The shape of buoyant coronal loops in a magnetic field and the eruption of coronal transients and prominences
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF00158500.pdf
Reference18 articles.
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3. Low, B. C.: 1982, Rev. Geophys. Space Phys. 20, 145.
4. Melville, J. P., Hood A, and Priest, E. R.: 1983, Solar Phys. 87, 301.
5. Parker, E. N.: 1955, Astrophys. J. 121, 491.
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