Flux emergence and interaction with a coronal field: 3D MHD simulations

Bibcode
2006IAUS..233...53A
DOI
10.1017/S1743921306001396
Archontis, V.; Moreno-Insertis, F.; Galsgaard, K.; Hood, A. W.
Bibliographical reference

Solar Activity and its Magnetic Origin, Proceedings of the 233rd Symposium of the International Astronomical Union held in Cairo, Egypt, March 31 - April 4, 2006, Edited by Volker Bothmer; Ahmed Abdel Hady. Cambridge: Cambridge University Press, 2006., pp.53-56

Advertised on:
0
2006
Number of authors
4
IAC number of authors
0
Citations
1
Refereed citations
1
Description
The dynamic process of magnetic flux emergence from the solar interior to the outer atmosphere may well be related with eruptive phenomena and intense events of the Solar activity. However, the physics of the emergence is not still well understood. Thus, we have performed 3D MHD simulations to study the rising motion of a twisted flux tube from the convection zone of the Sun and its interaction with a preexisting coronal magnetic field. The results show that the reconnection process depends criticaly on the initial relative orientation between the two magnetic flux systems into contact. On the other hand, the overal process of emergence depends mostly on the dynamics of the sub-photospheric plasma.
Type
Non-refereed

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