Physical Conditions in Solar Coronal Holes on the Base of Non-LTE Calculations

Details Physical Conditions in Solar Coronal Holes on the Base of Non-LTE Calculations Physical Conditions in Solar Coronal Holes on the Base of Non-LTE Calculations

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..259..235m&link_type=abstract

The Dynamic Sun, Proceedings of the Summerschool and Workshop held at the Solar Observatory Kanzelhöhe, Kärnten, Austria, August

Astronomy and Astrophysics

Astrophysics

Scientific paper

We show that the intensity variations of the He I 10830 Å and the
H Lyα lines which are observed in coronal holes and
quiet regions can be explained by the model variations in the upper
chromosphere.

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