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Solar wind‐generated current in the Lunar Dust Experiment
Author(s) -
Xie Lianghai,
Zhang Xiaoping,
Zheng Yongchun,
Guo Dawei
Publication year - 2016
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2016gl068640
Subject(s) - solar zenith angle , zenith , current (fluid) , solar wind , environmental science , exosphere , atmospheric sciences , altitude (triangle) , physics , drift current , electric field , convection , computational physics , geophysics , ion , meteorology , plasma , optics , geometry , mathematics , quantum mechanics , thermodynamics
Measurements from the Lunar Dust Experiment (LDEX) show that the current associated with lofted lunar dust lacks an altitude dependence, implying that the current may come from other sources. Here we present some evidences for solar wind (SW)‐generated current. Direct SW influx on the nightside can cause a large current, and the backscattered energetic neutral atoms (ENAs) on the dayside can bring a good correlation between the current and SW density. It is found that the current favors a lower SW speed and a smaller SW incident angle, but the dependences are also affected by the solar zenith angle (SZA) and the scattering function of ENAs. Picked‐up ions can enhance the current when the angle between the convection electric field and LDEX's normal is larger than 90°. But when the angle is smaller than 90°, the enhancement is negligible.