2019
DOI: 10.1016/j.jqsrt.2019.03.007
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Calibration model of polarimeters on board the Aerosol-UA space mission

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Cited by 14 publications
(20 citation statements)
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“…Over the past few decades, satellite remote sensing techniques have developed rapidly and extensively, and various (primarily photometric) instruments have been developed and deployed to monitor atmospheric aerosols from space (Bréon et al, 2011;Dubovik et al, 2019;King et al, 1999;Kokhanovsky et al, 2015;Li et al, 2009;Tanré et al, 2011). While the design and capabilities of the photometric observations are constantly evolving, the greatest improvement has been in the form of multi-angular multi-spectral polarimetry (MAP) measurements (Hansen et al, 1995;Hasekamp and Landgraf, 2007;Knobelspiesse et al, 2012;Mishchenko and Travis, 1997;Mishchenko et al, 2004;Waquet et al, 2009;Tanré et al, 2011). MAP measurements have enough inherent information content to greatly improve our understanding about aerosol properties.…”
Section: Introductionmentioning
confidence: 99%
“…Over the past few decades, satellite remote sensing techniques have developed rapidly and extensively, and various (primarily photometric) instruments have been developed and deployed to monitor atmospheric aerosols from space (Bréon et al, 2011;Dubovik et al, 2019;King et al, 1999;Kokhanovsky et al, 2015;Li et al, 2009;Tanré et al, 2011). While the design and capabilities of the photometric observations are constantly evolving, the greatest improvement has been in the form of multi-angular multi-spectral polarimetry (MAP) measurements (Hansen et al, 1995;Hasekamp and Landgraf, 2007;Knobelspiesse et al, 2012;Mishchenko and Travis, 1997;Mishchenko et al, 2004;Waquet et al, 2009;Tanré et al, 2011). MAP measurements have enough inherent information content to greatly improve our understanding about aerosol properties.…”
Section: Introductionmentioning
confidence: 99%
“…e spectral characteristics of the individual dichroic mirrors and spectral filters and the resulting characteristics for spectral channels 865 nm, 1378 nm, and 1620 nm of the optical units IR are shown in Figure 4. Note that the individual spectral transmittance values of the VIS and IR optical units will be taken into account in the calibration procedure described in detail in [14].…”
Section: Spectral Selection Systemmentioning
confidence: 99%
“…At this stage, we have not considered the following: the probable difference in the transmission coefficients of the different optical paths of ScanPol, the finite polarization contrast (extinction ratio) of polarizing prisms, the possible optical anisotropy of the camera lenses, and the other imperfections in the optical characteristics of the PSA ScanPol, which can also significantly affect the field parameters. [14,[16][17][18]. Because the mount and determination of the orientation of the polarizing axes of the Wollaston prisms are the simplest operations in the PSA ScanPol, it makes sense to investigate separately their effect on the accuracy of measuring the polarization parameters of the light flux.…”
Section: Mount Of Wollaston Prisms and Requirements To Eirmentioning
confidence: 99%
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