Evidence for arc SEC radio burst sources in the upper corona

Details Evidence for arc SEC radio burst sources in the upper corona Evidence for arc SEC radio burst sources in the upper corona

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...84..361m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 84, April 1983, p. 361-369. Research supported by the Australian Research Grants Committee.

Physics

2

Magnetohydrodynamic Waves, Plasma Radiation, Solar Corona, Solar Radio Bursts, Solar Spectra, Fine Structure, Particle Acceleration, Plasma Drift, Plasma Frequencies, Wave Propagation

Scientific paper

Some interpretations of solar S burst spectra are presented. It is shown
that the spectra provide evidence for small (≡ 500 km) radio
sources in the corona which radiate at the fundamental plasma frequency.
The possibility of S burst fringes corresponding to coronal MHD waves of
wavelength λ ≅ 103 km is discussed.

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