Acta Optica Sinica, Volume. 45, Issue 18, 1828011(2025)

Scientific Mission Design for Ultraviolet Hyperspectral Detection of Venus Cloud Layers (Invited)

Tao Li1, Xin Fang1、*, Liujun Zhong1, Dexin Lai1, Bo Li2, Yamin Wang3, Yonghe Zhang3, and Xin Ye2
Author Affiliations
  • 1CAS Center for Excellence in Comparative Planetology, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, Anhui , China
  • 2Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, Jilin , China
  • 3Innovation Academy for Microsatellites of Chinese Academy of Sciences, Shanghai 201203, China
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    References(35)

    [2] Nakamura M, Imamura T, Ishii N et al. AKATSUKI returns to Venus[J]. Earth, Planets and Space, 68, 75(2016).

    [3] Cardesín Moinelo A, Piccioni G, Ammannito E et al. Calibration of hyperspectral imaging data: VIRTIS-M onboard Venus express[J]. IEEE Transactions on Geoscience and Remote Sensing, 48, 3941-3950(2010).

    [29] Smrekar S, Dyar D, Helbert J et al. VERITAS (Venus Emissivity, Radio Science, InSAR, Topography and Spectroscopy): a proposed discovery mission[C]. EPS, C2020-447(2020).

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    Tao Li, Xin Fang, Liujun Zhong, Dexin Lai, Bo Li, Yamin Wang, Yonghe Zhang, Xin Ye. Scientific Mission Design for Ultraviolet Hyperspectral Detection of Venus Cloud Layers (Invited)[J]. Acta Optica Sinica, 2025, 45(18): 1828011

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    Paper Information

    Category: Remote Sensing and Sensors

    Received: May. 27, 2025

    Accepted: Aug. 28, 2025

    Published Online: Sep. 19, 2025

    The Author Email: Xin Fang (xinf@ustc.edu.cn)

    DOI:10.3788/AOS251150

    CSTR:32393.14.AOS251150

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