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...
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| Veröffentlicht in: | Advances in Astronomy and Space Physics |
|---|---|
| Datum: | 2011 |
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| Format: | Artikel |
| Sprache: | Englisch |
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Advances in astronomy and space physics
2011
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/118985 |
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| 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. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| _version_ | 1862594853203869696 |
|---|---|
| author | Baran, O.A. |
| author_facet | Baran, O.A. |
| citation_txt | 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. |
| collection | DSpace DC |
| container_title | Advances in Astronomy and Space Physics |
| description | 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 shifted towards the boundaries in large granules; the temperature inversion takes place. The temporal changes of the shapes of the reconstructed distributions of the temperature and the vertical velocity on the subgranulation scales has been investigated. Also the effect of finite resolution on spatial variations of the velocities and temperaturein the solar photosphere has been estimated.
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| first_indexed | 2025-11-27T12:52:00Z |
| format | Article |
| fulltext | |
| id | nasplib_isofts_kiev_ua-123456789-118985 |
| institution | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| isbn | 987-966-439-367-3 |
| language | English |
| last_indexed | 2025-11-27T12:52:00Z |
| publishDate | 2011 |
| publisher | Advances in astronomy and space physics |
| record_format | dspace |
| spelling | Baran, O.A. 2017-06-02T18:36:50Z 2017-06-02T18:36:50Z 2011 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. 987-966-439-367-3 https://nasplib.isofts.kiev.ua/handle/123456789/118985 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 shifted towards the boundaries in large granules; the temperature inversion takes place. The temporal changes of the shapes of the reconstructed distributions of the temperature and the vertical velocity on the subgranulation scales has been investigated. Also the effect of finite resolution on spatial variations of the velocities and temperaturein the solar photosphere has been estimated. The authors are grateful to Dr. N. G. Shchukina for kindly proving the results of observations and to Dr. R. I. Kostik for data reduction. en Advances in astronomy and space physics Advances in Astronomy and Space Physics Structure of convective flows of the real Solar granulation Article published earlier |
| spellingShingle | Structure of convective flows of the real Solar granulation Baran, O.A. |
| title | Structure of convective flows of the real Solar granulation |
| title_full | Structure of convective flows of the real Solar granulation |
| title_fullStr | Structure of convective flows of the real Solar granulation |
| title_full_unstemmed | Structure of convective flows of the real Solar granulation |
| title_short | Structure of convective flows of the real Solar granulation |
| title_sort | structure of convective flows of the real solar granulation |
| url | https://nasplib.isofts.kiev.ua/handle/123456789/118985 |
| work_keys_str_mv | AT baranoa structureofconvectiveflowsoftherealsolargranulation |