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INTERNATIONAL JOURNAL OF GEOMAGNETISM AND AERONOMY, VOL. 7, GI3002, doi:10.1029/2005GI000133, 2007

Discussion paper: Comments on physical properties of strongest perturbations on the Sun in the heliosphere and the magnetosphere

O. S. Veselovsky

Institute of Nuclear Physics, Moscow State University Moscow Russia
Also at Space Research Institute, Russian Academy of Sciences Moscow Russia


I. S. Yakovchouk

Institute of Nuclear Physics, Moscow State University Moscow Russia


Abstract

[1]  Strongest energy releases on the Sun are manifested as coronal mass ejections and solar flares. They are driven by subphotospheric thermal and electromagnetic energy fluxes. We consider recent examples showing that their heliospheric and magnetospheric consequences could be similar or rather different from case to case. Common and specific features can be expressed and delimited when using dimensionless parameters. A universal geometry scenario for these processes does not exist.

Received 24 December 2005; accepted 15 August 2007; published 20 November 2007.

Keywords: heliosphere; magnetosphere of the Sun; coronal mass ejections; solar flares.

Index Terms: 7519 Solar Physics, Astrophysics, and Astronomy: Flares; 2788 Magnetospheric Physics: Magnetic storms and substorms (7954); 7807 Space Plasma Physics: Charged particle motion and acceleration.

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Citation: Veselovsky, O. S., and I. S. Yakovchouk (2007), Discussion paper: Comments on physical properties of strongest perturbations on the Sun in the heliosphere and the magnetosphere, Int. J. Geomagn. Aeron., 7, GI3002, doi:10.1029/2005GI000133.