Structure of convective flows on supergranular scales in the solar photosphere

The exploration of the velocity field of the real solar convection was performed using neutral iron line λ ≈ 639.3 nm profile from the observations with high spatial resolution. The inverse procedure was applied for each profile to reproduce the velocity field in the solar photosphere. Acoustic wave...

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Bibliographic Details
Published in:Advances in Astronomy and Space Physics
Date:2012
Main Author: Baran, O.A.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2012
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119189
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Structure of convective flows on supergranular scales in the solar photosphere / O.A. Baran // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 153-156. — Бібліогр.: 14 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine