On the intermediate drift burst model

Details On the intermediate drift burst model On the intermediate drift burst model

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..110..381m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 110, no. 2, 1987, p. 381-389.

Physics

26

Drift Rate, Fine Structure, Solitary Waves, Stellar Models, Type 4 Bursts, Whistlers, Absorption Spectra, Coronal Loops, Emission Spectra, Magnetic Field Configurations, Solar Magnetic Field

Scientific paper

A modification of the presently existing intermediate drift burst model by Kuijpers (1975) and Bernold (1983) is suggested. It is shown that whistler solitons cannot be responsible for intermediate drift bursts. Here, they are interpreted as the radio signature of localized formstable whistler wave packets propagating along the magnetic field in a coronal loop. In the frame of this modified model, the magnetic field strengths derived from fiber burst data agree with previous estimates by Dulk and McLean (1978).

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