Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.133..307g&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 133, no. 2, 1987, p. 307-315.
Astronomy and Astrophysics
Astrophysics
1
Atmospheric Boundary Layer, Late Stars, Stellar Atmospheres, Stellar Temperature, Vertical Distribution, Abundance, Chromosphere, Electron Energy, Neutral Particles, Photosphere
Scientific paper
An attempt is made to demonstrate the possibility of the existence of one more layer - pinchrosphere - in the structure of atmospheres of late-type stars - later than G5. Pinchrosphere is the coolest layer with very low electron temperature, 5500 K. It is located on the photosphere and near the inner boundary of the chromosphere. Practically all elements in the pinchrosphere, particularly hydrogen and magnesium, are in a neutral state. The main physical parameters of the pinchrosphere are derived.
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