MHD mesoscale interactions at the magnetopause and driven reconnection

Research output: Chapter in Book/Report/Conference proceedingChapter

6 Scopus citations

Abstract

A brief review of the theoretical development of the planetary dynamo problem and theoretical models of the solar wind-magnetosphere interaction, such as the reconnection, viscous interaction and impulsive penetration models, is given. MHD mesoscale physics in the non-uniform plasma interaction region should be applied in order to understand how the energy of motion of the magnetofluids is transferred into electromagnetic (E-M) energy. A macro-particle description involving compressional and shear Alfvenons has been introduced to give the particle-like behavior of the corresponding MHD waves [Song and Lysak, 1994]. The driven nature of the solar windmagnetosphere interaction and driven reconnection are discussed in terms of the interactions between Alfvenons and between Alfvenons and the ambient magnetic field. A unified model of the solar wind-magnetosphere interaction may be established on the basis of Alfvenon dynamics.

Original languageEnglish (US)
Title of host publicationPhysics of the Magnetopause, 1995
EditorsP. Song, M.F. Thomsen, B.U.O. Sonnerup
PublisherBlackwell Publishing Ltd
Pages349-356
Number of pages8
ISBN (Electronic)9781118663974
ISBN (Print)9780875900476
DOIs
StatePublished - 1995

Publication series

NameGeophysical Monograph Series
Volume90
ISSN (Print)0065-8448
ISSN (Electronic)2328-8779

Bibliographical note

Funding Information:
Acknowledgments. We would like to thank B. U. O. Sonnerup for very helpful suggestions and comments on the paper. We have also benefited from discussions with many of our colleagues, including C. Cattell, W. Dai, R. Elphic, G. Fasel, K.-H. Glassmeier, J. T. Gosling, W. J. Heikkila, H. Kawano, H. Kuo, G. Le, J. Lemaire, N. Lin, T. Lui, R. N. Lundin, Z. Ma, P. Newell, A. Otto, E. N. Parker, T.-D. Phan, T. A. Potemra, G. Rostoker, C. T. Russell, D. Sibeck. This work has been sup ported in part by NSF Grants ATM-9111791 and ATM-9301043 and by NASA Grants NAGW-2653 and NAGW-2690.

Publisher Copyright:
© 1995 by the American Geophysical Union.

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