Expected IPS variations due to a disturbance described by a 3-D MHD model

Details Expected IPS variations due to a disturbance described by a 3-D MHD model Expected IPS variations due to a disturbance described by a 3-D MHD model

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36.1155t&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 36, Nov. 1988, p. 1155-1163.

Computer Science

11

Interplanetary Medium, Magnetohydrodynamic Stability, Scintillation, Solar Wind Velocity, Three Dimensional Models, Heliosphere, Interplanetary Magnetic Fields, Solar Flares, Time Dependence

Scientific paper

The variations of interplanetary scintillation due to a disturbance described by a three-dimensional, time-dependent, MHD model of the interplanetary medium are calculated. The resulting simulated IPS maps are compared with observations of real disturbances and it is found that there is some qualitative agreement. It is concluded that the MHD model with a more realistic choice of input conditions would probably provide a useful description of many interplanetary disturbances.

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