Solar radio continuum storms and a breathing magnetic field model

Details Solar radio continuum storms and a breathing magnetic field model Solar radio continuum storms and a breathing magnetic field model

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975srcs.book......&link_type=abstract

Solar radio continuum storms and a breathing magnetic field model. Final report., by . Separate print Washington Data Processin

Computer Science

Magnetic Field Configurations, Solar Magnetic Field, Solar Radio Emission, Microwave Frequencies, Solar Storms, Sunspots, Type 3 Bursts

Scientific paper

Radio noise continuum emissions observed in metric and decametric wave frequencies are, in general, associated with actively varying sunspot groups accompanied by the S-component of microwave radio emissions. These continuum emission sources, often called type I storm sources, are often associated with type III burst storm activity from metric to hectometric wave frequencies. This storm activity is, therefore, closely connected with the development of these continuum emission sources. It is shown that the S-component emission in microwave frequencies generally precedes, by several days, the emission of these noise continuum storms of lower frequencies. In order for these storms to develop, the growth of sunspot groups into complex types is very important in addition to the increase of the average magnetic field intensity and area of these groups. After giving a review on the theory of these noise continuum storm emissions, a model is briefly considered to explain the relation of the emissions to the storms.

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