• Acta Optica Sinica
  • Vol. 39, Issue 11, 1130003 (2019)
Tianhang Yang1、2、3, Xiuqing Hu4、*, Hanlie Xu4, Chunqiang Wu4, Chengli Qi4, and Mingjian Gu1、3
Author Affiliations
  • 1Key Laboratory of Infrared System Detection and Imaging Technology, Chinese Academy of Sciences, Shanghai 200083, China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • 3Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China
  • 4Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, National Satellite Meteorological Center, Beijing 100081, China
  • show less
    DOI: 10.3788/AOS201939.1130003 Cite this Article Set citation alerts
    Tianhang Yang, Xiuqing Hu, Hanlie Xu, Chunqiang Wu, Chengli Qi, Mingjian Gu. Radiation Calibration Accuracy Assessment of FY-3D Hyperspectral Infrared Atmospheric Sounder Based on Inter-Comparison[J]. Acta Optica Sinica, 2019, 39(11): 1130003 Copy Citation Text show less
    Inter-comparison processes of HIRAS and IASI
    Fig. 1. Inter-comparison processes of HIRAS and IASI
    Long-term latitude distributions of SNO events of HIRAS-IASI/A and HIRAS-IASI/B. (a) Latitude distribution of SNO events of HIRAS-IASI/A and HIRAS-IASI/B from April to December, 2018; (b) latitude distribution of SNO events of HIRAS-IASI/A during 10-12 June, 2018
    Fig. 2. Long-term latitude distributions of SNO events of HIRAS-IASI/A and HIRAS-IASI/B. (a) Latitude distribution of SNO events of HIRAS-IASI/A and HIRAS-IASI/B from April to December, 2018; (b) latitude distribution of SNO events of HIRAS-IASI/A during 10-12 June, 2018
    Pixel overlap rate of HIRAS-IASI versus pixel distance between HIRAS and IASI (nadir)
    Fig. 3. Pixel overlap rate of HIRAS-IASI versus pixel distance between HIRAS and IASI (nadir)
    Pixel matching of MERSI-II and HIRAS-IASI
    Fig. 4. Pixel matching of MERSI-II and HIRAS-IASI
    BT difference at 900 cm-1 between HIRAS and IASI/A versus ratio of standard deviation to mean of MERSI-II in channel 24 (ratio is below 0.01). The mean of HIRAS-IASI/A BT difference is 0.106 K and the standard deviation of BT difference is 0.485 K
    Fig. 5. BT difference at 900 cm-1 between HIRAS and IASI/A versus ratio of standard deviation to mean of MERSI-II in channel 24 (ratio is below 0.01). The mean of HIRAS-IASI/A BT difference is 0.106 K and the standard deviation of BT difference is 0.485 K
    Matching of HIRAS-IASI spectra. (a) HIRAS (solid line) and IASI (dash line) spectra simulated by LBLRTM for standard atmospheric profile; (b) BT difference between IASIH and HIRAS
    Fig. 6. Matching of HIRAS-IASI spectra. (a) HIRAS (solid line) and IASI (dash line) spectra simulated by LBLRTM for standard atmospheric profile; (b) BT difference between IASIH and HIRAS
    Spatial distributions of matching samples of HIRAS-IASI/A and HIRAS-IASI/B
    Fig. 7. Spatial distributions of matching samples of HIRAS-IASI/A and HIRAS-IASI/B
    Spectral distribution, mean deviation of BT, and standard deviation of BT difference for HIRAS-IASI/A and HIRAS-IASI/B(North and South Arctic regions). (a) HIRAS spectral distributions for HIRAS-IASI/A and HIRAS-IASI/B, the solid line represents the mean of BT(dark); (b) BT mean deviation of HIRAS-IASI/A and HIRAS-IASI/B; (c) standard deviation of BT differences of HIRAS-IASI/A and HIRAS-IASI/B
    Fig. 8. Spectral distribution, mean deviation of BT, and standard deviation of BT difference for HIRAS-IASI/A and HIRAS-IASI/B(North and South Arctic regions). (a) HIRAS spectral distributions for HIRAS-IASI/A and HIRAS-IASI/B, the solid line represents the mean of BT(dark); (b) BT mean deviation of HIRAS-IASI/A and HIRAS-IASI/B; (c) standard deviation of BT differences of HIRAS-IASI/A and HIRAS-IASI/B
    Mean deviation of BT for HIRAS-IASI/A and HIRAS-IASI/B versus mean of HIRAS BT. (a)(b) LWIR; (c)(d) MWIR; (e)(f) SWIR
    Fig. 9. Mean deviation of BT for HIRAS-IASI/A and HIRAS-IASI/B versus mean of HIRAS BT. (a)(b) LWIR; (c)(d) MWIR; (e)(f) SWIR
    Scatter plots of HIRAS-IASI/A BT differences versus HIRAS BT. (a) 678.125 cm-1; (b) 900.0 cm-1; (c) 1500.0 cm-1; (b) 2157.5 cm-1
    Fig. 10. Scatter plots of HIRAS-IASI/A BT differences versus HIRAS BT. (a) 678.125 cm-1; (b) 900.0 cm-1; (c) 1500.0 cm-1; (b) 2157.5 cm-1
    Scatter plots of HIRAS-IASI/B BT differences versus HIRAS BT. (a) 678.125 cm-1; (b) 900.0 cm-1; (c) 1500.0 cm-1; (b) 2157.5 cm-1
    Fig. 11. Scatter plots of HIRAS-IASI/B BT differences versus HIRAS BT. (a) 678.125 cm-1; (b) 900.0 cm-1; (c) 1500.0 cm-1; (b) 2157.5 cm-1
    Long-term sequences of BT differences of HIRAS-IASI/A in LWIR. (a) 750.00 cm-1; (b) 800.00 cm-1; (c) 950.00 cm-1
    Fig. 12. Long-term sequences of BT differences of HIRAS-IASI/A in LWIR. (a) 750.00 cm-1; (b) 800.00 cm-1; (c) 950.00 cm-1
    Long-term sequences of BT differences of HIRAS-IASI/A in MWIR. (a) 1300.00 cm-1; (b) 1500.00 cm-1; (c) 1700.00 cm-1
    Fig. 13. Long-term sequences of BT differences of HIRAS-IASI/A in MWIR. (a) 1300.00 cm-1; (b) 1500.00 cm-1; (c) 1700.00 cm-1
    Long-term sequences of BT differences of HIRAS-IASI/A in SWIR. (a) 2200.00 cm-1; (b) 2400.00 cm-1; (c) 2500.00 cm-1
    Fig. 14. Long-term sequences of BT differences of HIRAS-IASI/A in SWIR. (a) 2200.00 cm-1; (b) 2400.00 cm-1; (c) 2500.00 cm-1
    Instrument parameter characteristicHIRASIASI
    Satellite platformFY-3DMetOp-AMetOp-B
    Launch date2017-11-152006-10-192012-09-17
    Orbit height /km830.5817.0
    Local equatorial13:4009:30
    Spatial resolution(nadir) /km16.012.0
    Scan cycle /s108
    Detector array2×22×2
    Maximum optical path difference/cm0.82
    Spectral sampling resolution /cm-10.6250.25
    Apodized spectral resolution /cm-11.13750.5
    Number of channels2287 (non-apodized)2275(apodized)8461(apodized)
    Spectral coverage /μm15.38-8.80(LWIR)8.26-5.70(MWIR)4.64-3.92(SWIR)15.5-8.26(LWIR)8.26-5.00(MWIR)5.00-3.62(SWIR)
    Table 1. Instrument parameter characteristics of HIRAS and IASI
    ConditionCriteria
    FOV distance /km≤7
    Time difference /min≤10
    View angle difference|cos Zen1/cos Zen2|≤0.01
    FOV homogeneitySTDE/MEANE<0.01|MEANT-MEANE|<k·STDE
    Table 2. Matching criteria for SNOs of HIRAS-IASI
    Tianhang Yang, Xiuqing Hu, Hanlie Xu, Chunqiang Wu, Chengli Qi, Mingjian Gu. Radiation Calibration Accuracy Assessment of FY-3D Hyperspectral Infrared Atmospheric Sounder Based on Inter-Comparison[J]. Acta Optica Sinica, 2019, 39(11): 1130003
    Download Citation