MHD Equations: Deriving and Exploring Consequences

In summary, using the Maxwell equations, we can derive an expression for the magnetic field at high resistivity. At high resistivity, the magnetic field is approximately zero, leading to instabilities and disruptions in the plasma.
  • #1
Logarythmic
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Homework Statement


Two of the MHD equations can be written as

[tex]\vec{E} + \vec{v} \times \vec{B} = \eta \vec{J}[/tex]

[tex]\vec{\nabla} \times \vec{B} = \mu_0 \vec{J}[/tex]

where [itex]\eta[/tex] is the resistivity of the plasma.

Derive an expression for the magnetic field at a very high resistivity and describe the corresponding consequences for the behaviour of the magnetic field lines.

The Attempt at a Solution


I need a starter. I have no clue.. Use the maxwell equations?
 
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  • #2


Hello! I would suggest starting by using the Maxwell equations to derive an expression for the magnetic field at high resistivity. The Maxwell equations describe the relationship between electric and magnetic fields, and they are fundamental to understanding MHD (magnetohydrodynamics) equations.

To begin, let's rewrite the MHD equations in terms of the Maxwell equations:

1. \vec{\nabla} \cdot \vec{E} = \frac{\rho}{\epsilon_0} (Gauss's law)

2. \vec{\nabla} \cdot \vec{B} = 0 (Gauss's law for magnetism)

3. \vec{\nabla} \times \vec{E} = -\frac{\partial \vec{B}}{\partial t} (Faraday's law)

4. \vec{\nabla} \times \vec{B} = \mu_0 \vec{J} (Ampere's law)

Now, let's focus on the second MHD equation, \vec{\nabla} \times \vec{B} = \mu_0 \vec{J}. We can rearrange this equation to solve for \vec{B}:

\vec{B} = \frac{1}{\mu_0} \vec{\nabla} \times \vec{J}

Next, let's consider the high resistivity case, where \eta is very large. This means that the resistivity of the plasma is high, and therefore the current density \vec{J} is small. Plugging this into our equation for \vec{B}, we get:

\vec{B} = \frac{1}{\mu_0} \vec{\nabla} \times \vec{J} \approx \frac{1}{\mu_0} \vec{\nabla} \times 0 = 0

This tells us that at high resistivity, the magnetic field is approximately zero. This has significant consequences for the behaviour of magnetic field lines. In the absence of a strong magnetic field, the plasma will not be confined and will be free to move and expand. This can lead to instabilities and disruptions in the plasma, which can have negative effects on any plasma-based systems or experiments.

I hope this helps get you started on your solution. Remember to always use the fundamental equations and consider
 

1. What are MHD equations?

MHD equations, or magnetohydrodynamic equations, are a set of equations that describe the behavior of a plasma (ionized gas) that is influenced by both magnetic and electric fields.

2. How are MHD equations derived?

MHD equations are derived from the fundamental laws of physics, such as conservation of mass, momentum, and energy, as well as Maxwell's equations for electromagnetism.

3. What are some consequences of MHD equations?

Some consequences of MHD equations include the ability to describe and predict the behavior of plasmas in various scenarios, such as in astrophysical environments or in laboratory experiments.

4. How are MHD equations used in research?

MHD equations are used in a variety of research fields, including astrophysics, plasma physics, and engineering. They are also used in computer simulations to study and analyze complex plasma phenomena.

5. What are some limitations of MHD equations?

MHD equations have certain limitations, such as not taking into account certain effects like turbulence or collisions between particles. They also cannot fully describe highly nonlinear or turbulent plasma behavior.

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