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Two-dimensional pressure structure of a coronal loop

โœ Scribed by V. Krishan

Publisher
Springer
Year
1985
Tongue
English
Weight
291 KB
Volume
97
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

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By expressing the magnetic field and fluid velocity in terms of two Chandrasekhar-Kendall functions (n = 0, m = 0; n = 1, m = 0) we investigated the steady-state pressure profile inside a solar coronal loop. For constant density loops, we found a two-dimensional (radial and axial) structure of press

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