Principles of light guidance

# Principles of light guidance

## Principles of light guidance

- - - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - - -
##### Presentation Transcript

1. Principles of light guidance Early lightguides Luminous water fountains with coloured films over electric light sources built into the base were used for early public displays. These fountains use the same basic principle of light guidance as modern optical fibres. The same idea is still used today in fountains, advertising displays, car dashboards... Paris Exposition of 1889

2. Principles of light guidance How water can guide light • The water in the jet has a higher optical density, or refractive index, than the surrounding air. • The water-air surface then acts as a mirror for light propagating in the water jet. • Rays of light travel in straight lines and are reflected back into the jet when they reach its outer surface. • Hence the light rays follow the jet of water as it curves towards the ground under gravity.

3. Tyndall’s* demonstration for the classroom * or more accurately, “Colladon’s demonstration”

4. Optical fibres – threads of glass Human hair for comparison 50 – 80 mm Typical refractive indices: Cladding: ncl = 1.4440 Core: nco = 1.4512 Light is guided along the core by Total Internal Reflection Cladding helps isolate light from edge of fibre where losses and scattering are high

5. Total Internal Reflection Rays striking an interface between two dielectrics from the higher index side are totally internally reflected if the refracted ray angle calculated from Snell’s Law would otherwise exceed 90˚. If n1 = 1.470 and n2 =1.475, say, then qcrit = 85.28˚ within a fibre core

6. Bound rays vs Refracting Rays Bound rays zig-zag indefinitely along a fibre or waveguide Refracting rays decay rapidly as they propagate

7. Visible laser focused into an optical fibre This Argon laser excites both leaky modes and bound modes “Spatial transient” glow due to leaky modes scattering from acrylate jacket material Several Watts @ l = 514nm Light scatters off the air itself ! Bound modes continue for many km along the fibre, and are seen here due to Rayleigh scattering, the main cause of attenuation in modern fibres Rayleigh scattering is much reduced at longer infrared wavelengths

8. Applying Snell’s Law: Numerical Aperture Numerical Aperture is defined as NA = n0 sinawhere a is the cone half-angle for the emerging light rays, and n0 is the external index. In a simple way, NA characterises the light gathering ability of an optical fibre. Ray diagram Knowing the critical angle inside the fibre helps us calculate a, and hence the NA by successive applications of Snell’s Law:

9. An optical communications link So, where does this optical fibre fit into the overall picture?

10. Digitisation of analogue data Voice is sampled digitally about 8000 times every second, and each sample needs 8 bits of data to encode it, so a telephone conversation requires 64,000 bits/sec. Quality does not suffer by discrete sampling if it is fast enough. This is analogous to projecting 25 discrete movie frames per second, which fools the eye into seeing a continuous picture sequence.

11. Dispersion - a problem in step profile fibres Different rays propagate along step profile fibres at different rates - this is known as multimode dispersion. Pulse distortion is greater for fibres with many modes, and gets worse as the fibre length increases.

12. Dispersion in step profile fibres: How bad? A simple calculation can tell us how much dispersion to expect in a step profile multimode fibre. Consider a representative segment: The speed of light in the core is c / ncore. Hence the transit time through the segment for the axial ray is Of course, that’s the fastest possible time. The slowest is for the critical ray... The critical ray travels a distance S, where: Hence, the transit time for the critical ray is: We are interested in the time delay: Or more particularly, the time delay per unit length along the fibre: For typical multimode fibres, ncore ~1.48, nclad ~ 1.46 , so DT/L ~ 67 ns / km by this calculation. In fact, practical fibres exhibit DT/L ~ 10 - 50 ns / km, due to mode mixing.

13. Variation on a theme: Graded index fibre Shortest Path (physically) travels through the highest index region and is therefore slow. Longest Path (physically) travels through lower index some of the time and is faster With the correct graded index profile, all rays can have identical transit times, eliminating multimode dispersion !! Caution: There are still other types of dispersion present !

14. Chromatic Dispersion Even if we eliminate all types of multimode dispersion, pulses of light having different wavelengths still travel at different velocities in silica, so pulse spreading is still possible if we use a spread of wavelengths. This is called Material Dispersion and is responsible for rainbows etc. Together, Material Dispersion and Waveguide Dispersion are termed Chromatic Dispersion. The pulse spread is proportional to fibre length L and wavelength spread Dl. In the fundamental mode, the light spreads out differently into the cladding depending on wavelength. Hence, different wavelengths have different ‘effective refractive indices’. This is Waveguide Dispersion.

15. Transmission through an optical fibre Telecommunications engineers quantify the transmission of light through a system using logarithmic units called decibels (dB): Transmission in dB = 10 log10 (Pout / Pin) GAIN LOSS Lasers, amplifiers etc... Fibres, passive components etc...

16. The telecommunications windows

17. Attenuation mechanisms Several effects lead to loss of light in fibres: Absorption by impurity ions and atoms of the pure glass (eg, OH- ion) Absorption by vibrating molecular bonds (eg Si - O) Rayleigh Scattering by inhomogeneities frozen into the glass structure itself Each of these effects has a strong spectral dependence!