Physics
Scientific paper
Nov 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ssrv...24..259b&link_type=abstract
Space Science Reviews, vol. 24, Nov. 1979, p. 259-346. Research supported by the Department of Space of India.
Physics
4
Decametric Waves, High Resolution, Noise Storms, Radio Observation, Solar Corona, Solar Radio Bursts, Photosphere, Polarization Characteristics, Solar Wind, Spectral Resolution, Stellar Models
Scientific paper
The current knowledge of high resolution observations at decameter wavelengths of the quiet sun, the slowly varying component, type I to V bursts and noise storms are summarized. These observations produced important physical parameters of the solar corona and the dynamical processes around the 2 solar radius from the photosphere where transition from closed to open field lines takes place and the solar wind builds up. The decametric noise bursts, the angular sizes of noise storm sources, and polarization information of decametric continuum and bursts were discussed, showing that decametric solar burst intensities are deeply modulated by scintillations in the earth ionosphere. Models and theories of the metric and decametric noise storms proposed so far were examined, and a more satisfactory model which explains the 'BF' type bursts and conventional noise storms bursts at decametric wavelengths was suggested.
Bhonsle Rajaram V.
Degaonkar S. S.
Sawant Hanumant S.
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