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EUV transmission of Optical Blocking Filter and Optical Blocking Layer for Soft X-ray Imager (SXI) onboard Astro-H

机译:软X射线成像器(SXI)的光阻塞过滤器和光阻挡层的EUV传输(SXI)车载Astro-H

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We have developed the X-ray CCD camera system for the Soft X-ray Imager (SXI) which will be launched as focal plane detectors of X-ray telescope onboard the Japanese 6th X-ray astronomical satellite, Astro-H. The X-ray CCD is back-illuminated (BI) CCD which has an Optical Blocking Layer (OBL) directly coating its X-ray illumination surface with Aluminum-Polyimide-Aluminum instead of Optical Blocking Filter (OBF). The X-ray CCD is affected by large doses of extreme ultraviolet (EUV) radiation from Earth sun-lit atmosphere (airglow) in orbit. To evaluate the performance of polyimide that cut off EUV, we measured the EUV transmission of both OBL and OBF at various energy range between 15-72 eV by utilizing beam line located at the Photon Factory in High Energy Accelerator Research Organization (KEK-PF) in this March and June, and obtained the EUV transmission to be 3% at 41 eV which is as same as expected transmission from the designed thickness of polyimide layer.
机译:我们开发了软X射线成像仪(SXI)的X射线CCD摄像头系统,该系统将作为X射线望远镜的焦平面探测器推出,在日本第6 X射线天文卫星,Astro-H上坐在X射线望远镜的焦平面探测器。 X射线CCD是背部照明(BI)CCD,其具有与铝 - 聚酰亚胺 - 铝的X射线照明表面直接涂覆其X射线照射表面而不是光学阻挡过滤器(OBF)。 X射线CCD受到轨道中地球灯光气氛(释放)的大剂量极紫外(EUV)辐射的影响。为了评估切断EUV的聚酰亚胺的性能,通过利用位于高能量加速器研究组织(Kek-PF)的光子厂的光束线,测量了15-72eV之间的各种能量范围的EUV传输。在3月和6月,在41EV中获得了EUV变速器为3%,与从设计的聚酰亚胺层的设计厚度一样与预期的传输相同。

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