Nonlinear development of convective instability within slender flux tubes. II. The effect of radiative heat transport-Reference-Cited by-同舟云学术

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Nonlinear development of convective instability within slender flux tubes. II. The effect of radiative heat transport

Published:1985-03 Issue:1 Volume:6 Page:21-34
ISSN:0250-6335
Container-title:Journal of Astrophysics and Astronomy
language:en
Short-container-title:Astrophys Astron

Author:

Venkatakrishnan P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF02719526.pdf

Reference11 articles.

1. Antia, H. M., Chitre, S. M. 1979Solar Phys.,63, 67.

2. Chandrasekhar, S. 1961,Hydrodynamic and Hydromagnetic Stability, Clarendon Press, Oxford

3. Defouw, R. J. 1970,Solar Phys.,14, 42.

4. Hasan, S. S. 1984,Astr, Astrophys., (in press).

5. Kato, S. 1966,Publ. astr. Soc. Japan,18, 201.

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1. Magnetic Flux Tubes and Activity on the Sun;Lectures on Solar Physics;2003

2. Radiative Transfer Effects and the Dynamics of Small‐Scale Magnetic Structures on the Sun;The Astrophysical Journal;2000-11-20

3. Properties of Convective Instability in a Vertical Photospheric Magnetic Flux Tube;The Astrophysical Journal;1999-09

4. On the stability of stationary flows in thin magnetic flux tubes;Geophysical & Astrophysical Fluid Dynamics;1998-11

5. The Theory of Sunspots;Sunspots: Theory and Observations;1992

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