Hall cascades versus instabilities in neutron star magnetic fields
From MaRDI portal
Publication:3551085
DOI10.1051/0004-6361/200913452zbMath1183.85014arXiv0912.2656OpenAlexW3105268844WikidataQ56324925 ScholiaQ56324925MaRDI QIDQ3551085
Rainer Hollerbach, C. J. Wareing
Publication date: 8 April 2010
Published in: Astronomy & Astrophysics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0912.2656
turbulencemagnetohydrodynamics (MHD)stars: evolutionstars: neutronstars: magnetic fieldspulsars: general
Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Related Items (6)
Stability and instability of hydromagnetic Taylor-Couette flows ⋮ Cross and magnetic helicity in the outer heliosphere from Voyager 2 observations ⋮ Dissipation wavenumber and regularity for electron magnetohydrodynamics ⋮ Approximative analytic study of fermions in magnetar's crust; ultra-relativistic plane waves, Heun and Mathieu solutions and beyond ⋮ FERMIONS IN MAGNETAR'S CRUST IN TERMS OF HEUN DOUBLE CONFLUENT FUNCTIONS ⋮ A TOY MODEL FOR SCALARS IN TRANSIENT MAGNETIC FIELDS
This page was built for publication: Hall cascades versus instabilities in neutron star magnetic fields
