Cyclotron radio emission in plasma with steep temperature gradient

Details Cyclotron radio emission in plasma with steep temperature gradient Cyclotron radio emission in plasma with steep temperature gradient

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...94..105s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 94, Aug. 1984, p. 105-115.

Physics

1

Cyclotron Radiation, Electron Distribution, Plasma Radiation, Solar Radio Emission, Sunspots, Brightness Temperature, Centimeter Waves, Distribution Functions, Electron Energy, Temperature Gradients, Velocity Distribution

Scientific paper

In the paper it is investigated how the non-Maxwellian electron velocity distribution function associated with steep temperature gradient affects the cyclotron radio emission at centimeter wavelengths. The results obtained were used to calculate the distribution of the brightness temperature across a sunspot. The presence of the large electron temperature gradient in the transition region may lead to a significant increase of the observed brightness temperature (up to several tens of percent) in comparison with the brightness temperature obtained by assumption of the Maxwellian distribution function.

Affiliated with

Also associated with

No associations

Rating

Cyclotron radio emission in plasma with steep temperature gradient does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cyclotron radio emission in plasma with steep temperature gradient, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cyclotron radio emission in plasma with steep temperature gradient will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1678950