Multiple images in a thick mirror

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SUMMARY

The discussion centers on the reflection of light from thick glass mirrors, specifically addressing why 4% of light is reflected at the air/glass boundary. This percentage is derived from the formula R=(1-n/1+n)², where R represents the reflected light and n is the refractive index. For glass with a refractive index of 1.5, this results in a reflection of 4%. The conversation also highlights that the reflection percentage varies with different refractive indices, such as 11.1% for an index of 2 and 0.2% for an index of 1.1. The importance of front-surface reflective mirrors for applications in astronomy and laser work is also emphasized.

PREREQUISITES
  • Understanding of the refractive index in optics
  • Familiarity with the equation for light reflection at boundaries
  • Basic knowledge of optical materials, particularly glass
  • Awareness of applications in astronomy and laser technology
NEXT STEPS
  • Research the effects of surface irregularities on light reflection
  • Explore the properties of front-surface reflective mirrors in detail
  • Learn about the applications of different refractive indices in optical design
  • Investigate the impact of angle of incidence on light reflection
USEFUL FOR

Optical engineers, physicists, and anyone involved in the design and application of reflective surfaces in telescopes and laser systems will benefit from this discussion.

Fiona Rozario
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I understand that 4% of the light is reflected back from the glass surface in a thick glass mirror. But why 4%? Why not 5% or 10%? Will this percentage change if the glass has a lower refractive index?
 
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Where did you read that ? do you have a reference ?

I would expect the percentage to be reflected back from the air/glass boundary surface to be dependent on the quality of the glass and the smoothness of the surface
the rest would be transmitted through the glass and reflected off the rear reflection surface and back out again ( there would be transmission losses in the glass as part of the double traverse the light does as well)

lets see what others have to say :)

Dave
 
Fiona Rozario said:
I understand that 4% of the light is reflected back from the glass surface in a thick glass mirror. But why 4%? Why not 5% or 10%? Will this percentage change if the glass has a lower refractive index?

Neglecting surface irregularities and assuming the light strikes at a normal angle (perpendicular to the surface), the amount of light reflected by transparent surface is given by the equation R=(1-n/1+n)2, where R is the amount of light reflected and n is the refractive index. Glass with a refractive index of 1.5 gives us: R=(1-1.5/1+1.5)2, which comes out to be R=0.04, which is 4%.

With a refractive index of 2: R=(1-2/1+2)2, or R=0.111..., which is about 11.1%.

With a refractive index of 1.1: R=1-1.1/1+1.1)2, or R=0.002268, about 0.2%.

Finding the amount of light reflected when the light is striking at an angle other than normal is much more complicated.
 
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Drakkith said:
Neglecting surface irregularities and assuming the light strikes at a normal angle (perpendicular to the surface), the amount of light reflected by transparent surface is given by the equation R=(1-n/1+n)2, where R is the amount of light reflected and n is the refractive index. Glass with a refractive index of 1.5 gives us: R=(1-1.5/1+1.5)2, which comes out to be R=0.04, which is 4%.

With a refractive index of 2: R=(1-2/1+2)2, or R=0.111..., which is about 11.1%.

With a refractive index of 1.1: R=1-1.1/1+1.1)2, or R=0.002268, about 0.2%.

Finding the amount of light reflected when the light is striking at an angle other than normal is much more complicated.

Thank you!
 
This is why accurate mirrors as are needed for astronomy and laser work are front-surface reflective.
 
Danger said:
This is why accurate mirrors as are needed for astronomy and laser work are front-surface reflective.

Indeed. To my knowledge, pretty much all telescope mirrors are front-surface reflective.
 

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