The necessity of fundamental emission in type III bursts

Details The necessity of fundamental emission in type III bursts The necessity of fundamental emission in type III bursts

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41..439s&link_type=abstract

Solar Physics, vol. 41, Apr. 1975, p. 439-447.

Physics

5

Brightness Temperature, Plasma Frequencies, Plasma Waves, Radio Bursts, Type 3 Bursts, Emission Spectra, Harmonic Radiation, Plasma Density, Relativistic Particles, Shock Waves, Transverse Waves

Scientific paper

Previous observations of some type III bursts are investigated to determine whether conclusions that type III bursts occur near twice the plasma frequency between 10 and 215 solar radii are consistent with predictions based on nonlinear plasma theory. Transverse wave emission at the fundamental and harmonic is analyzed, and it is shown that the burst emission must be near the plasma frequency in the region between 10 and 50 solar radii in order to be consistent with the observed steep rise in brightness temperature for these bursts. Comparison of experimental and theoretical results indicates that type III emission in the 10 to 50-solar radii region occurs at the fundamental and that no conclusions can be made about emission beyond that region.-

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