Chemi-ionization and chemi-recombination processes in solar and stellar atmospheres.

Details Chemi-ionization and chemi-recombination processes in solar and stellar atmospheres. Chemi-ionization and chemi-recombination processes in solar and stellar atmospheres.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pobeo..54...35m&link_type=abstract

Publications of the Astronical Observatory of Belgrade, No. 54, p. 35 - 38

Astronomy and Astrophysics

Astronomy

Atomic Processes: Solar Atmosphere, Atomic Processes: Stellar Atmospheres

Scientific paper

Within the semi-classical approximation, chemi-ionization processes during symmetrical atom - Rydberg atom collisions were considered, as well as the inverse chemi-recombination processes during the scattering of free electrons by corresponding collisional ion-atom complexes and molecular ions. It has been shown that these processes must be taken into account when modelling the low-temperature layers of the solar atmosphere and atmospheres of some helium-rich stars.

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