Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Centrum voor Plasma-Astrofysica, Departement Wiskunde, Katholieke Universiteit Leuven, Belgium
LANL
Centrum voor Plasma-Astrofysica, Departement Wiskunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium Alamos National Laboratory, Los Alamos, NM 87545, USA
Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
Centrum voor Plasma-Astrofysica, Departement Wiskunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium and Plasma Theory Group, Los Alamos National Laboratory, Los Alamos, NM
Centrum voor Plasma-Astrofysica, Departement Wiskunde, Katholieke Universiteit, Leuven, Belgium
Centrum voor Plasma-Astrofysica, Departement Wiskunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium Theory Group, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
T-15, Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545
Theoretical Division, Los Alamos National Laboratory, Los Alamos, NM 87545 Alamos National Laboratory
LANL, MS: C305, Los Alamos, 87544, USA C305, Los Alamos, 87544, USA T-15 Plasma Theory Group, Los Alamos, NM 87545, USA C305, los alamos, 87544, USA Alamos National Lab, MS K717, Los Alamos, NM 87545, USA Alamos National Laboratory, T-15 Plasma Theory, Los Alamos, NM 87545, USA Alamos National Laboratory, K717, Los Alamos, NM 87545, USA Alamos National Laboratory, M.S. B216, Los Alamos, NM 87544, USA Theory, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
Centrum voor Plasma Astrofysica, Katholieke Universiteit Leuven, Heverlee, Belgium; Alamos Na
3-D Implicie-PIC Simulation Studies of Electrid Fields During Magnetic Reconnection
3d Flux Rope Dynamics Including Reconnection, Bouncing, And Guide Field Compression
3D Kinetic Simulations of the Onset of Collisionless Magnetic Reconnection
3D Magnetic reconnection: evolution of x-lines.
3D MHD simulation and the role of null points in coronal reconnection
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