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Inter-calibration of infrared channels of geostationary meteorological satellite imagers

机译:对地静止气象卫星图像红外通道的相互校准

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This article examines a method of inter-calibration for MSU-GS imager of the Russian Geostationary Earth Orbit (GEO) satellite Elektro-L No. 2. Since the launch (December 11, 2015), the satellite's radiation cooler has been operating in an abnormal mode, so the calibration of the IR channels of the MSU-GS imager differed from that pre-flight and, in general, could have a daily variability. To ensure the satellite’s further operation in orbit, it was necessary to calibrate imager channels at a frequency that would allow to identify daily calibration course to detect and compensate its sources. In order to do this, we have developed a special method of GEO-GEO inter-calibration. The calibration of MSU-GS was performed using SEVIRI imager installed on the GEO satellite Meteosat-10. SEVIRI was chosen as a reference instrument because its spectral channels are similar to those of MSU-GS. The MSU-GS was calibrated according to the regressions calculated from the simultaneously images of the field of regard selected between the sub-satellite points. The dynamic brightness temperature (BT) range was determined by deep convective clouds in high troposphere and warm ocean surface. Using the proposed method of inter-calibration, it was possible to confirm the absence of a significant daily variation of the calibration since November 2017. The amplitude of the variation smoothly increases from ~0.2K at high (~ 300K) BTs to ~ 1.0K when the temperature decreased to 200K. These estimates allow the use of the Fourier spectrometer IKFS 2 installed on the Russian Low-Earth-Orbit (LEO) satellite Meteor-M No. 2 to verify the developed GEO-GEO scheme of inter-calibration. Despite the specifics of the situation on board Elektro-L No. 2, the proposed method of GEO-GEO inter-calibration can be applied to radiometers of other neighboring satellites that differ in SSP and spatial resolution.
机译:本文研究了俄罗斯对地静止地球轨道(GEO)卫星Elektro-L 2号的MSU-GS成像仪的相互校准方法。自发射以来(2015年12月11日),该卫星的辐射冷却器一直在使用异常模式,因此MSU-GS成像仪的红外通道的校准与飞行前有所不同,并且通常每天都有变化。为了确保卫星在轨道上的进一步运行,有必要以一定的频率校准成像仪通道,以便确定每日校准过程以检测和补偿其来源。为此,我们开发了一种特殊的GEO-GEO相互校准方法。使用安装在GEO卫星Meteosat-10上的SEVIRI成像仪对MSU-GS进行校准。之所以选择SEVIRI作为参考仪器,是因为其光谱通道与MSU-GS相似。根据从亚卫星点之间选择的视场的同时图像计算出的回归值,对MSU-GS进行校准。动态亮度温度(BT)范围由对流层和温暖海洋表面的深对流云确定。使用建议的相互校准方法,可以确认自2017年11月以来,校准的每日变化不大。变化幅度从高(〜300K)BT时的〜0.2K平稳增加到〜1.0K。当温度降至200K时。这些估计值允许使用安装在俄罗斯低地球轨道(LEO)卫星Meteor-M 2号上的傅立叶光谱仪IKFS 2来验证已开发的GEO-GEO互校准方案。尽管Elektro-L No.2上的情况有特殊规定,但建议的GEO-GEO互校准方法可以应用于SSP和空间分辨率不同的其他相邻卫星的辐射计。

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