Mathematics – Probability
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..358...76b&link_type=abstract
Solar Polarization 4, ASP Conference Series, Vol. 358, Proceedings of the conference held 19-23 September, 2005, in Boulder, Col
Mathematics
Probability
Scientific paper
We present a dynamic model of the atmospheric magnetic field in which magnetic loop footpoints are controlled by photospheric flows computed through a N-body algorithm. This simulation reproduces a system whose behaviour is characterized by small scale (e.g., granular) advection flows that interact to form large spatial organization scales (e.g., meso- and super-granulation). In this model the passive advection of magnetic footpoints through photospheric spatio-temporal correlated flows causes the magnetic field to reconfigure as a consequence of magnetic reconnection processes. This approach, based on the dynamic model of multiple magnetic loops tep{b8 Hu03} and on an advective-interaction model proposed by tet{b8 Ra03}, naturally accounts for the observed probability distribution functions and waiting time statistics of the emitted magnetic energy.
Berrilli Francesco
Del Moro Dario
Egidi Alberto
Viticchie B.
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