《Table 3 PFA main specifications》
本系列图表出处文件名:随高清版一同展现
《The enhanced X-ray Timing and Polarimetry mission—eXTP》
Since they are based on very similar concepts in this section we discuss the optics of both the SFA and PFA.Thirteen X-ray grazing-incidence Wolter-I(parabola+hyperbola)optics modules will be implemented onboard eXTP.The SFA includes nine optics modules while four optics modules are designed for the PFA.The expected collecting area of each telescope is at 2 keV,and at 6 ke V.The FoV is 12 arcmin(in diameter).These figures already meet the requirement of~820 cm2at 2 keV1) .The requirement for the angular resolution of the PFA optics is<30 arcsec(HEW,goal is 15 arcsec),more demanding than the 1 arcmin(HEW)angular resolution required for the SFA optics.For both types of telescopes the focal length reference value is 525 cm.The maximum diameter of the mirror shells,allowed by the envelope for a single mirror of less than 600 mm in diameter,is about 510 mm.The weight of the optics module is expected to be~50 kg for the SFA and~100 kg for the PFA.In Table 1 we list the main parameters of the SFA and PFA optics.
图表编号 | XD0034876100 严禁用于非法目的 |
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绘制时间 | 2019.02.01 |
作者 | ShuangNan Zhang、Andrea Santangelo、Marco Feroci、YuPeng Xu、FangJun Lu、Yong Chen、Hua Feng、Shu Zhang、Sren Brandt、Margarita Hernanz、Luca Baldini、Enrico Bozzo、Riccardo Campana、Alessandra De Rosa、YongWei Dong、Yuri Evangelista、Vladimir Karas、Norbert Meidinger、Ali |
绘制单位 | Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences、Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences、Institut für Astronomie und Astrophysik, Eberha |
更多格式 | 高清、无水印(增值服务) |