dc.contributor.author |
Barletta, W |
|
dc.contributor.author |
Gershtein, S. S |
|
dc.contributor.author |
Krishan, V |
|
dc.contributor.author |
Reiser, M |
|
dc.contributor.author |
Sessler, A. M |
|
dc.contributor.author |
Xie, M |
|
dc.date.accessioned |
2008-08-04T11:11:08Z |
|
dc.date.available |
2008-08-04T11:11:08Z |
|
dc.date.issued |
1994 |
|
dc.identifier.citation |
Physica Scripta, Vol. T52, pp. 154 - 156 |
en |
dc.identifier.issn |
0281-1847 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/2989 |
|
dc.description |
Restricted Access |
|
dc.description.abstract |
Solar flare data are examined with an eye to seeing if they suggest collective acceleration of ions. That, in fact, seems to be the case. The collective acceleration mechanism of Gershtein is reviewed and the possibilities of the mechanism are discussed. |
en |
dc.format.extent |
3894 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
The Royal Swedish Academy of Sciences |
en |
dc.relation.uri |
http://www.iop.org/EJ/abstract/1402-4896/1994/T52/028 |
en |
dc.subject |
Acceleration mechanism of Gershtein, |
en |
dc.subject |
Solar Flare Data |
en |
dc.title |
Collective acceleration in solar flares |
en |
dc.type |
Article |
en |