Peculiarities of convective motions in the upper solar atmosphere. I-Reference-Cited by-同舟云学术

Peculiarities of convective motions in the upper solar atmosphere. I

Published:2010-10 Issue:5 Volume:26 Page:233-241
ISSN:0884-5913
Container-title:Kinematics and Physics of Celestial Bodies
language:en
Short-container-title:Kinemat. Phys. Celest. Bodies

Author:

Kostyk R. I.

Publisher

Allerton Press

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.3103/S0884591310050028.pdf

Reference24 articles.

1. M. I. Stodilka, “Temperature structure of the Actual Solar Granulation,” Kinem. Fiz. Nebes. Tel 19, 407–416 (2003) [Kinem. Phys. Celest. Bodies 19, 334 (2003)].

2. M. I. Stodilka, “Structure of Convective Motions in the Solar Photosphere,” Kinem. Fiz. Nebes. Tel 22, 260–270 (2006).

3. M. I. Stodilka, O. A. Baran, and S. Z. Malynych, “Peculiarities of the Convection in the Solar Photosphere,” Kinem. Fiz. Nebes. Tel 22, 173–182 (2006) [Kinem. Phys. Celest. Bodies 22, 134 (2006)].

4. M. I. Stodilka and O. A. Baran, “Structure of the Solar Photospheric Convection on Subgranulation Scales,” Kinem. Fiz. Nebes. Tel 24, 99–109 (2008) [Kinem. Phys. Celest. Bodies 24, 70 (2008)].

5. N. G. Shchukina and H. Bueno, “Fe I Lines in Cool Star Spectra: Non-LTE Effects in Atmosphere of Solar Type,” Kinem. Fiz. Nebes. Tel 14, 315–329 (1998).

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