Magnetic reconnection events in the interplanetary space
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Magnetic field and plasma measurements in teh period of 1975–1981 with 0. 18-h averages from Helios spacecrafts are analyzed. It is discovered that magnetic reconnection phenomena exist in the interplanetary space. By means of the reconstruction of magnetic field configuration in the azimuth angle plane, it is found that the magnetic reconnection event with time scale of the order of day is a significant form of magnetic reconnection phenomena in the interplanetary space, which consists of a mediate body (or a plasma bulk) and two magnetic separator lines. It could originate from coronal mass ejection event or magnetic cloud in the interplanetary space. Numerical simulation has reproduced the basic characteristics of the magnetic reconnection events.
Keywordsinterplanetary space magnetic reconnection heliospheric physics
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- 1.Hones, E. W., Jr., Magnetic reconnection in space and laboratory plasma, inGeophysical Monograph (ed. Hones, E. W., Jr.), Washington, D.C.: AGU Publishers, 1984, 30: 21.Google Scholar
- 2.Axford, W. I., Magnetic field reconnection,Magnetic Reconnection in Space and Laboratory Plasmas, Geophysical Monograph (ed. Hones, E. W., Jr.), Washington, D.C.: AGU Publishers, 1984, 30: 1.Google Scholar
- 3.Cowley, S. W. H., Magnetic reconnection, inSolar System Magnetic Fields (ed. Priest, E. R.), Dordrecht: D. Reidel Publishing Company, 1985, 121–155.Google Scholar
- 11.Burlaga, L. F. E., Magnetic clouds, inPhysics and Chemistry in Space and Solar Physics, Vol. 21,Physics of the Inner Heliosphere II (eds. Schwenn, R., Marsch, E.), Berlin, Heidelberg: Springer-Verlag, 1991, 1–19.Google Scholar