Study of the solar corona using radio and space observations

Details Study of the solar corona using radio and space observations Study of the solar corona using radio and space observations

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979colo.rept.....d&link_type=abstract

Final Technical Report, 1 Oct. 1978 - 31 Oct. 1979 Colorado Univ., Boulder.

Other

Coronas, Dynamic Characteristics, Magnetic Fields, Observation, Solar Corona, Energy Transfer, Light (Visible Radiation), Papers, Radio Bursts, Thermal Diffusivity

Scientific paper

Optical, radio and X-ray evidence of violent mass motions in the corona has existed for some years but only recently have the form, nature, frequency and implication of the transients become obvious. The observed properties of coronal transients concentrating on the white-light and radio manifestations. The possible mechanisims involved in the radio bursts are discussed. The estimates of various forms of energy are reviewed. It appears that the magnetic energy transported from the Sun by the transient exceeds that of any other form, and that magnetic forces dominate in the dynamics of the motions. The conversion of magnetic energy into mechanical energy, by expansion of the fields, provides a possible driving force for the coronal and interplanetary shock waves.

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