Charge exchange in laboratory and astrophysical plasmas

Details Charge exchange in laboratory and astrophysical plasmas Charge exchange in laboratory and astrophysical plasmas

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jphys..49....1p&link_type=abstract

(IAU, ESA, CNRS, et al., Colloquium on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas, 102nd, Beaulieu-sur-Me

Physics

Plasma Physics

3

Charge Exchange, Cosmic Plasma, Laboratories, Plasma Physics, Tokamak Devices, Chromosphere, Hydrogen Atoms, Molecular Excitation, Nuclear Fusion, Photoionization, Planetary Nebulae, Stellar Coronas

Scientific paper

Charge exchanges involving excited states of hydrogen are discussed, with a focus on both laboratory and astrophysical plasmas mainly composed of hydrogen isotopes and helium. Both passive and active sources of neutral hydrogen in laboratory plasmas are considered, and a review of ion-ion charge exchange is given. The discussion of charge exchange in astrophysical plasmas outlines both solar coronal plasmas and nebular plasmas. The specific areas studied include corona equilibrium, the chromosphere-corona transition region, ionization balance of H in nebulae, thermal balance of nebulae, and a consideration of planetary nebulae as important astrophysical laboratories for the study of charge exchange.

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