Calculating refraction in continuous refractive index

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SUMMARY

The discussion focuses on calculating the deflection angle θ of light from a distant star as it passes near the sun, using the refractive index formula n = √(1 + 5920/r). Participants emphasize the application of Snell's law to model the refraction through discrete layers of varying refractive index. The solution involves integrating the effects of an infinite number of thin layers, with each layer's refractive index dependent on the distance r from the sun. The need for additional data regarding the proximity of the light beam to the sun's surface is also highlighted.

PREREQUISITES
  • Understanding of Snell's law in optics
  • Familiarity with calculus, specifically integration techniques
  • Knowledge of refractive index concepts
  • Basic principles of light propagation in a medium
NEXT STEPS
  • Study the application of Snell's law in varying refractive indices
  • Learn about integration of functions in physics, particularly in optics
  • Research the concept of continuous refractive index and its implications
  • Explore the effects of gravitational lensing on light paths
USEFUL FOR

Students and educators in physics, particularly those focused on optics and gravitational effects, as well as anyone interested in advanced calculations involving light refraction near massive bodies like the sun.

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Homework Statement



The problem is page 5 on: http://www.physics.ox.ac.uk/olympiad/Downloads/PastPapers/Paper3_2010_.pdf

I will just summarise the question:

The refractive index of space,n, at a distance r from the sun is given by √(1+5920/r). The light from a distant star is deflected by a small angle θ. Using a simple model, calculate θ.

Homework Equations



Snell's law?

The Attempt at a Solution



I have no idea of how to get started with this question. I think that the model will involve some discrete layers but I still wouldn't know how to do the problem. Any help would really be appreciated.
 
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Yes, use Snell's law. Consider a ray of light that would pass some distance s from the sun passing through a thin annulus at radius r. You can calculate the angle at which it intersects that annulus and hence the small adjustment to its trajectory. I think you can treat s as unchanging, since the deflection is small.
 
Seems to me data is missing, especially how close to the sun's surface does the beam get. I suppose you could make your answer a function of that distance as another poster suggests.

Then I'd say you need to do an integration of an infinite number of infinitely thin layers with n a function of r. For each layer Snell's law would apply.
 

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