Velocity profiles of interplanetary shocks

Details Velocity profiles of interplanetary shocks Velocity profiles of interplanetary shocks

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.703c&link_type=abstract

In JPL Solar Wind Five p 703-709 (SEE N84-13067 03-92)

Physics

9

Interplanetary Medium, Radio Bursts, Seismic Waves, Shock Wave Profiles, Solar Corona, Shock Wave Propagation, Type 2 Bursts, Velocity Distribution, Wave Interaction

Scientific paper

The type 2 radio burst was identified as a shock propagating through solar corona. Radio emission from shocks travelling through the interplanetary (IP) medium was observed. Using the drift rates of IP type II bursts the velocity characteristics of eleven shocks were investigated. It is indicated that shocks in the IP medium undergo acceleration before decelerating and that the slower shocks take longer to attain their maximum velocity.

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