Polarization Science and Remote Sensing IX 2019
DOI: 10.1117/12.2530729
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Expected performance and error analysis for SPEXone, a multi-angle channeled spectropolarimeter for the NASA PACE mission

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Cited by 17 publications
(18 citation statements)
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“…The retrieval algorithm minimizes the difference between the MAP measurements and the forward model simulations computed from vector radiative transfer simulations (Zhai et al, 2009(Zhai et al, , 2010. By assuming the measurement and modeling uncertainties follow Gaussian statistical distributions, the retrieval parameters can be estimated through Bayesian theory using the cost function χ 2 to quantify the difference between the measurement and the forward model simulation (Rogers, 2000):…”
Section: Joint Aerosol and Ocean Color Retrieval Algorithmmentioning
confidence: 99%
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“…The retrieval algorithm minimizes the difference between the MAP measurements and the forward model simulations computed from vector radiative transfer simulations (Zhai et al, 2009(Zhai et al, , 2010. By assuming the measurement and modeling uncertainties follow Gaussian statistical distributions, the retrieval parameters can be estimated through Bayesian theory using the cost function χ 2 to quantify the difference between the measurement and the forward model simulation (Rogers, 2000):…”
Section: Joint Aerosol and Ocean Color Retrieval Algorithmmentioning
confidence: 99%
“…OCI will provide continuous spectral measurements from the ultraviolet (340 nm) to near-infrared (890 nm) with full width at half maximum of 5 nm resolution and sampling every 2.5 nm, plus a set of seven discrete shortwave infrared (SWIR) bands centered at 940, 1038, 1250, 1378, 1615, 2130, and 2260 nm. SPEXone performs multi-angle measurements at five along-track viewing angles of 0 • , ±20 • , and ±58 • , with a surface swath of 100 km and a continuous spectral range spanning 385-770 nm at resolutions of 2-3 nm for intensity and 10-40 nm for polarization (Rietjens et al, 2019). HARP2 is a wide field-of-view imager that measures the polarized radiances at 440, 550, 670, and 870 nm, where the 670 nm band will measure 60 viewing angles and the other bands 10 viewing angles, with a swath of 1556 km at nadir on the Earth's surface.…”
mentioning
confidence: 99%
“…OCI will provide continuous spectral measurements from the ultraviolet (340 nm) to near-infrared (890 nm) with Full Width Half Maximum of 5 nm resolution and sampling every 2.5 nm, plus a set of seven discrete shortwave infrared (SWIR) bands centered at 940, 1038, 1250, 1378, 1615, 2130, and 2260 nm. SPEXone performs multiangle measurements at 5 along track viewing angles of 0 • , ±20 • and ±58 • , with a surface swath of 100km, and a continuous spectral range spanning 385-770 nm at resolutions of 2-3 nm for intensity and 10-40 nm for polarization (Rietjens et al, 2019). HARP2 is a wide field-of-view imager that measures the polarized radiances at 440, 550, 670, and 870 nm, 2 https://doi.org/10.5194/amt-2020-507 Preprint.…”
Section: Introductionmentioning
confidence: 99%
“…HARP2 is a wide field-of-view imager that measures polarized radiances at 440, 550, 670, and 865 nm, where the 670 nm band will be at 60 viewing angles and the other bands at 10 viewing angles. SPEXone is a narrow swath imager that performs multi-angle measurements at 5 viewing angles of 0 • , ±20 • and ±58 • on ground, in a continuous spectral range spanning 385-770 nm with a resolution of 2-3 nm for intensity, and 10-40nm for polarization (Rietjens et al, 2019).…”
Section: Introductionmentioning
confidence: 99%