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 | ||
</math> | </math> | ||
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|+ MHD Equations and Their Applications | |||
! Equation/Formula !! Name !! Usefulness and Applications | |||
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| <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. | |||
|- | |||
| <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. | |||
|- | |||
| <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
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 | 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. |