Results 11 to 20 of about 40,435 (218)
Earth, Planets and Space, 2019 Coronal mass ejections (CMEs) cause disturbances in the environment of the Earth when they arrive at the Earth. However, the prediction of the arrival of CMEs still remains a challenge.
Kazumasa Iwai +5 more
doaj +3 more sources
MHD Simulation of Prominence-Cavity System [PDF]
Frontiers in Astronomy and Space Sciences, 2019 We present magnetohydrodynamic simulation of the evolution from quasi-equilibrium to onset of eruption of a twisted, prominence-forming coronal magnetic flux rope underlying a corona streamer. The flux rope is built up by an imposed flux emergence at the
Yuhong Fan, Tie Liu, Tie Liu
doaj +3 more sources
Simulations of Incompressible MHD Turbulence [PDF]
, 2000 56 pages, 30 figures, submitted to ApJ 59 pages, 31 figures, accepted to ...
Maron, Jason, Goldreich, Peter
openaire +6 more sources
MHD supersonic flow control: OpenFOAM simulation [PDF]
Труды Института системного программирования РАН, 2018 MHD flow control is a relevant topic in today’s aerospace engineering. An OpenFOAM density-based solver that is capable of handling MHD supersonic flow problems with constant magnetic field is developed.
A. I. Ryakhovskiy, A. A. Schmidt
doaj +3 more sources
The influence of Asymmetric Inflow Reconnection on the Diffusion Region in Resistive Space Plasmas [PDF]
Iranian Journal of Astronomy and Astrophysics, 2022 To investigate the effect of asymmetric magnetic reconnection on thedevelopment of the diffusion region and growth of magnetic islands induced duringreconnection (plasmoids), we use 2-dimensional resistive magnetohydrodynamics sim-ulations. In particular,
Hossein Lotfi, Mahboub Hosseinpour
doaj +1 more source
Empirical model of the Earth's cusp at low-altitudes
地球与行星物理论评, 2023 The Earth's cusp is a critical "window" for the solar wind plasma to enterthe low-altitude magnetosphere and ionosphere. However, the overall configuration of cusp has not been established.
Ziqian Liu +4 more
doaj +1 more source
Annales Geophysicae, 1999 Abstract. Two aspects of solar MHD are discussed in relation to the work of the MHD simulation group at KIS. Photospheric magneto-convection, the nonlinear interaction of magnetic field and convection in a strongly stratified, radiating fluid, is a key process of general astrophysical relevance.
M. Schüssler, M. Schüssler
openaire +6 more sources
Nihon Kikai Gakkai ronbunshu, 2021 Electromagnetic flow meter (EMF) has been applied to measure a flow rate of sodium in circular pipe using permanent magnet for a loop-type sodium-cooled Fast Reactor (SFR), such as Monju. To extend EMF to a tank-type SFR only with an annular flow channel
Takatoshi ASADA +4 more
doaj +1 more source
3D Radiative MHD Simulations of Starspots [PDF]
The Astrophysical Journal, 2020 Abstract There are no direct spatially resolved observations of spots on stars other than the Sun, and starspot properties are inferred indirectly through lightcurves and spectropolarimetric data. We present the first self-consistent 3D radiative MHD computations of starspots on G2V, K0V, and M0V stars, which will help us to better ...
Mayukh Panja +2 more
openaire +3 more sources
AIP Advances, 2023 Collisionless magnetic reconnection typically requires kinetic treatment that is, in general, computationally expensive compared to fluid-based models. In this study, we use the magnetohydrodynamics with an adaptively embedded particle-in-cell (MHD-AEPIC)
Dion Li +4 more
doaj +1 more source