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Recent Sensor Designs for Earth Observation

机译:最近的地球观测传感器设计

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摘要

The large number of missions associated with ESA's Copernicus program has necessitated several new image sensor designs for earth observation (or living planet) applications as each instrument needs to be highly optimized. Whilst the majority of these sensors have utilised CCD technology, the use of CMOS is starting to increase. New CCD designs and technology trends for hyperspectral applications such as Sentinel 4, Sentinel 5, Sentinel 5 precursor (TropOMI), Flex and 3MI are described. In these the sensor design has been optimized to provide highest possible signal levels with lowest possible noise in combination with higher frame rates and reduced image smear. CMOS sensors for MTG (Meteosat Third Generation) and METImage are then described. Both use extremely large pixels, up to 250μm square, at high line rates. Radiation test data and key performance measurements are shown for MTG and for a test device that has been made for METImage. Finally, newer developments including back-illumination and means for achieving a TDI function in standard-processed CMOS are briefly described.
机译:与ESA的Copernicus计划相关的大量任务已经需要用于地球观测(或活片)应用的几个新的图像传感器设计,因为每个仪器都需要高度优化。虽然这些传感器的大部分利用了CCD技术,但是使用CMOS开始增加。描述了Sentinel 4,Sentinel 5,Sentinel 5前体(Tropomi),Flex和3Mi的高光谱应用的新CCD设计和技术趋势。在这些中,传感器设计已被优化,以提供具有最低可能噪声的最高可能的信号电平,以及更高的帧速率和降低的图像涂抹。然后描述MTG(Meteosat第三代)和Metimage的CMOS传感器。两者都使用极大的像素,高达250μm平方,高线速率。辐射测试数据和关键性能测量显示为MTG和已经为Metimage制造的测试设备。最后,简要描述了包括后照明和用于在标准处理的CMOS中实现TDI函数的较新的发展。

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