Results 91 to 100 of about 4,318 (239)
Context: Coronal magnetic null points have been implicated as possible locations for localised heating events in 2D models. We investigate this possibility about fully 3D null points.
Thurgood, J. O. +5 more
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The branch of physics known as magnetohydrodynamics (MHD) emerged in the middle of the 20th century. MHD models, being substantially nonlinear, are quite challenging for theoretical study and allow nontrivial consideration only in particular limited ...
Anatoly A. Gurchenkov, Ivan A. Matveev
doaj +1 more source
The mathematical analysis of viscous magnetohydrodynamics (MHD) models is of great interest in recent years. In this paper, a finite element Galerkin method is employed for the estimation of an unknown time-dependent convection coefficient and source in ...
Miglena N. Koleva, Lubin G. Vulkov
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Three dimensional magnetohydrodynamics of fusion plasmas [PDF]
The primary aim of the research on nuclear fusion is to obtain a new energy source to help satisfying a growing and sustainable consumption. This objective has to be reached through scientific research, both from the physics point of view and through the
Veranda, Marco
core
Compression of the Earth's magnetotail by interplanetary shocks directly drives transient magnetic flux closure [PDF]
peer reviewedWe use a novel method to evaluate the global opening and closure of magnetic flux in the terrestrial system, and to analyse two interplanetary shock passages that occurred during magnetically quiet periods.
Palmroth, Minna +26 more
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The underlying investigation reports the effects of the magnetohydrodynamics (MHD) and non-linear slip coefficients on the coating thickness of the web/substrate during the blade coating process.
Muhammad Asif Javed +4 more
doaj +1 more source
In this brief note we study the n-dimensional magnetohydrodynamic equations with hyper-viscosity and zero resistivity.
Tran, Chuong Van +5 more
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Magnetic reconnection in flux-tubes undergoing spinning footpoint motions [PDF]
Aims.Photospheric motions acting on the coronal magnetic field have the potential to build up huge amounts of magnetic energy. The energy may be released through magnetic reconnection, and so a detailed understanding of the 3D process is crucial if its ...
I. De Moortel +4 more
core +1 more source
A two-component phenomenology for the evolution of MHD turbulence
Incompressible MHD turbulence with a mean magnetic field B₀ develops anisotropic spectral structure and can be simply described only by including at least two distinct fluctuation components.
Dmitruk, Pablo +2 more
core
SWIFF : space weather integrated forecasting framework [PDF]
This research has received funding from the European Commission’s FP7 Program with the grant agreement SWIFF (Project No. 2633430, swiff.eu). The KU Leuven simulations were conducted on the computational resources provided by the PRACE Tier-0 Project No.
Viviane Pierrard +84 more
core +1 more source

