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首页> 外文会议>Conference on Interferometry in Space Pt.1, Aug 26-28, 2002, Waikoloa, Hawaii, USA >Hypertelescope imaging: from exo-planets to neutron stars
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Hypertelescope imaging: from exo-planets to neutron stars

机译：超望远镜成像：从系外行星到中子星

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摘要

"Densified-pupil multi-aperture imaging arrays", also called hypertelescopes, provide a path towards rich images obtained directly at the focal plane. They typically involve a large Fizeau arrangement, with a small attached "pupil densifier" serving to gain luminosity at the expense of field . At scales ranging from kilometers to perhaps a million kilometers, such architectures appear of interest for stellar physics, galaxies, cosmology, and neutron star imaging with the larger sizes. Ground testing is initiated and space versions are proposed, particularly to NASA for its Terrestrial Planet Finder. The coronagraphic imaging achievable with this space version is expected to improve the detection sensitivity by attenuating the sky background contribution. Subsequent larger (150 km) versions can in principle resolve the "green spots" on an Earth seen at several parsecs. Current design work for a precursor array of "flying mirrors" driven by solar sails in geostationary orbit will be presented.
机译：也被称为超望远镜的“瞳孔多孔径成像阵列”为直接在焦平面获得的丰富图像提供了一条路径。它们通常涉及大型的Fizeau装置，并带有小型的“瞳孔致密剂”，以获取光度，但以牺牲现场为代价。这种结构的规模从几公里到大约一百万公里不等，对更大尺寸的恒星物理学，星系，宇宙学和中子星成像很有用。已开始进行地面测试，并提出了太空版本，特别是针对NASA的“地球行星搜索器”。预期通过这种空间版本可获得的冠状成像可以通过减弱天空背景贡献来提高检测灵敏度。随后的较大版本（150公里）原则上可以解决几秒钟差距处出现的地球上的“绿点”。将介绍在对地静止轨道上由太阳帆驱动的“飞行镜”前体阵列的当前设计工作。

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