Observational aspects of the study of plasma turbulence in solar flares

Details Observational aspects of the study of plasma turbulence in solar flares Observational aspects of the study of plasma turbulence in solar flares

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jqsrt..44..177f&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 44, July 1990, p. 177-184.

Physics

Plasma Diagnostics, Plasma Frequencies, Plasma Turbulence, Solar Flares, Spectral Line Width, Balmer Series, Chromosphere, Plasma Oscillations

Scientific paper

Using two techniques (the polarization method and the Baranger-Mozer
method) a study has been made of plasma turbulence in solar emission
features. The study suggests the conclusion that the 0.02-0.03 plasma
turbulence level (E = 1-2 kV/cm seems to be the highest achieved in
flares.

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