Properties of metre-wavelength solar bursts associated with interplanetary type II emission

Details Properties of metre-wavelength solar bursts associated with interplanetary type II emission Properties of metre-wavelength solar bursts associated with interplanetary type II emission

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...91..159r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 91, March 1984, p. 159-168.

Physics

22

Interplanetary Space, Solar Flares, Solar Terrestrial Interactions, Type 2 Bursts, Very High Frequencies, Frequency Distribution, Magnetic Storms, Space Plasmas, Statistical Analysis

Scientific paper

A statistical analysis is used to determine the properties of metre-wavelength events which are associated with interplanetary type II bursts. It is found that the likelihood of an interplanetary type II burst is greatly increased if: (1) an associated metre-wavelength type II has a starting frequency less than 45 MHz; (2) a strong metre-wavelength continuum is present; (3) the type II contains herringbone fine structure; and (4) the metre-wavelength activity is accompanied by strong, long-lasting Hα and soft X-ray events.

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