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The formation of solar prominences by magnetic reconnection and condensation
Home
Publications
The formation of solar prominences by magnetic reconnection and condensation
The formation of solar prominences by magnetic reconnection and condensation
GP
G. W. Pneuman
G. W. Pneuman
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1 October 1983
journal article
Published by
Springer Science and Business Media LLC
in
Solar Physics
Vol. 88
(1)
https://doi.org/10.1007/bf00196189
Abstract
No abstract available
Keywords
EVACUATED
LORENTZ
THERMAL CONDUCTION
FIELD LINES
RECONNECTION
HYDROSTATIC EQUILIBRIUM
HELICES
MAGNETIC FIELD
DOWNFLOW
NEUTRAL LINE
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