2020
DOI: 10.1109/tgrs.2019.2959830
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FY-3D HIRAS Radiometric Calibration and Accuracy Assessment

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Cited by 27 publications
(15 citation statements)
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“…A curious point to note here is that one of the few channels to improve (down by −3%) is AMSU‐A channel 14, the highest temperature peaking channel, that suffers the largest degradation in the MO54R907 and NOAA54R812 experiments. It is not clear at this stage what is the reason for the global system degradation and further investigations will be conducted, although it may be related to unresolved calibration issues affecting the detector nonlinearity correction and polarization parameters (Wu et al ., 2020).…”
Section: Resultsmentioning
confidence: 99%
“…A curious point to note here is that one of the few channels to improve (down by −3%) is AMSU‐A channel 14, the highest temperature peaking channel, that suffers the largest degradation in the MO54R907 and NOAA54R812 experiments. It is not clear at this stage what is the reason for the global system degradation and further investigations will be conducted, although it may be related to unresolved calibration issues affecting the detector nonlinearity correction and polarization parameters (Wu et al ., 2020).…”
Section: Resultsmentioning
confidence: 99%
“…FengYun-3 is a Chinese second-generation sun-synchronous meteorological satellite [28]. HIRAS is the first infrared Fourier detection instrument carried on Fengyun-3D [29]. The main goal is to observe the infrared radiation emitted by the Earth-Atmosphere system with high spectral resolution in the 0.38-15.38 µm spectral range.…”
Section: Data 211 Satellite Datamentioning
confidence: 99%
“…Ideally, the FTS measurement is linearly proportional to the incident spectral radiance. However, according to the instrumentation study and data analysis of some existing remote sensing IR FTS, such as MetOp/IASI [8], SNPP/CrIS [9], FY-3D/HIRAS [10], the signal chain nonlinearity is expected to be one dominant source of uncertainty associated with the measured spectra [11][12]. Generally, the measurement directly recorded on a FTS detector is called interferogram, which is converted by the inverse Fourier transform of the incident light spectrum.…”
Section: Introductionmentioning
confidence: 99%