Introduction of Lunar Ionosphere Research by RO Method
WANG Zhen1, WANG Na1, PING Jinsong2
Author information+
1. Xinjiang Astronomical Observatory,Chinese Academy of Sciences 2. Key Laboratory of Lunar and Planetary Exploration Research, National Astronomical Observatories, CAS
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History+
Received
Revised
27 Jul 2014
17 Aug 2014
Issue Date
20 May 2022
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 ~10-14 /m2, after subtracting this trend component from the original observation data obtained at the tracking station.
WANG Zhen, WANG Na, PING Jinsong.
Introduction of Lunar Ionosphere Research by RO Method. Journal of Deep Space Exploration, 2014, 1(3): 220‒225 https://doi.org/10.15982/j.issn.2095-7777.2014.03.010
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