100 micr'/> Determination of CERES Flight models 1 and 2 sensors zero-radiance response variability with elevation and azimuth scan angles, on-orbit aboard TERRA Spacecraft
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Determination of CERES Flight models 1 and 2 sensors zero-radiance response variability with elevation and azimuth scan angles, on-orbit aboard TERRA Spacecraft

机译:确定TERRES航天器在轨的CERES飞行模型1和2传感器的零辐射响应随仰角和方位角的变化

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The Clouds and the Earth's Radiant Energy System (CERES) instrument has scanning thermistor bolometers that measure broadband radiances in the shortwave (0.3 - 5.0 micrometer), total (0.3 - >100 micrometer) and 8 -12 micrometer water vapor window regions. The CERES Flight models Ⅰ and Ⅱ (FM1 and FM2) instruments were launched aboard the Earth Observing System-Terra platform on December 1999. The CERES instrument can operate in fixed as well as rotating azimuth positions with the elevation head moving in full scan or short scan modes. The sensor measurements have shown a dependency on observation geometry during each of these scan modes of operation. The zero radiance offsets of the sensors were measured using end caps (low emittance aluminum targets) on the ground at each elevation observation angle in fixed azimuth scan mode. The Terra spacecraft have conducted two sets of calibration maneuvers viewing the deep space on-orbit in March and April 2003. During these tests where the spacecraft is constantly pitched to view the cold space (3 degree K blackbody), zero radiance offsets were measured for the CERES sensors in all scan modes of operation. This paper describes the procedures used to determine the zero radiance scan offsets for CERES sensors. The measured offset values calculated from ground and in-flight tests for the FM1 and FM2 sensors are also presented.
机译:云和地球的辐射能系统(CERES)仪器具有扫描热敏电阻测辐射热计,可测量短波(0.3-5.0微米),总辐射(0.3-> 100微米)和8 -12微米水蒸气窗口区域的宽带辐射。 CERESⅠ和Ⅱ飞行模型(FM1和FM2)仪器于1999年12月在地球观测系统-Terra平台上发射。CERES仪器可在固定和旋转方位角位置操作,仰角头可在全扫描或短距离内移动扫描模式。在这些扫描操作模式的每一个中,传感器的测量结果都显示出对观测几何形状的依赖性。在固定方位角扫描模式下,在每个仰角观察角处,使用端盖(低辐射铝靶)在地面上测量传感器的零辐射偏移。 Terra航天器在2003年3月和2003年4月进行了两组校准操作,以观察深空轨道。在这些测试中,航天器不断俯仰以观察冷空间(3度K黑体),测量了零辐射偏移量。所有扫描操作模式下的CERES传感器。本文介绍了用于确定CERES传感器的零辐射扫描偏移量的过程。还介绍了根据地面和飞行中FM1和FM2传感器计算得出的偏移值。

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