Magnetic topologies in the solar corona due to four discrete photospheric flux regions

DOI10.1080/03091920410001715575zbMath1206.85016OpenAlexW2087281794MaRDI QIDQ3080181

Daniel S. Brown, Colin Beveridge, Eric R. Priest

Publication date: 5 March 2011

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091920410001715575

zbMATH Keywords

magnetic fieldtopologysolar corona

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (3)

Dynamical systems and topology of magnetic fields in conducting medium ⋮ A topological analysis of the magnetic breakout model for an eruptive solar flare ⋮ Magnetic diffusion and the motion of field lines

Cites Work

• Magnetic reconnection at three-dimensional null points
• Topological bifurcations in three–dimensional magnetic fields

This page was built for publication: Magnetic topologies in the solar corona due to four discrete photospheric flux regions