activity
20072024
most citedMagnetic field evolution in magnetar crusts through three dimensional simulations

103 citations · 785 across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.SR2024★ 1 cited

Shear-driven magnetic buoyancy in the solar tachocline: Dependence of the mean electromotive force on diffusivity and latitude

Craig D. Duguid, Paul J. Bushby, Toby S. Wood

The details of the dynamo process that is responsible for driving the solar magnetic activity cycle are still not fully understood. In particular, whilst differential rotation prov…

physics.flu-dyn2024

Stratified Resistive Tearing Instability

Scott J. Hopper, Toby S. Wood, Paul J. Bushby

Resistive tearing instabilities are common in fluids that are highly electrically conductive and carry strong currents. We determine the effect of stable stratification on the tear…

astro-ph.HE2023★ 1 cited

Three-dimensional magneto-thermal evolution of off-centred dipole magnetic field configurations in neutron stars

Andrei P. Igoshev, Rainer Hollerbach, Toby Wood

Off-centred dipole configurations have been suggested to explain different phenomena in neutron stars, such as natal kicks, irregularities in polarisation of radio pulsars and prop…

astro-ph.SR2023★ 3 cited

Shear-driven magnetic buoyancy in the solar tachocline: The mean electromotive force due to rotation

Craig D. Duguid, Paul J. Bushby, Toby S. Wood

The leading theoretical paradigm for the Sun's magnetic cycle is an -dynamo process, in which a combination of differential rotation and turbulent, helical flows produces a lar…

physics.flu-dyn2022

Validity of sound-proof approximations for magnetic buoyancy

John B. Moss, Toby S. Wood, Paul J. Bushby

The presence of acoustic waves in models of compressible flows can present complications for analytical and numerical analysis. Therefore, several methods have been developed to fi…

astro-ph.HE2022★ 9 cited

Three-Dimensional Magnetothermal Simulations of Magnetar Outbursts

Davide De Grandis, Roberto Turolla, Roberto Taverna +3

The defining trait of magnetars, the most strongly magnetized neutron stars (NSs), is their transient activity in the X/-bands. In particular, many of them undergo phases of enh…