Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..359..164m&link_type=abstract
Numerical Modeling of Space Plasma Flows: Astronum-2006 ASP Conference Series, Volume 359, Proceedings of the Conference Held 26
Astronomy and Astrophysics
Astronomy
Scientific paper
It is suggested that emerging flux build up magnetic energy in the solar corona that could become the source of flares or jets. Emerging flux also plays an important role in active region formation and disappearance. To investigate these phenomena, it is necessary to study the evolution of an emerging flux from the convection zone to the corona. The solar atmosphere is highly stratified by gravity. For example, the density ratio between photosphere and corona is about ˜ 10^8. However, to study emerging flux process by numerical simulations, it is needed to treat this process with that highly stratified calculation domain. In this paper, we introduce our numerical simulation results for (1) X-ray jets associated with emerging flux and magnetic reconnection in the solar corona, (2) twisted magnetic flux tube emergence into the solar corona, and (3) surge caused by emerging flux tube.
Isobe Hiroaki
Miyagoshi Takashi
Shibata Kazunari
Yokoyama Tadashi
No associations
LandOfFree
Magnetohydrodynamic Numerical Simulations of Emerging Flux and Associated Active Phenomena in the Solar Atmosphere 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 Magnetohydrodynamic Numerical Simulations of Emerging Flux and Associated Active Phenomena in the Solar Atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetohydrodynamic Numerical Simulations of Emerging Flux and Associated Active Phenomena in the Solar Atmosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1241231