Calculating refraction in continuous refractive index

In summary, the question asks for the calculation of the deflection angle of light from a distant star passing through a medium with a variable refractive index, given by √(1+5920/r). The suggested approach is to use Snell's law and consider the angle at which the light intersects an annulus at a distance r from the sun. The deflection can then be calculated by integrating over an infinite number of thin layers, with the refractive index changing as a function of distance. However, further information is needed, such as the distance at which the light passes through the medium.
  • #1
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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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  • #2
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.
 
  • #3
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.
 

FAQ: Calculating refraction in continuous refractive index

What is the formula for calculating refraction in continuous refractive index?

The formula for calculating refraction in continuous refractive index is n1 sinθ1 = n2 sinθ2, where n1 is the refractive index of the initial medium, θ1 is the angle of incidence, n2 is the refractive index of the final medium, and θ2 is the angle of refraction.

How do you determine the refractive index of a medium?

The refractive index of a medium can be determined by measuring the speed of light in that medium and dividing it by the speed of light in a vacuum. This is also known as Snell's Law, and the resulting value is a dimensionless quantity.

What factors can affect the refractive index of a medium?

The refractive index of a medium can be affected by factors such as temperature, pressure, and the wavelength of light passing through it. Changes in these factors can cause the refractive index to vary, resulting in changes in the angle of refraction.

How does the refractive index vary in different mediums?

The refractive index varies in different mediums due to the density and composition of the medium. Materials with a higher density and different chemical makeup will have a higher refractive index, meaning that light will travel slower through these mediums.

What is the practical application of calculating refraction in continuous refractive index?

Calculating refraction in continuous refractive index is used in a variety of practical applications, such as designing lenses for cameras and glasses, determining the shape and size of lenses for corrective vision, and understanding how light travels through different mediums in scientific experiments.

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