Computer Science
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992chjss..12....9w&link_type=abstract
Chinese Journal of Space Science (ISSN 0254-6124), vol. 12, no. 1, p. 9-16.
Computer Science
1
Conductive Heat Transfer, Magnetohydrodynamics, Solar Corona, Solar Prominences, Thermal Radiation, Dynamic Response, Hydrodynamic Equations, Radial Distribution, Thermal Conductivity
Scientific paper
Using the magnetohydrodynamic equations with complete energy equation, the dynamic response under the magnetostatic equilibrium in the solar corona caused by the radial ejection of cold mass at the solar surface is studied numerically. The results may explain the formation of the solar prominence and the propagation of accompanying coronal disturbance. It also shows that the effects of thermal conduction and radiative loss on the fundamental property of a disturbance propagation is very small, and it may be that they do not play a role of importance in the formation of prominence.
Wang Ai-Hua
Wang Shui
Wu Shi Tsan
No associations
LandOfFree
A numerical simulation for the propagation of disturbance in the solar corona. II - The effects of thermal conduction and radiation 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 A numerical simulation for the propagation of disturbance in the solar corona. II - The effects of thermal conduction and radiation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A numerical simulation for the propagation of disturbance in the solar corona. II - The effects of thermal conduction and radiation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-936340