Zobrazeno 1 - 10
of 101
pro vyhledávání: '"Sorathia, Kareem A."'
Autor:
Zhang, Binzheng, Delamere, Peter A., Yao, Zhonghua, Bonfond, Bertrand, Lin, D., Sorathia, Kareem A., Brambles, Oliver J., Lotko, William, Garretson, Jeff S., Merkin, Viacheslav G., Grodent, Denis, Dunn, William R., Lyon, John G.
Jupiter's bright persistent polar aurora and Earth's dark polar region indicate that the planets' magnetospheric topologies are very different. High-resolution global simulations show that the reconnection rate at the interface between the interplane
Externí odkaz:
http://arxiv.org/abs/2006.14834
Akademický článek
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Autor:
Zhang, Binzheng, Sorathia, Kareem A., Lyon, John G., Merkin, Viacheslav G., Garretson, Jeffrey S., Wiltberger, Michael
Efficient simulation of plasmas in various contexts often involves the use of meshes that conform to the intrinsic geometry of the system under consideration. We present here a description of a new magnetohydrodynamic code, Gamera (Grid Agnostic MHD
Externí odkaz:
http://arxiv.org/abs/1810.10861
Akademický článek
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When matter orbits around a central mass obliquely with respect to the mass's spin axis, the Lense-Thirring effect causes it to precess at a rate declining sharply with radius. Ever since the work of Bardeen & Petterson (1975), it has been expected t
Externí odkaz:
http://arxiv.org/abs/1309.0290
Orbiting disks may exhibit bends due to a misalignment between the angular momentum of the inner and outer regions of the disk. We begin a systematic simulational inquiry into the physics of warped disks with the simplest case: the relaxation of an u
Externí odkaz:
http://arxiv.org/abs/1303.5465
Autor:
Zhang, Binzheng, Sorathia, Kareem A., Lyon, John G., Merkin, Viacheslav G., Wiltberger, Michael
Publikováno v:
In Journal of Computational Physics 1 January 2019 376:276-294
Grid-based magnetohydrodynamic (MHD) simulations have proven invaluable for the study of astrophysical accretion disks. However, the fact that angular momentum transport in disks is mediated by MHD turbulence (with structure down to very small scales
Externí odkaz:
http://arxiv.org/abs/1106.4019
We have identified the presence of large-scale, low-frequency dynamo cycles in a long-duration, global, magnetohydrodynamic (MHD) simulation of black hole accretion. Such cycles had been seen previously in local shearing box simulations, but we discu
Externí odkaz:
http://arxiv.org/abs/1009.1882
We analyze a suite of global magnetohydrodynamic (MHD) accretion disk simulations in order to determine whether scaling laws for turbulence driven by the magnetorotational instability, discovered via local shearing box studies, are globally robust. T
Externí odkaz:
http://arxiv.org/abs/1002.3611