Title of article :
What are the physical mechanisms of eruptions and CMEs? Original Research Article
Author/Authors :
Brigitte Schmieder، نويسنده , , Guillaume Aulanier، نويسنده ,
Issue Information :
دوهفته نامه با شماره پیاپی سال 2012
Pages :
9
From page :
1598
To page :
1606
Abstract :
CMEs are due to physical phenomena that drive both, eruptions and flares in active regions. Eruptions/CMEs must be driven from initially force-free current-carrying magnetic field. Twisted flux ropes, sigmoids, current lanes and pattern in photospheric current maps show a clear evidence of currents parallel to the magnetic field. Eruptions occur starting from equilibria which have reached some instability threshold. Revisiting several data sets of CME observations we identified different mechanisms leading to this unstable state from a force free field. Boundary motions related to magnetic flux emergence and shearing favor the increase of coronal currents leading to the large flares of November 2003. On the other hand, we demonstrated by numerical simulations that magnetic flux emergence is not a sufficient condition for eruptions. Filament eruptions are interpreted either by a torus instability for an event occurring during the minimum of solar activity either by the diffusion of the magnetic flux reducing the tension of the restraining arcade. We concluded that CME models (tether cutting, break out, loss of equilibrium models) are based on these basic mechanisms for the onset of CMEs.
Keywords :
Coronal mass ejection , Active region , Electric currents , MHD simulations of eruptions
Journal title :
Advances in Space Research
Serial Year :
2012
Journal title :
Advances in Space Research
Record number :
1133938
Link To Document :
بازگشت