A torsional wave model for solar radio pulsations

Details A torsional wave model for solar radio pulsations A torsional wave model for solar radio pulsations

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...87..177t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 87, Aug. 1983, p. 177-186.

Physics

16

Magnetohydrodynamic Waves, Pulsed Radiation, Solar Oscillations, Solar Radio Emission, Electromagnetic Pulses, Synchrotron Radiation

Scientific paper

One of the widely accepted models for solar radio pulsations invokes radial oscillations of a magnetic flux tube. Due to acoustic, radiative damping, this theory does not easily explain the long length of the pulse trains, the large modulation depths or the great stability of the pulse repetition rate often observed. Torsional waves efficiently modulate synchrotron emission, and since they do not undergo radiative damping, can produce stable pulse repetition rates and long pulse trains.

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