dc.contributor.author |
Venkatakrishnan, P |
|
dc.date.accessioned |
2008-09-15T14:57:50Z |
|
dc.date.available |
2008-09-15T14:57:50Z |
|
dc.date.issued |
1990-08 |
|
dc.identifier.citation |
Solar Physics, Vol. 128, No. 2, pp. 371 - 376 |
en |
dc.identifier.issn |
0038-0938 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3629 |
|
dc.description.abstract |
We demonstrate that magnetic tension vanishes at regions of large magnetic shear on the polarity inversion line. The characteristics of these tension-free fields depend on the density of the medium and, therefore, change as a consequence of instabilities which modify the density. These instabilities may possibly evolve into solar flares. We suggest this as a possible explanation for the observed occurrence of flares at locations of large magnetic shear along the polarity inversion line. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Kluwer Academic Publishers |
en |
dc.relation.uri |
http://dx.doi.org/10.1007/BF00838473 |
en |
dc.subject |
Solar Flares |
en |
dc.subject |
Magnetic shear |
en |
dc.title |
Loss of magnetic tension in pre-flare magnetic configurations |
en |
dc.type |
Article |
en |