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.
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.
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After completing this section, you will be able to:
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.
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.
⟵ 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
The refractive index \(n\) of any material is calculated from light passing from air into the denser medium.
\(c = \text{Speed of light in a vacuum}\)
\(v = \text{Speed of light in the denser medium}\)
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.
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.
Per second there would be more of the shorter wavelengths (UV) than the longer (infrared).
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 bNormal is simply another term for a line drawn perpendicular (at right angles) to another line, in this case the interface between two mediums.
The refractive index (\(n\) or RI) is calculated using the equation below:
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.
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.
The sine of an angle is calculated from the side lengths of a right angle triangle.
Similarly,
Refractive index is usually measured with some kind of refractometer.
These articles include the use of the refractive index and can both be found at JAIC Online.
In this section, you have learned:
After completing this section, you will be able to:
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.
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.
The mirror for the Hubble telescope was polished to within an accuracy of 30 nanometers. It took two years.
Light hitting a rough surface like a pigment particle is scattered.
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.
The combination of reflections and the refractive index of materials needs to be taken into account for exhibitions and picture framing.
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.
When light travels from a denser medium to a lighter one, the light is bent away from the normal.
If the light strikes the interface at a critical angle, all the light is reflected back into the denser medium.
Light will be totally internally reflected if the following condition is met:
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.
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:
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.
A similar concept is used in attenuated total reflectance Fourier-transform infrared spectroscopy (ATR FTIR)
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.
These articles on the concept of reflection can be found at JAIC Online.
You have learned:
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