Stochastic Growth Theory of Type III Solar Radio Emission

Details Stochastic Growth Theory of Type III Solar Radio Emission Stochastic Growth Theory of Type III Solar Radio Emission

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...418..506r&link_type=abstract

Astrophysical Journal v.418, p.506

Astronomy and Astrophysics

Astronomy

39

Plasmas, Sun: Radio Radiation, Sun: Solar Wind

Scientific paper

The recently developed stochastic growth theory of type III radio
sources is extended to predict their electromagnetic volume emissivities
and brightness temperatures. Predicted emissivities are consistent with
spacecraft observations and independent theoretical constraints.

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