New observations of solar noise storm radiation at decameter wavelengths

Details New observations of solar noise storm radiation at decameter wavelengths New observations of solar noise storm radiation at decameter wavelengths

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132..155t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, March 1991, p. 155-171. University of Maryland-supported research.

Physics

9

Decametric Waves, Noise Storms, Photosphere, Solar Corona, Solar Radio Bursts, Solar Storms, Magnetic Field Configurations, Solar Activity Effects, Solar Electrons, Solar Magnetic Field

Scientific paper

Multifrequency observations of storm continuum and other radio bursts are presented. Based on their positional study and their correlation with other coronal and photospheric features, the storm source is located in the magnetic field lines lying above a single bipolar active region. Energetic electrons trapped in the magnetic structures above the spots must be responsible for the storm radiation. Spontaneous emission of Langmuir waves by anisotropic distributions can explain both storm continumm and bursts self-consistently.

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