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Victorian Physics Teachers Conference 2002 Physics Oration

Victorian Physics Teachers Conference 2002 Physics Oration . Photonics: Light waves for communication New waves in education Dr Andrew Stevenson Manager, Educational Development Photonics Institute Pty Ltd GPO Box 464 Canberra ACT 2601. Outline . What is photonics?

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Victorian Physics Teachers Conference 2002 Physics Oration

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  1. Victorian Physics Teachers Conference 2002Physics Oration Photonics: Light waves for communication New waves in education Dr Andrew Stevenson Manager, Educational Development Photonics Institute Pty Ltd GPO Box 464 Canberra ACT 2601

  2. Outline • What is photonics? • Evolution of optical communications • Important physical principles • Photonics technology and frontiers • The Photonics industry now and in 2010 • Outlook for careers in photonics • Tertiary study options • Photonics Institute - how can we help?

  3. What is Photonics? The use of photons, the fundamental particles of light to transmit, store and process information.

  4. Why do we need Photonics? • The principal driver for the photonics industry is growing demand for faster, more efficient communications. • World Internet traffic is tripling each year (more users each day, spending more time on-line, downloading more Mbytes / hour) • Photonics technologies enable the provision of extremely high bandwidth to meet this growing demand.

  5. Evolution of optical communication x More speed x More channels = Greater bandwidth

  6. Evolution of optical communication • Modulating light to transmit information • 1. Smoke signals / fires / lanterns / heliographs / mirrors • Slow “digital” encoding, simple intensity modulation • Very trivial messages (“All clear”, “Send help”) • More of a broadcast than a dedicated channel • 2. Claude Chappe invents first “optical telegraph” • Slow “digital” encoding, using shapes • Sophisticated codes to improve information content • Reasonably fast and reliable • Trained humans needed to encode / decode • Europe’s first telecommunications network

  7. Evolution of optical communication Claude Chappe d’Auteroche (1763 - 1805) Claude’s statue (1893 - 1942) Claude’s portrait Melted down during WW2 to make ammunition Claude’s machine

  8. Evolution of optical communication Some of Claude’s stations survive to this day ... These are analogous to today’s fibre optic “repeater stations” A map of Europe’s first telecommunications network Lines established 1793 - 1852

  9. Evolution of optical communication • Modulating light to transmit information • To speed up communications, it is necessary to take humans “out of the loop”. • A fully automatic optical link is required. • Bell’s Photophone ( ~ 1880) • Machine codes & decodes in real time, no delays • Intensity modulation of light • Analogue encoding of signal in modulated light • Audio (vocal) bandwidth for fairly rapid information transmission (as good as any conversation!) • Single (dedicated) communication channel

  10. Evolution of optical communication … interrupted by a phone call during a meeting... Alexander Graham Bell (1847 - 1922) ...

  11. Evolution of optical communication Bell’s Photophone (3 June 1880, 4 years after the telephone) Sunlight is focussed onto a small lightweight mirror on a special cantilevered mount Speaker’s voice is mechanically concentrated to vibrate the mirror at acoustic frequencies The mirror modulates (steers) the light in time with the voice The fluctuating sunlight is directed by the mirror to a selenium receiver that produces changes in the current driving a speaker coil, reproducing the original voice (hopefully). Sketches from Bell’s own notebook

  12. Evolution of optical communication • Modulating light to transmit information • 3. Early optical fibre links - Multimode fibre, LED sources • (1960’s, 1970’s) • Intensity modulation of an LED (analogue or digital) • Bandwidth usually limited by multimode fibre dispersion: longer distance <-> smaller bandwidth • Over short links, bandwidth limited by LED modulation rate (usually less than 300 Mbit/s) • Useful over fairly short links / Local Area Networks

  13. Evolution of optical communication • Modulating light to transmit information • 4. Modern single-mode fibre links, Laser sources • (1980’s onwards) • Fibre supports one optical “mode” - small dispersion • Can modulate laser diodes up to a several GHz • Far higher bandwidths are possible using an in-line intensity modulator after the laser diode • The only solution for long-haul high bit rate optical communication links • Dense Wavelength Division Multiplexing (DWDM) lets us encode signals on many wavelength channels at once - uses more of the available optical bandwidth

  14. Evolution of optical communication • The long distance optical ‘medium’ • 1. Open Air: Beacon fires / semaphore flags on hilltops • Day or Night operation only, depending on method used • Vulnerable to weather, sleepy observers • Not secure - easy to eavesdrop • Coding and decoding can be complex OR • Messages take a long time to send • (Tradeoff between bandwidth and complexity)

  15. Evolution of optical communication • The long distance optical ‘medium’ • 2. Open Air: Lasers on rooftops, building-to-building • 24 hours a day operation • Large bandwidth (~ 1GHz) • Collimated beam (but not totally secure) • Potential danger (eyes), • Vulnerable to weather / obstructions ??? • Useful range ~ 1km, due to beam distortion • Potentially useful for the “last mile”

  16. Evolution of optical communication Building-to-Building (“B2B”) Laser communications One possible solution to span the “last mile” with an optical frequency connection Laser transceivers in customer premises are placed near windows in line of site from a hub 1.3 metres Fairly large!

  17. Evolution of optical communication • The long distance optical ‘medium’ • 3. Lightpipes - a nice idea perhaps, but then again... • Large bandwidth • Sensitive to changes of temperature, alignment etc • Many reflection losses if solid glass lenses are used • Complex, not practical, not economic

  18. Evolution of optical communication • The long distance optical ‘medium’ • 4. Optical Fibres • Huge bandwidth (esp. when using many wavelengths) • Flexible, temperature insensitive, low loss, few alignment issues • Cheap and able to be mass produced • Standard long distance communication medium

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