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Results from Solar Reflective Band End-to-End Testing for VIIRS F1 Sensor Using T-SIRCUS

机译:使用T-SIRCUS对VIIRS F1传感器进行太阳能反射带端到端测试的结果

摘要

Verification of the Visible Infrared Imager Radiometer Suite (VIIRS) End-to-End (E2E) sensor calibration is highly recommended before launch, to identify any anomalies and to improve our understanding of the sensor on-orbit calibration performance. E2E testing of the Reflective Solar Bands (RSB) calibration cycle was performed pre-launch for the VIIRS Fight 1 (F1) sensor at the Ball Aerospace facility in Boulder CO in March 2010. VIIRS reflective band calibration cycle is very similar to heritage sensor MODIS in that solar illumination, via a diffuser, is used to correct for temporal variations in the instrument responsivity. Monochromatic light from the NIST T-SIRCUS was used to illuminate both the Earth View (EV), via an integrating sphere, and the Solar Diffuser (SD) view, through a collimator. The collimator illumination was cycled through a series of angles intended to simulate the range of possible angles for which solar radiation will be incident on the solar attenuation screen on-orbit. Ideally, the measured instrument responsivity (defined here as the ratio of the detector response to the at-sensor radiance) should be the same whether the EV or SD view is illuminated. The ratio of the measured responsivities was determined at each collimator angle and wavelength. In addition, the Solar Diffuser Stability Monitor (SDSM), a ratioing radiometer designed to track the temporal variation in the SD BRF by direct comparison to solar radiation, was illuminated by the collimator. The measured SDSM ratio was compared to the predicted ratio. An uncertainty analysis was also performed on both the SD and SDSM calibrations.
机译:强烈建议在发射前对可见红外成像辐射计套件(VIIRS)端对端(E2E)传感器校准进行验证,以识别任何异常情况并增进我们对传感器在轨校准性能的了解。反射太阳波段(RSB)校准周期的E2E测试是在2010年3月在科罗拉多州博尔德(Boulder CO)的Ball Aerospace工厂为VIIRS Fight 1(F1)传感器进行的发射前进行的。VIIRS反射波段校准周期与传统传感器MODIS非常相似在这种情况下,太阳光通过漫射器用于校正仪器响应度的时间变化。来自NIST T-SIRCUS的单色光用于通过积分球照明地球视图(EV),并通过准直仪照明太阳漫射器(SD)视图。准直仪照明通过一系列角度进行循环,这些角度旨在模拟太阳辐射将在轨道上入射到太阳衰减屏幕上的可能角度范围。理想情况下,无论是照亮EV还是SD视图,所测得的仪器响应度(此处定义为检测器响应与传感器辐射度之比)都应该相同。在每个准直器角度和波长下确定所测响应度的比率。此外,准直仪对太阳漫射器稳定性监视器(SDSM)进行了照明,它是一种比例辐射计,旨在通过与太阳辐射直接比较来跟踪SD BRF的时间变化。将测得的SDSM比率与预测比率进行比较。还对SD和SDSM校准都进行了不确定性分析。

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