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中国自主木星冰卫星冰下液态海洋探测刍议
徐曦煜1,2, 朱迪1, 杨双宝1
1.中国科学院 国家空间科学中心 微波遥感技术重点实验室, 北京 100190;2.中国科学院 遥感与数字地球研究所 遥感科学国家重点实验室, 北京 100094
摘要:
木星冰卫星(尤其是“木卫2”)在整个太阳系中有非常独特的探测价值,也是当前国际深空探测最前沿、最受关注的领域之一。在对国外相关探测技术归纳总结的同时,结合木星冰卫星冰下海洋探测的若干科学问题,次表层模型、温度廓线及探测深度、电离层的影响等方面,提供了几种木星冰卫星冰下液态水海洋探测的新思路,并给出了一些初步的系统框架设计和次表层介电特性仿真分析等结果。通过对新方法、新模式的探索,有望对我国自主木星冰卫星的次表层液态海洋探测起到良好的借鉴作用。
关键词:  木星冰卫星  液态海洋  次表层  高度计  电离层
DOI:10.15982/j.issn.2095-7777.2019.06.009
分类号:P353;V447
基金项目:国家自然科学基金资助项目(41876209);遥感科学国家重点实验室开放基金资助项目(OFSLRSS201705)
Remarks on Chinese Autonomous Exploration of the Liquid Oceans beneath the Icy Moons’Surfaces of Jupiter System
XU Xiyu1,2, ZHU Di1, YANG Shuangbao1
1.The Key Laboratory of Microwave Remote Sensing, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;2.State Key Laboratory of Remote Sensing Science, Institute of Remote Sensing and Digital Earth, Chinese Academy of Sciences, Beijing 100094, China
Abstract:
Icy Moons of Jupiter System (especially Europa) have abundant exploring value,and they are among the hottest objectives in solar system exploration throughout the world. In this paper,the recent advances in pertinent exploration technology in the international community are summarized, and some science issues, such as sub-surface model, temperature profile, penetration depth,and the influence of icy moons' ionosphere,are addressed. A few new ideas are presented,a preliminary system framework is proposed,and some simulation results of the sub-surface dielectric property are shown. The forthcoming Chinese autonomous Jupiter system exploration mission focusing on the exploration of the liquid oceans beneath the icy moons' surfaces is expected to benefit much from the investigation of new methodology and new configuration in this paper.
Key words:  Jupiter ice moons  liquid ocean  subsurface  altimeter  ionosphere