Minimagnetospheres above the Lunar Surface and the Formation of Lunar Swirls

被引:46
作者
Bamford, R. A. [1 ,3 ]
Kellett, B. [1 ]
Bradford, W. J. [1 ]
Norberg, C. [2 ]
Thornton, A. [3 ]
Gibson, K. J. [3 ]
Crawford, I. A. [4 ]
Silva, L. [5 ]
Gargate, L. [5 ]
Bingham, R. [6 ,7 ]
机构
[1] Rutherford Appleton Lab, RAL Space, Didcot OX11 0QX, Oxon, England
[2] Swedish Inst Space Phys, SE-98128 Kiruna, Sweden
[3] Univ York, Dept Phys, York Plasma Inst, York YO10 5DD, N Yorkshire, England
[4] Univ London Birkbeck Coll, Dept Earth & Planetary Sci, London WC1E 7HX, England
[5] Inst Super Tecn, P-104900 Lisbon, Portugal
[6] Univ Strathclyde, Glasgow, Lanark, Scotland
[7] Rutherford Appleton Lab, Cent Laser Facil, Didcot OX11 0QX, Oxon, England
基金
英国工程与自然科学研究理事会;
关键词
SOLAR-WIND; PROSPECTOR; MISSION; PLASMAS; MOON;
D O I
10.1103/PhysRevLett.109.081101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this paper we present in situ satellite data, theory, and laboratory validation that show how small-scale collisionless shocks and minimagnetospheres can form on the electron inertial scale length. The resulting retardation and deflection of the solar wind ions could be responsible for the unusual "lunar swirl'' patterns seen on the surface of the Moon.
引用
收藏
页数:5
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