Sources of interplanetary shocks

Details Sources of interplanetary shocks Sources of interplanetary shocks

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..15..355l&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 15, no. 8-9, p. 355-364

Computer Science

1

Interplanetary Space, Shock Waves, Solar Corona, Solar Flares, Solar Wind, Spatial Dependencies, Stellar Mass Ejection, Temporal Distribution, Data Correlation, Data Reduction, Density Distribution, Shock Wave Profiles, Solar Cycles, Stellar Models, Velocity Distribution

Scientific paper

The sources of interplanetary shocks are reviewed from the standpoint of today's knowledge. Recent progress from both new and accumulated observations and models indicates that contributions from the two major sources of the shocks: Coronal Mass Ejections (CMEs) and stream interactions, have distinctive radial, latitudinal and temporal dependencies. The need for global statistical surveys over serveral solar cycles, and models that take into account the complexity of the solar wind, is apparent from this current perspective.

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