Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...239l...1g&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 239, no. 1-2, Nov. 1990, p. L1-L4.
Astronomy and Astrophysics
Astrophysics
35
Solar Radiation, Solar Radio Bursts, Radiation Spectra, Radio Emission, Synchrotron Radiation
Scientific paper
Observational evidence is presented for coherent solar radio spike radiation at harmonics up to s = 6, showing that, contrary to the predictions of the common electron cyclotron maser theories, millisecond spike burst radiation between 300 and 3000 MHz is not restricted to the fundamental frequency and its very lowest harmonics (s = 2,3). Radiation spectra were recorded by two frequency-agile receivers near Zurich (Switzerland), between 100 and 3000 MHz, at high time and frequency resolution. Harmonic ratios close to 2:3 and 3:4 were found, and some events showed three bands with ratios close to 2:3:4; in one case, three very similar separated branches of individual spike bursts were found with a frequency ratio of 3.0:4.0:5.05. It is suggested that these observations may be interpreted in terms of relativistic gyrosynchrotron maser.
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