Structure of convective flows of the real Solar granulation

The temperature and velocity field within granular cells has been studied by solving the nonequilibrium inverse radiative transfer problem using neutral iron line λ ≈ 523.4 nm profiles. The results are the following: the temperature and velocity maxima do not always coincide and the maxima can be sh...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Datum:2011
1. Verfasser: Baran, O.A.
Format: Artikel
Sprache:English
Veröffentlicht: Advances in astronomy and space physics 2011
Schriftenreihe:Advances in Astronomy and Space Physics
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/118985
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Structure of convective flows of the real Solar granulation / O.A. Baran // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 53-56. — Бібліогр.: 15 назв. — англ.

Institution

Digital Library of Periodicals of National Academy of Sciences of Ukraine