Radio Tracking of a White-Light Coronal Mass Ejection from Solar Corona to Interplanetary Medium

Details Radio Tracking of a White-Light Coronal Mass Ejection from Solar Corona to Interplanetary Medium Radio Tracking of a White-Light Coronal Mass Ejection from Solar Corona to Interplanetary Medium

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...529l..53r&link_type=abstract

The Astrophysical Journal, Volume 529, Issue 1, pp. L53-L56.

Astronomy and Astrophysics

Astronomy

26

Sun: Solar-Terrestrial Relations, Sun: Activity, Sun: Corona, Sun: Flares, Sun: Radio Radiation

Scientific paper

For a solar flare/coronal mass ejection (CME) event on 1999 May 3, type II radio emissions were observed from the metric through the hectometric wavelength regimes. By comparing the dynamics of the CME with that implied by the frequency range and frequency drift rates of the type II radio emissions, it is concluded that the decametric-hectometric type II radio emissions were associated with the CME. The dynamics implied by the metric type II radio burst suggest a distinct coronal shock, associated with the flare, which only produced radio emissions in the low corona.

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