activity
20002019
most citedHARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics

801 citations · 921 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2019★ 17 cited

Numerical investigation of the dynamics of linear spin fields on Kerr background I. Late time tails of spin fields

Károly Csukás, István Rácz, Gábor Zsolt Tóth

The time evolution of linear fields of spin and on Kerr black hole spacetimes are investigated by solving the homogeneous Teukolsky equation numerically. Th…

physics.ao-ph2017

Large-scale vorticity generation and kinetic energy budget along the U.S. West Coast

Gábor Tóth, Viktória Homonnai, Imre M. Jánosi

We attempt to evaluate energy budget over a restricted but extremely well studied oceanic region along the shorelines of Oregon and California. The analysis is based on a recently…

astro-ph.EP2017★ 48 cited

The dehydration of water worlds via atmospheric losses

Chuanfei Dong, Zhenguang Huang, Manasvi Lingam +3

We present a three-species multi-fluid MHD model (H, HO and e), endowed with the requisite atmospheric chemistry, that is capable of accurately quantifying the magn…

physics.space-ph2015★ 51 cited

The role of the Hall effect in the global structure and dynamics of planetary magnetospheres: Ganymede as a case study

John C. Dorelli, Alex Glocer, Glyn Collinson +1

We present high resolution Hall MHD simulations of Ganymede's magnetosphere demonstrating that Hall electric fields in ion-scale magnetic reconnection layers have significant globa…

astro-ph2003★ 801 cited

HARM: A Numerical Scheme for General Relativistic Magnetohydrodynamics

Charles F. Gammie, Jonathan C. McKinney, Gábor Tóth

We describe a conservative, shock-capturing scheme for evolving the equations of general relativistic magnetohydrodynamics. The fluxes are calculated using the Harten, Lax, and van…

astro-ph2000★ 4 cited

Pulsar wind nebulae in supernova remnants

E. van der Swaluw, A. Achterberg, Y. A. Gallant +1

A spherically symmetric model is presented for the interaction of a pulsar wind with the associated supernova remnant. This results in a pulsar wind nebula whose evolution is coupl…