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..153p&link_type=abstract

Journal de Physique Colloque, Tome 49, C1, p. 153 - 163

Astronomy and Astrophysics

Astrophysics

9

H Ii Regions:Plasma, Planetary Nebulae:Plasma, Plasma:Charge Transfer, Plasma:H Ii Regions, Plasma:Planetary Nebulae, Plasma:Solar Chromosphere, Plasma:Solar Corona, Solar Chromosphere:Plasma, Solar Corona:Plasma

Scientific paper

Charge exchanges are important for the ionization balance of many ions in either warm coronal plasmas or photoionized plasmas of astrophysics. Lines produced by charge exchange have been discovered in the spectrum of nebulae and probably the solar chromosphere. Introduction of charge exchanges modifies earlier views about the structure of some astrophysical objects. The nebulae appear as valuable "laboratories" to check theoretical charge exchange cross sections at very low energy. It is suggested that the detection of charge exchange lines in the solar spectrum would provide new insights into the dynamics of the interface between the chromosphere and the corona. It is pointed out that charge exchanges between heavy particles may have significant effects in the ionization front of some nebulae.

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