Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242..692s&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Feb. 15, 1990, p. 692-697. Research supported by S
Astronomy and Astrophysics
Astrophysics
22
Atomic Collisions, Collision Rates, Electron Scattering, Hydrogen Atoms, Hydrogen Plasma, Plasma Temperature, Astrophysics, Born Approximation, Oscillator Strengths
Scientific paper
Extensive electron-hydrogen atom scattering calculations have recently been performed using a hybrid model which employs intermediate energy R-matrix theory, pseudostate close-coupling, and the second Born approximation. The resulting 1s-2s and 1s-2p cross-sections have been integrated over a Maxwellian electron energy distribution to yield effective collision strengths and rate coefficients for excitation to the n = 2 levels of the hydrogen atom. These parameters are reported for plasma temperatures ranging from 5000 to 500,000, and are fitted to simple analytic formulas.
Burke James P.
Scholz T. T.
Scott M. P.
Walters H. R. J.
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