Turbulent Stark effect - Possible observational manifestations in solar flares

Details Turbulent Stark effect - Possible observational manifestations in solar flares Turbulent Stark effect - Possible observational manifestations in solar flares

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jqsrt..44..171t&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 44, July 1990, p. 171-175.

Physics

1

Plasma Oscillations, Plasma Turbulence, Solar Flares, Stark Effect, High Frequencies, Low Frequencies, Spectral Line Width

Scientific paper

For a variety of turbulence generation mechanisms in solar flares, an analysis is made of the mutual orientation of the electric field vectors of HF and LF plasma oscillations. Examination has been carried out separately for the three separate structural parts of a flare: the energy-release region, flare loops, and the chromospheric flare itself. The most favorable conditions for gaps to appear on hydrogen line profiles and consequently for HF turbulence diagnostics are found to exist in the lower parts of the flare loops. In order to detect the LF turbulence, it is useful to carry out spectral observations in the flare-ribbon region in the chromosphere.

Affiliated with

Also associated with

No associations

Rating

Turbulent Stark effect - Possible observational manifestations in solar flares 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 Turbulent Stark effect - Possible observational manifestations in solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbulent Stark effect - Possible observational manifestations in solar flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1095490