Simulations of radiatively cooled magnetic reconnection driven by pulsed power

Magnetic reconnection is an important process in astrophysical environments, as it reconfigures magnetic field topology and converts magnetic energy into thermal and kinetic energy. In extreme astrophysical systems, such as black hole coronae and pulsar magnetospheres, radiative cooling modifies the...

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Veröffentlicht in:	Journal of plasma physics 2024-04, Vol.90 (2), Article 905900215
Hauptverfasser:	Datta, Rishabh, Crilly, Aidan, Chittenden, Jeremy P., Chowdhry, Simran, Chandler, Katherine, Chaturvedi, Nikita, Myers, Clayton E., Fox, William R., Hansen, Stephanie B., Jennings, Chris A., Ji, Hantao, Kuranz, Carolyn C., Lebedev, Sergey V., Uzdensky, Dmitri A., Hare, Jack D.
Format:	Artikel
Sprache:	eng
Schlagworte:	70 PLASMA PHYSICS AND FUSION TECHNOLOGY Accretion disks Aspect ratio astrophysical plasmas Black holes Cooling Cooling rate Current sheets Energy Exploding wires Internal energy Kinetic energy Local thermodynamic equilibrium Mach number Magnetic fields Magnetic islands Numerical analysis plasma instabilities plasma simulation Pulsar magnetospheres Pulsars Radiation Radiation effects Radiation transport Simulation Three dimensional models Topology Transportation planning
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