Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands
Abstract Since its launch on September 6, 2008, HJ-1A has been in the orbit for 13 years. The CCD1 sensor on the HJ-1A has four reflected solar bands. Since the calibration frequency is limited to the annual site calibration, cross-calibration is an effective method to improve the calibration freque...
Main Authors: | , , , , , |
---|---|
Format: | Article |
Language: | English |
Published: |
Nature Publishing Group
2021-04-01
|
Series: | Scientific Reports |
Online Access: | https://doi.org/10.1038/s41598-021-86619-y |
id |
doaj-bef237b54af84577bb92e2366d3f4024 |
---|---|
record_format |
Article |
spelling |
doaj-bef237b54af84577bb92e2366d3f40242021-04-04T11:32:07ZengNature Publishing GroupScientific Reports2045-23222021-04-0111111410.1038/s41598-021-86619-yLong-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bandsLi Liu0Tingting Shi1Hailiang Gao2Xuewen Zhang3Qijin Han4Xinkai Hu5China Center for REsources Satellite Data and Application (CRESDA)National Resource Center for Chinese Materia Medical, China Academy of Chinese Medical SciencesAerospace Information Research Institute, Chinese Academy of SciencesChina Center for REsources Satellite Data and Application (CRESDA)China Center for REsources Satellite Data and Application (CRESDA)College of Surveying and Mapping Engineering, Guilin University of TechnologyAbstract Since its launch on September 6, 2008, HJ-1A has been in the orbit for 13 years. The CCD1 sensor on the HJ-1A has four reflected solar bands. Since the calibration frequency is limited to the annual site calibration, cross-calibration is an effective method to improve the calibration frequency. In this paper, we use 420 image pairs of HJ-1A CCD1 and Terra MODIS over the Dunhuang test site for gains calculation, where we take MODIS as the reference sensor. The spectral band adjustment factors (SBAFs) for cross-calibration are then calculated to compensate for the spectral mismatch. The cross-calibration results are also validated by the field calibration results. From 2008 to 2019, a total of six campaigns have been cross-calibrated on the same day. The gain difference between the site calibration and cross-calibration is less than 3%. The long-term cross-calibration results further indicate that due to the adjustment of HJ-1A CCD gain state in October 2009, an abrupt change occurred 405 days after launch. After 12 years of on-orbit operation, the attenuation rate has reached 23.51%, 21.89%, 8.11%, and 13.37%, respectively by the end of 2019 based on the cross-calibration results.https://doi.org/10.1038/s41598-021-86619-y |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Li Liu Tingting Shi Hailiang Gao Xuewen Zhang Qijin Han Xinkai Hu |
spellingShingle |
Li Liu Tingting Shi Hailiang Gao Xuewen Zhang Qijin Han Xinkai Hu Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands Scientific Reports |
author_facet |
Li Liu Tingting Shi Hailiang Gao Xuewen Zhang Qijin Han Xinkai Hu |
author_sort |
Li Liu |
title |
Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands |
title_short |
Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands |
title_full |
Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands |
title_fullStr |
Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands |
title_full_unstemmed |
Long-term cross calibration of HJ-1A CCD1 and Terra MODIS reflective solar bands |
title_sort |
long-term cross calibration of hj-1a ccd1 and terra modis reflective solar bands |
publisher |
Nature Publishing Group |
series |
Scientific Reports |
issn |
2045-2322 |
publishDate |
2021-04-01 |
description |
Abstract Since its launch on September 6, 2008, HJ-1A has been in the orbit for 13 years. The CCD1 sensor on the HJ-1A has four reflected solar bands. Since the calibration frequency is limited to the annual site calibration, cross-calibration is an effective method to improve the calibration frequency. In this paper, we use 420 image pairs of HJ-1A CCD1 and Terra MODIS over the Dunhuang test site for gains calculation, where we take MODIS as the reference sensor. The spectral band adjustment factors (SBAFs) for cross-calibration are then calculated to compensate for the spectral mismatch. The cross-calibration results are also validated by the field calibration results. From 2008 to 2019, a total of six campaigns have been cross-calibrated on the same day. The gain difference between the site calibration and cross-calibration is less than 3%. The long-term cross-calibration results further indicate that due to the adjustment of HJ-1A CCD gain state in October 2009, an abrupt change occurred 405 days after launch. After 12 years of on-orbit operation, the attenuation rate has reached 23.51%, 21.89%, 8.11%, and 13.37%, respectively by the end of 2019 based on the cross-calibration results. |
url |
https://doi.org/10.1038/s41598-021-86619-y |
work_keys_str_mv |
AT liliu longtermcrosscalibrationofhj1accd1andterramodisreflectivesolarbands AT tingtingshi longtermcrosscalibrationofhj1accd1andterramodisreflectivesolarbands AT hailianggao longtermcrosscalibrationofhj1accd1andterramodisreflectivesolarbands AT xuewenzhang longtermcrosscalibrationofhj1accd1andterramodisreflectivesolarbands AT qijinhan longtermcrosscalibrationofhj1accd1andterramodisreflectivesolarbands AT xinkaihu longtermcrosscalibrationofhj1accd1andterramodisreflectivesolarbands |
_version_ |
1721542610040913920 |