Physics
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cophc..59...95p&link_type=abstract
Computer Physics Communications, Volume 59, Issue 1, p. 95-103.
Physics
18
Scientific paper
A numerical code is presented for the computation of the temporal evolution of an externally driven cylindrical plasma column in the framework of linearized compressible and resistive magnetohydrodynamics. The partial differential equations are solved with a semi-discretization method using cubic and quadratic finite elements for the spatial discretization and a fully implicit time advance. This numerical technique yields very accurate results even for small values of the resistivity. With this code it is, amongst others, possible to simulate the heating of solar coronal loops by the resonant absorption of waves that inpitch on them in order to determine the role of this dissipation mechanism in coronal heating. In particular, it is necessary to find out how the time scales of this heating mechanism compare to the life of the coronal loops.
Present address: JET Joint Undertaking, Theory Division, Abingdon, Oxfordshire OX14 3EA, England.
Goossens Marcel
Kerner Wolfgang
Poedts Stefaan
No associations
LandOfFree
Temporal evolution of resonant absorption in solar coronal loops 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 Temporal evolution of resonant absorption in solar coronal loops, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Temporal evolution of resonant absorption in solar coronal loops will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-780187