Results 91 to 100 of about 2,051 (189)

Formation of Stationary Magnetohydrodynamic Outflows from a Disk by Time‐dependent Simulations [PDF]

, 1997
M. M. Romanova, G. V. Ustyugova, A. V. Koldoba, В. М. Чечеткин, R. V. E. Lovelace   +4 more
openalex   +1 more source

Three-dimensional Magnetohydrodynamic Simulations of Periodic Variations of Ganymede’s Footprint

The Astrophysical Journal
Alfvénic power is generated through the interaction between the mini-magnetosphere of Ganymede and the corotating flow of the Jovian plasma, contributing to the formation of the Ganymede auroral footprint at Jupiter’s ionosphere.
Tao Yan, Binzheng Zhang, Junjie Chen, Zhiqi Zheng, Ziyi Yang, Shengyi Ye, Jun Cui   +6 more
doaj   +1 more source

Learning effective physical laws for generating cosmological hydrodynamics with Lagrangian deep learning. [PDF]

Proc Natl Acad Sci U S A, 2021
Dai B, Seljak U.
europepmc   +1 more source

On the effect of oscillatory phenomena on Stokes inversion results. [PDF]

Philos Trans A Math Phys Eng Sci, 2021
Keys PH, Steiner O, Vigeesh G.
europepmc   +1 more source

Magnetohydrodynamic simulations of accretion disks around a weakly magnetized neutron star in strong gravity [PDF]

, 2001
Y. Kato, Masahiko Hayashi, S. Miyaji, Ryōji Matsumoto   +3 more
openalex   +1 more source

Unveiling the Connection between the Alfvénic Oval and the Open–Closed Field Line Boundary at Ganymede

The Astrophysical Journal
Alfvén waves generated by the interactions between the Ganymede magnetosphere and the fast-corotating Jovian plasma carry a significant amount of energy.
Tao Yan, Binzheng Zhang, Junjie Chen, Ziyi Yang, Shengyi Ye, Jun Cui   +5 more
doaj   +1 more source

Magnetohydrodynamic Simulation of a Solar Flare with Chromospheric Evaporation Effect Based on the Magnetic Reconnection Model [PDF]

, 2001
T. Yokoyama, Kazunari Shibata
openalex   +1 more source

Comparative Analysis of Hall Effect Implementations in Hall Magnetohydrodynamics

The Astrophysical Journal
There is no standard numerical implementation of the Hall effect, which is one of the nonideal magnetohydrodynamic (MHD) effects. Numerical instability arises when a simple implementation is used, in which the Hall electric field is added to the electric
Kazunari Iwasaki, Kengo Tomida
doaj   +1 more source

Three‐dimensional Magnetohydrodynamic Simulations of Radiatively Cooling, Pulsed Jets [PDF]

, 2001
A. H. Cerqueira, E. M. de Gouveia Dal Pino   +1 more
openalex   +1 more source

Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and <i>γ</i>-Ray Bursts. [PDF]

Front Astron Space Sci, 2021
Ruiz M, Shapiro SL, Tsokaros A.
europepmc   +1 more source