dc.contributor.author |
Rosa, R. K |
|
dc.contributor.author |
Karlicky, M |
|
dc.contributor.author |
Zanandrea, A |
|
dc.contributor.author |
Sych, R. A |
|
dc.contributor.author |
Hanumant, S. S |
|
dc.contributor.author |
Krishan, V |
|
dc.date.accessioned |
2013-04-29T09:16:59Z |
|
dc.date.available |
2013-04-29T09:16:59Z |
|
dc.date.issued |
2005-09 |
|
dc.identifier.citation |
AIP Conference Proceedings, Vol. 784, pp. 567-573 |
en |
dc.identifier.isbn |
0-7354-0273-6 |
|
dc.identifier.issn |
0094-243X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/6049 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
Solar magnetic loop structures can exist in a broad range of spatio-temporal scales and their mutual interactions are described by nonlinear processes of magnetic reconnection triggered as a secondary regime by a primary MHD instability. From the application of wavelet analysis on decimetric time series as a counterpart of spatio-temporal flare loop observations we derive, using Tajima's model for quasi-periodic MHD coalescence, possible ranges of minimum Sagdeev potential. From this parameter we obtain the Alfven period of nonlinear oscillation for a typical mutual solar loop interaction observed by SOHO and TRACE. |
en |
dc.language.iso |
en |
en |
dc.publisher |
American Institute of Physics |
en |
dc.relation.uri |
http://dx.doi.org/10.1063/1.2077220 |
en |
dc.rights |
© American Institute of Physics |
en |
dc.subject |
Solar flares |
en |
dc.subject |
Magnetohydrodynamics |
en |
dc.subject |
Spectral analysis |
en |
dc.title |
Characterization of solar multi-scaling magnetic loop interactions |
en |
dc.type |
Article |
en |