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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| Published in: | Advances in Astronomy and Space Physics |
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| Date: | 2012 |
| Main Author: | |
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2012
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| 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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