Abstract
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.
- Received 28 April 2012
- Publisher error corrected 24 August 2012
DOI:https://doi.org/10.1103/PhysRevLett.109.081101
© 2012 American Physical Society
Corrections
24 August 2012
Erratum
Publisher’s Note: Minimagnetospheres above the Lunar Surface and the Formation of Lunar Swirls [Phys. Rev. Lett. 109, 081101 (2012)]
R. A. Bamford, B. Kellett, W. J. Bradford, C. Norberg, A. Thornton, K. J. Gibson, I. A. Crawford, L. Silva, L. Gargaté, and R. Bingham
Phys. Rev. Lett. 109, 099902 (2012)
Focus
Magnetic Fields Explain Lunar Surface Features
Published 20 August 2012
A proposed explanation for puzzling features on the Moon involving small-scale magnetic fields has now been verified with a scaled-down version in the lab.
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