We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flux emergence simulation. The simulation domain ranges from the top of the solar interior to the low corona. A twisted magnetic flux tube emerges from the solar interior and into the atmosphere where it interacts with the ambient magnetic field. By studying the connectivity of the evolving magnetic field, we are able to better understand the process of flux rope formation in the solar atmosphere. In the simulation, two flux ropes are produced as a result of flux emergence. Each has a different evolution resulting in different topological structures. These are determined by plasma flows and magnetic reconnection. As the flux rope is the basic st...
Context. There has been suggestions that the initial subsurface magnetic field in flux emergence mod...
Context. Interplanetary coronal mass ejections (ICMEs) originate from the eruption of complex magnet...
Context. Interplanetary coronal mass ejections (ICMEs) originate from the eruption of complex magnet...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flu...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flu...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydro-dynamic (MHD) so...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flu...
Aims. We investigate the formation of flux ropes in a flux emergence region and their rise into the ...
International audienceAims: We investigate the formation of flux ropes in a flux emergence region an...
International audienceAims: We investigate the formation of flux ropes in a flux emergence region an...
Aims. We model the emergence of magnetized plasma from the top of the convection zone to the lower c...
We have simulated the three-dimensional (3D) emergence and interaction of two twisted flux tubes, wh...
Large-scale solar eruptions are believed to have a magnetic flux rope as the core structure. However...
Magnetic flux emergence is the subject of how magnetic fields from the solar interior can rise and e...
We have studied the emergence of a weakly twisted magnetic flux tube from the upper convection zone ...
Context. There has been suggestions that the initial subsurface magnetic field in flux emergence mod...
Context. Interplanetary coronal mass ejections (ICMEs) originate from the eruption of complex magnet...
Context. Interplanetary coronal mass ejections (ICMEs) originate from the eruption of complex magnet...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flu...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flu...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydro-dynamic (MHD) so...
We present an analysis of the formation of atmospheric flux ropes in a magnetohydrodynamic solar flu...
Aims. We investigate the formation of flux ropes in a flux emergence region and their rise into the ...
International audienceAims: We investigate the formation of flux ropes in a flux emergence region an...
International audienceAims: We investigate the formation of flux ropes in a flux emergence region an...
Aims. We model the emergence of magnetized plasma from the top of the convection zone to the lower c...
We have simulated the three-dimensional (3D) emergence and interaction of two twisted flux tubes, wh...
Large-scale solar eruptions are believed to have a magnetic flux rope as the core structure. However...
Magnetic flux emergence is the subject of how magnetic fields from the solar interior can rise and e...
We have studied the emergence of a weakly twisted magnetic flux tube from the upper convection zone ...
Context. There has been suggestions that the initial subsurface magnetic field in flux emergence mod...
Context. Interplanetary coronal mass ejections (ICMEs) originate from the eruption of complex magnet...
Context. Interplanetary coronal mass ejections (ICMEs) originate from the eruption of complex magnet...