Pulsations of microwave emission as a consequence of oscillatory transients in the solar atmosphere

Details Pulsations of microwave emission as a consequence of oscillatory transients in the solar atmosphere Pulsations of microwave emission as a consequence of oscillatory transients in the solar atmosphere

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...93..301z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 93, July 1984, p. 301-304.

Physics

4

Magnetoacoustic Waves, Microwave Emission, Solar Activity, Solar Oscillations, Solar Radio Bursts, Transient Oscillations, Magnetohydrodynamic Flow, Plasma Currents, Solar Atmosphere, Solar Magnetic Field

Scientific paper

The authors offer a new interpretation of the origin of oscillations in active regions. Quasi-periodic oscillation trains with periods of 3 min, 5 min, and ≅7 min arise due to slow oscillatory transients which accompany the appearance of plasma flow along the sunpot's magnetic field. In oscillatory transients of the fast type, occurring in current loop systems, the typical period of oscillations shifts towards values of the order of a second.

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