the relativistic highly magnetized plasma aiming to explain Crab flares In tearing mode instability of a relativistic current layer (see also Lyutikov 2003a;
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Explosive reconnection of double tearing modes in relativistic plasmas
30 août 2013 · Explosive reconnection of double tearing modes in relativistic plasmas: application to the Crab flares H Baty,1‹ J Petri1‹ and S Zenitani2‹
[PDF] Explosive reconnection in magnetars
opment of tearing mode in magnetically-dominated relativistic plasma msec Finally, we discuss how reconnection may explain other magnetar phenomena
[PDF] Explosive reconnection of the double tearing mode in relativistic
24 avr 2015 · Explosive reconnection of the double tearing mode in relativistic plasmas Application to the Crab J ér ôme P étri1 Hubert Baty1
[PDF] Particle acceleration in explosive relativistic reconnection - CORE
the relativistic highly magnetized plasma aiming to explain Crab flares In tearing mode instability of a relativistic current layer (see also Lyutikov 2003a;
[PDF] Tohir AKRAMOV La reconnexion magnétique explosive - Thèses
with DTM dynamics and the particles are accelerated up to relativistic velocities In addition, the effect Keywords: Magnetic reconnection - Resistive instability - Double-tearing modes - Ma- 3 Instabilité explosive du mode de double-tearing 63 2 1 Le concept de la MHD parfaite: dans un plasma hautement conducteur,
Fast magnetic reconnection: The ideal tearing instability in classic
29 jan 2018 · instability in classic, Hall, and relativistic plasmas E Papini1, S Magnetic reconnection is believed to be the driver of many explosive phenomena The e- folding growth time τt of the fastest reconnecting mode, calculated
[PDF] Explosive nonlinear growth of double tearing mode: plasmoid
Explosive nonlinear growth of double tearing mode: plasmoid formation and test particle Magnetic reconnection is a fundamental process in astrophysical and laboratory plasmas, where a to a fast and explosive reconnection phase during the non linear evolution of double tearing modes relativistic Lorentz equations
[PDF] RESEARCH REPORT - International Nuclear Information System
Numerical Study of Explosive Tearing Mode Instability normal to the plasma sheet stabilizes both the electron and ion linear by magnetic reconnection, Phys Terasawa,T and A Nishida, Simultaneous observations of relativistic electron
pdf Explosive reconnection of the double tearing mode in
The pulsar linked to its surrounding nebula the pulsar and its magnetosphere source of relativistic e±pairs rL= 106m the cold ultra-relativistic wind streaming to the nebula the shocked wind composed of particles heated after crossing the MHD shock rts= 3 × 1015m= 0 1 pc ? main source of radiation observed in radio optics X-rays and gamma-
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