Mm- to cm-wavelength time delays in solar burst emission burst emission and the effect of varying magnetic field

Details Mm- to cm-wavelength time delays in solar burst emission burst emission and the effect of varying magnetic field Mm- to cm-wavelength time delays in solar burst emission burst emission and the effect of varying magnetic field

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8219124c&link_type=abstract

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Physics

Magnetic Variations, Solar Magnetic Field, Solar Radio Bursts, Time Lag, Emission Spectra, Maxima, Temporal Resolution, Wavelengths

Scientific paper

Certain solar bursts measured in the mm to cm wave range of frequencies present maximum emission not coincident in time. In some cases the emission is delayed towards lower frequencies which is in apparent contradiction with what would be expected in geometries commonly assumed in thermal models. An explanation is given which places the primary source at the top of a magnetic loop, the collisionless fronts formed moving downwards into the solar chromosphere with the addition of time varying magnetic field effects. The explanation predicts observed time delays for wavelengths situated in the optically thin part of the gyrosynchrotron burst emission spectrum.

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