Determination of the electron concentration inhomogeneity in the quiet solar prominence

Details Determination of the electron concentration inhomogeneity in the quiet solar prominence Determination of the electron concentration inhomogeneity in the quiet solar prominence

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13c..61v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 13, p. 61

Physics

Solar Electrons, Electron Density Profiles, Solar Prominences, Nonuniform Plasmas, Balmer Series, Radiation Distribution, H Lines, Continuous Spectra

Scientific paper

We propose a method to determine the intensity of the recombination
radiation distribution at the hydrogen Balmer limit from electron
concentration values. The method is based on an analysis of the
continuum spectrum strengthening near the Balmer limit and is applicable
to emission features that are optically thin in the Balmer continuum.

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