气象科技进展
氣象科技進展
기상과기진전
Advances in Meteorological Science and Technology
2013年
4期
71-83
,共13页
胡秀清%孙凌%刘京晶%丁雷%王向华%李元%张勇%徐娜%陈林
鬍秀清%孫凌%劉京晶%丁雷%王嚮華%李元%張勇%徐娜%陳林
호수청%손릉%류경정%정뢰%왕향화%리원%장용%서나%진림
衰减率%仪器性能跟踪%中分辨率光谱成像仪%反射太阳波段定标%替代定标
衰減率%儀器性能跟蹤%中分辨率光譜成像儀%反射太暘波段定標%替代定標
쇠감솔%의기성능근종%중분변솔광보성상의%반사태양파단정표%체대정표
Degradation rate%instrument monitoring%Medium Resolution Spectral Imager (MERSI)%solar reflective band calibration%vicarious calibration (VC)
中分辨率光谱成像仪(MERSI)是搭载在我国第二代极轨气象卫星风云三号(FY-3)上的一个主要仪器。总结了MERSI在仪器设计、定标算法、发射前及在轨性能以及仪器性能验证等方面的信息。针对MERISI可见光星上定标器(VOC)的跟踪监测发现,在过去两年,它的太阳反射波段(RSBs)发生了显著的衰减,特别是较短波长通道(<500nm)衰减量超过10%,最大衰减发生在第8波段,约20%。但波长较长通道的性能相对稳定,衰减量小于5%。两个短波红外通道电子增益出现随机跃动,导致发射后的定标系数存在频繁波动。以上结果与其他两种替代定标方法相比(即中国遥感卫星辐射校正场定标,简称场地定标和基于Terra/MODIS敦煌沙漠场景交叉定标),结论一致。MERSI针对大气顶辐射亮度或反射率定标的总不确定度小于5%。定标结果为FY-3A/MERSI定标系数的更新提供了重要的参考和评估。
中分辨率光譜成像儀(MERSI)是搭載在我國第二代極軌氣象衛星風雲三號(FY-3)上的一箇主要儀器。總結瞭MERSI在儀器設計、定標算法、髮射前及在軌性能以及儀器性能驗證等方麵的信息。針對MERISI可見光星上定標器(VOC)的跟蹤鑑測髮現,在過去兩年,它的太暘反射波段(RSBs)髮生瞭顯著的衰減,特彆是較短波長通道(<500nm)衰減量超過10%,最大衰減髮生在第8波段,約20%。但波長較長通道的性能相對穩定,衰減量小于5%。兩箇短波紅外通道電子增益齣現隨機躍動,導緻髮射後的定標繫數存在頻繁波動。以上結果與其他兩種替代定標方法相比(即中國遙感衛星輻射校正場定標,簡稱場地定標和基于Terra/MODIS敦煌沙漠場景交扠定標),結論一緻。MERSI針對大氣頂輻射亮度或反射率定標的總不確定度小于5%。定標結果為FY-3A/MERSI定標繫數的更新提供瞭重要的參攷和評估。
중분변솔광보성상의(MERSI)시탑재재아국제이대겁궤기상위성풍운삼호(FY-3)상적일개주요의기。총결료MERSI재의기설계、정표산법、발사전급재궤성능이급의기성능험증등방면적신식。침대MERISI가견광성상정표기(VOC)적근종감측발현,재과거량년,타적태양반사파단(RSBs)발생료현저적쇠감,특별시교단파장통도(<500nm)쇠감량초과10%,최대쇠감발생재제8파단,약20%。단파장교장통도적성능상대은정,쇠감량소우5%。량개단파홍외통도전자증익출현수궤약동,도치발사후적정표계수존재빈번파동。이상결과여기타량충체대정표방법상비(즉중국요감위성복사교정장정표,간칭장지정표화기우Terra/MODIS돈황사막장경교차정표),결론일치。MERSI침대대기정복사량도혹반사솔정표적총불학정도소우5%。정표결과위FY-3A/MERSI정표계수적경신제공료중요적삼고화평고。
The Medium Resolution Spectral Imager (MERSI) is a key instrument onboard Fengyun-3 (FY-3), the second generation of polar-orbiting meteorological satellites in China. This paper summarizes the knowledge of MERSI instrument in terms of sensor design, calibration algorithm, prelaunch and on-orbit characterization, and performance veriifcation. The calibration monitoring of its relfective solar bands (RSBs) is primarily conducted using a visible onboard calibrator and found that it has a signiifcant degradation on the order of 10%in its shorter RSB bands (<500 nm), with the largest in band 8 of about 20%during the past two years. However, the performance at longer wavelength bands is relatively stable with a change of less than 5%. It is shown that the postlaunch calibration of the two short-wavelength infrared bands has frequent lfuctuations because of random jumps in their electronic gains. These results are consistently veriifed by two kinds of vicarious calibration (VC) methods:China Radiometric Calibration Sites VC and intercalibration using Terra/Moderate Resolution Imaging Spectroradiometer over Dunhuang desert. The overall uncertainty in the MERSI top-of-atmosphere radiance or relfectance is less than 5%. These results provide the important reference and evaluation for the update of the FY-3A/MERSI calibration coefifcients.