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Application of an artificial neural network to predict the entrance length of three-dimensional magnetohydrodynamics channel flow
In this paper, a feed-forward, back-propagation neural network was employed for modeling the three-dimension magnetohydrodynamics (MHD) develo**...
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Analysis of DC Inductive Arc Restriking Characteristics of HVDC Relays
Arc restriking will prolong the arc extinguishing time and increase the erosion of the contacts, seriously reduces the electrical life and... -
Second law analysis of MHD third-grade fluid flow through the microchannel
The present study analyses the phenomena of entropy generation of magneto third-grade fluid flow through the microchannel. The significance of Joule...
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Unsteady MHD Casson fluid flow with heat transfer passed over a porous rigid plate with stagnation point flow: Two-parameter Lie scaling approach
This study examined the steady flow of Casson fluid over a rigid porous plate in an infinite region with magnetohydrodynamic (MHD), thermal radiation...
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Dynamics of carbon nanotubes on Reiner–Philippoff fluid flow over a stretchable Riga plate
In this discussion, the influence of carbon nanotubes on fluid flow is explored with the aim of optimizing, facilitating and improving heat transfer...
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Computational Estimate of the DT-to-DD Neutron Yield Ratio for Plasma Focus Chambers
AbstractThe paper presents a computational estimate of the DT-to-DD neutron yield ratio for a spherical plasma-focus chamber PF9. The computations...
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A unified framework for global auroral morphologies of different planets
Planetary magnetic fields control energetic particles in their space environments and guide particles to polar atmospheres, where they produce...
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Current Status of MHD Simulations for Space Weather
In this chapter, we review the status of the art of the three-dimensional (3D) time-dependent magnetohydrodynamic (MHD) models of solar wind. We... -
Unsteady MHD flow of Maxwell fluid with Caputo–Fabrizio non-integer derivative model having slip/non-slip fluid flow and Newtonian heating at the boundary
The purpose of this manuscript is to investigate the unsteady magnetohydrodynamics flow of a Maxwell fluid with conjugate effects of heat and mass...
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Entropy generation in MHD nanofluid flow induced by a slendering stretching sheet with activation energy, viscous dissipation and Joule heating impacts
This research article looks at entropy generation and activation energy analysis on hydromagnetic and thermally radiated nanofluid flow generated by...
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Mixed convection MHD nanofluid flow over a wedge with temperature-dependent heat source
The present work investigates the transfer of heat, mass and fluid flow at the boundary layer of a nanofluid past a wedge in the presence of a...
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The Sun’s Alfvén Surface: Recent Insights and Prospects for the Polarimeter to Unify the Corona and Heliosphere (PUNCH)
The solar wind is the extension of the Sun’s hot and ionized corona, and it exists in a state of continuous expansion into interplanetary space. The...
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Eleven-Year Cycle of Solar Magnetic Activity: Observations, Theories, and Numerical Model Predictions
The record of sunspot observations spans 400 years and shows an 11-year solar activity cycle. How the Sun generates magnetic fields to produce... -
Analysis of Acoustic Wave Phenomena in Radiation Magnetic Hydrodynamics
Abstract —The propagation of linear acoustic disturbances in an infinite, homogeneous, gray radiating plasma, initially in mechanical and radiation...
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Global Smooth Axisymmetic Solutions of the Boussinesq Equations for Magnetohydrodynamics Convection
In this paper, we consider global axisymmetric smooth solutions for the Boussinesq equation for magnetohydrodynamics convection without magnetic...
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Theoretical and Observed Signs of Excitation of Small-Scale Magnetic Fluctuations in the Depth of the Sun
AbstractAn actual problem today is the search for observed evidence of the existence of deep small-scale magnetic fields of the Sun. In this regard,...
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Jets with Kelvin-Helmholtz waves at the Earth’s magnetopause under pure southward IMF conditions
The Kelvin-Helmholtz (KH) waves have been frequently observed during the northward interplanetary magnetic field (IMF) but have been much less...
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Evolution of Viscous Electrically Conducting Fluid Flow on a Rotating Wall in the Presence of a Magnetic Field with Account for the Induction and Diffusion Effects
AbstractThe evolution of a viscous conducting fluid flow on a rotating plate in the presence of a magnetic field is studied. The analytical solution...
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A Finite Volume MHD Code in Spherical Coordinates for Background Solar Wind
A second-order Godunov-type finite volume method (FVM) to advance the equations of single-fluid solar wind plasma magnetohydrodynamics (MHD) in time...