Deriving the Properties of Coronal Pressure Fronts in 3D: Application to the 2012 May 17 Ground Level Enhancement
Université Toulouse III - Paul Sabatier · Université Fédérale de Toulouse Midi-Pyrénées · +12 more institutions
Abstract
We study the link between an expanding coronal shock and the energetic particles measured near Earth during the ground level enhancement of 2012 May 17. We developed a new technique based on multipoint imaging to triangulate the three-dimensional (3D) expansion of the shock forming in the corona. It uses images from three vantage points by mapping the outermost extent of the coronal region perturbed by the pressure front. We derive for the first time the 3D velocity vector and the distribution of Mach numbers, M FM, of the entire front as a function of time. Our approach uses magnetic field reconstructions of the coronal field, full magnetohydrodynamic simulations and imaging inversion techniques. We find that…
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Authors
15- APA. P. RouillardCorresponding
Université Toulouse III - Paul Sabatier, Université Fédérale de Toulouse Midi-Pyrénées, Institut de Recherche en Astrophysique et Planétologie
- IPIllya Plotnikov
Université Toulouse III - Paul Sabatier, Université Fédérale de Toulouse Midi-Pyrénées, Institut de Recherche en Astrophysique et Planétologie
- RPRui Pinto
Université Toulouse III - Paul Sabatier, Université Fédérale de Toulouse Midi-Pyrénées, Institut de Recherche en Astrophysique et Planétologie
- MTMargot Tirole
Université Toulouse III - Paul Sabatier, Université Fédérale de Toulouse Midi-Pyrénées, Institut de Recherche en Astrophysique et Planétologie
- MLM. Lavarra
Université Toulouse III - Paul Sabatier, Université Fédérale de Toulouse Midi-Pyrénées, Institut de Recherche en Astrophysique et Planétologie
Topics & keywords
- Physics
- Coronal mass ejection
- Mach number
- Shock (circulatory)
- Corona (planetary geology)
- Solar wind
- Magnetic cloud
- Magnetohydrodynamics