Magnetic Reconnection in the Near Venusian Magnetotail

Author:

Zhang T. L.12,Lu Q. M.1,Baumjohann W.2,Russell C. T.3,Fedorov A.4,Barabash S.5,Coates A. J.6,Du A. M.7,Cao J. B.8,Nakamura R.2,Teh W. L.2,Wang R. S.2,Dou X. K.1,Wang S.1,Glassmeier K. H.9,Auster H. U.9,Balikhin M.10

Affiliation:

1. Chinese Academy of Sciences Key Laboratory of Geospace Environment, University of Science and Technology of China, Hefei 230026, China.

2. Space Research Institute, Austrian Academy of Sciences, Graz 8042, Austria.

3. Institute of Geophysics and Planetary Physics, University of California, Los Angeles (UCLA), CA 90095–1567, USA.

4. Centre d’Etude Spatiale des Rayonnements, Toulouse 31028, France.

5. Swedish Institute of Space Physics, Kiruna 98128, Sweden.

6. Mullard Space Science Laboratory, University College London, London RH5 6NT, UK.

7. Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.

8. Space Science Institute, Beihang University, Beijing 100191, China.

9. Institut für Geophysik und Extraterrestrische Physik, Technischen Universität Braunschweig, Braunschweig 38106, Germany.

10. Department of Automatic Control and Systems Engineering, University of Sheffield, Sheffield S1 3JD, UK.

Abstract

Magnetic Reconnection Magnetic reconnection (MR) has been observed in the magnetospheres of planets with an intrinsic magnetic field, such as Earth, Mercury, Jupiter, and Saturn. MR is a universal plasma process that occurs in regions of strong magnetic shear and converts magnetic energy into kinetic energy. On Earth, MR is responsible for magnetic storms and auroral events. Using data from the European Space Agency Venus Express spacecraft, Zhang et al. (p. 567 , published online 5 April; see the Perspective by Slavin ) present surprising evidence for MR in the magnetosphere of Venus, which is a nonmagnetized body.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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