Coronal and interplanetary Type 2 radio emission

Details Coronal and interplanetary Type 2 radio emission Coronal and interplanetary Type 2 radio emission

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sici.symp...25c&link_type=abstract

In Alabama Univ., Huntsville. STIP Symposium on Physical Interpretation of Solar/Interplanetary and Cometary Intervals p 25 (SEE

Physics

Interplanetary Medium, Intervals, Radio Emission, Solar Corona, Solar Radio Bursts, Shock Waves, Solar Wind, Stellar Mass Ejection, X Ray Spectra

Scientific paper

Several observations suggest that the disturbances which generate coronal (meter wavelength) type II radio bursts are not driven by coronal mass ejections (CMEs). A new analysis using a large sample of metric radio bursts and associated soft X-ray events provides further support for the original hypothesis that type II-producing disturbances are blast waves generated at the time of impulsive energy release in flares. Interplanetary (IP) shocks, however, are closely associated with CMEs. The shocks responsible for IP type II events (observed at kilometer wavelengths) are associated with the most energetic CMEs.

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