Fine spectral structures in decametric noise storms and coronal irregularities

Details Fine spectral structures in decametric noise storms and coronal irregularities Fine spectral structures in decametric noise storms and coronal irregularities

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983srs..work..127s&link_type=abstract

Solar radio storms, p. 127 - 141

Physics

Decametric Waves, Solar Corona, Solar Magnetic Field, Solar Storms, Absorption Spectra, Bandwidth, Curvature, Drift Rate, Plasma Frequencies, Solar Wind

Scientific paper

With high sensitivity/time/frequency resolution various spectral features in decametric noise storms burst were observed. These various spectral features, are explained in terms of propagation effect and/or induced scattering of Langmuir waves to transverse waves on thermal ions, by various researchers. Recently a few more powerful decametric radio telescopes have gone into operation. Various aspects of decametric noise storms are updated and a possible noise storm model explaining fine spectral features is discussed.

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