Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes

Details Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..399v&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 399-402 (2010).

Computer Science

Solar Magnetism, Corona, Magnetohydrodynamics, Magnetic Field Effects, Electric And Magnetic Fields, Solar Magnetism, Coronal Mass Ejection, Magnetohydrodynamics And Plasmas, Magnetosheath

Scientific paper

It is widely accepted that magnetic disturbances around fast interplanetary magnetic clouds can play an important role in their geo-effectiveness. An analytical solution for magnetic field in the sheath region of a cylindrical magnetic cloud with an elliptical cross-section is proposed. Upstream magnetic field can have an arbitrary direction. Normal magnetic field components are conserved through the bow shock with a high accuracy.

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