Author Affiliations
1School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China2National Satellite Meteorological Center, China Meteorological Administration, Beijing 100081, China3Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, China Meteorological Administration, Beijing 100081, China4Shanghai Institute of Technology Physics, Chinese Academy of Sciences, Shanghai 200083, Chinashow less
Fig. 1. Focal plane of MERSI-II
Fig. 2. Polar island images of earth observed by MERSI-II with equalization enhancement (2019-07-18). (a) Band 20; (b) band 21
Fig. 3. Fire point target images of earth observed by MERSI-II with Gaussian enhancement (2019-03-18). (a) Band 20; (b) band 21
Fig. 4. Polar island images of earth observed by MERSI-II with Gaussian enhancement (2019-07-18). (a) Band 6; (b) band 7
Fig. 5. Lunar images obtained by single-detector multi-frame scanning in short-wave infrared focal plane (2017-12-26). (a) Band 5 detector 5; (b) band 6 detector 5
Fig. 6. Lunar images obtained by single-detector multi-frame scanning in mid and long wave infrared focal plane (2017-12-26). (a) Band 21 detector 5; (b) band 23 detector 5
Fig. 7. Schematic of crosstalk from bands in mid and long wave infrared focal plane. (a) Lunar pseudo-color image of band 20 detector 5; (b) schematic of the lunar arrangement of each band
Fig. 8. Lunar images of band 20 before and after crosstalk correction (2017-12-26). (a) Without correction; (b) with correction
Fig. 9. Lunar image of band 20 before and after crosstalk correction (2018-01-25). (a) Without correction; (b) with correction
Fig. 10. Earth images of band 20 before and after crosstalk correction (2018-01-29). (a) Without correction; (b) with correction
Wavelength range | Band | Wavelength /μm | Source of crosstalk | Crosstalk proportion |
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| 1 | 0.470 | No | | Visible (VIS) | 2 | 0.550 | No | | | 3 | 0.650 | No | | | 4 | 0.865 | No | | | 5 | 1.380 | From detectors | 25%--40% | Short-wave infrared (SWIR) | 6 | 1.640 | From detectors | 7%--20% | | 7 | 2.130 | No | | | 8 (det1) | 0.412 | From detectors | 3%--4% | | 9 | 0.443 | No | | | 10 | 0.490 | No | | | 11 | 0.555 | No | | | 12 | 0.670 | No | | | 13 | 0.709 | No | | Visible and near-infrared (VNIR) | 14 | 0.746 | No | | | 15 | 0.865 | No | | | 16 | 0.905 | No | | | 17 | 0.936 | No | | | 18 | 0.940 | No | | | 19 | 1.030 | No | | | 20 | 3.800 | From bands | 1.3%--3% | Mid and long wave infrared (MLWIR) | 21 | 4.050 | From bands | 1.2%--1.7% | | 22 | 7.200 | From bands | Saturation | | 23 | 8.550 | From bands | 3.5%--5% | Long-wave infrared (LWIR) | 24 | 10.800 | From bands | 1.5%--2.5% | | 25 | 12.000 | From bands | 0%--1% |
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Table 1. Crosstalk detection results of all bands of MERSI-II
Detector | Band 21 | Band 23 | Band 22 |
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Det1 | 0.00105634 | 1.22514515×10-3 | 0.00086126 | Det2 | 0.00544265 | 3.43000244×10-4 | 0.00128618 | Det3 | 0.00217129 | 1.09546923×10-3 | 0.00149434 | Det4 | 0.00365741 | 6.22984547×10-5 | 0.00100561 | Det5 | -0.00042805 | 5.82319004×10-4 | 0.00124892 | Det6 | 0.02883502 | 2.74452948×10-4 | 0.00197744 | Det7 | 0.00882859 | 1.02648869×10-3 | 0.00065176 | Det8 | 0.00263379 | 7.59549995×10-4 | 0.00150834 | Det9 | 0.00177946 | 6.57615186×10-4 | 0.00068722 | Det10 | 0.00385918 | 1.03962834×10-3 | 0.00109455 |
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Table 2. Crosstalk coefficient summary of band 20 detector 5 (2017-12-26)