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...
| Main Authors: | , , , , , , , , , , , , , , |
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| Format: | Article |
| Published: |
Cambridge University Press
2024
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| Online Access: | https://hdl.handle.net/1721.1/155295 |