A numerical simulation of the interaction between a magnetic cloud and a high-speed stream

Details A numerical simulation of the interaction between a magnetic cloud and a high-speed stream A numerical simulation of the interaction between a magnetic cloud and a high-speed stream

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22...69h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 1, p. 69-75.

Astronomy and Astrophysics

Astrophysics

Scientific paper

A numerical simulation has been carried out of the interaction between a magnetic cloud and a tail-gating high-speed stream observed on 1978-08-27/28. The simulation has largely reproduced the observed profiles at 1 au. The results of the simulation show that the system led to the formation of a forward fast and a forward slow shock (originating in the cloud) and a rearward fast shock (originating in the stream), whose properties are modified in varying degrees by the cloud-stream interaction. Under the pursuit of the stream, the expansion of the magnetic cloud is suppressed at its rear end, and a high-temperature, high-density and strong magnetic field structure is formed there.

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