Physics
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..125..277w&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 125, Feb. 1990, p. 277-293.
Physics
20
Magnetohydrodynamics, Simulation, Solar Physics, Solar Prominences, Condensation, Conductive Heat Transfer, Stellar Models
Scientific paper
The effects of condensation and thermal conduction on the formation of Kippenhahn-Schlueter (K-S) type prominences in quiet regions (QP) due to symmetric mass injection are investigated. To implement this investigation a self-consistent, two-dimensional, nonplanar, time-dependent MHD simulation model is developed. In the model, various values of the injection velocity, density, and magnetic field strength are used to determine the most favorable conditions for the QP formation. Based on these simulation results, it is found that the formation of a K-S type field configuration should be considered as a dynamic process which needs both condensation amd mass injection to supply enough mass to maintain such a configuration to complete the quiescent prominence formation process.
An Chang-Hyuk
Bao Jingdong
Tandberg-Hanssen Einar
Wu Shi Tsan
No associations
LandOfFree
The role of condensation and heat conduction in the formation of prominences - an MHD simulation 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 The role of condensation and heat conduction in the formation of prominences - an MHD simulation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The role of condensation and heat conduction in the formation of prominences - an MHD simulation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1843694