Remote radio tracking of CMEs in the solar corona and interplanetary medium

Details Remote radio tracking of CMEs in the solar corona and interplanetary medium Remote radio tracking of CMEs in the solar corona and interplanetary medium

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..653r&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 653-656 (1999).

Physics

2

Solar Wind Plasma, Sources Of Solar Wind, Radio, Microwave

Scientific paper

We use dynamic spectra that display the observed radio intensity as a function of inverse frequency and time for tracking CME associated radio emissions through the interplanetary medium. The analyses of these radio emissions directly reveal the dynamics of the CME-driven shock as well as the nature of the radiation mechanism. For the two examples illustrated, we deduce that the type II radio emissions were generated primarily at the harmonic of the plasma frequency and in the upstream region of the CME-driven shock. For the two events, which have very different speeds, we found no evidence for significant deceleration of the CME-driven shock as it propagated through the interplanetary medium.

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