Nonaxisymmetric Hall instability: A key to understanding magnetars
It is generally accepted that the nonlinear, dynamical evolution of magnetic fields in the interior of neutron stars plays a key role in the explanation of the observed phenomenology. Understanding the transfer of energy between toroidal and poloidal components, or between different scales, is of pa...
| Główni autorzy: | , |
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| Format: | Artykuł |
| Język: | English |
| Wydane: |
American Physical Society
2019-12-01
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| Seria: | Physical Review Research |
| Dostęp online: | http://doi.org/10.1103/PhysRevResearch.1.032049 |