Fast/slow Alfven waves in High/Low Beta Plasma?

In summary: WileyIn summary, Alfven waves are sound waves in a plasma, and their propagation speed depends on the plasma beta value, which is the ratio of plasma pressure to magnetic pressure. For a more thorough understanding, you can refer to various textbooks and online resources on plasma physics and electrodynamics.
  • #1
Alita1984
1
0
Guys can you please tell me how fast/slow Alfven waves propogate in High/Low Beta Plasma? I need to derive equation cannot find any clue on that! Please be so kind to help me please!:rolleyes:
 
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  • #3
MHD wave theory borders on crackpot.
 
  • #4
Thread closed for Moderation...
 
  • #5
Thread re-opened.
 
  • #6
Crackpot? That's news to me. Alfven won the Nobel Prize. Aren't Alfven waves just sound waves in a plasma?

It is true that Alfven came up with a cosmological theory that turned out to be wrong and that crackpots have latched onto it, but Alfven can't be blamed for that.
 
  • #7
You can find the general theory of plasma waves in hot (or cold) plasmas (any beta) in this chapter:

http://psl.postech.ac.kr/material/lecture/chap3.pdf

In principle, you can identify the cold limit and the Alfven wave and see how it transform in hot plasmas.

See also the cold text:

http://psl.postech.ac.kr/material/lecture/chap1.pdf

The reference above is rather lengthy, you may find similar material in a more compact presentation, with google.
My preferred reference on plasma electrodynamics is:

Principles of plasma electrodynamics, Springer

A more specialized book on Alfven waves might help you too:

The Physics of Alfven Waves
 

Related to Fast/slow Alfven waves in High/Low Beta Plasma?

1. What are fast/slow Alfven waves?

Fast/slow Alfven waves are types of plasma waves that propagate through a plasma, which is an ionized gas consisting of positively and negatively charged particles. These waves are named after Hannes Alfven, a Swedish scientist who first described them in the 1940s. Fast Alfven waves are characterized by high frequency oscillations and require a high-beta plasma, while slow Alfven waves have lower frequency oscillations and can propagate in both high and low beta plasmas.

2. What is a high/low beta plasma?

Beta (β) is a parameter that describes the ratio of plasma pressure to magnetic pressure in a plasma. A high-beta plasma has a high pressure compared to its magnetic field, while a low-beta plasma has a low pressure compared to its magnetic field. This parameter is important because it determines the behavior of plasma waves, including fast and slow Alfven waves.

3. How do fast/slow Alfven waves differ from each other?

In addition to their different frequency characteristics, fast and slow Alfven waves also have different properties and behaviors. Fast Alfven waves can only propagate in a high-beta plasma and are typically associated with strong magnetic fields. Slow Alfven waves, on the other hand, can propagate in both high and low beta plasmas and are often associated with weaker magnetic fields. Additionally, fast Alfven waves can only propagate in the direction of the magnetic field, while slow Alfven waves can also propagate perpendicular to the magnetic field.

4. What are the applications of studying fast/slow Alfven waves in high/low beta plasma?

Studying fast/slow Alfven waves in high/low beta plasma has many practical applications. These waves play a role in the dynamics of solar flares and other space weather events. Understanding their behavior can also help us better understand and predict the behavior of plasma in fusion reactors, which use magnetic fields to confine and heat plasma to extremely high temperatures. Additionally, these waves are being studied for potential use in plasma-based propulsion systems for spacecraft.

5. How are fast/slow Alfven waves in high/low beta plasma studied?

There are various methods used to study fast/slow Alfven waves in high/low beta plasma. Some of these include laboratory experiments using plasma devices, numerical simulations on computers, and observations from spacecraft and satellites. Researchers also use theoretical models and mathematical equations to understand the behavior of these waves in different plasma environments.

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