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Pneuman, G.W. (1983) The formation of solar prominences by magnetic reconnection and condensation. Solar Physics, 88 (1). doi:10.1007/bf00196189

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Reference TypeJournal (article/letter/editorial)
TitleThe formation of solar prominences by magnetic reconnection and condensation
JournalSolar Physics
AuthorsPneuman, G.W.Author
Year1983 (October)Volume88
Issue1
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/bf00196189Search in ResearchGate
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Mindat Ref. ID8917642Long-form Identifiermindat:1:5:8917642:7
GUID0
Full ReferencePneuman, G.W. (1983) The formation of solar prominences by magnetic reconnection and condensation. Solar Physics, 88 (1). doi:10.1007/bf00196189
Plain TextPneuman, G.W. (1983) The formation of solar prominences by magnetic reconnection and condensation. Solar Physics, 88 (1). doi:10.1007/bf00196189
In(1983, October) Solar Physics Vol. 88 (1) Springer Science and Business Media LLC

See Also

These are possibly similar items as determined by title/reference text matching only.

Kopp, R.A., Pneuman, G.W. (1976) Magnetic reconnection in the corona and the loop prominence phenomenon. Solar Physics, 50 (1). doi:10.1007/bf00206193
Hildner, E. (1974) The formation of solar quiescent prominences by condensation. Solar Physics, 35 (1). 123-136 doi:10.1007/bf00156962
Anzer, U., Pneuman, G. W. (1982) Magnetic reconnection and coronal transients. Solar Physics, 79 (1). 129-147 doi:10.1007/bf00146978
Pneuman, G. W. (1980) Eruptive prominences and coronal transients. Solar Physics, 65 (2). 369-385 doi:10.1007/bf00152800
Pneuman, G.W. (1986) Driving mechanisms for the solar wind. Space Science Reviews, 43 (1). doi:10.1007/bf00175327
Pneuman, G. W. (1984) Evolution of rising helical prominences in a nonuniform atmosphere. Solar Physics, 94 (2). 299-313 doi:10.1007/bf00151320
Pneuman, G. W. (1971) The rotation of magnetic loop systems in the solar atmosphere. Solar Physics, 19 (1). 16-31 doi:10.1007/bf00148819
Mason, Stephen F., Bessey, R. J. (1983) The formation of prominences by thermal instability: A numerical study. Solar Physics, 83 (1). 121-134 doi:10.1007/bf00148247
Pneuman, G.W. (1967) Solar flares as resulting from the temporary interruption of energy flow to the corona: A case of hydromagnetic resonance. Solar Physics, 2 (4). doi:10.1007/bf00146494
Smith, DeanF., Pneuman, G.W. (1972) Particle motions in coronal streamers and type III radio bursts. Solar Physics, 25 (2). doi:10.1007/bf00192343
Ballester, J.L., Kleczek, J. (1983) Kinematics of solar prominences. Solar Physics, 87 (2). doi:10.1007/bf00224839
 
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