Characteristics of shocks in the solar corona, as inferred from radio, optical, and theoretical investigations

Details Characteristics of shocks in the solar corona, as inferred from radio, optical, and theoretical investigations Characteristics of shocks in the solar corona, as inferred from radio, optical, and theoretical investigations

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ssrv...32...11m&link_type=abstract

(Slovenska Akademia Vied, IAU, and COSPAR, Study of Travelling Interplanetary Phenomena Workshop on Shock Waves in the Solar Cor

Computer Science

31

Magnetohydrodynamic Waves, Shock Wave Propagation, Solar Corona, Solar Flares, Type 2 Bursts, Computerized Simulation, Velocity Distribution

Scientific paper

Solar radio bursts of spectral type II provide one of the chief diagnostics for the propagation of shocks through the solar corona. Radio data on the shocks are compared with computer models for propagation of fast-mode MHD shocks through the solar corona. Data on coronal shocks and high-velocity ejecta from solar flares are then discussed in terms of a general model consisting of three main velocity regimes.

Affiliated with

Also associated with

No associations

Rating

Characteristics of shocks in the solar corona, as inferred from radio, optical, and theoretical investigations 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 Characteristics of shocks in the solar corona, as inferred from radio, optical, and theoretical investigations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristics of shocks in the solar corona, as inferred from radio, optical, and theoretical investigations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1020240