How Deeply Can We See Into the Sun?

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SUMMARY

This discussion focuses on the depth of visibility into the Sun, emphasizing that visibility varies with the line of sight. It clarifies that what we observe is light emitted from a low-density plasma, contrasting it with the challenges of seeing through fog. The conversation confirms that wavelength significantly influences visibility, as the photon mean free path, which is dependent on wavelength, determines how deeply we can see into the Sun. The product of the mean free path and plasma density ultimately dictates optical depth.

PREREQUISITES
  • Understanding of photon mean free path
  • Knowledge of plasma physics
  • Familiarity with optical properties of light
  • Basic concepts of wavelength and its effects on visibility
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  • Research the relationship between photon mean free path and plasma density
  • Explore the principles of plasma physics in astrophysics
  • Study the effects of wavelength on light scattering and absorption
  • Investigate optical depth in astrophysical contexts
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Astronomers, astrophysicists, and students interested in solar physics and the optical properties of stellar plasmas.

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How deeply into the Sun can we see?
What are we actually seeing?
Is wavelength related to how much we can see into the sun?
 
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blumfeld0 said:
How deeply into the Sun can we see?

Varies with the line of sight.
What are we actually seeing?

Light emitted from a low density plasma, kinda like the opposite of trying to see through fog over a great distance (since the plasma is emitting, rather than scattering and blocking the light)

Is wavelength related to how much we can see into the sun?

Yes, because the photon mean free path (how far photons travel before being scattered or absorbed) is wavelength dependent, and it is the product of the mean free path and density that determine how 'deep' we can see optically.
 
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