Type IIIb bursts and their fine structure in frequency band 18-30 MHz

Details Type IIIb bursts and their fine structure in frequency band 18-30 MHz Type IIIb bursts and their fine structure in frequency band 18-30 MHz

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1206..445m&link_type=abstract

ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: Proceedings of the 4th Gamow International Conference on Astrophysics and Cosmology Afte

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Astronomical Observations, Radio Telescopes, Astronomical Spectra, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Radio Telescopes And Instrumentation, Heterodyne Receivers, Spectroscopy And Spectrophotometry

Scientific paper

This paper deals with Type IIIb bursts, which were observed in the frequency band from 18 to 30 MHz. These bursts have fine frequency structures contrary to usual Type III bursts. The main properties of Type IIIb bursts such as number of striae in a burst, their frequency drift rates, durations, frequency widths of stria, emission fluxes are presented. It is also shown that parameters of stria bursts depend on the position of active areas on the solar disk.

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