Mathematics – Probability
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh22a0850e&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH22A-0850
Mathematics
Probability
7509 Corona, 7519 Flares, 7526 Magnetic Reconnection (2723, 7835), 7529 Photosphere
Scientific paper
A numerical model for nanoflares is proposed to describe probability density functions (PDF) and waiting time statistics of the emitted magnetic energy and to guess PDF of quiet-Sun magnetic field strength. In the simulation, footpoints of reconnecting magnetic loops are advected by photospheric flows computed via a n-body algorithm. The model simulates a system whose behavior is characterized by small scale (i.e., granulation) flows that interact to develop large organization scales (i.e., mesogranulation). Such spatio-temporal correlated flows, incessantly supply , remove and convey the passive magnetic footpoints onto the photospheric surface, triggering reconnections and magnetic field reconfigurations.
Berrilli Francesco
Del Moro Dario
Egidi Alberto
Viticchie B.
No associations
LandOfFree
Numerical Simulations of Nanoflares: PDFs of Released Energy, Waiting Times and Quiet- Sun Magnetic Field Elements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Numerical Simulations of Nanoflares: PDFs of Released Energy, Waiting Times and Quiet- Sun Magnetic Field Elements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical Simulations of Nanoflares: PDFs of Released Energy, Waiting Times and Quiet- Sun Magnetic Field Elements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1416460