Results 191 to 200 of about 258,872 (345)
The purpose of this work is to investigate the effect of thermal radiation on convective heat transfer for an electrically conducting hybrid nanofluid moving perpendicularly through a microchannel with parallel plates heated under isothermal conditions ...
Sajjan Kiran+3 more
doaj +1 more source
Anomalous Substorm Signatures During Sudden Solar‐Wind Pressure Enhancements
Abstract Magnetospheric substorms, characterized by the rapid release of energy stored in the magnetotail, play a central role in space weather dynamics. These events are typically triggered by enhanced magnetic reconnection between the Earth's magnetic field and the interplanetary magnetic field (IMF).
Shipra Sinha+4 more
wiley +1 more source
Variation of Model‐Predicted Reconnection Voltages Applied to Uranus' Dayside Magnetosphere
Abstract Uranus provides a key missing piece for fundamentally understanding solar wind‐magnetospheric interactions due to its location in the outer solar system. Whether the viscous‐like interaction overtakes global magnetic reconnection as the dominant process at the magnetopause of the outer planets remains unresolved.
S. Zomerdijk‐Russell+2 more
wiley +1 more source
Stagnation electrical MHD nanofluid mixed convection with slip boundary on a stretching sheet
K. Hsiao
semanticscholar +1 more source
Ballooning Modes in Three-dimensional MHD Equilibria with Shear [PDF]
D. Correa-Restrepo
openalex +1 more source
Abstract The auroral current and electrodynamic structures II sounding rocket mission launched two payloads from Andøya Rocket Range into a post‐dusk discrete auroral arc and observed field‐aligned electron dispersions near inverted‐V precipitation.
C. Feltman+8 more
wiley +1 more source
Non-unique solutions for electron MHD [PDF]
We consider the electron magnetohydrodynamics (MHD) equation on the 3D torus $\mathbb T^3$. For a given smooth vector field $H$ with zero mean and zero divergence, we can construct a weak solution $B$ to the electron MHD in the space $L^\gamma_tW^{1,p}_x$ for appropriate $(\gamma, p)$ such that $B$ is arbitrarily close to $H$ in this space.
arxiv
Alfven — A two-dimensional code based on shasta, solving the radiative, diffusive MHD equations [PDF]
William J. Weber+2 more
openalex +1 more source