A self-consistent model for the storm radio emission from the sun

Details A self-consistent model for the storm radio emission from the sun A self-consistent model for the storm radio emission from the sun

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132..173t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, March 1991, p. 173-193. University of Maryland-supported research.

Physics

12

Electron Capture, Electrostatic Waves, Self Consistent Fields, Solar Radio Bursts, Solar Radio Emission, Solar Storms, Brightness Temperature, Solar Activity, Solar Electrons, Solar Magnetic Field

Scientific paper

A self-consistent theoretical model for storm continuum and bursts is presented in which the Langmuir waves are emitted spontaneously by an anisotropic loss-cone distribution of electrons trapped in the magnetic field above active regions. These high-frequency electrostatic waves are assumed to coalesce with lower-hybrid waves excited either by the trapped protons or by weak shocks, making the observed brightness temperature equal to the effective temperature of the Langmuir waves. It is shown that whenever the collisional damping is more than the negative damping due to the anisotropic distribution, there is a steady emission of Langmuir waves responsible for the storm continuum.

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