On the field configuration in magnetic clouds

Details On the field configuration in magnetic clouds On the field configuration in magnetic clouds

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.731g&link_type=abstract

In JPL Solar Wind Five p 731-733 (SEE N84-13067 03-92)

Computer Science

Numerical Analysis

30

Interplanetary Medium, Magnetic Clouds, Magnetic Effects, Magnetic Properties, Magnetohydrodynamics, Plasma Clouds, Azimuth, Dynamic Models, Magnetic Fields, Numerical Analysis, Radial Velocity, Space Charge

Scientific paper

Interplanetary magnetic clouds are represented by cylindrically symmetric equilibrium solutions of the MHD-equations. The radial magnetic pressure gradient of the force-free field is balanced by the curvature stress. The field inside is essentially parallel to the cylinder axis, far outside it is oriented in azimuthal direction. These configurations therefore differ from the non-selfconsistent model proposed by Klein and Burlaga (1982), where the field lines are tightly wound even near the axis.

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