Sep 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aspc..184...38s&link_type=abstract
Third Advances in Solar Physics Euroconference: Magnetic Fields and Oscillations, ASP Conference Series vol.184, p. 38-54. Eds.
Physics
15
Magnetic Fields, Flux Tubes, Convection, Polarization, Stokes Profiles, Simultations
Scientific paper
We propose that the observed fragmentation of magnetic elements is due to their inherent liability to the interchange instability. The convective collapse and numerical simulations of the formation of intense magnetic flux sheets including spectral signatures of the formation process are discussed. We suggest that the mean downflow measured in magnetic elements is due to a fraction of an ensemble of magnetic elements being in the formation phase at any given time. It is shown that observed Stokes V profiles of magnetic elements are actua lly an average of spatially strongly varying profiles with a delicate balance of positive and negative contributions to the area asymmetry.
No associations
LandOfFree
Flux Tube Dynamics 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 Flux Tube Dynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flux Tube Dynamics will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1769599