Refractive Index

Foundation for Advancement in Conservation


© 2008

Introduction

Conservators need to understand the principles of the refractive index of materials when doing restorations. The physics for this subject is reasonably complex. I am going to make some simplifications to several of the concepts involved.

Those of you who really want to do the math should read through the article on refractive index on Wikipedia.

Contents

This tutorial is divided into the following sections:

Please complete each section in order, as the information builds on that covered in previous sections. You can return to any section later.

Press Ctrl+Shift+F to search.

Refractive Index Learning Objectives

After completing this section, you will be able to:

What Is Refractive Index?

The refractive index is all about the apparent changes that we see in the speed of light when it travels through a different medium such as water.

The physicests Essen and Gordon-Smith confirmed that the speed of light in a vacuum was 300,000,000 meters per second (give or take a few thousand meters).

Conservators would need to use the refractive index of an adhesive if they were repairing a transparent material such as glass.

Light Waves

Animated GIF of a sine wave

All energy (including light) travels in waves. The wavelength is measured from the top of one wave to the top of the next. The amplitude is the height of the wave.

Electromagnetic Spectrum

Diagram of electromagnetic wavelengths, from gamma rays at 0.1 angstrom, through visible light at 400 to 700 nanometers, down to long waves at one meter.

⟵ High energy end



We perceive only a very small part of the total electromagnetic spectrum as light and color.

The shorter the wavelength, the higher the energy.



⟵ Low energy end

Mathematical Definition

The refractive index \(n\) of any material is calculated from light passing from air into the denser medium.

\(n = \frac{c}{v}\)

\(c = \text{Speed of light in a vacuum}\)

\(v = \text{Speed of light in the denser medium}\)

The light travels more slowly through the denser medium because of interactions between its energy and the electron clouds. The light travels at the same wavelength in both the air and the denser medium but the frequency is slower in the dense medium.

Units of Measurement of Frequency

The frequency of light is measured in Hertz (Hz) or cycles per second.

Imagine standing at a finish line, counting the number of wave peaks as they pass.

Diagram showing the difference in wavelength between infrared and ultraviolet light

Per second there would be more of the shorter wavelengths (UV) than the longer (infrared).

Bending Path of Light

Diagram showing the path of light as it passes through a denser medium

The path of light bends as it passes from the lighter to denser medium, then bends back to its original path as it leaves.

angle a = angle a   angle b = angle b

Normal Angle

Image of a paintbrush in a glass of water, with a vertical dashed line demonstrating the changed path of the light Diagram showing the normal angle between two mediums

Normal is simply another term for a line drawn perpendicular (at right angles) to another line, in this case the interface between two mediums.

Calculation of RI

The refractive index (\(n\) or RI) is calculated using the equation below:

Diagram showing the angle of incidence i and angle of refraction r


\(n = \frac{\color{darkred}{\sin i}}{\color{darkblue}{\sin r}}\)

On the whole conservators are not expected to calculate the refractive index, although they do need to be able to use the information it gives.

Calculation of RI Cont.

If you know the refractive index of any two materials, then you can calculate the amount that the light will be bent from Snell's law.

Diagram showing the angle of incidence i or refractive index A entering the denser medium, and the angle of refraction r or refractive index B within the denser medium

\(\require{color}\frac{\color{darkred}\text{Sine} \ i}{ \color{darkblue}\text{Sine} \ r} =\frac{\color{darkblue}\text{Refractive index B}}{ \color{darkred}\text{Refractive index A}}\)

\(\color{darkred}\text{Sine }\ i\ \times \ \text{Refractive index A} \color{black} = \color{darkblue}\text{Sine}\ r \times \text{Refractive index B} \)

Sine of an Angle: Definition

The sine of an angle is calculated from the side lengths of a right angle triangle.

Image of a right triangle, with angle a between the adjacent side and the hypoteneuse, opening towards the the opposite side.

\(\sin \angle a = \frac{\text{Length of opposite side}}{\text{Length of hypoteneuse}}\)

Similarly,

\(\cos a = \frac{adjacent}{hypoteneuse}\)

\(\tan a = \frac{opposite}{adjacent}\)

Measurement of RI

Image of a refractometer

Refractive index is usually measured with some kind of refractometer.

Refractive Index: References

These articles include the use of the refractive index and can both be found at JAIC Online.

Augerson, Christopher C.; Messinger, John M.; "Controlling the Refractive Index of epoxy adhesives with acceptable yellowing after aging"; JAIC 1993, 32 (3). 311–314.

Nagy, Eleonora E.; "Fills for white marble: properties of seven fillers and two thermosetting resins"; JAIC 1998, 37 (1). 69–87.

Refractive Index: Summary

In this section, you have learned:

  • How visible light fits into the electromagnetic spectrum
  • The equation that defines refractive index
  • How to calculate the refractive index
  • How Snell's law is used to calculate the amount light will be bent

Reflection

Image of a laser reflecting off a mirror in front of a protractor, showing an angle of fifty degrees before and after reflecting

Reflection: Learning Objectives

After completing this section, you will be able to:

Reflection, Color, and Texture

Macro image of green gouache

The way light reflects off an object determines, to a large extent, the color and texture of the surface.

This is important for filling and in-painting.

Specular Reflection

When light hits a smooth surface some of it is reflected and some of it is refracted. Reflection from a smooth surface, like a mirror, is called specular reflection.

Diagram showing that the angle of incoming light a and reflected light b are equal, with refracted light entering the denser medium at a different angle

Hubble Telescope Example

Photo of the Hubble Space Telescope mirror being polished

The mirror for the Hubble telescope was polished to within an accuracy of 30 nanometers. It took two years.

A small miscalculation in the shape need for the surface meant that light at the edges and the center reflected back to different points on the receiver, causing a halo.

Image showing a photo taken in 1993 next to one taken in 1994, showing the improved sharpness. The link includes another photo taken in 2018 after the mirror was refined further. Images before and after corrective "surgery" was carried out in space.

Diffuse Reflection

Light hitting a rough surface like a pigment particle is scattered.

Diagram showing light bouncing off a rough surface in different directions

Combination of Reflection and Refraction

Light is reflected and refracted when it hits the boundary between any two different materials. This can get quite complicated.

The amount of light that is reflected at each boundary depends on the differences in the refractive indices.

Combination of Reflection and Refraction

The combination of reflections and the refractive index of materials needs to be taken into account for exhibitions and picture framing.

Diagram of light passing from air, into water, then glass, with some reflecting off the boundary each time to return in three parallel lines

Critical Angle

The critical angle depends on the ratio between the two refractive indices shown below.

When light travels from a lighter medium (low refractive index) to a denser medium (high refractive index) the light is bent towards the normal. Diagram of light entering a denser medium and bending towards the normal

When light travels from a denser medium to a lighter one, the light is bent away from the normal. Diagram of light entering a lighter medium and bending away from the normal

If the light strikes the interface at a critical angle, all the light is reflected back into the denser medium.Diagram of light reflecting at the interface with no refraction

Critical Angle

Photo of a diamond

Light will be totally internally reflected if the following condition is met:

\(\frac{n_2}{n_1}\leq 1\)

The refractive index of the lighter medium divided by the refractive index of the denser medium is equal to or less than 1.

For light moving from glass into air (or into a vacuum), the critical angle is approximately 41.8º.

The critical angle for diamond is about 24.4º. Jewelers cut diamonds so that most of the light is internally reflected.

Application of Total Internal Reflection

We can find the physics of total internal reflection put to good use in the cool fiber optic lighting that is used in exhibitions and some scientific equipment. The fiber in fiber optics consists of:

Diagram of an optic fiber, with a core, usually made of glass, cladding that reflects the light, and a buffer coating that protects the fiber

More on Fiber Optics

Diagram of an optical fiber with the buffer on the outside, cladding between, and the core in the center

The light is shone down a glass core that has a high refractive index.

The light reflects from the cladding which has a much smaller refractive index.

The light will reflect from the cladding and travel down the glass core even when the fiber is bent.

ATR FTIR

A similar concept is used in attenuated total reflectance Fourier-transform infrared spectroscopy (ATR FTIR)

Diagram showing infrared light reflecting off the sample and a mirror parallel to it multiple times

Infrared light is shone along a sample cell. At each reflection point it enters the sample for a few microns. An absorption spectrum is produced from the sampling points.

Reflection: References

These articles on the concept of reflection can be found at JAIC Online.

Baas, Valerie; Foster, Christopher; Trentelmen, Karen; "The effects of four different wet treatments on albumen photograph"; JAIC 1999, 38 (2). 176–185.

Mayer, Lance; Myers, Gay; "American Impressionism, matteness, and varnishing"; JAIC 2004, 43 (3). 237–254.

Sease, Catherine; "Light Piping: a new lighting system for museum cases"; JAIC 1993, 32 (3). 279–290.

Reflection: Summary

You have learned:

  • How light reflection contributes to color and texture of a surface
  • The difference between specular and diffuse reflection
  • How the combination of reflection and refraction needs to be accounted for in exhibiting artwork
  • How the critical angle can be used to determine how much light is internally reflected
  • Several practical applications of knowledge of the critical angle

Credits

Researched and written by Sheila Fairbrass Siegler

Instructional Design by Cyrelle Gerson of Webucate Us

Project Management by Eric Pourchot

Special thanks to members of the Association of North American Graduate Programs in Conservation (ANAGPIC) and the AIC Board of Directors for reviewing these materials.

This project was conceived at a Directors Retreat organized by the Getty Conservation Institute and was developed with grant funding from the Getty Foundation.

Converted to HTML5 by Avery Bazemore, 2021

© 2008 Foundation for Advancement in Conservation