Properties of metre-wavelength solar bursts associated with coronal mass ejections

Details Properties of metre-wavelength solar bursts associated with coronal mass ejections Properties of metre-wavelength solar bursts associated with coronal mass ejections

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..105..149r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 105, May 1986, p. 149-171. DOD-supported research.

Physics

19

Coronal Loops, Solar Corona, Solar Radio Bursts, Stellar Mass Ejection, Continuous Radiation, Electron Acceleration, Frequency Distribution, Radio Spectra, Solar X-Rays, Type 2 Bursts, Velocity Distribution

Scientific paper

An investigation is made to determine the relationship between a coronal mass ejection (CME) and the characteristics of associated metre-wave activity. It is found that (1) the CME width and leading edge velocity can be highly influential in determining the intensity, spectral complexity and frequency coverage of both type II and continuum bursts; (2) the presence of a CME is possibly a necessary condition for the production of a metric continuum event and (3) metric continuum bursts as well as intense, complex type II events are preferentially associated with strong, long lasting soft X-ray events.

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