Statistics – Computation
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985sssmp..28..978w&link_type=abstract
Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 28, Sept. 1985, p
Statistics
Computation
Computational Astrophysics, Magnetohydrodynamics, Plasma Dynamics, Solar Corona, Atmospheric Physics, Computational Fluid Dynamics, Lines Of Force, Magnetic Field Configurations, Rarefied Plasmas, Solar Magnetic Field
Scientific paper
This paper reconsiders the characteristics of the propagation of a disturbance in the solar corona by means of a magnetohydrodynamic model and the full-implicit continuous Eulerian scheme in the spherical coordinates. To simulate the magnetic configuration of the solar atmosphere, a method in combination with analytical and numerical methods is used to obtain a streamlike magnetic field structure. With this magnetic field model, the dynamic response in the solar corona caused by a radial ejection of cold mass in the neighborhood of the equator at the solar surface and the accompanying physical processes are discussed. Some significant physical phenomena have been discovered. The results explain the formation of the solar prominence and the accompanying coronal transient.
Wang Anzhong
Wang Shuang
No associations
LandOfFree
Numerical simulation for propagation of disturbance in solar corona 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 simulation for propagation of disturbance in solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical simulation for propagation of disturbance in solar corona will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-803290