MODULE 5 · SYLLABUS 5.10 · LEVEL 1

Chapter 7: Fibre Optics

How light is guided along a glass fibre by total internal reflection, the terms you need (core, cladding, numerical aperture, modes, attenuation, dispersion, bend radius), the advantages and drawbacks against copper, terminations, splices and couplers, the fibre-optic data bus, and fibre on aircraft.

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🎯 What you'll learn
  • Total internal reflection, core and cladding, critical angle and numerical aperture
  • Cable construction, single-mode and multimode (step-index and graded-index) fibre
  • Light sources and detectors; attenuation, dispersion, decibels and bend radius
  • Advantages and disadvantages of fibre against electrical wire
  • Terminations, splices, couplers, control terminals and remote terminals — the fibre-optic data bus
  • Applications on aircraft and handling, cleaning and safety
📖 The lesson

How a fibre guides light

An optical fibre is a hair-thin strand of very pure glass (or plastic) that carries information as pulses of light instead of electrical current. It has two layers of glass with slightly different refractive indices: the central core (higher index, n₁) and the surrounding cladding (lower index, n₂).

Light guided by total internal reflection cladding n₂ (lower) core n₁ (higher) acceptance cone steeper than the cone: escapes, lost ▲ beyond the critical angle → totally reflected sin θc = n₂ / n₁ · numerical aperture NA = sin θa = √(n₁² − n₂²) ≈ 0.2–0.3 for multimode fibre
Total internal reflection. The core has a slightly higher refractive index than the cladding. Light that meets the boundary at more than the critical angle is reflected completely back into the core, so it zig-zags along the fibre with very little loss. Only light entering within the acceptance cone (set by the numerical aperture) is guided; the rest escapes.
  • When light passes from a denser to a less dense medium it bends away from the normal. Beyond the critical angle (sin θc = n₂/n₁) it cannot escape at all and is totally internally reflected. Light launched into the core at a shallow enough angle therefore bounces along the fibre, trapped, even around gentle bends.
  • The acceptance angle is the largest angle to the fibre axis at which entering light is still guided. Its sine is the numerical aperture (NA) = √(n₁² − n₂²), typically 0.2–0.3 for multimode glass fibre. A large NA collects light easily from an LED.
Cross-section of a fibre cable outer jacket strength member (aramid yarn) buffer / coating 250–900 µm cladding — 125 µm core — 9 µm SM, 50 / 62.5 µm MM Glass or plastic? Glass (silica) fibre: low loss, long distances, high bandwidth Plastic optical fibre (POF): ≈ 1 mm core, cheap, easy to terminate — short links only Wavelengths (infrared — invisible) 850 nm · 1 300 nm · 1 550 nm lowest loss ≈ 0.2 dB/km at 1 550 nm
Construction. The light travels in the tiny core; the cladding keeps it there. A plastic buffer protects the glass, an aramid strength member takes any pull so the fibre itself is never stretched, and the jacket protects the whole cable. Aircraft cables add tougher, fire-resistant materials.

Fibre types

Step-index multimode core 50–62.5 µm (or 1 mm POF) in out Graded-index multimode index falls gradually from the centre in out Single-mode core ≈ 9 µm — one path only in out different ray paths arrive at different times (modal dispersion) → the pulse spreads → less bandwidth
Modes. In a thick multimode core, light takes many paths of different lengths, so a short pulse spreads out — modal dispersion. Graded-index fibre slows the central rays so all paths arrive nearly together. Single-mode fibre has a core so small that only one path exists — the highest bandwidth, but it needs a laser source and very precise connectors.
  • Multimode step-index: a large core (50 or 62.5 µm in glass, about 1 mm in plastic optical fibre) with a sharp change of index at the cladding. Light follows many paths (modes) of different lengths, so pulses spread — modal dispersion limits bandwidth and distance. Cheap, easy to couple light into, used with LEDs for short links.
  • Multimode graded-index: the core's index falls gradually from the centre outwards, so rays travelling the longer, outer paths move faster. All modes arrive almost together — much higher bandwidth than step-index.
  • Single-mode (monomode): a core of about 9 µm carries only one mode, so there is no modal dispersion — the highest bandwidth and longest distances. It needs a laser source and very precise alignment at connectors and splices.
  • Sources: LEDs (cheap, wide beam, multimode) and laser diodes or VCSELs (narrow, powerful, fast — single-mode and high-speed multimode). Detectors: PIN photodiodes and, for weak signals, avalanche photodiodes (APD). Aircraft fibre normally uses invisible infrared at 850 nm or 1 300 nm.

Fibre-optic terms

TermMeaning
AttenuationLoss of light power along the fibre (absorption and scattering), in dB/km. 3 dB is half the power, 10 dB one tenth.
DispersionSpreading of light pulses with distance — modal (multimode) and chromatic (different wavelengths travel at different speeds). It limits bandwidth.
BandwidthThe data rate (or frequency) a given length of fibre can carry, often in MHz·km.
Bend radiusThe tightest curve allowed. Tighter bends let light escape (macrobend loss) and can crack the glass. Microbends are tiny kinks from crushing or over-tight ties.
Insertion lossThe loss added by a connector, splice or coupler, in dB.
Back reflection (return loss)Light reflected back towards the source by a poor joint — it can upset lasers.
Numerical apertureThe light-gathering ability of the fibre — the sine of the acceptance angle.
ModeOne possible path of light through the fibre.

Fibre compared with electrical wire

AdvantagesDisadvantages
  • Immune to EMI, HIRF and lightning-induced currents — light is not affected by electromagnetic fields
  • Radiates nothing — no crosstalk, and hard to tap (secure)
  • Very wide bandwidth — huge data rates
  • Light and small for the data carried
  • Electrical isolation — no ground loops, no sparks (safe near fuel), no short circuits
  • Low loss over long distances; does not corrode
  • More expensive components and terminations
  • Fragile — damaged by tight bends, crushing, pulling and vibration
  • Needs special tools, training and test equipment to terminate, repair and test
  • Connectors are very sensitive to dirt
  • Cannot carry electrical power
  • Needs electrical/optical converters at each end
  • Repairs (splicing) are slower than wire repairs

Terminations, splices and couplers

  • Terminations: the fibre is stripped, bonded (usually with epoxy) or crimped into a precision ferrule or terminus, and the end face is polished flat so that two fibres meet core-to-core with physical contact. Aircraft use rugged connectors — for example multi-way MIL-DTL-38999 shells with fibre termini, or ARINC 801 connectors — rather than office types.
  • Splices join fibres permanently. A fusion splice melts the two ends together with an electric arc (lowest loss, about 0.1 dB or less). A mechanical splice aligns them in a sleeve with index-matching gel.
  • Couplers split or combine light. A tee coupler taps light off a line; a star coupler mixes the light from every input and shares it among all outputs — transmissive (separate input and output fibres) or reflective (light is reflected back to all fibres).

The fibre-optic data bus

A fibre-optic data bus connects terminals through couplers instead of wires. A control terminal (bus controller) manages the traffic, and remote terminals in each system send and receive when commanded — the same idea as MIL-STD-1553B, which has a fibre version (MIL-STD-1773). Ethernet and AFDX links can also run on fibre, point-to-point between end systems and switches.

Fibre-optic data bus with a star coupler star coupler Control terminal bus controller Remote terminal 1 Remote terminal 2 Remote terminal 3 Remote terminal 4 Remote terminal 5 Couplers Star: light from any input is shared among all outputs (transmissive or reflective) — each terminal hears all Tee: taps a little light off a line; loss grows with every tee Control terminal runs the bus; remote terminals answer it — like a 1553 bus on fibre (MIL-STD-1773)
Couplers and terminals. A passive star coupler mixes the light from each input and shares it among all the outputs, so every terminal receives every message. A control terminal manages the bus and remote terminals respond to it. Tee couplers tap light from a single line but add loss at every tap.

Fibre optics on aircraft

  • Data networks: parts of the avionics and cabin networks on aircraft such as the Airbus A380 and Boeing 787 run on fibre, especially long runs and high-rate links.
  • In-flight entertainment: the high-bandwidth video distribution to the cabin.
  • Fly-by-light: flight control signals on fibre, immune to HIRF and lightning — flying on the Kawasaki P-1 maritime patrol aircraft and in research.
  • Sensors: fibre-optic gyros in some attitude and heading reference units, and optical sensors in hazardous areas such as fuel tanks.
  • Lighting: fibre is used to pipe light for some panel and cabin lighting effects.

Handling, cleaning and safety

Connector end-face inspection (fibre microscope) Clean connect Dust / oil film clean, re-inspect Scratched core re-polish or replace Chipped replace terminus inspect → clean → inspect again before every mating · fit dust caps the moment a connector is opened
Keep it clean. A single speck of dust on a 9 µm core can block most of the light, and mating a dirty connector can scratch both end faces. Every connector is inspected with a fibre microscope, cleaned with approved materials, and inspected again before it is mated.
  • Respect the minimum bend radius (typically 10 to 20 times the cable diameter — use the value in the wiring practices manual), do not crush cables under clamps or over-tighten ties, and never pull on the fibre itself.
  • Fit dust caps as soon as a connector is opened. Inspect, clean and re-inspect every end face before mating, using lint-free wipes or approved cleaning tools and solvent.
  • Test with an optical light source and power meter (insertion loss) or an OTDR (optical time-domain reflectometer), which locates breaks and bad joints by timing reflected light.
  • Never look into a fibre or connector — the infrared light is invisible and a laser source can damage your eyes, even when the fibre seems dark. Use a microscope with a filter, or a video probe, with the source switched off.
  • Fibre off-cuts are tiny glass needles: collect them in a marked container and keep them away from skin, eyes and food.
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