Help with EM waves travelling through a plasma

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SUMMARY

The discussion focuses on the propagation of electromagnetic (EM) waves through plasma, specifically in the context of intelligent beings attempting to communicate with Earth using radio waves swept from 10 to 50 MHz. It is established that during solar flares, frequencies between 24.25 and 28 MHz are blocked by the radiation belt plasma, indicating the need to deduce the plasma frequency and magnetic field. Key concepts include identifying the type of plasma waves, their cutoff regions, and the relationship between plasma density and the background magnetic field (B0). The discussion emphasizes the importance of understanding wave properties and resonances in plasma physics.

PREREQUISITES
  • Understanding of electromagnetic wave propagation in plasma
  • Familiarity with plasma frequency and its significance
  • Knowledge of the relationship between plasma density and magnetic fields
  • Basic concepts of wave cutoffs and resonances in plasma physics
NEXT STEPS
  • Study Chen's "Introduction to Plasma Physics and Controlled Fusion" for foundational knowledge on plasma waves
  • Research the properties of electromagnetic waves in plasma, focusing on cutoff frequencies
  • Explore the mathematical relationship between plasma density and magnetic field strength
  • Investigate the effects of solar flares on radio wave propagation through plasma
USEFUL FOR

Students preparing for exams in plasma physics, researchers studying electromagnetic wave interactions with plasma, and professionals in astrophysics or space communication technologies.

can't.do.phys
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I've been given a practice question for an exam and I can't quite get it started. The question is: Intelligent beings on a distant planet try and communicate with Earth by sending powerful radio waves swept in frequency from 10 to 50MHz per minute. The linearly polarized emissions must pass through a radiation belt plasma in such a way that E and k are perpendicular to B0. It is found that during solar flares on their sun, frequencies between 24.25 and 28MHz do not get through their radiation belt. From this deduce the plasma frequency and magnetic field there.
I think I have to figure out the group velocity but does it also have to do with the cut off region of a plasma frequency? and how do I connect it all together to find out the plasma density and magnetic field? I'm so confused.
 
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First you need to identify what type plasma wave(s) are being used. There are a multitude of different EM waves that propagate in a plasma. Some of them have k parallel to the background B others have k perpendicular to B. The same is true with the perturbed E and background B.

Once you have narrowed down the possible waves, start looking at their properties. Do they have cutoffs? Do they have any resonances? Are there frequencies where these waves are evanescent (they don't propagate)?

How do you relate these cut-offs and such to the plasma density or background B?

I suggest looking at Chen's Introduction to Plasma Physics and Controlled Fusion for a detailed introduction to plasma waves.
 

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