Non-resonant nonlinear coupling of magnetohydrodynamic waves in inhomogeneous media [PDF]
V. M. Nakariakov, D. Tsiklauri, TD Arber
openalex +1 more source
Non-ideal magnetohydrodynamics on a moving mesh II: Hall effect [PDF]
Oliver Zier +2 more
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∇ ⋅ B, Outer Boundary, and Biot–Savart in Magnetosphere MHD Simulations
Abstract We examine the size of ∇⋅B $\nabla \cdot \mathbf{B}$ and outer surface boundary integrals in estimating the surface magnetic field from magnetohydrodynamic (MHD) simulations. Maxwell's equations tell us ∇⋅B=0 $\nabla \cdot \mathbf{B}=0$, which may be violated due to numerical error. MHD models such as the Space Weather Modeling Framework (SWMF)
Dean Thomas +4 more
wiley +1 more source
Investigation of entropy generation in the magnetohydrodynamic electroosmotic peristaltic flow of Cu–Al2O3/H2O hybrid nanofluid via a curved channel [PDF]
Hani Alahmadi +3 more
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Are Cusp‐Aligned Arcs the Equivalent of Auroral Streamers in a Closed Magnetosphere?
Abstract We present the first observations of a 3‐hour quasi‐periodic intensification of the polar auroras during a prolonged interval of strongly‐northward interplanetary magnetic field (IMF). This takes the form of a localized spot of auroral emission that appears near the pole which subsequently spreads sunward and antisunward to produce a sun ...
S. E. Milan +7 more
wiley +1 more source
Rotational effect of a cylinder on hydro-thermal characteristics in a partially heated square enclosure using CNT-water nanofluid. [PDF]
Azad AK +4 more
europepmc +1 more source
Spontaneous Hot Flow Anomalies in Earth's Foreshock
Abstract In recent years, we have learned that foreshock transients play an influential role in solar wind coupling with Earth's magnetosphere. These transients include spontaneous hot flow anomalies (SHFAs), which are characterized by dips in magnetic field magnitude and ion density, enhanced temperature, decelerated and deflected solar wind flow, and
D. Rojas‐Castillo +2 more
wiley +1 more source
MHD rotating flow over a stretching surface: The role of viscosity and aggregation of nanoparticles. [PDF]
Alqahtani AM +5 more
europepmc +1 more source
Relativistic Magnetohydrodynamics [PDF]
openaire +1 more source
Abstract Ultra‐low‐frequency (ULF) waves play a critical role in magnetospheric dynamics, yet their transient growth and resonant electron interactions remain poorly understood. We develop a first‐principle model of toroidal mode field line resonances that captures wave growth, saturation, and phase mixing.
J. Liu +3 more
wiley +1 more source

