Type III bursts and coronal temperature

Details Type III bursts and coronal temperature Type III bursts and coronal temperature

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...71..381k&link_type=abstract

Solar Physics, vol. 71, June 1981, p. 381-384.

Physics

Plasma-Particle Interactions, Relativistic Electron Beams, Solar Corona, Solar Temperature, Type 3 Bursts, Distribution Functions, Electrostatic Waves, Flux Density, Plasma Density

Scientific paper

Numerical solution of the interaction of evolutionary electron beam with
coronal plasma shows that the velocity of packet of the generated
Langmuir's waves increases with the increase of coronal temperature.
This effect can be manifested by a dependence of the drift of type III
bursts on the coronal temperature.

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