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月球电离层掩星探测研究

王震 王娜 平劲松

深空探测学报Issue(3):220-225,6.
深空探测学报Issue(3):220-225,6.DOI:10.15982/j.issn.2095-7777.2014.03.010

月球电离层掩星探测研究

Introduction of Lunar Ionosphere Research by RO Method

王震 1王娜 2平劲松1

作者信息

  • 1. 中国科学院新疆天文台,乌鲁木齐 830011
  • 2. 中国科学院国家天文台 月球与深空探测重点实验室,北京 100012
  • 折叠

摘要

Abstract

To measure the thin plasma layer above the surface of the moon,via using radio occultation technique and coherent radio waves of the S/X band,dual-frequency measurements could be acquired at a given Earth-based receiving station.On the line-sight direction,the terrestrial ionosphere,interplanetary plasma and thin lunar ionosphere are mixed together,in order to investigate the relatively pure variation of ionospheric total electron content (TEC) surrounding the moon,Using the trend extrapolation method,the terrestrial ionosphere and interplanetary disturbance error influence could be eliminated,so as to estimate the fitting trend component.The TEC of lunar ionosphere is obtained about 10 -1 4/m2 ,after subtracting this trend component from the original observation data obtained at the tracking station.

关键词

月球电离层/电子总含量 (TEC)/无线电掩星

Key words

lunar ionosphere/total electron content/radio occultation

分类

天文与地球科学

引用本文复制引用

王震,王娜,平劲松..月球电离层掩星探测研究[J].深空探测学报,2014,(3):220-225,6.

基金项目

国家重点基础研究发展计划(973计划)项目(2015CB857101) (973计划)

深空探测学报

2096-9287

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