}(\lambda_1,\lambda_2,z)=\frac{\ln \left[ \frac{\alpha(\lambda_1,z)}{\alpha(\lambda_2,z)} \right] }{\ln \left[ \frac{\lambda_2}{\lambda_1} \right]}
giuseppe@125 67 :label: eq_kalpha
giuseppe@125 68
giuseppe@125 69 This quantity is size dependent assuming larger values for smaller particles and ranges between -1 for very big particles and 4 for molecules.
giuseppe@125 70
giuseppe@125 71 Similarly to the Angstrom exponent, the backscatter related Angstrom exponent can be calculated as:
giuseppe@125 72
giuseppe@125 73 .. math::
giuseppe@125 74 k_{\beta}(\lambda_1,\lambda_2,z)=\frac{\ln \left[ \frac{\beta(\lambda_1,z)}{\beta(\lambda_2,z)} \right] }{\ln \left[ \frac{\lambda_2}{\lambda_1} \right]}
giuseppe@125 75 :label: eq_kbeta
giuseppe@125 76
giuseppe@125 77 As for the Angstrom exponent this quantity is size dependent assuming larger values for smaller particles. However, it has to be noted that it is
giuseppe@125 78 even more sensitive than Angstrom exponent to the size of the particles, because the backscatter itself is more size-related than the extinction coefficient.
giuseppe@125 79
giuseppe@125 80
giuseppe@125 81
giuseppe@125 82
giuseppe@125 83 1.2 Basic concepts for the retrieval of aerosol optical properties
giuseppe@125 84 ------------------------------------------------------------------
giuseppe@125 85
giuseppe@125 86
giuseppe@125 87 ACTRIS/EARLINET is mainly based on Raman lidar stations, i.e. lidars equipped with elastic channel (detection channel at the same wavelength of transmitted laser beam) and an additional channel for detecting the N2 Raman-shifted signal. This additional channel allows the direct measurement of the aerosol extinction (Ansmann et al., 1990). This means having the capability of independent retrieval of extinction and backscatter coefficient in good signal-to-noise ratio conditions, using the retrieved extinction in the elastic lidar equation reported above. Whenever this is not possible an assumption about the relationship between extinction and backscatter is needed for solving the lidar equation affecting the overall uncertainty of the aerosol backscatter coefficient. Within ACTRIS/EARLINET, aerosol extinction profiles are reported only when the Raman channel capability is used and therefore only with direct assessed measurement of the extinction coefficient profile.
giuseppe@125 88
giuseppe@125 89 Solving the N2 Raman lidar equation involves a derivative respect to the range of the logarithm of the signal. This procedure is complex from mathematical point of view and needs for specific smoothing approaches. Within EARLINET many efforts have been done for comparing the different suitable procedures (Pappalardo et al., 2004): the linear fit has been identified as the most appropriate one. Two options are available the weighted and not weighted linear fit.
giuseppe@125 90
giuseppe@125 91 For what concerns the aerosol backscatter coefficient profiles, the SCC can provide aerosol products in a flexible way choosing from a set of possible pre-defined analysis procedures: it enables the retrieval of particle backscatter coefficients with the elastic technique by using both the Klett method (Klett, 1981; Fernald, 1984) and the iterative algorithm (Di Girolamo et al., 1995), but also the computation of particle backscatter coefficient profiles after the Raman method (Ansmann et al., 1992).
giuseppe@125 92
giuseppe@125 93 Statistical errors are calculated starting from the statistical errors affecting the lidar detected signals: the statistical errors affecting the optical properties can be calculated using the Monte Carlo or error propagation law. The provided errors do not include the uncertainties related to the assumption made in the retrieval algorithms like: the uncertainty to the atmospheric molecular profile, the wavelength dependence of the extinction, the absence of aerosol in the backscatter calibration range and more relevant the lidar ratio values assumption in the elastic backscatter method and the calibration of the depolarization channels. The quantification of the resulting overall error is still under investigation and object of studies within ACTRIS/EARLINET. The current approach is to reduce as much as possible such errors improving the quality assurance procedures together with the calibration centre and selecting the best possible approaches (e.g. intensifying the scheduling of the depolarization calibration procedures).

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