Computer Science – Numerical Analysis
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..115...81a&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 115, no. 1, 1988, p. 81-92.
Computer Science
Numerical Analysis
6
Magnetic Field Configurations, Magnetohydrodynamics, Mass Transfer, Solar Magnetic Field, Solar Prominences, Chromosphere, Gravitational Effects, Numerical Analysis, Plasma Density, Solar Corona, Velocity Distribution
Scientific paper
The authors have studied chromospheric mass injection into an overlying coronal dipole magnetic field using a 2-D ideal magnetohydrodynamic (MHD) numerical model. The results indicate that such injection can produce magnetic field deformation conducive to active region prominences - namely, Kippenhahn-Schlüter (K-S) type configurations for stable support of injected plasma. Optimum conditions for such dynamical formation of K-S-type field configurations are shown: To form a K-S-type magnetic field configuration, a narrow range of injection density, velocity, and magnetic field strength must be used; spicule-like asymmetric mass injection seems favorable.
An Chang-Hyuk
Bao Jingdong
Wu Shi Tsan
No associations
LandOfFree
Numerical simulation of mass injection for the formation of prominence magnetic field configurations. I - Asymmetric injection 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 of mass injection for the formation of prominence magnetic field configurations. I - Asymmetric injection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical simulation of mass injection for the formation of prominence magnetic field configurations. I - Asymmetric injection will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1693086