Persistent 1.5s oscillations superimposed at a solar burst observed at two mm-wavelengths

Details Persistent 1.5s oscillations superimposed at a solar burst observed at two mm-wavelengths Persistent 1.5s oscillations superimposed at a solar burst observed at two mm-wavelengths

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8327948z&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Microwaves, Oscillations, Radio Astronomy, Solar Radio Bursts, Cross Correlation, Emission Spectra, Interferometry, Magnetically Trapped Particles, Optical Thickness, Sunspots

Scientific paper

Long-enduring quasi-periodic oscillations (1.5s) superimposed to a solar burst were observed simultaneously at two different mm-wavelengths (22 GHz and 44 GHz). The oscillations were present throughout the burst duration (about 10 min), and were delayed at 44 GHz with respect to 22 GHz by 0.3s. The relatives amplitude of the oscillation was of about 20 percent at 44 GHz and of about 5 percent at 22 GHz. Interferometer measurements at 10.6 GHz indicated the burst source stable within 1 arcsec. HeD3 line flare indicated two persistent small spots separated by about 10 arcsec. The 22/44 GHz burst position has good correspondence with the HeD3 spots' location. The oscillations displays features which appear to distinguish them from ultrafast time structures found in other bursts. One possible interpretation was suggested by assuming a modulation of the gyrosynchrotron emission of trapped electrons by a variable magnetic field on a double burst source, optically thin at 44 GHz and with optical thickness or approximately 0.3 at 22 GHz.

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