Polarization and emission mode of solar radio spikes

Details Polarization and emission mode of solar radio spikes Polarization and emission mode of solar radio spikes

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...245..299g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 245, no. 1, May 1991, p. 299-309. Research supported by CNR and Ministero dell

Mathematics

Logic

48

Polarized Electromagnetic Radiation, Solar Corona, Solar Flares, Solar Radio Emission, Type 3 Bursts, H Alpha Line, Microwave Emission, Type 4 Bursts

Scientific paper

The observed polarization characteristics of solar millisecond
decimetric and microwave spike emission are discussed. The effect of
these characteristics on the emission mode is considered. It is found
that strong polarization is not inherent to all spike observations. Any
polarization degree may be observed with similar probability.

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