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20112022
most citedA Solution Accurate, Efficient and Stable Unsplit Staggered Mesh Scheme for Three Dimensional Magnetohydrodynamics

164 citations · 646 across the 18 of their papers we have counts for

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5 papers · 1 filter

astro-ph.SR2022★ 19 cited

Hydrodynamics and survivability during post-main-sequence planetary engulfment

Ricardo Yarza, Naela Razo Lopez, Ariadna Murguia-Berthier +6

The engulfment of substellar bodies (SBs, such as brown dwarfs and planets) by giant stars is a possible explanation for rapidly rotating giants, lithium-rich giants, and the prese…

astro-ph.SR2018★ 11 cited

The Rise of a Magnetic Flux Tube in a Background Field: Solar Helicity Selection Rules

Bhishek Manek, Nicholas Brummell, Dongwook Lee

The buoyant transport of magnetic fields from the solar interior towards the surface plays an important role in the emergence of active regions, the formation of sunspots and the o…

astro-ph.SR2013★ 14 cited

Three-dimensional numerical simulation of magnetohydrodynamic-gravity waves and vortices in the solar atmosphere

K. Murawski, I. Ballai, A. K. Srivastava +1

With the adaptation of the FLASH code we simulate magnetohydrodynamic-gravity waves and vortices as well as their response in the magnetized three-dimensional (3D) solar atmosphere…

astro-ph.SR2013★ 90 cited

The Post-Merger Magnetized Evolution of White Dwarf Binaries: The Double-Degenerate Channel of Sub-Chandrasekhar Type Ia Supernovae and the Formation of Magnetized White Dwarfs

Suoqing Ji, Robert T. Fisher, Enrique Garcia-Berro +6

Type Ia supernovae (SNe Ia) play a crucial role as standardizable cosmological candles, though the nature of their progenitors is a subject of active investigation. Recent observat…

astro-ph.SR2011★ 134 cited

Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence

Alexei G. Kritsuk, Aake Nordlund, David Collins +13

We employ simulations of supersonic super-Alfvenic turbulence decay as a benchmark test problem to assess and compare the performance of nine astrophysical MHD methods actively use…