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Explanation of Different Shapes of Planetaries in Terms of Movement in Magnetic and Gravitational Fields

Published online by Cambridge University Press:  14 August 2015

E. Woyk (Eliška Chvojková)
E. Woyk (Eliška Chvojková)*
Affiliation:
Astronomical Institute, Czechoslovak Academy Of Sciences, Czechoslovakia

Abstract

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Many features observed in solar prominences, planetary nebulae and the terrestrial magnetosphere (e.g. the filamentary structure, suspended clouds and arcs or toroids hovering above the equator) lead to the conviction that magnetic fields play a significant role in these objects. The magnetic mechanism (Woyk, 1967) described briefly below may be able to explain the shapes of all known planetaries. The field intensity sufficient for supporting the mechanism described need not exceed about 10−6–10−4G.

Type
Session IV – Structure and Dynamics
Information
Symposium - International Astronomical Union , Volume 34: Planetary Nebulae , 1968 , pp. 275 - 278
Copyright
Copyright © Reidel 1968 

References

Chvojková, E. (1965) Bull. Astr. Inst. Čsl., 16, 63.Google Scholar
Chvojková, E., Klepešta, J. (1965) Bull. Astr. Inst. Čsl., 16, 70.Google Scholar
Woyk, E. (1967) J. atmos. terr. Phys., 29, 465.Google Scholar