Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-28T00:29:13.606Z Has data issue: false hasContentIssue false

Filamentary Currents and the Magnetic Conditions on the Sun

Published online by Cambridge University Press:  16 November 2021

Abstract

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Part 5.
Copyright
Copyright © Academic Press 1962 

References

1. Hewish, A. The Scattering of Radio Waves in the Solar Corona, M.N. 118, 534, 1958.Google Scholar
2. Vitkevich, V. V. and Panorkin, B. N. The Structure of the Solar Super-corona, Astr. J. Moscow 36, 544, 1959.Google Scholar
3. Högbom, J. A. The Structure and Magnetic Field of the Solar Corona, M.N. 120, 530, 1960.Google Scholar
4. Kippenhahn, R. and Schlüter, A. A Theory of Solar Prominences, Z. Astrophys. 43, 36, 1957.Google Scholar
5. Jensen, E. On the Dynamics of Prominences and Coronal Condensations, Astrophys. Norveg. 6, 93, 1959.Google Scholar
6. Lüst, R. and Zirin, H. Condensation of Prominences from the Corona, Z. Astrophys. 49, 8, 1960.Google Scholar
7. Alfvén, H. Filamentary Structure Produced by an Electric Current in a Plasma, Ark. Fys. 19, 375, 1961.Google Scholar
8. Alfvén, H. Cosmical Electrodynamics, p. 157, 68, Oxford 1950 and Proc. roy. Soc. A233, 296, 1955.Google Scholar
9. Alfvén, H. and Lehnert, B. The Sun’s General Magnetic Field, Nature 178, 1339, 1956.Google Scholar
10. Babcock, H. W. and Babcock, H. D. The Sun’s Magnetic Field, Astrophys. J. 121, 349, 1955.Google Scholar
11. Babcock, H. D. The Sun’s Polar Magnetic Field, Astrophys. J. 130, 364, 1959.Google Scholar