MHD Fluid: Difference between revisions

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\frac{D\rho}{Dt} + \rho \nabla \cdot u = 0
\frac{D\rho}{Dt} + \rho \nabla \cdot u = 0
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|+ MHD Equations and Their Applications
! Equation/Formula !! Name !! Usefulness and Applications
|-
| <math display="block">\rho \left(\frac{Du}{Dt}\right) = -\nabla P + J \times B + \eta \nabla^2 u</math> || MHD Momentum Equation || Describes the conservation of momentum in magnetized fluids. Applications include understanding fluid motion in plasmas, astrophysical phenomena, and magnetic confinement in fusion experiments.
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| <math display="block">\frac{\partial B}{\partial t} = \nabla \times (u \times B - \eta \nabla B)</math> || MHD Induction Equation || Governs the evolution of the magnetic field. Used in studies of magnetic reconnection, dynamo processes, and the behavior of magnetic fields in astrophysical systems.
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| <math display="block">E + u \times B = \eta J</math> || Ideal MHD Ohm's Law || Relates electric fields, fluid velocity, and magnetic fields. Essential for understanding the electrical behavior of magnetized plasmas in fusion research and space plasma physics.
|-
| <math display="block">\rho \left(\frac{D\varepsilon}{Dt}\right) = -P \nabla \cdot u + \nabla \cdot (k \nabla T) + \eta J^2</math> || MHD Energy Equation || Describes the conservation of energy in magnetized fluids. Applied in studies of magnetic confinement devices, astrophysical plasmas, and space weather modeling.
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| <math display="block">\frac{D\rho}{Dt} + \rho \nabla \cdot u = 0</math> || Ideal MHD Frozen-in Flux Equation || Expresses the conservation of mass and the 'frozen-in' property of magnetic flux in ideal MHD. Important for understanding plasma dynamics in fusion research, solar wind interactions, and astrophysical accretion processes.
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Revision as of 14:36, 11 February 2024






MHD Equations and Their Applications
Equation/Formula Name Usefulness and Applications
MHD Momentum Equation Describes the conservation of momentum in magnetized fluids. Applications include understanding fluid motion in plasmas, astrophysical phenomena, and magnetic confinement in fusion experiments.
MHD Induction Equation Governs the evolution of the magnetic field. Used in studies of magnetic reconnection, dynamo processes, and the behavior of magnetic fields in astrophysical systems.
Ideal MHD Ohm's Law Relates electric fields, fluid velocity, and magnetic fields. Essential for understanding the electrical behavior of magnetized plasmas in fusion research and space plasma physics.
MHD Energy Equation Describes the conservation of energy in magnetized fluids. Applied in studies of magnetic confinement devices, astrophysical plasmas, and space weather modeling.
Ideal MHD Frozen-in Flux Equation Expresses the conservation of mass and the 'frozen-in' property of magnetic flux in ideal MHD. Important for understanding plasma dynamics in fusion research, solar wind interactions, and astrophysical accretion processes.


Symbol Definitions in MHD Equations
Symbol Name(s) Definition
Fluid Density Density of the fluid in the MHD equations.
Material Derivative Rate of change of a quantity moving with the fluid.
Pressure Fluid pressure in the MHD equations.
Current Density Current density vector in the MHD equations.
Magnetic Field Magnetic field vector in the MHD equations.
Magnetic Diffusivity Magnetic diffusivity in the MHD equations.
Nabla Operator Vector differential operator (gradient, divergence, or curl) in the MHD equations.
Cross Product Cross product of two vectors in the MHD equations.
Electric Field Electric field vector in the MHD equations.
Fluid Velocity Velocity vector of the fluid in the MHD equations.
Time Derivative of Magnetic Field Rate of change of the magnetic field with respect to time.
Specific Internal Energy Specific internal energy of the fluid in the MHD equations.
Thermal Conductivity Thermal conductivity of the fluid in the MHD equations.
Divergence Operator Divergence of a vector field in the MHD equations.
Material Derivative of Specific Internal Energy Rate of change of specific internal energy moving with the fluid.
Curl Operator Curl of a vector field in the MHD equations.
Material Derivative of Density Rate of change of fluid density moving with the fluid.