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SDO EVE CCD and thin foil filter characterization and selection

机译:SDO EVE CCD和薄箔滤光片的特性和选择

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摘要

The NASA Solar Dynamics Observatory (SDO), scheduled for launch in 2009, incorporates a suite of instruments including the EUV Variability Experiment (EVE). The Multiple EUV Grating Spectrograph (MEGS) channels use concave reflection gratings to image solar spectra onto CCDs that are operated at -100℃. MEGS provides 0.1 nm spectral resolution between 5-105nm every 10 seconds with an absolute accuracy of better than 25% over the SDO 5-year mission. Characterizations and selection testing of the CCDs and the thin foil filters for SDO EVE have been performed with both in-band and visible illumination. CCD selection was based on results from testing in LASP facility Calibration and Test Equipment (CTE3) as well as results from at testingMIT. All CCDs meet the requirements for electronics gain, flat field, Quantum Efficiency (QE), dark current, reverse clock, CTE, bad pixels and the -120℃ survival test. The thin foil filters selection was based on tests performed at LASP facilities and NIST. All filters provide > 10~6 attenuation of visible light with the proper EUV transmission needed for order sorting capabilities and are free of critical pinholes.
机译:计划于2009年发射的NASA太阳动力学天文台(SDO)结合了包括EUV可变性实验(EVE)在内的一系列仪器。多重EUV光栅光谱仪(MEGS)通道使用凹面反射光栅将太阳光谱成像到在-100℃下运行的CCD上。 MEGS每10秒提供0.1 nm的光谱分辨率,范围为5-105nm,绝对精度超过SDO 5年任务的25%。 CCD和用于SDO EVE的薄箔滤光片的特性测试和选择测试已经在带内和可见光下进行了。 CCD的选择基于LASP设备校准和测试设备(CTE3)中的测试结果以及testMIT的结果。所有CCD都满足以下要求:电子增益,平坦场,量子效率(QE),暗电流,反向时钟,CTE,不良像素和-120℃生存测试。薄箔过滤器的选择基于在LASP设施和NIST进行的测试。所有滤光片都能提供大于10〜6的可见光衰减,并具有订单分类功能所需的适当EUV透射率,并且没有严重的针孔。

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