Time profiles of solar radio spikes

Details Time profiles of solar radio spikes Time profiles of solar radio spikes

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...231..202g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 1, May 1990, p. 202-212.

Astronomy and Astrophysics

Astrophysics

85

Electron Beams, Solar Corona, Solar Radio Bursts, Decimeter Waves, Solar Radio Emission, Type 3 Bursts

Scientific paper

High-resolution observations are carried out to study the time profiles of individual solar radio spikes. The time profiles show a characteristic exponential decay with frequency dependent decay rates. On the assumption of the plasma hypothesis, the following empirical relation between T and the electron density n was found the emitting region.

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