| Full text | |
| Author(s): |
Rosa, RR
;
Karlicky, M
;
Zanandrea, A
;
Sych, RA
;
Sawant, HS
;
Krishan, V
;
DeGouveiaDal Pino, EM
;
Lugones, G
;
Lazarian, A
Total Authors: 9
|
| Document type: | Journal article |
| Source: | MAGNETIC FIELDS IN THE UNIVERSE: FROM LABORATORY AND STARS TO PRIMORDIAL STRUCTURES; v. 784, p. 7-pg., 2005-01-01. |
| 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. (AU) | |
| FAPESP's process: | 03/06665-2 - Robert Andreevich Sych | Institute of Solar Terrestrial Physics - Rússia |
| Grantee: | Reinaldo Roberto Rosa |
| Support Opportunities: | Research Grants - Visiting Researcher Grant - International |