Type II solar radio bursts, interplanetary shocks, and energetic particle events

Details Type II solar radio bursts, interplanetary shocks, and energetic particle events Type II solar radio bursts, interplanetary shocks, and energetic particle events

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...282..339c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 282, July 1, 1984, p. 339-344. Previously announced in STAR as N83-17435.

Physics

Plasma Physics

85

Energetic Particles, International Sun Earth Explorer 3, Plasma Physics, Radio Astronomy, Radio Bursts, Frequency Ranges, Radio Frequencies, Solar Corona, Solar Flares, Wavelengths

Scientific paper

Using the ISEE-3 radio astronomy experiment data 37 interplanetary (IP) type II bursts have been identified in the period September 1978 to December 1981. These events and the associated phenomena are listed. The events are preceded by intense, soft X ray events with long decay times (LDEs) and type II and/or type IV bursts at meter wavelengths. The meter wavelength type II bursts are usually intense and exhibit herringbone structure. The extension of the herringbone structure into the kilometer wavelength range results in the occurrence of a shock accelerated (SA) event. The majority of the interplanetary type II bursts are associated with energetic particle events. These results support other studies which indicate that energetic solar particles detected at 1 A.U. are generated by shock acceleration. From a preliminary analysis of the available data there appears to be a high correlation with white light coronal transients.

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