Physics – Fluid Dynamics
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004gapfd..98..429b&link_type=abstract
Geophysical and Astrophysical Fluid Dynamics, vol. 98, Issue 5, p.429-445
Physics
Fluid Dynamics
11
Scientific paper
Many dynamic phenomena in the solar corona are driven by the complex and ever-changing magnetic field. It is helpful, in trying to model these phenomena, to understand the structure of the magnetic field, i.e. the magnetic topology. We study here the topological structure of the coronal magnetic field arising from four discrete photospheric flux patches, for which we find that seven distinct, topologically stable states are possible; the changes between these are caused by six types of bifurcation. Two bifurcation diagrams are produced, showing how the changes occur as the relative positions and strengths of the flux patches are varied. A method for extending the analysis to higher numbers of sources is discussed.
Beveridge Colin
Brown Scott D.
Priest Eric R.
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