Annotation
We prove the stability of a previously obtained temperature-versus-thickness distribution in the solar chromosphere-corona transition region. The temperature distribution has been obtained on the assumption that the plasma heating by classical heat flux is balanced by the energy loss due to radiation.
Received: 2011 January 25
Approved: 2011 November 11
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 State Institute of Astronomy, Moscow State University, Moscow, 119191, Russia
Sternberg State Institute of Astronomy, Moscow State University, Moscow, 119191, Russia
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