Radiative recombination in some ions of astrophysical interest

Details Radiative recombination in some ions of astrophysical interest Radiative recombination in some ions of astrophysical interest

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...52..417n&link_type=abstract

Solar Physics, vol. 52, May 1977, p. 417-422. Research supported by the University Grants Commission.

Astronomy and Astrophysics

Astrophysics

Atomic Excitations, Gas Ionization, Radiative Recombination, Recombination Coefficient, Solar Atmosphere, Astronomical Models, Astrophysics, Ionization Cross Sections, Monatomic Gases, Photoionization, Solar Corona, Solar Physics, Solar Spectra, Temperature Effects

Scientific paper

Radiative recombination coefficients for some quadruply and quintuply
ionized atoms present in the sun and its atmosphere are investigated in
the temperature range from 10 to 10,000 K by using the method of
detailed balance. Simple expressions are given for a quick estimation.

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