Optical Fibre Communication Systems

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Presentation transcript:

Optical Fibre Communication Systems Lecture 2: Nature of Light and Light Propagation Professor Z Ghassemlooy Northumbria Communications Laboratory School of Informatics, Engineering and Technology The University of Northumbria U.K. http://soe.unn.ac.uk/ocr

Contents Wave Nature of Light Particle Nature of Light Electromagnetic Wave Reflection, Refraction, and Total Internal Reflection Ray Properties in Fibre Types of Fibre Fibre Characteristics Attenuation Dispersion Bandwidth Distance Product Summary

G Ekspong, Stockholm University, Sweden, 1999. Wave Nature of Light Newton believed in the particle theory of light. He explained the straight-line casting of sharp shadows of objects placed in a light beam. but he could not explain the textures of shadows Wave theory: Explains the interference where the light intensity can be enhanced in some places and diminished in other places behind a screen with a slit or several slits. The wave theory is also able to account for the fact that the edges of a shadow are not quite sharp. This theory describes: Propagation, reflection, refraction and attenuation G Ekspong, Stockholm University, Sweden, 1999.

Wave Nature of Light - contd. 1864 James Clerk Maxwell His mathematical theory of electromagnetism led to the view that light is of electromagnetic nature, propagating as a wave from the source to the receiver. 1880s Heinrich Hertz Discovered experimentally the existence of electromagnetic waves at radio-frequencies. Wave theory does not describe the absorption of light by a photosensitive materials 1900-20 Max Planck, Neils Bohr and Albert Einstein Invoked the idea of light being emitted in tiny pulses of energy

Particle Nature of Light Light behaviour can be explained in terms of the amount of energy imparted in an interaction with some other medium. In this case, a beam of light is composed of a stream of small lumps or QUANTA of energy, known as PHOTONS. Each photon carries with it a precisely defined amount of energy defined as: Wp = h*f Joules (J) where; h = Plank's constant = 6.626 x 10-34 J.s, f = Frequency Hz The convenient unit of energy is electron volt (eV), which is the kinetic energy acquired by an electron when accelerated to 1 eV = 1.6 x 10-19 J. Even although a photon can be thought of as a particle of energy it still has a fundamental wavelength, which is equivalent to that of the propagating wave as described by the wave model. This model of light is useful when the light source contains only a few photons.

Electromagnetic Spectrum

Electromagnetic Radiation Carries energy through space (includes visible light, dental x-rays, radio waves, heat radiation from a fireplace) The wave is composed of a combination of mutually perpendicular electric and magnetic fields the direction of propagation of the wave is at right angles to both field directions, this is known as an ELECTROMAGNETIC WAVE EM wave move through a vacuum at 3.0 x 108 m/s ("speed of light") Speed of light in a vacuum

The Wave Equation Solutions to Maxwell’s equations:   Plane wave: phase fronts  Plane wave: Spherical wave:

One Dimensional EM Wave For most purposes, a travelling light wave can be presented as a one-dimensional, scalar wave provided it has a direction of propagation. Such a wave is usually described in terms of the electric field E. Wavelength  Eo Phase z A plane wave propagating in the direction of z is: The propagation constant (or wave number) Phase velocity n = Propagation medium refractive index

Polarization Light is a transverse, electromagnetic wave, where the transverse nature of it can be demonstrated through polarization. Unpolarized light source: The electric field is vibrating in many directions; all perpendicular to the direction of propagation. Polarized light source: The vibration of the electric field is mostly in one direction. Any direction is possible as long as it's perpendicular to the propagation. Horizontal Vertical Diognal

Group Velocity A pure single frequency EM wave propagate through a wave guide at a Phase velocity However, non-monochromatic waves travelling together will have a velocity known as Group Velocity: 1.44 1.46 1.49 500 1700 1900 n ng  (nm) Ref. index Where the fibre group index is:

Reflection and Refraction of Light Medium 1 1 2 n1 n2 n1 < n2 1 2 n2 n1 n1 > n2 1 Reflected ray Refracted Incident 2 Boundary Medium 2 Using the Snell's law at the boundary we have: n1 sin 1 = n2 sin 2 or n1 cos 1 = n2 cos 2 1 = The angle of incident

Total Internal Reflection n1 > n2 1 As 1 increases (or 1 decreases) then there is no reflection The incident angle 1 =  c = Critical Angle Beyond the critical angle, light ray becomes totally internally reflected 1>c n2 n1 n1 > n2 1<c 1 When 1 = 90o (or c = 0o) n1 sin 1 = n2 Thus the critical angle

Ray Propagation in Fibre - Bound Rays  > c,  > max c 5 3 a 2 1  4 Core n1 Air (no =1) Cladding n2 From Snell’s Law: n0 sin  = n1 sin (90 - )  = max when  = c Thus, n0 sin max = n1 sin c

Ray Propagation in Fibre - contd. Or n0 sin max = n1 (1 - sin2 c)0.5 Since Then NA determines the light gathering capabilities of the fibre

Ray Propagation in Fibre - contd. Therefore n0 sin max = NA Fibre acceptance angle Note Relative refractive index difference Thus 0.14< NA < 1

Modes in Fibre A fiber can support: many modes (multi-mode fibre). a single mode (single mode fiber). The number of modes (V) supported in a fiber is determined by the indices, operating wavelength and the diameter of the core, given as. or V<2.405 corresponds to a single mode fiber. By reducing the radius of the fiber, V goes down, and it becomes impossible to reach a point when only a single mode can be supported.

Basic Fibre Properties Cylindrical Dielectric Waveguide Low loss Usually fused silica Core refractive index > cladding refractive index Operation is based on total internal reflection Buffer coating Cladding Core

Types of Fibre There are two main fibre types: (1) Step index: Multi-mode Single mode (2) Graded index multi-mode Total number of guided modes M for multi-mode fibres: Multi-mode SI Multi-mode GI

Step-index Multi-mode Fibre Output pulse Input pulse n2 = 1.46 Advantages: Allows the use of non-coherent optical light source, e.g. LED's Facilitates connecting together similar fibres Imposes lower tolerance requirements on fibre connectors. Cost effective dn=0.04,100 ns/km Disadvantages: Suffer from dispersion (i.e. low bandwidth (a few MHz) High power loss

Graded-index Multi-mode Fibre Output pulse Input pulse Advantages: Allows the use of non-coherent optical light source, e.g. LED's Facilitates connecting together similar fibres Imposes lower tolerance requirements on fibre connectors. Reduced dispersion compared with STMMF dn = 0.04,1ns/km Disadvantages: Lower bandwidth compared with STSMF High power loss compared with the STSMF

Step-index Single-mode Fibre Output pulse Input pulse dn = 0.005, 5ps/km Advantages: Only one mode is allowed due to diffraction/interference effects. Allows the use high power laser source Facilitates fusion splicing similar fibres Low dispersion, therefore high bandwidth (a few GHz). Low loss (0.1 dB/km) Disadvantages: Cost

Single Mode Fiber - Power Distribution Guided Evanescent Optical power Intensity profile of the fundamental mode

Fibre Characteristics The most important characteristics that limit the transmission capabilities are: Attenuation (loss) Dispersion (pulse spreading)

Attenuation - Standard Fibre 180 nm SM-fiber, InGaAsP DFB-laser, ~ 1990 Optical amplifiers InGaAsP FP-laser or LED 80nm 600 800 1000 1200 1400 1600 1800 0.2 0.5 1.0 2.0 5 10 0.1 Wavelength (nm) Attenuation (dB/km) MM-fibre, GaAs-laser or LED 1st window- 1975 2nd window 1980 3rd window 1985 Fourth Generation, 1996, 1.55 mm WDM-systems 1300 nm 1550 nm Bandwidth = 1.142 x 1014 Hz |1300 nm + 2.2475 1014 Hz |1550 nm

Attenuation (Loss ) - contd. Fibre Pi Po L Po (L)= Pi (0).e- pL The output power Fibre attenuation coefficient (p =  scattering +  absorption +  bending) Or in dB/km, fibre attenuation

Fibre Attenuation - contd. In a typical system, the total loss could bas 20-30 dB, before it needs amplification. So, at 0.2 dB/km, this corresponds to a distance of 100-150 km. Attenuation along the fibre link can be measured using Optical Time Domain Reflectometer

Fibre Dispersion Data carried in an optical fibre consists of pulses of light energy consists of a large number of frequencies travelling at a given rate. There is a limit to the highest data rate (frequency) that can be sent down a fibre and be expected to emerge intact at the output. This is because of a phenomenon known as Dispersion (pulse spreading), which limits the "Bandwidth” of the fibre. si(t) T so(t) Output pulse  L Many modes Cause of Dispersion: Chromatic (Intramodal) Dispersion Modal (Intermodal) Dispersion

Chromatic Dispersion It is a result of group velocity being a function of wavelength. In any given mode different spectral components of a pulse traveling through the fibre at different speed. It depends on the light source spectral characteristics. Laser  = 1-2 nm  = R.M.S Spectral width LED (many modes)  = 40 nm wavelength May occur in all fibre, but is the dominant in single mode fibre Main causes: Material dispersion - different wavelengths => different speeds Waveguide dispersion: different wavelengths => different angles

Material Dispersion Refractive index of silica is frequency dependent. Thus different frequency (wavelength) components travel at different speed RMS pulse broadening Where material dispersion coefficient: 0.8 1.0 1.2 1.4 1.6 1.7 -100 100 175 Dmat  2nd window Note: Negative sign, indicates that low wavelength components arrives before higher wavelength components.

However it is significant in monomode fibres. Waveguide Dispersion This results from variation of the group velocity with wavelength for a particular mode. Depends on the size of the fibre. This can usually be ignored in multimode fibres, since it is very small compared with material dispersion. However it is significant in monomode fibres. 0.8 1.0 1.2 1.4 1.6 1.7 -100 100 175 Dmat  Waveguide dispersion Total dispersion Material dispersion

Modal (Intermodal) Dispersion Lower order modes travel travelling almost parallel to the centre line of the fibre cover the shortest distance, thus reaching the end of fibre sooner. The higher order modes (more zig-zag rays) take a longer route as they pass along the fibre and so reach the end of the fibre later. Mainly in multimode fibres 1 2 Cladding n2 Core n1 c  

Modal Dispersion - SIMMF The time taken for ray 1 to propagate a length of fibre L gives the minimum delay time: The time taken for the ray to propagate a length of fibre L gives the maximum delay time: Since The delay difference Since relative refractive index difference Thus

Modal Dispersion - SIMMF For 1, and For a rectangular input pulse, the RMS pulse broadening due to modal dispersion at the output of the fibre is: Total dispersion = chromatic dispersion + modal dispersion

Modal Dispersion - GIMMF The delay difference the RMS pulse broadening

Dispersion - Consequences I- Frequency Limitation (Bandwidth) 1 L = L1 1 T L B 1 L = L2 > L1 Intersymbol interference Maximum frequency limitation of signal, which can be sent along a fibre Intersymbol interference (ISI), which is unacceptable in digital systems which depend on the precise sequence of pulses. II- Distance: A given length of fibre, has a maximum frequency (bandwidth) which can be sent along it. To increase the bandwidth for the same type of fibre one needs to decrease the length of the fibre.

Bandwidth Limitations Maximum channel bandwidth B: For non-return-to-zero (NRZ) data format: B = BT /2 For return-to-zero (RZ) data format: B = BT Where the maximum bit rate BT = 1/T, and T = bit duration. For zero pulse overlap at the output of the fibre BT <= 1/2 where  is the pulse width. For MMSF: BT (max) = 1/2Ts For a Gaussian shape pulse:BT  0.2/rms where rms is the RMS pulse width. For MMSF: BT (max) =0.2/ modal or BT (max) =0.2/ T Total dispersion

Bandwidth Distance Product (BDP) The BDP is the bandwidth of a kilometer of fibre and is a constant for any particular type of fibre. Bopt * L = BT * L (MHzkm) For example, A multimode fibre has a BDP of 20 MHz.km, then:- - 1 km of the fibre would have a bandwidth of 20 MHz - 2 km of the fibre would have a bandwidth of 10 MHz Typical B.D.P. for different types of fibres are: Multimode 6 - 25 MHz.km Single Mode 500 - 1500 MHz.km Graded Index 100 - 1000 MHZ.km

Bandwidth Distance Product Bit rate B (Gbps) 0.1 1 10 100 1000 10,000 Source spectral width = 1 nm Source spectral width < 1 nm Distance L (km) Dmat = 17 ps/km.nm

Controlling Dispersion For single mode fibre: Wavelength 1300: - Dispersion is very small - Loss is high compared to 1550 nm wavelength Wavelength 1550: - Dispersion is high compared with 1300 nm - Loss is low Limitation due to dispersion can be removed by moveing zero-diepersion point from 1300 nm to 1550 nm. How? By controlling the waveguide dispersion. Fibre with this property are called Dispersion-Shifted Fibres

Controlling Dispersion 1.1 1.2 1.3 1.4 1.5 1.6 1.7 -20 20 Standard Dispersion shifted flattened Wavelength ( m m) -10 10

Summary Nature of light : Particle and wave Light is part of EM spectrum Phase and group velocities Reflection, refraction and total internal reflection etc. Types of fibre Attenuation and dispersion