An Alternative Approach to Explaining Magnetospheric Processes

dc.creatorPonomarev, E. A.
dc.creatorSedykh, P. A.
dc.date2004-07-28
dc.date.accessioned2026-07-07T05:52:22Z
dc.date.available2026-07-07T05:52:22Z
dc.descriptionThis paper gives a brief outline of the progression from the first substorm model developed in [Ponomarev, 1985; Sedykh, Ponomarev, 2002] based on C.F. Kennel's ideas, to the present views about the mechanism by which solar wind kinetic energy is converted to electromagnetic energy at the Bow Shock and by which this energy is transferred to the magnetosphere in the form of current; about the transformation of the energy of this current to gas kinetic energy of convecting plasma tubes, and, finally, the back transformation of gas kinetic energy to electromagnetic energy in secondary magnetospheric MHD generators. The questions of the formation of the magnetospheric convection system, the nature of substorm break-up, and of the matching of currents in the magnetosphere-ionosphere system are discussed.
dc.descriptionThe paper was presented on the International Conference on Substorms-7 (Levi,Lapland,Finland; 21-27 March 2004)
dc.identifierhttps://arxiv.org/abs/physics/0407139
dc.identifierhttp://arxiv.org/abs/physics/0407139
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/86301
dc.subjectSpace Physics
dc.subjectGeophysics
dc.titleAn Alternative Approach to Explaining Magnetospheric Processes
dc.typetext

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