The force-free twisted magnetosphere of a neutron star – II. Degeneracies of the Grad–Shafranov equation
Author:
Affiliation:
1. Departament de Física Aplicada, Universitat d'Alacant, Ap. Correus 99, E-03080 Alacant, Spain
2. Departament d'Astronomia i Astrofísica, Universitat de València, Dr. Moliner 50, E-46100 Burjassot, València, Spain
Funder
MINECO
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/474/1/625/22141290/stx2814.pdf
Reference27 articles.
1. The force-free twisted magnetosphere of a neutron star
2. Long-term evolution of the force-free twisted magnetosphere of a magnetar
3. THERMOPLASTIC WAVES IN MAGNETARS
4. On the existence of force-free magnetic fields
5. Magnetic field configurations of a magnetar throughout its interior and exterior – core, crust and magnetosphere
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2. Modelling force-free neutron star magnetospheres using physics-informed neural networks;Monthly Notices of the Royal Astronomical Society;2023-06-16
3. Three-dimensional Dynamics of Strongly Twisted Magnetar Magnetospheres: Kinking Flux Tubes and Global Eruptions;The Astrophysical Journal Letters;2023-04-01
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