Results 101 to 110 of about 69,070 (213)

Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics [PDF]

, 2017
We present Phantom, a fast, parallel, modular and low-memory smoothed particle hydrodynamics and magnetohydrodynamics code developed over the last decade for astrophysical applications in three dimensions. The code has been developed with a focus on stellar, galactic, planetary and high energy astrophysics and has already been used widely for studies ...
arxiv   +1 more source

Laboratory observation of a nonlinear interaction between shear Alfv\'{e}n waves

, 2005
An experimental investigation of nonlinear interactions between shear Alfv\'{e}n waves in a laboratory plasma is presented. Two Alfv\'{e}n waves, generated by a resonant cavity, are observed to beat together, driving a low frequency nonlinear psuedo-mode
B. Brugman, C. A. Kletzing, D. A. Gurnett, H. Wong, J. W. Belcher, P. Pribyl, T. A. Carter, W. Lybarger   +7 more
core   +1 more source

Evolution of Force‐Free Magnetic Structure in the Dayside Ionosphere of Mars

Journal of Geophysical Research: Space Physics, Volume 130, Issue 4, April 2025.
Abstract Magnetic fields measured in the ionosphere of Mars by the magnetometers onboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) and the Mars Global Surveyor (MGS) spacecraft display a wide range of spatial scales, ranging from global to small‐scale.
T. E. Cravens, O. Hamil, A. R. Renzaglia, S. R. Shaver, S. A. Ledvina, C. S. Kennedy   +5 more
wiley   +1 more source

Multispecies MHD Simulations of the Crustal Field Influence at the Mars Magnetotail Current Sheet

Journal of Geophysical Research: Space Physics, Volume 130, Issue 4, April 2025.
Abstract The magnetotail current sheet of Mars exhibits a dawn‐to‐dusk asymmetry that has been seen in satellite observations and MHD simulations. However, the influence of season has not been thoroughly investigated in MHD simulations. This investigation incorporates seasonal variations, driven by planetary eccentricity and solar variability, within ...
N. A. Quartey, M. W. Liemohn
wiley   +1 more source

Review of Conductive Reciprocating Liquid Metal Magnetohydrodynamic Generators

Energies
Reciprocating liquid metal magnetohydrodynamic (MHD) power generation is a new MHD power generation method in which the working fluid is a single-phase liquid metal with a low melting point and high conductivity.
Lingzhi Zhao, Aiwu Peng
doaj   +1 more source

Pulsed power accelerator for material physics experiments

Physical Review Special Topics. Accelerators and Beams, 2015
We have developed the design of Thor: a pulsed power accelerator that delivers a precisely shaped current pulse with a peak value as high as 7 MA to a strip-line load.
D. B. Reisman, B. S. Stoltzfus, W. A. Stygar, K. N. Austin, E. M. Waisman, R. J. Hickman, J.-P. Davis, T. A. Haill, M. D. Knudson, C. T. Seagle, J. L. Brown, D. A. Goerz, R. B. Spielman, J. A. Goldlust, W. R. Cravey   +14 more
doaj   +1 more source

Magnetic Effects at the Edge of the Solar System: MHD Instabilities, the de Laval nozzle Effect and an Extended Jet

, 2004
To model the interaction between the solar wind and the interstellar wind, magnetic fields must be included. Recently Opher et al. 2003 found that, by including the solar magnetic field in a 3D high resolution simulation using the University of Michigan ...
Baranov V. B., Baranov V. B., D. L. DeZeeuw, Dahlburg R. B., Frisch P. C., G. Toth, I. Sokolov, L. Bettarini, M. Opher, M. Velli, P. C. Liewer, Parker E. N., Pogorolev N. V., Ratkiewicz R., Ratkiewicz R., T. I. Gombosi, W. Manchester, Washimi H.   +17 more
core   +2 more sources

The Magnetic Topology of AR13664 Leading to Its First Halo CME

Journal of Geophysical Research: Space Physics, Volume 130, Issue 4, April 2025.
Abstract In the first half of May 2024, the solar active region (AR) NOAA 13664 was responsible for generating the strongest geomagnetic storm in over 20 years through an enhanced production of coronal mass ejections (CMEs). A key factor in this production was the complex magnetic topology of AR13664.
D. MacTaggart, T. Williams, O. P. M. Aslam   +2 more
wiley   +1 more source

Numerical simulations of imbalanced strong magnetohydrodynamic turbulence

, 2009
Magnetohydrodynamics (MHD) is invoked to address turbulent fluctuations in a variety of astrophysical systems. MHD turbulence in nature is often anisotropic and imbalanced, in that Alfvenic fluctuations moving in opposite directions along the background ...
Beresnyak, Beresnyak, Boldyrev, Chandran, Cho, Grappin, Haugen, Iroshnikov, Kadomtsev, Lithwick, Lithwick, Lithwick, Maron, Marsch, Perez, Podesta   +15 more
core   +1 more source

Computation of inverse magnetic cascades [PDF]

, 1981
Inverse cascades of magnetic quantities for turbulent incompressible magnetohydrodynamics are reviewed, for two and three dimensions. The theory is extended to the Strauss equations, a description intermediate between two and three dimensions appropriate
Montgomery, D.
core   +1 more source