In many astrophysical and fusion applications the CFL stability condition implies strong computational efforts. We propose here a magneto-inductive (Darwin) plasma model, which neglects retardation effects so that the electromagnetic propagation speed is effectively infinite. In this way long timescale phenomena can be investigated without the need to explicitly resolve wave propagation. By neglecting the solenoidal part of the displacement current in Ampere’s law and setting up the vector potential as a divergence-free field, the Maxwell- Darwin equations are converted from hyperbolic to elliptic partial differential equations, which can then be solved with the help of tree methods. Our purpose is to formulate a mesh-free model based on pa...
Efforts are currently being directed towards a fully implicit, electromagnetic, JFNK-based solver, m...
In this paper, we study the exterior boundary value problems of the Darwin model to the Maxwell's eq...
We present a meshless method for magnetohydrodynamics by evolving the vector potential of magnetic f...
In many astrophysical and fusion applications the CFL stability condition implies strong computation...
A new approach to Darwin or magnetoinductive plasma simulation is presented which combines a mesh-fr...
A new type of mesh-free plasma simulation model is presented, capable of modelling particle systems ...
For many astrophysical and most magnetic fusion applications, the purely electromagnetic modes gener...
To study the transport phenomena of energetic particles in plasmas, a new type of mesh-free plasma s...
Maxwell's equations are the foundation of electromagnetics, its extensive applications make com...
In plasma simulations, where the speed of light divided by a characteristic length is at a much high...
The Darwin model of electromagnetic interaction is presented as a self-consistent theory, and is sho...
We present a new Vlasov code for collisionless plasmas in the nonrelativistic regime. A Darwin appro...
This dissertation describes a new algorithm for simulating low frequency, kinetic phenomena in plasm...
The Darwin field model addresses an approximation to Maxwell's equations where radiation effects are...
Degree granted in Engineering-Applied Science.Typescript.SPEC. COLL. HAS ARCHIVAL COPY; MICRO. ROOM ...
Efforts are currently being directed towards a fully implicit, electromagnetic, JFNK-based solver, m...
In this paper, we study the exterior boundary value problems of the Darwin model to the Maxwell's eq...
We present a meshless method for magnetohydrodynamics by evolving the vector potential of magnetic f...
In many astrophysical and fusion applications the CFL stability condition implies strong computation...
A new approach to Darwin or magnetoinductive plasma simulation is presented which combines a mesh-fr...
A new type of mesh-free plasma simulation model is presented, capable of modelling particle systems ...
For many astrophysical and most magnetic fusion applications, the purely electromagnetic modes gener...
To study the transport phenomena of energetic particles in plasmas, a new type of mesh-free plasma s...
Maxwell's equations are the foundation of electromagnetics, its extensive applications make com...
In plasma simulations, where the speed of light divided by a characteristic length is at a much high...
The Darwin model of electromagnetic interaction is presented as a self-consistent theory, and is sho...
We present a new Vlasov code for collisionless plasmas in the nonrelativistic regime. A Darwin appro...
This dissertation describes a new algorithm for simulating low frequency, kinetic phenomena in plasm...
The Darwin field model addresses an approximation to Maxwell's equations where radiation effects are...
Degree granted in Engineering-Applied Science.Typescript.SPEC. COLL. HAS ARCHIVAL COPY; MICRO. ROOM ...
Efforts are currently being directed towards a fully implicit, electromagnetic, JFNK-based solver, m...
In this paper, we study the exterior boundary value problems of the Darwin model to the Maxwell's eq...
We present a meshless method for magnetohydrodynamics by evolving the vector potential of magnetic f...