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

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Showing astro-ph.SRShow all

10 papers · 1 filter

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…

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…

astro-ph.SR2016★ 103 cited

Magnetic field evolution in magnetar crusts through three dimensional simulations

Konstantinos N. Gourgouliatos, Toby Wood, Rainer Hollerbach

Current models of magnetars require extremely strong magnetic fields to explain their observed quiescent and bursting emission, implying that the field strength within the star's o…

astro-ph.SR2015★ 103 cited

Three-dimensional simulations of the magnetic stress in a neutron star crust

Toby S. Wood, Rainer Hollerbach

We present the first fully self-consistent three-dimensional model of a neutron star's magnetic field, generated by electric currents in the star's crust via the Hall effect. We fi…

astro-ph.SR2013★ 41 cited

Dynamics of the solar tachocline III: Numerical solutions of the Gough and McIntyre model

Luis A. Acevedo-Arreguin, Pascale Garaud, Toby S. Wood

We present the first numerical simulations of the solar interior to exhibit a tachocline consistent with the Gough and McIntyre (1998) model. We find nonlinear, axisymmetric, stead…

astro-ph.SR2013★ 61 cited

Energy conservation and gravity waves in sound-proof treatments of stellar interiors: Part II Lagrangian constrained analysis

Geoffrey M. Vasil, Daniel Lecoanet, Benjamin P. Brown +2

The speed of sound greatly exceeds typical flow velocities in many stellar and planetary interiors. To follow the slow evolution of subsonic motions, various sound-proof models att…