Physics
Scientific paper
Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216...48b&link_type=abstract
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 48-51 (2010).
Physics
Magnetohydrodynamics, Solar Corona, Magnetic Field Effects, Magnetohydrodynamic Waves, Plasma Turbulence, Magnetohydrodynamics, Corona, Interplanetary Magnetic Fields, Magnetohydrodynamic Waves, Plasma Turbulence
Scientific paper
A short review is given about the self-consistent MHD model of solar coronal heating recently proposed by Bigot et al. (2008) in which the dynamical effect of the background magnetic field along a coronal structure is taken into account through exact results from Alfvén wave turbulence. The main properties of the model are given as well as the heating rate and the microturbulent velocity obtained in the case of coronal loops. The conclusion is that Alfvén wave turbulence may produce an efficient background heating for the solar corona.
Bigot Barbara
Galtier Sebastien
Politano Helene
No associations
LandOfFree
Solar Coronal Heating via Alfvén Wave Turbulence 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 Solar Coronal Heating via Alfvén Wave Turbulence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Coronal Heating via Alfvén Wave Turbulence will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1423447