Enhancement of the solar X-ray line intensities due to dielectronic recombination as an excitation process

Details Enhancement of the solar X-ray line intensities due to dielectronic recombination as an excitation process Enhancement of the solar X-ray line intensities due to dielectronic recombination as an excitation process

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41...97a&link_type=abstract

Solar Physics, vol. 41, Mar. 1975, p. 97-107. Research supported by the Council of Scientific and Industrial Research and Aligar

Physics

6

Electron Impact, Line Spectra, Recombination Reactions, Solar Spectra, Solar X-Rays, X Ray Spectra, Atomic Excitations, Electron Density (Concentration), Electron Recombination, Ion Recombination, Radiant Flux Density, Spectrum Analysis

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1975SoPh...41...97A

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