On the origin of continuum emission during decametric solar noise storms

Details On the origin of continuum emission during decametric solar noise storms On the origin of continuum emission during decametric solar noise storms

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96..371l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, April 1985, p. 371-380.

Physics

1

Continuous Radiation, Decametric Waves, Noise Storms, Solar Radio Emission, Solar Storms, Electron Distribution, Solar Corona, Solar Magnetic Field, Solar Wind

Scientific paper

The stationary current of diffusely-distributed super-thermal electrons along a weakly inhomogeneous coronal magnetic field is considered as a possible model of the noise storm continuum source in decametric wavelengths. It is shown that the realization of such a streaming leads to a considerably increased level of plasma noise in the diffuse component region and then to enhanced radio emission from this region.

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