The Chinese Hα Solar Explorer(CHASE) mission: An overview  被引量:14

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作  者:Chuan Li Cheng Fang Zhen Li MingDe Ding PengFei Chen Ye Qiu Wei You Yuan Yuan MinJie An HongJiang Tao XianSheng Li Zhe Chen Qiang Liu Gui Mei Liang Yang Wei Zhang WeiQiang Cheng JianXin Chen ChangYa Chen Qiang Gu QingLong Huang MingXing Liu ChengShan Han HongWei Xin ChangZheng Chen YiWei Ni WenBo Wang ShiHao Rao HaiTang Li Xi Lu Wei Wang Jun Lin YiXian Jiang LingJie Meng Jian Zhao 

机构地区:[1]School of Astronomy and Space Science, Nanjing University [2]Key Laboratory for Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education [3]Shanghai Institute of Satellite Engineering [4]Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences [5]Shanghai Academy of Spaceflight Technology [6]China Center for Resources Satellite Data and Application [7]China Aerospace Science and Technology Corporation [8]Key and Special Project Center of China National Space Administration (CNSA)

出  处:《Science China(Physics,Mechanics & Astronomy)》2022年第8期2-9,共8页中国科学:物理学、力学、天文学(英文版)

基  金:supported by China National Space Administration(CNSA)。

摘  要:The Chinese Hα Solar Explorer(CHASE), dubbed “Xihe”—Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration(CNSA). The CHASE mission is designed to test a newly developed satellite platform and to acquire the spectroscopic observations in the Hα waveband. The Hα Imaging Spectrograph(HIS)is the scientific payload of the CHASE satellite. It consists of two observational modes: raster scanning mode and continuum imaging mode. The raster scanning mode obtains full-Sun or region-of-interest spectral images from 6559.7 to 6565.9 ? and from 6567.8 to 6570.6 ? with 0.024 ? pixel spectral resolution and 1 min temporal resolution. The continuum imaging mode obtains photospheric images in continuum around 6689 ? with the full width at half maximum of 13.4 ?. The CHASE mission will advance our understanding of the dynamics of solar activity in the photosphere and chromosphere. In this paper, we present an overview of the CHASE mission including the scientific objectives, HIS instrument overview, data calibration flow, and first results of on-orbit observations.

关 键 词:space-based telescope solar physics CHROMOSPHERE photosphere 

分 类 号:V476.4[航空宇航科学与技术—飞行器设计]

 

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