2020
DOI: 10.3390/rs12111878
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Comparison of the Lunar Models Using the Hyper-Spectral Imager Observations in Lijiang, China

Abstract: A lunar observation campaign was conducted using a hyper-spectral imaging spectrometer in Lijiang, China from December 2015 to February 2016. The lunar hyper-spectral images in the visible to near-infrared region (VNIR) have been obtained in different lunar phases with absolute scale established by the National Institute of Metrology (NIM), China using the lamp–plate calibration system. At the same time, the aerosol optical depth (AOD) is measured regularly by a lidar and a lunar CE318U for atmospheric charact… Show more

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Cited by 7 publications
(7 citation statements)
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“…Total lunar spectral irradiance for a given set of illumination and viewing angles and distances can be modeled empirically based on prior lunar irradiance characterization as a function of geometry. Such a lunar spectral-irradiance model (Kieffer and Stone, 2005) has been in common use for nearly two decades, and improved models are an active research area (Stone et al, 2020;Taylor et al, 2021;Wang et al, 2020;Sun and Xiong, 2021;Kieffer, 2021a;Kieffer, 2022) Lunar irradiance is polarized (Dollfus,1962), up to several percent at common calibration geometries, passing through zero at phase angles near 24°. Polarization has been largely ignored in lunar calibration to date, but modern measurements (see http://calvalportal.ceos.org/lime-documents) are being made after nearly a century gap.…”
Section: The Moonmentioning
confidence: 99%
“…Total lunar spectral irradiance for a given set of illumination and viewing angles and distances can be modeled empirically based on prior lunar irradiance characterization as a function of geometry. Such a lunar spectral-irradiance model (Kieffer and Stone, 2005) has been in common use for nearly two decades, and improved models are an active research area (Stone et al, 2020;Taylor et al, 2021;Wang et al, 2020;Sun and Xiong, 2021;Kieffer, 2021a;Kieffer, 2022) Lunar irradiance is polarized (Dollfus,1962), up to several percent at common calibration geometries, passing through zero at phase angles near 24°. Polarization has been largely ignored in lunar calibration to date, but modern measurements (see http://calvalportal.ceos.org/lime-documents) are being made after nearly a century gap.…”
Section: The Moonmentioning
confidence: 99%
“…For instance, the Sea-viewing Wide Field-of-view Sensor (SeaWiFS) mission used the Moon exclusively to perform a time-dependent calibration in orbit to within 0.2% uncertainty (Eplee et al, 2006). Improved lunar models are an active research area (Kieffer, 2021a(Kieffer, , 2022Stone et al, 2020;Sun & Xiong, 2021;Taylor et al, 2021;Y. Wang et al, 2020).…”
Section: The Moonmentioning
confidence: 99%
“…For instance, the Sea‐viewing Wide Field‐of‐view Sensor (SeaWiFS) mission used the Moon exclusively to perform a time‐dependent calibration in orbit to within 0.2% uncertainty (Eplee et al., 2006). Improved lunar models are an active research area (Kieffer, 2021a, 2022; Stone et al., 2020; Sun & Xiong, 2021; Taylor et al., 2021; Y. Wang et al., 2020). Lunar irradiance is polarized (Dollfus, 1962), up to several percent at common calibration geometries, passing through zero at phase angles near 24°.…”
Section: Calibration and Monitoringmentioning
confidence: 99%
“…Moreover, the measurements showed a stronger linear relationship between the spectral irradiance ratio and wavelength for the different lunar phases, as did the model, which is related to an effect called phase reddening. The results on phase angle and spectral agreement are available in [160]. The instrument remains operational and accumulated data are being analyzed currently, while its successor is undergoing extensive testing and expects to provide a level of automation well above the GLIS.…”
Section: Lijing Projectmentioning
confidence: 99%