The shape of a magnetic cloud in the solar wind

Details The shape of a magnetic cloud in the solar wind The shape of a magnetic cloud in the solar wind

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..583r&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, July-Aug. 1991, p. 583-586. In Russian.

Computer Science

2

Magnetic Clouds, Solar Flares, Solar Magnetic Field, Solar Wind, Toroidal Plasmas, Dynamic Pressure, Hydrostatic Pressure, Interplanetary Medium, Magnetic Field Configurations

Scientific paper

A self-consistent theoretical method is used to determine the shape of a magnetic cavity arising in the solar wind under the effect of the motion of a toroidal flare-generated magnetic cloud. Under the effect of solar-wind dynamic pressure, the cloud is compressed in the front part, while a magnetic tail is formed in the rear part. When the hydrostatic pressure of the solar wind is taken into account, the study indicates that collapse of the tail can occur and that a closed magnetic cavity of nonaxisymmetric toroidal configuration can be formed.

Affiliated with

Also associated with

No associations

Rating

The shape of a magnetic cloud in the solar wind does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The shape of a magnetic cloud in the solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The shape of a magnetic cloud in the solar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1727071