Annotation
The distribution of the temperature versus the thickness in the chromosphere-corona transition region of the solar atmosphere on the assumption that the plasma heating by classical heat flux is balanced by the energy loss by radiation. It is shown that the transition region between the corona and chromosphere is a thin layer, to which, however, a simple collision approximation may be applied.
Received: 2010 May 14
Approved: 2011 April 13
PACS:
96.60.Na Chromosphere
96.60.P- Corona
96.60.Xy Transition region
96.60.P- Corona
96.60.Xy Transition region
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
O.V. Ptitsyna, B.V. Somov
Sternberg Astronomical Institute, Moscow University, Moscow, Russia
Sternberg Astronomical Institute, Moscow University, Moscow, Russia
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