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首页> 外文期刊>Applied optics >Celestial body irradiance determination from an underfilled satellite radiometer: application to albedo and thermal emission measurements of the Moon using CERES
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Celestial body irradiance determination from an underfilled satellite radiometer: application to albedo and thermal emission measurements of the Moon using CERES

机译:利用未充满的卫星辐射计确定天体的辐照度:应用CERES应用于月球的反照率和热辐射测量

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摘要

The Clouds and the Earth's Radiant Energy System (CERES) is a program that measures the Earth radiation budget (ERB) from two polar orbiting satellite platforms. CERES radiometers are designed to make stable broadband measurements of scattered solar and emitted thermal radiative flux leaving Earth with an accuracy of 1percent or better. Using versatile and programmable scan modes, it is also possible for every CERES instrument to view the Moon on each orbit. However, until now, it has not been possible to derive absolute measurements of lunar irradiance using CERES because the Moon's disk fills only 10percent of the telescope field of view. This work presents a method of integrating CERES raster-scan data in order to obtain a measurement of the average scattered solar and emitted thermal radiance from the entire lunar disk. The technique results in excellent agreement between CERES instruments on different satellites as to lunar albedo and emitted thermal flux. The average broadband Moon albedo is measured by CERES at a value of 0.1362 (+-2-3percent) when normalized to a static lunar phase angle of 7 deg using the U.S. Geological Survey lunar irradiance Robotic Lunar Observatory model. The method for the first time also yields very accurate measurements of the thermal irradiance emitted from the Moon. These suggest an average long-wave flux of 977 Wm~(-2) (+-2-3percent at 7 deg phase), implying an approximate mean surface temperature of around 92 deg C. Statistical analysis on available data suggests that a CERES instrument performing monthly lunar measurements could utilize the Moon as a stability target and reduce calibration drifts to 0.3percent per decade or less within an instrument's lifetime. Given the success of the technique, a solar calibration system is proposed that will allow precise tracking of an ERB instrument's optical degradation using the Sun.
机译:云与地球辐射能系统(CERES)是一个程序,用于测量来自两个极轨道卫星平台的地球辐射预算(ERB)。 CERES辐射计旨在对离开地球的散射太阳光和发射的热辐射通量进行稳定的宽带测量,精度为1%或更高。使用通用的可编程扫描模式,每台CERES仪器也可以在每个轨道上观察月球。但是,到目前为止,由于月球盘仅占望远镜视场的10%,因此无法使用CERES得出月球辐照度的绝对测量值。这项工作提出了一种集成CERES光栅扫描数据的方法,以便获得整个月球盘的平均散射太阳辐射和辐射热辐射的测量值。该技术使不同卫星上的CERES仪器之间在月球反照率和发射热通量方面具有极好的一致性。当使用美国地质调查局的月球辐照度自动月球观测仪模型将其标准化为7度的静态月相角时,CERES测得的平均宽带月球反照率值为0.1362(+-2-3%)。首次使用该方法还可以对月球发出的热辐射进行非常精确的测量。这些表明平均长波通量为977 Wm〜(-2)(在7度相位时为+ -2-3%),这意味着大约平均表面温度约为92摄氏度。对现有数据的统计分析表明,CERES仪器每月进行一次月球测量可以利用月球作为稳定目标,并在仪器的使用寿命内将校准漂移降低到每十年小于或等于0.3%。考虑到该技术的成功,提出了一种太阳能校准系统,该系统将允许使用太阳精确跟踪ERB仪器的光学退化。

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  • 来源
    《Applied optics》 |2008年第27期|共13页
  • 作者

    Grant Matthews;

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