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Advanced Geosynchronous Studies Imager: an all-reflective off-center off-axis focal telescope for Earth observation

机译:先进的地球同步研究成像仪:用于地球观测的全反射偏心离轴聚焦望远镜

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Abstract: An unobscured, f/4, Earth scanning telescope was designed by optimizing an off-center, off-axis Cassegrain telescope with a unit magnification spherical camera mirror. A flat scan mirror in front of the 30-cm diameter telescope directs the 1-degree field-of-view. Observation form geosynchronous orbit results in sunlight illumination of the scanning, primary, and secondary mirrors near satellite local midnight. The 'all-reflective' design has a primary- secondary spacing of 87-cm. A field stop helps control stay sunlight illumination of the camera mirror and beam division optics. Exit pupil stops further control stray illumination. Sub-satellite pixel image scale is 1/2-, 1-, and 2-km over the spectral range 0.4- to 13.5-microns. The general requirements are for the first diffraction dark ring to be imaged on the pixels. The flat image plane is separated into four bands using dichroic beamsplitters and flat mirrors to accommodate linear array detector technology. Sub-band channels are defined with filters in near contact with the detectors. All but the visible detectors are enclosed behind transmission windows so that all bands can be operated without thermal vacuum facilities during ground testing. All transmission elements are 'wedged' to correct for astigmatism introduced by using them in converging light. The powered mirrors and scan flat are to be silicon carbide. The mechanical structure will be a near-zero expansion graphite fiber reinforced plastic. Tolerance analysis and thermal modeling show optical element displacements well below requirements. Instrument volume corresponds approximately to that of the current GOES Imager. !4
机译:摘要:通过使用单位放大率球面相机镜优化偏心,偏轴的卡塞格林望远镜,设计了一种无遮挡的f / 4地球扫描望远镜。直径30厘米望远镜前面的平面扫描镜可引导1度视野。地球同步轨道的观测结果导致了卫星当地午夜附近的扫描镜,主镜和副镜的阳光照射。 “全反射”设计的主副间隔为87厘米。视场光阑有助于控制摄像机镜和分光镜的太阳光照射。出瞳停止进一步控制杂散照明。在0.4至13.5微米的光谱范围内,亚卫星像素的图像比例为1 / 2-,1-和2-km。一般要求是将第一个衍射黑环成像在像素上。使用二向色分束器和平面镜将平面图像平面分为四个波段,以适应线性阵列检测器技术。子带通道由与检测器紧密接触的滤波器定义。除可见光探测器外,所有探测器都被封闭在透射窗的后面,因此在地面测试期间,所有波段都可以在没有热真空设施的情况下运行。所有的透射元件都被“楔形”以校正在会聚光中使用它们所引入的像散。电动反射镜和扫描平面应为碳化硅。机械结构将是接近零膨胀的石墨纤维增强塑料。公差分析和热模型表明光学元件的位移远低于要求。仪器体积大约相当于当前GOES Imager的体积。 !4

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