Geometrical Optics Fiber Optics Fiberoptics: First Lightguide

Total Page:16

File Type:pdf, Size:1020Kb

Geometrical Optics Fiber Optics Fiberoptics: First Lightguide Phys 322 Lecture 15 Chapter 5 Geometrical Optics Fiber optics Fiberoptics: first lightguide 1870: water as a light guide John Tyndall 1820-1893 Fiberoptics: first optical communication Alexander Graham Bell 1847-1922 1880: photophone 4 years after inventing a telephone! Fiber optics: communications 1960: First laser 1966: coupling with fibers for communication 1970: 1% of light transmitted over 1 km (losses 20 dB/km) Today: over 96% of power transmitted over 1 km Why light? - frequencies ~1015 Hz Theoretical bandwidth limit: each oscillation is 1 bit, bandwidth is ~1014 bytes/second (100,000 GB/s) Speech ~3 kB/s: can support ~10 billion phone connections over one fiber simultaneously! DVD quality videophone: ~10 million channels! Note: Modern fiber systems record 100 Tb/s http://www.newscientist.com/article/mg21028095.500-ultrafast-fibre-optics-set-new-speed- record.html What is an Optical Fiber? An optical fiber is a waveguide for light consists of : core inner part where wave propagates cladding outer part used to keep wave in core buffer protective coating jacket outer protective shield Design of optical fibers Core: Thin glass center of the fiber that carries the light Cladding: Surrounds the core and reflects the light back into the core Buffer coating: Plastic protective coating ncore > ncladding Microstructure fiber Air holes In microstructure fiber, air holes act as the cladding surrounding a glass core. Such fibers have different dispersion properties. Core Such fiber has many applications, from medical imaging to optical clocks. Propagation of light in an optical fiber Light travels through the core bouncing from the reflective walls. The walls absorb very little light from the core allowing the light wave to travel large distances. Some signal degradation occurs due to imperfectly constructed glass used in the cable. The best optical fibers show very little light loss -- less than 10%/km at 1,550 nm. Maximum light loss occurs at the points of maximum curvature. Fiberoptics: single core fiber losses Consider large fiber: diameter D >> can use geometric optics Path length traveled by ray: l L / cost Number of reflections: l N 1 D /sint Example: Using Snell’s Law for t: L = 1 km, D = 50 m, n =1.6, = 30o f i Lsin N i 1 N = 6,580,000 2 2 D n f sin i Note: frustrated internal reflection, irregularities losses! Step Index Fiber: TIR escapes core escapes core cladding nt core ni stuck in core i i i nt critical angle sinc nti (pg 121) For total internal ni reflection need i c for TIR nc<nf Cladding - NA of a Step Index Fiber transparent layer core of a fiber nc (reduces losses and f/#) n nf i 90-t t max must be > critical angle NA noutside sinmax 2 2 n f nc NAstep ni 2 2 NA in air NAstep n f nc Fiber and f/# 2 2 n f nc sinmax ni Angle max defines the light gathering efficiency of the fiber, or numerical aperture NA: 2 2 NA ni sinmax n f nc 1 And f/# is: f /# Largest NA=1 2NA Typical NA = 0.2 … 1 Bundles Bundles can collect light from larger area and be still flexible Flexible light carriers Coherent bundles: flexible image carriers Fibers are arranged in a coherent fashion Data transfer limitations 1. Distance is limited by losses in a fiber. Losses are measured in decibels (dB) per km of fiber (dB/km), i.e. in logarithmic scale: 10 P P L /10 P - output power o o o log 10 P - input power L P P i i i L - fiber length Example: Po/Pi over 1 km 10 dB 1:10 20 dB 1:100 30 dB 1:1000 Workaround: use light amplifiers to boost and relay the signal 2. Bandwidth is limited by pulse broadening in fiber and processing electronics Attenuation page 297 IR absorption Rayleigh Scattering absorption and scattering in fiber in the IR: “low-OH” versus “high-OH” Pulse broadening Dispersion: The Basics Light propagates at a finite speed fastest ray slowest ray fastest ray: one traveling down middle (“axial mode”) slowest ray: one entering at highest angle (“high order” mode) will be a difference in time for these two rays Types of Dispersion in Fibers modal time delay from path length differences usually the biggest culprit in step-index material n() : different times to cross fiber (note: smallest effect ~ 1.3 m) waveguide changes in field distribution (important for SM) non-linear n can become intensity-dependent NOTE: GRIN fibers tend to have less modal dispersion because the ray paths are shorter Effect of Dispersion initial pulse farther down farther still time time time modal example: step index ~ 24 ns km -1 GRIN ~ 122 ps km-1 Fibers carry modes of light 2 D number of modes NA 0 a mode is : •a solution to the wave equation • a given path/distribution of light (pg 196) higher # modes gives more light, which is not always desirable Example of # of Modes @ 850nm Silica step-index fiber has nf = 1.452, nc = 1.442 (NA = 0.205) SELFOC graded index fiber with same NA diameter 2.5 50 200 400 1000 (microns) # step-index 1.5 580 9.3 E3 37 E3 230 E3 modes # GRIN 1.8 716 11 E3 46 E3 1150 E3 modes high # modes implies classical optics NA and # of Modes killed ray propagated ray large NA small NA Pulse broadening Multimode fiber: there are many rays (modes) with different OPLs and initially short pulses will be broadened (intermodal dispersion) For ray along axis: tmin L v f Ln f c 2 For ray entering at max: tmax l v f Ln f cnc The initially short pulse will be broadened by: Ln f n f Making nc close to nf t tmax tmin 1 reduces the effect! c nc Pulse broadening: example nf = 1.5 nc=1.489 Estimate the bandwidth limit for 1000 km transmission. Solution: 6 Ln f n f 10 1.5 1.5 5 t 1 1 s 3.7 10 s 37s 8 c nc 310 1.489 Even the shortest pulse will become ~37 s long 1 kilobits per second Bandwidth ~ 5 27 kbps 3.7 10 s = ONLY 3.3 kbytes/s Multimode fibers are not used for communication! Graded Index Fiber nc nf varies n quadratically nc like a “restoring” force ! Types of fibers nc nf nc step-index multimode nc nf nc step-index singlemode nc nf GRIN nc Single mode fiber To avoid broadening need to have only one path, or mode Single mode fiber: there is only one path, all other rays escape from the fiber clad core jacket Geometric optics does not work anymore: need wave optics. Single mode fiber core is usually only 2-7 micron in diameter Single mode fiber: broadening clad Problem: shorter the pulse, broader core the spectrum. refraction index depends on wavelength jacket ‘Transform’ limited pulse product of spectral full width at half maximum (fwhm) by time duration fwhm: ft 0.2 A 10 fs pulse at 800 nm is ~40 nm wide spectrally If second derivative of n is not zero this pulse will broaden in fiber rapidly Solitons: special pulse shapes that do not change while propagating Critical Bend radius An example: I need a fiber that will conduct NIR light. I have to keep a tight pulse pattern. It must couple into an LED. What do I do? Putting It All together (a) I needed a fiber that will conduct get a low OH fiber NIR light. (b) I had to keep a tight pulse pattern. you want low dispersion: SM or a GRIN fiber, low diameter, low NA (c) It must couple into an LED. The LED has a high divergence angle; better get a bright one. A laser might be better, and use a GRIN lens to couple. These are design considerations, as well as cost! Phys 322 Lecture 15 Chapter 5 Geometrical Optics Optical systems Human eye Human eye Most of the bending n1.376 Iris serves as aperture stop. Diameter changes from ~2 mm in dark to ~8 mm in bright light Note: it also contracts to increase sharpness when doing close work. collagen n1.337 (protein polymer) blind spot Floating specs (floaters): muscae volitantes http://en.wikipedia.org/wiki/Floater The cornea, iris, and lens The cornea is a thin membrane that has an index of refraction of around 1.38. It protects the eye and refracts light (more than the lens does!) as it enters the eye. Some light leaks through the cornea, especially when it’s blue. The iris controls the size of the pupil, an opening that allows light to enter through. The lens is jelly-like lens with an index of refraction of 1.386-1.406 (GRIN lens). This lens bends so that the vision process can be fine tuned. When you squint, you are bending this lens and changing its properties so that your vision is clearer. The ciliary muscles bend and adjust the lens. Accommodation 1 1 1 so si f 1 1 1 nl 1 f R1 R2 change focus closest: young adult ~12 cm middle-aged ~30 cm 60 yrs old ~100 cm (Birds: change curvature of cornea) Crystalline lens of an eye Lens: 9x4mm, consists of ~22,000 layers of cortical fibers n = 1.386…1.406 http://www.bartleby.com/107/illus887.html http://www.owlnet.rice.edu/~psyc351/imagelist.htm Correcting vision Nearsighted eye and glasses Farsighted eye and glasses Physiological optics: dioptric power D 1 1 1 Instead of f use dioptric power D: D nl 1 f R1 R2 1 1 1 For 2 thin lenses closely spaced: D D1 D 2 f f1 f2 For intact unaccommodated eye D=58.6 D (Diopter) Far point: the object point whose image lies on the retina for unaccommodated eye Normal eye: far point is Nearsightedness (myopia) - far point is closer, D > 58.6 D Farsightedness (hyperopia) - far point is behind the lens, D < 58.6 D Near point: the closest object point whose image could be projected on the retina with accommodated eye Example: nearsightedness (myopia) Far point is closer, D > 58.6 D Suppose far point = 2 m The additional lens must make image si=-2 m for so= 2 m (assume lens-eye distance is small, contact lens) 1 1 1 1 1 Lens f = -2 m, or D=-0.5 D f so si 2m For spectacle lens distance d away from eyes: D l D Dl - distant lens power (d from eye) c 1 D d l Dc - equivalent contact lens power Astigmatism The lens has different radii of curvature in different planes test pattern: normal eye astigmatic eye http://www.thineyeglasses.com/glossary/astigmatism.htm Correction: cylindrical lenses More complex: sphero-cylindrical lenses.
Recommended publications
  • SYLLABUS Optical Fiber Communication
    Optical Fiber Communication 10EC72 SYLLABUS Optical Fiber Communication Subject Code : 10EC72 IA Marks : 25 No. of Lecture Hrs/Week : 04 Exam Hours : 03 Total no. of Lecture Hrs. : 52 Exam Marks : 100 PART - A UNIT - 1 OVERVIEW OF OPTICAL FIBER COMMUNICATION: Introduction, Historical development, general system, advantages, disadvantages, and applications of optical fiber communication, optical fiber waveguides, Ray theory, cylindrical fiber (no derivations in article 2.4.4), single mode fiber, cutoff wave length, mode filed diameter. Optical Fibers: fiber materials, photonic crystal, fiber optic cables specialty fibers. 8 Hours UNIT - 2 TRANSMISSION CHARACTERISTICS OF OPTICAL FIBERS: Introduction, Attenuation, absorption, scattering losses, bending loss, dispersion, Intra modal dispersion, Inter modal dispersion. 5 Hours UNIT - 3 OPTICAL SOURCES AND DETECTORS: Introduction, LED’s, LASER diodes, Photo detectors, Photo detector noise, Response time, double hetero junction structure, Photo diodes, comparison of photo detectors. 7 Hours UNIT - 4 FIBER COUPLERS AND CONNECTORS: Introduction, fiber alignment and joint loss, single mode fiber joints, fiber splices, fiber connectors and fiber couplers. 6 Hours Dept of ECE, SJBIT Page 1 Optical Fiber Communication 10EC72 PART - B UNIT - 5 OPTICAL RECEIVER: Introduction, Optical Receiver Operation, receiver sensitivity, quantum limit, eye diagrams, coherent detection, burst mode receiver operation, Analog receivers. 6 Hours UNIT - 6 ANALOG AND DIGITAL LINKS: Analog links – Introduction, overview of analog links, CNR, multichannel transmission techniques, RF over fiber, key link parameters, Radio over fiber links, microwave photonics. Digital links – Introduction, point–to–point links, System considerations, link power budget, resistive budget, short wave length band, transmission distance for single mode fibers, Power penalties, nodal noise and chirping.
    [Show full text]
  • Introduction to Optical Communication Systems
    1. Introduction to Optical Communication Systems Optical Communication Systems and Networks Lecture 1: Introduction to Optical Communication Systems 2/ 52 Historical perspective • 1626: Snell dictates the laws of reflection and refraction of light • 1668: Newton studies light as a wave phenomenon – Light waves can be considered as acoustic waves • 1790: C. Chappe “invents” the optical telegraph – It consisted in a system of towers with signaling arms, where each tower acted as a repeater allowing the transmission coded messages over hundred km. – The first Optical telegraph line was put in service between Paris and Lille covering a distance of 200 km. • 1810: Fresnel sets the mathematical basis of wave propagation • 1870: Tyndall demonstrates how a light beam is guided through a falling stream of water • 1830: The optical telegraph is replaced by the electric telegraph, (b/s) until 1866, when the telephony was born • 1873: Maxwell demonstrates that light can be considered as electromagnetic waves http://en.wikipedia.org/wiki/Claude_Chappe Optical Communication Systems and Networks Lecture 1: Introduction to Optical Communication Systems 3/ 52 Historical perspective • 1800: In Spain, Betancourt builds the first span between Madrid and Aranjuez • 1844: It is published the law for the deployment of the optical telegraphy in Spain – Arms supporting 36 positions, 10º separation Alphabet containing 26 letters and 10 numbers – Spans: Madrid - Irún, 52 towers. Madrid - Cataluña through Valencia, 30 towers. Madrid - Cádiz, 59 towers. • 1855: It is published the law for the deployment of the electrical telegraphy network in Spain • 1880: Graham Bell invents the “photofone” for voice communications TRANSMITTER RECEIVER The transmitter consists of a The receiver is also a mirror made to be vibrated by parabolic reflector in which a the person’s voice, and then selenium cell is placed in its modulating the incident light focus to collect the variations beam towards the receiver.
    [Show full text]
  • Wireless Networks
    SUBJECT WIRELESS NETWORKS SESSION 2 WIRELESS Cellular Concepts and Designs" SESSION 2 Wireless A handheld marine radio. Part of a series on Antennas Common types[show] Components[show] Systems[hide] Antenna farm Amateur radio Cellular network Hotspot Municipal wireless network Radio Radio masts and towers Wi-Fi 1 Wireless Safety and regulation[show] Radiation sources / regions[show] Characteristics[show] Techniques[show] V T E Wireless communication is the transfer of information between two or more points that are not connected by an electrical conductor. The most common wireless technologies use radio. With radio waves distances can be short, such as a few meters for television or as far as thousands or even millions of kilometers for deep-space radio communications. It encompasses various types of fixed, mobile, and portable applications, including two-way radios, cellular telephones, personal digital assistants (PDAs), and wireless networking. Other examples of applications of radio wireless technology include GPS units, garage door openers, wireless computer mice,keyboards and headsets, headphones, radio receivers, satellite television, broadcast television and cordless telephones. Somewhat less common methods of achieving wireless communications include the use of other electromagnetic wireless technologies, such as light, magnetic, or electric fields or the use of sound. Contents [hide] 1 Introduction 2 History o 2.1 Photophone o 2.2 Early wireless work o 2.3 Radio 3 Modes o 3.1 Radio o 3.2 Free-space optical o 3.3
    [Show full text]
  • Letter from Alexander Graham Bell to Alexander Melville Bell, February 26, 1880, with Transcript
    Library of Congress Letter from Alexander Graham Bell to Alexander Melville Bell, February 26, 1880, with transcript ALEXANDER GRAHAM BELL TO HIS FATHER A. MELVILLE BELL 904 14th Street, N. W., Washington, D. C. Feb. 26th, 1880. Dear Papa: I have just written to Mamma about Mabel's baby and I now write to you about my own! Only think! — Two babies in one week! The first born at 904 14th Street — on the fifteenth inst., the other at my laboratory on the nineteenth. Both strong vigorous healthy young things and both destined I trust to grow into something great in the future. Mabel's baby was light enough at birth but mine was LIGHT ITSELF! Mabel's baby screamed inarticulately but mine spoke with distinct enunciation from the first. I have heard articulate speech produced by sunlight! I have heard a ray of the sun laugh and cough and sing! The dream of the past year has become a reality — the “ Photophone ” is an accomplished fact. I am not prepared at present to go into particulars and can only say that with Mr. Tainter's assistance I have succeeded in preparing crystalline selenium of so low a resistance and so sensitive to light that we have been enabled to perceive variations of light as sounds in the telephone. In this way I have been able to hear a shadow, and I have even perceived by ear the passage of a cloud across the sun's disk. Can Imagination picture what the future of this invention is to be! I dream of so many important and wonderful applications that I cannot bring myself to make known my discovery — until I have demonstrated the practicability of some of these schemes.
    [Show full text]
  • Alexander Graham Bell
    WEEK 2 LEVEL 7 Alexander Graham Bell Alexander Graham Bell is the famous inventor of the telephone. Born in Scotland on March 3, 1847, he was the second son of Alexander and Eliza Bell. His father taught students the art of speaking clearly, or elocution, and his mother played the piano. Bell’s mother was almost deaf. His father’s career and his mother’s hearing impairment influenced the course of his career. He became a teacher of deaf people. As a child, Bell didn’t care for school, and he eventually dropped out. He did like to solve problems though. For example, when he was only 12, he invented a new farm implement. The tool removed the tiny husks from wheat grains. After the deaths of his two brothers from tuberculosis, Bell and his parents moved from Europe to Canada in 1870. They thought the climate there was healthier than in Scotland. A year later, Bell moved to the United States. He got a job teaching at the Boston School for Deaf Mutes. © 2019 Scholar Within, Inc. WEEK 2 LEVEL 7 One of his students was a 15-year-old named Mabel Hubbard. He was 10 years older than she was, but they fell in love and married in 1877. The Bells raised two daughters but lost two sons who both died as babies. Bell’s father-in-law, Gardiner Hubbard, knew Bell was interested in inventing things, so he asked him to improve the telegraph. Telegraph messages were tapped out with a machine using dots and dashes known as Morse code.
    [Show full text]
  • Long-Range Free-Space Optical Communication Research Challenges Dr
    Long-Range Free-Space Optical Communication Research Challenges Dr. Scott A. Hamilton, MIT Lincoln Laboratory and Prof. Joseph M. Khan, Stanford University The substantial benefits of free-space optical (FSO) or laser communications (lasercom) have been well known to system designers for quite some time, c.f. [1]. The free-space channel, similar to the fiber channel, provides many benefits at optical frequencies compared to radio frequencies (RF) including extremely wide unregulated bandwidth and tightly confined beams (i.e. narrow beam divergence), both of which enable low size, weight and power (SWaP) terminals. However, significant challenges are still perceived: stochastic intensity fluctuations in a received optical signal after propagating through the atmosphere, power-starved link mode of operation, and narrow transmit beams that must be precisely pointed and tracked. Since the late 1970’s the United States [2], Europe [3] and Japan [4] have actively been developing FSO technology motivated primarily for long-haul spaceborne communication systems. While early efforts were focused on maturing FSO technology, the past decade has seen significant progress toward demonstrating the practicality of FSO for multiple applications. The first high-rate demonstration of FSO between a satellite in Geosynchronous (GEO) orbit and the ground was achieved by the US during the GeoLITE experiment in 2001. A short time later, the European Space Agency (ESA) demonstrated a 50- Mbps FSO link operating at 800-nm wavelengths between their Artemis GEO satellite and: i) another ESA spacecraft in Low-Earth orbit (LEO) in 2001 [5]; ii) a ground station located in Tenerife, Spain in 2001 [6]; and iii) an airplane flying at altitudes as low as 6,000 meters outfitted with an FSO terminal developed by France’s Astrium EADS in 2006 [7].
    [Show full text]
  • Optical Communications and Networks - Review and Evolution (OPTI 500)
    Optical Communications and Networks - Review and Evolution (OPTI 500) Massoud Karbassian [email protected] Contents Optical Communications: Review Optical Communications and Photonics Why Photonics? Basic Knowledge Optical Communications Characteristics How Fibre-Optic Works? Applications of Photonics Optical Communications: System Approach Optical Sources Optical Modulators Optical Receivers Modulations Optical Networking: Review Core Networks: SONET, PON Access Networks Optical Networking: Evolution Summary 2 Optical Communications and Photonics Photonics is the science of generating, controlling, processing photons. Optical Communications is the way of interacting with photons to deliver the information. The term ‘Photonics’ first appeared in late 60’s 3 Why Photonics? Lowest Attenuation Attenuation in the optical fibre is much smaller than electrical attenuation in any cable at useful modulation frequencies Much greater distances are possible without repeaters This attenuation is independent of bit-rate Highest Bandwidth (broadband) High-speed The higher bandwidth The richer contents Upgradability Optical communication systems can be upgraded to higher bandwidth, more wavelengths by replacing only the transmitters and receivers Low Cost For fibres and maintenance 4 Fibre-Optic as a Medium Core and Cladding are glass with appropriate optical properties!!! Buffer is plastic for mechanical protection 5 How Fibre-Optic Works? Snell’s Law: n1 Sin Φ1 = n2 Sin Φ2 6 Fibre-Optics Fibre-optic cable functions
    [Show full text]
  • Free Space Optics Vs Radio Frequency Wireless Communication
    I.J. Information Technology and Computer Science, 2016, 9, 1-8 Published Online September 2016 in MECS (http://www.mecs-press.org/) DOI: 10.5815/ijitcs.2016.09.01 Free Space Optics Vs Radio Frequency Wireless Communication Rayan A. Alsemmeari and Sheikh Tahir Bakhsh Faculty of Computing and Information Technology, King Abdulaziz University, Saudi Arabia E-mail: {ralsemmeari, stbakhsh}@kau.edu.sa Hani Alsemmeari Institute of Public Administration Information and Technology department E-mail: [email protected] Abstract—This paper presents the free space optics (FSO) but on very low data rates. Laser technology enhanced and radio frequency (RF) wireless communication. The the use of free space optics and is now highly dependent paper explains the feature of FSO and compares it with on the laser technology. FSO in original form was the already deployed technology of RF communication in developed by the NASA and used for the military terms of data rate, efficiency, capacity and limitations. purposes in different era as fast communication link. The The data security is also discussed in the paper for technology has many commonalities with the fiber optics identification of the system to be able to use in normal technology but behaves differently in the field due to the circumstances. These systems are also discussed in a way method of transmission for both the technologies [5, 6]. that they could efficiently combine to form the single RF technology is very old technology for system with greater throughput and higher reliability. communication. It is the wireless technology for data communication. It is considered to be in use for more Index Terms—Free Space Optics, Radio frequency, than 100 years.
    [Show full text]
  • Comparative Study of Optical and RF Communication Systems H
    I . , , comparative study of optical and RF Communication Systems for a MrJrs Mission H. Hernmati, K. Wilson, M. Sue, D. Rascoe, F. Lansing, h4. Wilhelm, L. Harcke, and C. Chen Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 AIISTRACT We luwc performed a study on tclcconmnmication sj’s[cnrs for a hypothetical mission to Mars. The objcctivc cf t hc study was to evaluate and compare lhc bcncfils that .rnicrowavc. (X-band. and Ka-band) and Optical conmumications $clmo]ogi$s afford to future missions. TIE lclcconmwnicatio]; systems were required to return data ‘atlcr launch and in-ohit at 2.7 AU with daily data volumes of 0.1, 1, or 10 Gbits. Space-borne tcnnimls capable of delivering each of the three data rates WCJC proposed and charactcnmd in terms of mass, power consumption, sire, and cost. The estimated panwnctcw for X- band, Ka-band, and Optical frcqucncics arc compared and presented here. For data volumes of 0.1 and 1 Gigs-bit pcr day, the X-band downlink system has a mass 1.5 times that of Ka-band, and 2.5 times that of Optical systcm. Ka-band oftcrcd about 20% power saving at 10 Gbit/day over X-band. For all data volumes, the optical communication terminals were lower in mass than the RF terminals. For data volumes of 1 and 10 Gb/day, the space-borne optical terminal also had a lower required DC power. ln all three cases, optical communications had a slightly higher development cost for the space tcnninal, 1. 1NTI{OD[JCTION The deep space cxTloration program has been steadily increasing the frequcncic$ used for planctmy radio communication since the inception of NASA in 1957.
    [Show full text]
  • Alexander Graham Bell 1847-1922
    NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA BIOGRAPHICAL MEMOIRS VOLUME XXIII FIRST MEMOIR BIOGRAPHICAL MEMOIR OF ALEXANDER GRAHAM BELL 1847-1922 BY HAROLD S. OSBORNE PRESENTED TO THE ACADEMY AT THE ANNUAL MEETING, 1943 It was the intention that this Biographical Memoir would be written jointly by the present author and the late Dr. Bancroft Gherardi. The scope of the memoir and plan of work were laid out in cooperation with him, but Dr. Gherardi's untimely death prevented the proposed collaboration in writing the text. The author expresses his appreciation also of the help of members of the Bell family, particularly Dr. Gilbert Grosvenor, and of Mr. R. T. Barrett and Mr. A. M. Dowling of the American Telephone & Telegraph Company staff. The courtesy of these gentlemen has included, in addition to other help, making available to the author historic documents relating to the life of Alexander Graham Bell in the files of the National Geographic Society and in the Historical Museum of the American Telephone and Telegraph Company. ALEXANDER GRAHAM BELL 1847-1922 BY HAROLD S. OSBORNE Alexander Graham Bell—teacher, scientist, inventor, gentle- man—was one whose life was devoted to the benefit of mankind with unusual success. Known throughout the world as the inventor of the telephone, he made also other inventions and scientific discoveries of first importance, greatly advanced the methods and practices for teaching the deaf and came to be admired and loved throughout the world for his accuracy of thought and expression, his rigid code of honor, punctilious courtesy, and unfailing generosity in helping others.
    [Show full text]
  • Optical Satellite Communication Toward the Future of Ultra High
    No.466 OCT 2017 Optical Satellite Communication toward the Future of Ultra High-speed Wireless Communications No.466 OCT 2017 National Institute of Information and Communications Technology CONTENTS FEATURE Optical Satellite Communication toward the Future of Ultra High-speed Wireless Communications 1 INTERVIEW New Possibilities Demonstrated by Micro-satellites Morio TOYOSHIMA 4 A Deep-space Optical Communication and Ranging Application Single photon detector and receiver for observation of space debris Hiroo KUNIMORI 6 Environmental-data Collection System for Satellite-to-Ground Optical Communications Verification of the site diversity effect Kenji SUZUKI 8 Optical Observation System for Satellites Using Optical Telescopes Supporting safe satellite operation and satellite communication experiment Tetsuharu FUSE 10 Development of "HICALI" Ultra-high-speed optical satellite communication between a geosynchronous satellite and the ground Toshihiro KUBO-OKA TOPICS 12 NICT Intellectual Property -Series 6- Live Electrooptic Imaging (LEI) Camera —Real-time visual comprehension of invisible electromagnetic waves— 13 Awards 13 Development of the “STARDUST” Cyber-attack Enticement Platform Cover photo Optical telescope with 1 m primary mirror. It receives data by collecting light from sat- ellites. This was the main telescope used in experiments with the Small Optical TrAn- sponder (SOTA). This optical telescope has three focal planes, a Cassegrain, a Nasmyth, and a coudé. The photo in the upper left of this page shows SOTA mounted in a 50 kg-class micro- satellite. In a world-leading effort, this was developed to conduct basic research on technology for 1.5-micron band optical communication between low-earth-orbit sat- ellite and the ground and to test satellite-mounted equipment in a space environment.
    [Show full text]
  • Fundamentals of Optical Communications
    FundamentalsFundamentals ofof OpticalOptical CommunicationsCommunications Raj Jain The Ohio State University Nayna Networks Columbus, OH 43210 Milpitas, CA 95035 Email: [email protected] http://www.cis.ohio-state.edu/~jain/ ©2002 Raj Jain 1 OverviewOverview ! Characteristics of Light ! Optical components ! Fibers ! Sources ! Receivers, ! Switches ©2002 Raj Jain 2 ElectromagneticElectromagnetic SpectrumSpectrum ! Infrared light is used for optical communication ©2002 Raj Jain 4 AttenuationAttenuation andand DispersionDispersion Dispersion 0 850nm 1310nm 1550nm©2002 Raj Jain 5 WavebandsWavebands O E S C L U 770 910 1260 1360 14601530 1625 1565 1675 ©2002 Raj Jain 6 WavebandsWavebands (Cont)(Cont) O E S C L U 770 910 1260 1360 1460 1530 1625 1565 1675 Band Descriptor Range (nm) 770-910 O Original 1260-1360 E Extended 1360-1460 S Short Wavelength 1460-1530 C Conventional 1530-1565 L Long 1565-1625 U Ultralong 1625-1675 ©2002 Raj Jain 7 OpticalOptical ComponentsComponents Fiber Sources Mux Amplifier Demux Receiver ! Fibers ! Sources/Transmitters ! Receivers/Detectors ! Amplifiers ! Optical Switches ©2002 Raj Jain 8 TypesTypes ofof FibersFibers II ! Multimode Fiber: Core Diameter 50 or 62.5 μm Wide core ⇒ Several rays (mode) enter the fiber Each mode travels a different distance ! Single Mode Fiber: 10-μm core. Lower dispersion. Cladding Core ©2002 Raj Jain 9 ReducingReducing ModalModal DispersionDispersion ! Step Index: Index takes a step jump ! Graded Index: Core index decreases parabolically ©2002 Raj Jain 11 TypesTypes ofof FibersFibers IIII
    [Show full text]