Structure of convective flows of the real Solar granulation

Домашня сторінка
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Фізико-технічні та математичні науки
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Відділення фізики і астрономії
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Advances in Astronomy and Space Physics
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Advances in Astronomy and Space Physics, 2011, том 1
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Advances in Astronomy and Space Physics, 2011, вип. 1-2
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dc.contributor.author	Baran, O.A.
dc.date.accessioned	2017-06-02T18:36:50Z
dc.date.available	2017-06-02T18:36:50Z
dc.date.issued	2011
dc.identifier.citation	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.	uk_UA
dc.identifier.isbn	987-966-439-367-3
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/118985
dc.description.abstract	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.	uk_UA
dc.description.sponsorship	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.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Advances in astronomy and space physics	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Structure of convective flows of the real Solar granulation	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA