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Tampilkan postingan dengan label Teknologi. Tampilkan semua postingan

Jumat, 12 November 2010

Fiber-optic communication

Fiber-optic communication is a method of transmitting information from one place to another by sending pulses of light through an optical fiber. The light forms an electromagnetic carrier wave that is modulated to carry information. First developed in the 1970s, fiber-optic communication systems have revolutionized the telecommunications industry and have played a major role in the advent of the Information Age. Because of its advantages over electrical transmission, optical fibers have largely replaced copper wire communications in core networks in the developed world.

The process of communicating using fiber-optics involves the following basic steps: Creating the optical signal involving the use of a transmitter, relaying the signal along the fiber, ensuring that the signal does not become too distorted or weak, receiving the optical signal, and converting it into an electrical signal.

Optical fiber is used by many telecommunications companies to transmit telephone signals, Internet communication, and cable television signals. Due to much lower attenuation and interference, optical fiber has large advantages over existing copper wire in long-distance and high-demand applications. However, infrastructure development within cities was relatively difficult and time-consuming, and fiber-optic systems were complex and expensive to install and operate. Due to these difficulties, fiber-optic communication systems have primarily been installed in long-distance applications, where they can be used to their full transmission capacity, offsetting the increased cost. Since 2000, the prices for fiber-optic communications have dropped considerably. The price for rolling out fiber to the home has currently become more cost-effective than that of rolling out a copper based network. Prices have dropped to $850 per subscriber in the US and lower in countries like The Netherlands, where digging costs are low.

Since 1990, when optical-amplification systems became commercially available, the telecommunications industry has laid a vast network of intercity and transoceanic fiber communication lines. By 2002, an intercontinental network of 250,000 km of submarine communications cable with a capacity of 2.56 Tb/s was completed, and although specific network capacities are privileged information, telecommunications investment reports indicate that network capacity has increased dramatically since 2004.

Band Description Wavelength Range
O band original 1260 to 1360 nm
E band extended 1360 to 1460 nm
S band short wavelengths 1460 to 1530 nm
C band conventional ("erbium window") 1530 to 1565 nm
L band long wavelengths 1565 to 1625 nm
U band ultralong wavelengths 1625 to 1675 nm
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Kamis, 07 Oktober 2010

Antenna Polarization

The polarization of an antenna is the polarization of the wave radiated by the antenna. At a given position, the polarization describes the orientation of the electric field.

Suppose an electromagnetic wave, radiated by an antenna, has an electric field E ( a vector) with two components: E x and E y.

electric field with components

We are going to explore the figure traced by the tip of vector E at a given position along the z axis as the time changes.

Let us assume that the components E x and E y of electric field E are given by

electric field with components
where a is the amplitude of component E x and b is the amplitude of component E . Phi is the difference of phase between the two components.

Tutorial using an applet

Press the button below "press here to start". The left is for controling parameters a, b and Phi and to start or stop the animation. Time t in the expressions giving the electric field is changed by steps or continuously. The electric field vector E changes in magnitude and direction. The extremity of the vector field E describes a curve: This curve defines the polarization.

1 - Linear polarization

Use the scrollbar to set Phi to 0. Set a = 1 and b = 1. (these values might be set already). Press the button "START/STOPT animation". The trace of the field vector E should be linear of the hence this is linear polarization. Change a and b and observe the angle of the segment changing.

The condition for linear polarization is that Phi should take values such as : Phi = n*Pi, where n is an integer. Use different values for Phi = n*Pi and check that the polarization is linear.

2 - Circular polarization



Set a = b = 1 and Phi to 0.5Pi. Press the button "START/STOPT animation". The trace is now a circle.

The conditions for circular polarization is that Phi should take values such as : Phi = (n+1)Pi/2. Example: Phi = Pi/2 , 3Pi/2, -Pi/2 ... and a = b. Take different values for Phi and a and b according the stated conditions and check that the polarization is circular.

3 - Elliptical polarization



Set a = b = 1 and Phi to any value other than 0, Pi, 0.5Pi, say 0.7Pi for example. Press the button "START/STOPT animation". The trace is now an ellipse.

The conditions for elliptical polarization is that Phi should take values such as : Phi = (n+1)Pi/2. Example: Phi = Pi/2 , 3Pi/2, -Pi/2... Take different values for Phi according the stated conditions and check that the polarization is an ellipse if a is NOT equal to b.
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Karakteristik Antena







Pengarahan

Pengarahan atau direktivity antena adalah perbandingan antara intensitas radiasi (daya tiap unit sudut ruang) pada arah tertentu U(θ, Ф) terhadap intensitas radiasi rata-rata Uo (dari seluruh permukaan) pancaran. Semakin besar direktivitas maka lebar berkas antena semakin sempit. Dalam penggunaan praktis yang dimaksud directivity merupakan direktivitas maksimum yaitu pada arah sumbu pancar (pada arah pancaran maksimal).

Direktivitas suatu antena didefinisikan sebagai : directivity.JPG


Gain (Penguatan)

Macam - macam referensi atau pembanding yang biasa digunakan yaitu isotropis, dimana efisiensi antena isotropis adalah 100 %, dipol λ/2, horn, dll. antena bergantung pada direktivitas antena dan efisiensi antena. Hubungan ketiganya dapat dirumuskan sebagai berikut : gain 2.JPG

Dimana η adalah factor efisiensi antena (0≤ η ≤ 1 atau 0 ≤ η ≥ 100% )

Satuan gain yang menggunakan isotropik sebagai antena referensi adalah dBi.

Antena dengan beam ke satu arah tertentu dimana memiliki gain/penguatan yang tinggi. Kebanyakan antena susunan tipe ini memiliki beam tunggal yang tegak lurus terhadap antena tersebut, dimana jarak antara patch adalah jarak antar patch.JPG Jarak antar elemen yang kurang dari λo/2 dihindari karena adanya saluran penyepadan. Sedangkan untuk jarak yang lebih dari λo tidak dipakai karena untuk mencegah timbulnya gratting lobe.

Sedangkan rumus yang berguna untuk memperkirakan gain dari antena susunan mikrostrip adalah : gain 3.JPG

dimana : A = D1.D2

D1 = Lebar efektif antena dengan jarak yang sama (didefinisikan sebagai jumlah jarak antara tepi ke tepi elemen ditambah dengan spasi antar elemen; (n + 1) x spasi horisontal.

D2 = Tinggi antenas susunan dengan definisi yang serupa dengan D1; (m + 1) x spasi vertikal.

α = Redaman (dB/satuan panjang).


Bandwidth

Bandwidth atau lebar pita frekuensi dari suatu antena adalah daerah frekuensi kerja suatu antena yang dibatasi oleh VSWR tertentu. Biasanya bandwidth dibatasi pada VSWR ≤ 1,5. Pada antena pita lebar atau broadband, bandwidth merupakan perbandingan antara frekuensi atas dengan frekuensi bawah, contoh : bandwidth 10:1 mengindikasikan bahwa frekuensi atas 10 kali lebih tinggi dari frekuensi bawah. Sedangkan pada antena pita sempit atau narrowband, bandwidth dinyatakan dalam persentase dari perbedaan frekuensi (atas dikurangi bawah) yang melewati frekuensi tengah bandwidth, contoh: bandwidth 5% mengindikasikan bahwa perbedaan frekuensi adalah 5% dari frekuensi tengah bandwidth. Adapun persamaan untuk mendapatkan bandwith yang diinginkan dinyatakan dengan : bandwith.JPG

dimana :BW = bandwidth lebar pita, MHz untuk VSWR <>

f = frekuensi operasi, GHz

t = tebal bahan, dalam inchi (kebanyakan ketebalan board tersedia dalam satuan 1/32 inchi = 0,794 mm)

bandwith antena.JPG


Polarisasi

Polarisasi antena pada arah tertentu didefinisikan sebagai polarisasi dari gelombang yang dipancarkan oleh antena tersebut. Jika antena sebagai penerima maka polarisasi antena adalah polarisasi dari gelombang datang pada arah tertentu yang menghasilkan daya terima maksimum.

polarisasi linear, eliptis, sirkular.JPG

Jenis polarisasi dapat diketahui dengan persamaan rasio kuat medan elektrik.

ratio kuat medan.JPG


Diagram Arah

Diagram arah yaitu suatu grafik yang menunjukkan pola pancaran atau penerimaan suatu antena sebagai fungsi dari arahnya. Penggambaran penampang melintangnya dengan arah vertikal dan horizontal dengan polarisasi elektrik dan magnetik. Berkas antena ditunjukkan dengan sudut pancaran antena yang tajam, sehingga pancarannya lebih kuat untuk penerimaan. Berkas antena ini memiliki luas yang disebut luas berkas (beam area) yaitu luas sudut ruang yang mewakili arah pancaran daya dari antena.

pola radiasi antena.JPG

Dalam diagram arah diatas terdapat tiga daerah pancaran yaitu: 1lobe utama (main lobe), 2lobe sisi samping(side lobe),3lobe sisi belakang (back lobe). FNBW (First Null Beamwidth) _ sudut saat penerimaan daya pertama kali. HPBW (Half Power Beamwidth) _ sudut yang dibentuk oleh dua arah yang mempunyai intensitas radiasi ½ kali (- 3 dB) dari intensitas radiasi maksimumnya; sudut ini terletak dalam sebuah bidang yang merupakan arah maksimum beam.


Impedansi Antena

Impedansi antena didefinisikan sebagai perbandingan antara medan elektrik terhadap medan magnetik pada suatu titik, dengan kata lain pada sepasang terminal maka impendansi antena bisa didefinisikan sebagai perbandingan antara tegangan terhadap arus pada terminal tersebut.

impedansi.JPG

Impedansi antena merupakan hal yang penting dalam perancangan antenna karena sebenarnya antena itu sendiri berfungsi sebagai penyepadan impedansi antenna tersebut dengan impedansi saluran. Penyepadan ini perlu dilakukan supaya terjadi transfer daya maksimum dari sumber ke antena atau sebaliknya. Impedansi suatu saluran (antena) ditentukan oleh ukuran, konstruksi fisik dan bahan serta frekuensi kerja antena tersebut.


Efisiensi Antena

Efisiensi total antena digunakan untuk menghitung rugi-rugi pada terminal input dan pada struktur antena. Beberapa rugi-rugi terjadi karena:

· Pemantulan (refleksi) karena ketidaksepadanan impendansi antara saluran dengan antena.

· Rugi – rugi konduksi dan dielektrika yang terjadi pada antena.


VSWR (Voltage Standing Wave Ratio)

VSWR adalah perbandingan antara tegangan maksimum dan minimum pada suatu gelombang berdiri akibat adanya pantulan gelombang yang disebabkan tidak matching-nya impedansi input antena dengan saluran feeder.

vswr.JPG

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Jenis - Jenis Antena (Omni, Parabolik, Grid, Sectoral)

Apakah Antena itu? Secara sederhana, antena adalah alat untuk mengirim dan menerima gelombang elektromagnetik, bergantung kepada pemakaian dan penggunaan frekuensinya, antena bisa berwujud berbagai bentuk, mulai dari seutas kabel, dipole, ataupun yagi, dsb. Antena adalah alat pasif tanpa catu daya(power), yang tidak bisa meningkatkan kekuatan sinyal radio, dia seperti reflektor pada lampu senter, membantu mengkonsentrasi dan memfokuskan sinyal.

Kekuatan dalam mengkonsentrasi dan memfokuskan sinyal radio, satuan ukurnya adalah dB. Jadi ketika dB bertambah, maka jangkauan jarak yang bisa ditempuhpun bertambah. Jenis antena yang akan dipasang harus sesuai dengan sistem yang akan kita bangun, juga disesuaikan dengan kebutuhan penyebaran sinyalnya. Secara umum ada dua jenis antena yaitu :

1. Directional
2. Omni Directional

Fungsi

Fungsi antena adalah untuk mengubah sinyal listrik menjadi sinyal elektromagnetik, lalu meradiasikannya (Pelepasan energy elektromagnetik ke udara / ruang bebas). Dan sebaliknya, antena juga dapat berfungsi untuk menerima sinyal elektromagnetik (Penerima energy elektromagnetik dari ruang bebas ) dan mengubahnya menjadi sinyal listrik. Pada radar atau sistem komunikasi satelit, sering dijumpai sebuah antena yang melakukan kedua fungsi (peradiasi dan penerima) sekaligus. Namun, pada sebuah teleskop radio, antena hanya menjalankan fungsi penerima saja.

Karakter antena

Ada beberapa karakter penting antena yang perlu dipertimbangkan dalam memilih jenis antena untuk suatu aplikasi (termasuk untuk digunakan pada sebuah teleskop radio), yaitu pola radiasi, directivity, gain, dan polarisasi. Karakter-karakter ini umumnya sama pada sebuah antena, baik ketika antena tersebut menjadi peradiasi atau menjadi penerima, untuk suatu frekuensi, polarisasi, dan bidang irisan tertentu. Misalnya, David Welkinson (0806322514) ingin membeli antena maka untuk mendapatkan antena yang sesuai dengan fungsi yang dinginkan, ia harus memimilih antena dengan karakter yang sesuai dengan fungsi yang dia inginkan.

• Pola radiasi

Pola radiasi antena adalah plot 3-dimensi distribusi sinyal yang dipancarkan oleh sebuah antena, atau plot 3-dimensi tingkat penerimaan sinyal yang diterima oleh sebuah antena. Pola radiasiantena dibentuk oleh dua buah pola radiasi berdasar bidang irisan, yaitu pola radiasi pada bidang irisan arah elevasi (pola elevasi) dan pola radiasi pada bidang irisan arah azimuth (pola azimuth).

Kedua pola di atas akan membentuk pola 3-dimensi. Pola radiasi 3-dimensi inilah yang umum disebut sebagai pola radiasi antena dipol. Sebuah antena yang meradiasikan sinyalnya sama besar ke segala arah disebut sebagai antena isotropis. Antena seperti ini akan memiliki pola radiasi berbentuk bola Namun, jika sebuah antena memiliki arah tertentu, di mana pada arah tersebut distribusi sinyalnya lebih besar dibandingkan pada arah lain, maka antena ini akan memiliki directivity Semakin spesifik arah distribusi sinyal oleh sebuah antena, maka directivity antena tersebut.

Antena dipol termasuk non-directive antenna. Dengan karakter seperti ini, antena dipol banyak dimanfaatkan untuk sistem komunikasi dengan wilayah cakupan yang luas. Pada astronomi radio, antena dipol digunakan pada teleskop radio untuk melakukan pengamatan pada rentang High Frekuensi (HF). Bentuk data yang dapat diperoleh adalah variabilitas intensitas sinyal yang dipancarkan oleh sebuah objek astronomi. Namun, karena antena dipol tidak memiliki directivity pada arah tertentu, teleskop radio elemen tunggal yang menggunakan antena jenis ini tidak dapat digunakan untuk melakukan pencitraan.

• Gain

Gain (directive gain) adalah karakter antena yang terkait dengan kemampuan antena mengarahkan radiasi sinyalnya, atau penerimaan sinyal dari arah tertentu. Gain bukanlah kuantitas yang dapat diukur dalam satuan fisis pada umumnya seperti watt, ohm, atau lainnya, melainkan suatu bentuk perbandingan. Oleh karena itu, satuan yang digunakan untuk gain adalah desibel.

• Polarisasi

Polarisasi didefinisikan sebagai arah rambat dari medan listrik. Antena dipol memiliki polarisasi linear vertikal . Mengenali polarisasi antena amat berguna dalam sistem komunikasi, khususnya untuk mendapatkan efisiensi maksimum pada transmisi sinyal. Pada astronomi radio, tujuan mengenali polarisasi sinyal yang dipancarkan oleh sebuah objek astronomi adalah untuk mempelajari medan magnetik dari objek tersebut.
Ada beberapa hal yang perlu diperhatikan dalam pola radiasi, yang pertama adalah Half-power Beamwidth (HPBW), atau yang biasa dikenal sebagai beanwidth suatu antena. Dalam astronomi radio, beamwidth adalah resolusi spasial dari sebuah teleskop radio, yaitu diameter sudut minimun dari dua buah titik yang mampu dipisahkan oleh teleskop radio tersebut. Secara teori, beamwidth untuk antena yang berbentuk parabola dapat ditentukan.

Antena Directional

Antena jenis ini merupakan jenis antena dengan narrow beamwidth, yaitu punya sudut pemancaran yang kecil dengan daya lebih terarah, jaraknya jauh dan tidak bisa menjangkau area yang luas, antena directional mengirim dan menerima sinyal radio hanya pada satu arah, umumnya pada fokus yang sangat sempit, dan biasanya digunakan untuk koneksi point to point, atau multiple point, macam antena direktional seperti antena grid, dish "parabolic", yagi, dan antena sectoral.

Antena Omni-Directional

Antena ini mempunyai sudut pancaran yang besar (wide beamwidth) yaitu 3600; dengan daya lebih meluas, jarak yang lebih pendek tetapi dapat melayani area yang luas Omni antena tidak dianjurkan pemakaian-nya, karena sifatnya yang terlalu luas se-hingga ada kemungkinan mengumpulkan sinyal lain yang akan menyebabkan inter-ferensi. antena omnidirectional mengirim atau menerima sinyal radio dari semua arah secara sama, biasanya digunakan untuk koneksi multiple point atau hotspot.

Type Antena

1. Antena Omnidirectional


Sebuah antena Omnidirectional adalah antena daya sistem yang memancar secara seragam dalam satu pesawat dengan bentuk pola arahan dalam bidang tegak lurus. This pattern is often described as "donut shaped". Pola ini sering digambarkan sebagai "donat berbentuk". Omnidirectional antenna can be used to link multiple directional antenna in outdoor point-to-multipoint communication systems including cellular phone connections and TV broadcasts. Antena Omnidirectional dapat digunakan untuk menghubungkan beberapa antena directional di outdoor point-to-multipoint komunikasi systems termasuk sambungan telepon selular dan siaran TV.

Antena omni mempunyai sifat umum radiasi atau pancaran sinyal 360-derajat yang tegak lurus ke atas. Omnidirectional antena secara normal mempunyai gain sekitar 3-12 dBi. Yang digunakan untuk hubungan Point-To-Multi-Point ( P2Mp) atau stu titik ke banyak titik di sekitar daerah pancaran. Yang baik bekerja dari jarak 1-5 km, akan menguntungkan jika client atau penerima menggunalan directional antenna atau antenna yang ter arah.Yang ditunjukkan di bawah adalah pola pancaran khas RFDG 140 omnidirectional antena. Radiasi yang horisontal dengan pancaran 360-derjat. Radiasi yang horisontal pada dasarnya E-Field.yang berbeda dengan, polarisasi yang vertikal adalah sangat membatasi potongan sinyal yang di pancarkan. Antena ini akan melayani atau hanya memberi pancaran sinyal pada sekelilingnya atau 360 derjat, sedamgkan pada bagian atas antena tidak memiliki sinyal radiasi.

Pola radiasi dari antenna Omni



2. Antena Grid


Antena ini merupakan salah satu antena wifi yang populer. Sudut pola pancaran antena ini lebih fokus pada titik tertentu sesuai pemasangannya.

3. Antena Parabolik

– Dipakai untuk jarak menengah atau jarak jauh
– Gain-nya bisa antara 18 sampai 28 dBi


Pola radiasi dari antena Parabolik


Kelebihan antenna parabola
  • Dapat digunakan untuk menerima 3 satellite sekaligus tanpa harus menggerakkan antenna.
  • Dapat menampilkan gambar dari semua TV dari satelit yang ditangkap dalam sekejap.
  • Kondisi permanent sehingga tidak gampang goyah terhadap posisi.
  • Signal quality dapat maksimum

Kekurangan antenna parabola
  • Tidak dapat digunakan menangkap satelit lebih dari 5
  • Membutuhkan lebih banyak LNBF
  • Channel yang diterima lebih sedikit

4. Antena Sectoral

Antena Sectoral hampir mirip dengan antena omnidirectional. Yang juga digunakan untuk Access Point to serve a Point-to-Multi-Point (P2MP) links. Beberapa antenna sectoral dibuat tegak lurus , dan ada juga yang horizontal.
Antena sectoral mempunyai gain jauh lebih tinggi dibanding omnidirectional antena di sekitar 10-19 dBi. Yang bekerja pada jarak atau area 6-8 km. Sudut pancaran antenna ini adalah 45-180 derajat dan tingkat ketinggian pemasangannya harus diperhatikan agar tidak terdapat kerugian dalam penangkapan sinyal.

Pola pancaran yang horisontal kebanyakan memancar ke arah mana antenna ini di arahkan sesuai dengan jangkauan dari derajat pancarannya, sedangkan pada bagian belakang antenna tidak memiliki sinyal pancaran.
Antenna sectoral ini jika di pasang lebih tinggi akan menguntungkan penerimaan yang baik pada suatu sector atau wilayah pancaran yang telah di tentukan.


Pola radiasi dari antena Sektoral


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Jumat, 20 Agustus 2010

Optical Fiber ( Fiber Optik )

A bundle of optical fibers
A TOSLINK fiber optic audio cable being illuminated at one end

An optical fiber is made up of the core, (carries the light pulses), the cladding (reflects the light pulses back into the core) and the buffer coating (protects the core and cladding from moisture, damage, etc.). Together, all of this creates a fiber optic which can carry up to 10 million messages at any time using light pulses. Fiber optics is the overlap of applied science and engineering concerned with the design and application of optical fibers. Optical fibers are widely used in fiber-optic communications, which permits transmission over longer distances and at higher bandwidths (data rates) than other forms of communications. Fibers are used instead of metal wires because signals travel along them with less loss and are also immune to electromagnetic interference. Fibers are also used for illumination, and are wrapped in bundles so they can be used to carry images, thus allowing viewing in tight spaces. Specially designed fibers are used for a variety of other applications, including sensors and fiber lasers.

Light is kept in the core of the optical fiber by total internal reflection. This causes the fiber to act as a waveguide. Fibers which support many propagation paths or transverse modes are called multi-mode fibers (MMF), while those which can only support a single mode are called single-mode fibers (SMF). Multi-mode fibers generally have a larger core diameter, and are used for short-distance communication links and for applications where high power must be transmitted. Single-mode fibers are used for most communication links longer than 550 meters (1,800 ft).

Joining lengths of optical fiber is more complex than joining electrical wire or cable. The ends of the fibers must be carefully cleaved, and then spliced together either mechanically or by fusing them together with an electric arc. Special connectors are used to make removable connections.


History

Daniel Colladon first described this "light fountain" or "light pipe" in an 1842 article entitled On the reflections of a ray of light inside a parabolic liquid stream. This particular illustration comes from a later article by Colladon, in 1884.

Fiber optics, though used extensively in the modern world, is a fairly simple and old technology. Guiding of light by refraction, the principle that makes fiber optics possible, was first demonstrated by Daniel Colladon and Jacques Babinet in Paris in the early 1840s. John Tyndall included a demonstration of it in his public lectures in London a dozen years later.[1] Tyndall also wrote about the property of total internal reflection in an introductory book about the nature of light in 1870: "When the light passes from air into water, the refracted ray is bent towards the perpendicular... When the ray passes from water to air it is bent from the perpendicular... If the angle which the ray in water encloses with the perpendicular to the surface be greater than 48 degrees, the ray will not quit the water at all: it will be totally reflected at the surface.... The angle which marks the limit where total reflection begins is called the limiting angle of the medium. For water this angle is 48°27', for flint glass it is 38°41', while for diamond it is 23°42'."[2][3]

Practical applications, such as close internal illumination during dentistry, appeared early in the twentieth century. Image transmission through tubes was demonstrated independently by the radio experimenter Clarence Hansell and the television pioneer John Logie Baird in the 1920s. The principle was first used for internal medical examinations by Heinrich Lamm in the following decade. In 1952, physicist Narinder Singh Kapany conducted experiments that led to the invention of optical fiber. Modern optical fibers, where the glass fiber is coated with a transparent cladding to offer a more suitable refractive index, appeared later in the decade.[1] Development then focused on fiber bundles for image transmission. The first fiber optic semi-flexible gastroscope was patented by Basil Hirschowitz, C. Wilbur Peters, and Lawrence E. Curtiss, researchers at the University of Michigan, in 1956. In the process of developing the gastroscope, Curtiss produced the first glass-clad fibers; previous optical fibers had relied on air or impractical oils and waxes as the low-index cladding material. A variety of other image transmission applications soon followed.

In the late 19th and early 20th centuries, light was guided through bent glass rods to illuminate body cavities. Alexander Graham Bell invented a 'Photophone' to transmit voice signals over an optical beam.[4]

It is said that, Jun-ichi Nishizawa, a Japanese scientist at Tohoku University, also proposed the use of optical fibers for communications, in 1963, as stated in his own book published in 2004 in India.[5] Nishizawa invented other technologies that contributed to the development of optical fiber communications as well.[6] Nishizawa later invented the graded-index optical fiber as a channel for transmitting light from semiconductor lasers.[7]

The groundbreaking event happened in around 1965, Charles K. Kao and George A. Hockham of the British company Standard Telephones and Cables (STC) were the first to promote the idea that the attenuation in optical fibers could be reduced below 20 decibels per kilometer (dB/km), allowing fibers to be a practical medium for communication.[8] They proposed that the attenuation in fibers available at the time was caused by impurities, which could be removed, rather than fundamental physical effects such as scattering. They correctly and systematically theorized the light-loss properties for optical fiber, and pointed out the right material to manufacture such fibers — silica glass with high purity. This discovery led to Kao being awarded the Nobel Prize in Physics in 2009.[9]

NASA used fiber optics in the television cameras that were sent to the moon. At the time its use in the cameras was 'classified confidential' and only those with the right security clearance or those accompanied by someone with the right security clearance were permitted to handle the cameras.[10]

The crucial attenuation level of 20 dB/km was first achieved in 1970, by researchers Robert D. Maurer, Donald Keck, Peter C. Schultz, and Frank Zimar working for American glass maker Corning Glass Works, now Corning Incorporated. They demonstrated a fiber with 17 dB/km attenuation by doping silica glass with titanium. A few years later they produced a fiber with only 4 dB/km attenuation using germanium dioxide as the core dopant. Such low attenuations ushered in optical fiber telecommunications and enabled the Internet. In 1981, General Electric produced fused quartz ingots that could be drawn into fiber optic strands 25 miles (40 km) long.[11]

Attenuations in modern optical cables are far less than those in electrical copper cables, leading to long-haul fiber connections with repeater distances of 70–150 kilometers (43–93 mi). The erbium-doped fiber amplifier, which reduced the cost of long-distance fiber systems by reducing or even in many cases eliminating the need for optical-electrical-optical repeaters, was co-developed by teams led by David N. Payne of the University of Southampton, and Emmanuel Desurvire at Bell Labs in 1986. The more robust optical fiber commonly used today utilizes glass for both core and sheath and is therefore less prone to aging processes. It was invented by Gerhard Bernsee in 1973 of Schott Glass in Germany.[12]

In 1991, the emerging field of photonic crystals led to the development of photonic-crystal fiber[13] which guides light by means of diffraction from a periodic structure, rather than total internal reflection. The first photonic crystal fibers became commercially available in 2000.[14] Photonic crystal fibers can be designed to carry higher power than conventional fiber, and their wavelength dependent properties can be manipulated to improve their performance in certain applications.

Applications

Optical fiber communication

Optical fiber can be used as a medium for telecommunication and networking because it is flexible and can be bundled as cables. It is especially advantageous for long-distance communications, because light propagates through the fiber with little attenuation compared to electrical cables. This allows long distances to be spanned with few repeaters. Additionally, the per-channel light signals propagating in the fiber have been modulated at rates as high as 111 gigabits per second by NTT,[15][16] although 10 or 40 Gb/s is typical in deployed systems.[17][18] Each fiber can carry many independent channels, each using a different wavelength of light (wavelength-division multiplexing (WDM)). The net data rate (data rate without overhead bytes) per fiber is the per-channel data rate reduced by the FEC overhead, multiplied by the number of channels (usually up to eighty in commercial dense WDM systems as of 2008). The current laboratory fiber optic data rate record, held by Bell Labs in Villarceaux, France, is multiplexing 155 channels, each carrying 100 Gb/s over a 7000 km fiber.[19] Nippon Telegraph and Telephone Corporation have also managed 69.1 Tb/s over a single 240 km fibre (multiplexing 432 channels, equating to 171 Gb/s per channel).[20] Bell Labs also broke a 100 Petabit per second kilometer barrier (15.5 Tb/s over a single 7000 km fibre).[21]

For short distance applications, such as creating a network within an office building, fiber-optic cabling can be used to save space in cable ducts. This is because a single fiber can often carry much more data than many electrical cables, such as 4 pair Cat-5 Ethernet cabling.[vague] Fiber is also immune to electrical interference; there is no cross-talk between signals in different cables and no pickup of environmental noise. Non-armored fiber cables do not conduct electricity, which makes fiber a good solution for protecting communications equipment located in high voltage environments such as power generation facilities, or metal communication structures prone to lightning strikes. They can also be used in environments where explosive fumes are present, without danger of ignition. Wiretapping is more difficult compared to electrical connections, and there are concentric dual core fibers that are said to be tap-proof.[22]

Fiber optic sensors

Fibers have many uses in remote sensing. In some applications, the sensor is itself an optical fiber. In other cases, fiber is used to connect a non-fiberoptic sensor to a measurement system. Depending on the application, fiber may be used because of its small size, or the fact that no electrical power is needed at the remote location, or because many sensors can be multiplexed along the length of a fiber by using different wavelengths of light for each sensor, or by sensing the time delay as light passes along the fiber through each sensor. Time delay can be determined using a device such as an optical time-domain reflectometer.

Optical fibers can be used as sensors to measure strain, temperature, pressure and other quantities by modifying a fiber so that the quantity to be measured modulates the intensity, phase, polarization, wavelength or transit time of light in the fiber. Sensors that vary the intensity of light are the simplest, since only a simple source and detector are required. A particularly useful feature of such fiber optic sensors is that they can, if required, provide distributed sensing over distances of up to one meter.

Extrinsic fiber optic sensors use an optical fiber cable, normally a multi-mode one, to transmit modulated light from either a non-fiber optical sensor, or an electronic sensor connected to an optical transmitter. A major benefit of extrinsic sensors is their ability to reach places which are otherwise inaccessible. An example is the measurement of temperature inside aircraft jet engines by using a fiber to transmit radiation into a radiation pyrometer located outside the engine. Extrinsic sensors can also be used in the same way to measure the internal temperature of electrical transformers, where the extreme electromagnetic fields present make other measurement techniques impossible. Extrinsic sensors are used to measure vibration, rotation, displacement, velocity, acceleration, torque, and twisting. A solid state version of the gyroscope using the interference of light has been developed. The fiber optic gyroscope (FOG) has no moving parts and exploits the Sagnac effect to detect mechanical rotation.

A common use for fiber optic sensors are in advanced intrusion detection security systems, where the light is transmitted along the fibre optic sensor cable, which is placed on a fence, pipeline or communication cabling, and the returned signal is monitored and analysed for disturbances. This return signal is digitally processed to identify if there is a disturbance, and if an intrusion has occurred an alarm is triggered by the fiber optic security system.

Other uses of optical fibers

A frisbee illuminated by fiber optics
Light reflected from optical fiber illuminates exhibited model
Fiber optic front sight on a hand gun

Fibers are widely used in illumination applications. They are used as light guides in medical and other applications where bright light needs to be shone on a target without a clear line-of-sight path. In some buildings, optical fibers are used to route sunlight from the roof to other parts of the building (see non-imaging optics). Optical fiber illumination is also used for decorative applications, including signs, art, and artificial Christmas trees. Swarovski boutiques use optical fibers to illuminate their crystal showcases from many different angles while only employing one light source. Optical fiber is an intrinsic part of the light-transmitting concrete building product, LiTraCon.

Optical fiber is also used in imaging optics. A coherent bundle of fibers is used, sometimes along with lenses, for a long, thin imaging device called an endoscope, which is used to view objects through a small hole. Medical endoscopes are used for minimally invasive exploratory or surgical procedures (endoscopy). Industrial endoscopes (see fiberscope or borescope) are used for inspecting anything hard to reach, such as jet engine interiors.

In spectroscopy, optical fiber bundles are used to transmit light from a spectrometer to a substance which cannot be placed inside the spectrometer itself, in order to analyze its composition. A spectrometer analyzes substances by bouncing light off of and through them. By using fibers, a spectrometer can be used to study objects that are too large to fit inside, or gasses, or reactions which occur in pressure vessels.[23][24][25]

An optical fiber doped with certain rare earth elements such as erbium can be used as the gain medium of a laser or optical amplifier. Rare-earth doped optical fibers can be used to provide signal amplification by splicing a short section of doped fiber into a regular (undoped) optical fiber line. The doped fiber is optically pumped with a second laser wavelength that is coupled into the line in addition to the signal wave. Both wavelengths of light are transmitted through the doped fiber, which transfers energy from the second pump wavelength to the signal wave. The process that causes the amplification is stimulated emission.

Optical fibers doped with a wavelength shifter are used to collect scintillation light in physics experiments.

Optical fiber can be used to supply a low level of power (around one watt) to electronics situated in a difficult electrical environment. Examples of this are electronics in high-powered antenna elements and measurement devices used in high voltage transmission equipment.

A growing trend in iron sights for arms, is the use of short pieces of optical fiber for contrast enhancement dots, made in such a way that ambient light falling on the length of the fiber is concentrated at the tip, making the dots slightly brighter than the surroundings. This method is most commonly used in front sights, but many makers offer sights that use fiber optics on front and rear sights. Fiber optic sights can now be found on handguns, rifles, and shotguns, both as aftermarket accessories and a growing number of factory guns.[26]

Principle of operation

An optical fiber is a cylindrical dielectric waveguide (nonconducting waveguide) that transmits light along its axis, by the process of total internal reflection. The fiber consists of a core surrounded by a cladding layer, both of which are made of dielectric materials. To confine the optical signal in the core, the refractive index of the core must be greater than that of the cladding. The boundary between the core and cladding may either be abrupt, in step-index fiber, or gradual, in graded-index fiber.

Index of refraction

The index of refraction is a way of measuring the speed of light in a material. Light travels fastest in a vacuum, such as outer space. The actual speed of light in a vacuum is about 300,000 kilometres (186 thousand miles) per second. Index of refraction is calculated by dividing the speed of light in a vacuum by the speed of light in some other medium. The index of refraction of a vacuum is therefore 1, by definition. The typical value for the cladding of an optical fiber is 1.46. The core value is typically 1.48. The larger the index of refraction, the slower light travels in that medium. From this information, a good rule of thumb is that signal using optical fiber for communication will travel at around 200 million meters per second. Or to put it another way, to travel 1000 kilometers in fiber, the signal will take 5 milliseconds to propagate. Thus a phone call carried by fiber between Sydney and New York, a 12000 kilometer distance, means that there is an absolute minimum delay of 60 milliseconds (or around 1/16th of a second) between when one caller speaks to when the other hears. (Of course the fiber in this case will probably travel a longer route, and there will be additional delays due to communication equipment switching and the process of encoding and decoding the voice onto the fiber).

Total internal reflection

When light traveling in a dense medium hits a boundary at a steep angle (larger than the "critical angle" for the boundary), the light will be completely reflected. This effect is used in optical fibers to confine light in the core. Light travels along the fiber bouncing back and forth off of the boundary. Because the light must strike the boundary with an angle greater than the critical angle, only light that enters the fiber within a certain range of angles can travel down the fiber without leaking out. This range of angles is called the acceptance cone of the fiber. The size of this acceptance cone is a function of the refractive index difference between the fiber's core and cladding.

In simpler terms, there is a maximum angle from the fiber axis at which light may enter the fiber so that it will propagate, or travel, in the core of the fiber. The sine of this maximum angle is the numerical aperture (NA) of the fiber. Fiber with a larger NA requires less precision to splice and work with than fiber with a smaller NA. Single-mode fiber has a small NA.

Multi-mode fiber

The propagation of light through a multi-mode optical fiber.
A laser bouncing down an acrylic rod, illustrating the total internal reflection of light in a multi-mode optical fiber.

Fiber with large core diameter (greater than 10 micrometers) may be analyzed by geometrical optics. Such fiber is called multi-mode fiber, from the electromagnetic analysis (see below). In a step-index multi-mode fiber, rays of light are guided along the fiber core by total internal reflection. Rays that meet the core-cladding boundary at a high angle (measured relative to a line normal to the boundary), greater than the critical angle for this boundary, are completely reflected. The critical angle (minimum angle for total internal reflection) is determined by the difference in index of refraction between the core and cladding materials. Rays that meet the boundary at a low angle are refracted from the core into the cladding, and do not convey light and hence information along the fiber. The critical angle determines the acceptance angle of the fiber, often reported as a numerical aperture. A high numerical aperture allows light to propagate down the fiber in rays both close to the axis and at various angles, allowing efficient coupling of light into the fiber. However, this high numerical aperture increases the amount of dispersion as rays at different angles have different path lengths and therefore take different times to traverse the fiber.

Optical fiber types.

In graded-index fiber, the index of refraction in the core decreases continuously between the axis and the cladding. This causes light rays to bend smoothly as they approach the cladding, rather than reflecting abruptly from the core-cladding boundary. The resulting curved paths reduce multi-path dispersion because high angle rays pass more through the lower-index periphery of the core, rather than the high-index center. The index profile is chosen to minimize the difference in axial propagation speeds of the various rays in the fiber. This ideal index profile is very close to a parabolic relationship between the index and the distance from the axis.

Single-mode fiber

The structure of a typical single-mode fiber.
1. Core: 8 µm diameter
2. Cladding: 125 µm dia.
3. Buffer: 250 µm dia.
4. Jacket: 400 µm dia.

Fiber with a core diameter less than about ten times the wavelength of the propagating light cannot be modeled using geometric optics. Instead, it must be analyzed as an electromagnetic structure, by solution of Maxwell's equations as reduced to the electromagnetic wave equation. The electromagnetic analysis may also be required to understand behaviors such as speckle that occur when coherent light propagates in multi-mode fiber. As an optical waveguide, the fiber supports one or more confined transverse modes by which light can propagate along the fiber. Fiber supporting only one mode is called single-mode or mono-mode fiber. The behavior of larger-core multi-mode fiber can also be modeled using the wave equation, which shows that such fiber supports more than one mode of propagation (hence the name). The results of such modeling of multi-mode fiber approximately agree with the predictions of geometric optics, if the fiber core is large enough to support more than a few modes.

The waveguide analysis shows that the light energy in the fiber is not completely confined in the core. Instead, especially in single-mode fibers, a significant fraction of the energy in the bound mode travels in the cladding as an evanescent wave.

The most common type of single-mode fiber has a core diameter of 8–10 micrometers and is designed for use in the near infrared. The mode structure depends on the wavelength of the light used, so that this fiber actually supports a small number of additional modes at visible wavelengths. Multi-mode fiber, by comparison, is manufactured with core diameters as small as 50 micrometers and as large as hundreds of micrometers. The normalized frequency V for this fiber should be less than the first zero of the Bessel function J0 (approximately 2.405).

Special-purpose fiber

Some special-purpose optical fiber is constructed with a non-cylindrical core and/or cladding layer, usually with an elliptical or rectangular cross-section. These include polarization-maintaining fiber and fiber designed to suppress whispering gallery mode propagation.

Photonic-crystal fiber is made with a regular pattern of index variation (often in the form of cylindrical holes that run along the length of the fiber). Such fiber uses diffraction effects instead of or in addition to total internal reflection, to confine light to the fiber's core. The properties of the fiber can be tailored to a wide variety of applications.

Mechanisms of attenuation

Light attenuation by ZBLAN and silica fibers

Attenuation in fiber optics, also known as transmission loss, is the reduction in intensity of the light beam (or signal) with respect to distance traveled through a transmission medium. Attenuation coefficients in fiber optics usually use units of dB/km through the medium due to the relatively high quality of transparency of modern optical transmission media. The medium is usually a fiber of silica glass that confines the incident light beam to the inside. Attenuation is an important factor limiting the transmission of a digital signal across large distances. Thus, much research has gone into both limiting the attenuation and maximizing the amplification of the optical signal. Empirical research has shown that attenuation in optical fiber is caused primarily by both scattering and absorption.

Light scattering

Specular reflection
Diffuse reflection

The propagation of light through the core of an optical fiber is based on total internal reflection of the lightwave. Rough and irregular surfaces, even at the molecular level, can cause light rays to be reflected in random directions. This is called diffuse reflection or scattering, and it is typically characterized by wide variety of reflection angles.

Light scattering depends on the wavelength of the light being scattered. Thus, limits to spatial scales of visibility arise, depending on the frequency of the incident light-wave and the physical dimension (or spatial scale) of the scattering center, which is typically in the form of some specific micro-structural feature. Since visible light has a wavelength of the order of one micrometre (one millionth of a meter) scattering centers will have dimensions on a similar spatial scale.

Thus, attenuation results from the incoherent scattering of light at internal surfaces and interfaces. In (poly)crystalline materials such as metals and ceramics, in addition to pores, most of the internal surfaces or interfaces are in the form of grain boundaries that separate tiny regions of crystalline order. It has recently been shown that when the size of the scattering center (or grain boundary) is reduced below the size of the wavelength of the light being scattered, the scattering no longer occurs to any significant extent. This phenomenon has given rise to the production of transparent ceramic materials.

Similarly, the scattering of light in optical quality glass fiber is caused by molecular level irregularities (compositional fluctuations) in the glass structure. Indeed, one emerging school of thought is that a glass is simply the limiting case of a polycrystalline solid. Within this framework, "domains" exhibiting various degrees of short-range order become the building blocks of both metals and alloys, as well as glasses and ceramics. Distributed both between and within these domains are micro-structural defects which will provide the most ideal locations for the occurrence of light scattering. This same phenomenon is seen as one of the limiting factors in the transparency of IR missile domes.[27]

At high optical powers, scattering can also be caused by nonlinear optical processes in the fiber.[28][29]

UV-Vis-IR absorption

In addition to light scattering, attenuation or signal loss can also occur due to selective absorption of specific wavelengths, in a manner similar to that responsible for the appearance of color. Primary material considerations include both electrons and molecules as follows:

1) At the electronic level, it depends on whether the electron orbitals are spaced (or "quantized") such that they can absorb a quantum of light (or photon) of a specific wavelength or frequency in the ultraviolet (UV) or visible ranges. This is what gives rise to color.

2) At the atomic or molecular level, it depends on the frequencies of atomic or molecular vibrations or chemical bonds, how close-packed its atoms or molecules are, and whether or not the atoms or molecules exhibit long-range order. These factors will determine the capacity of the material transmitting longer wavelengths in the infrared (IR), far IR, radio and microwave ranges.

The design of any optically transparent device requires the selection of materials based upon knowledge of its properties and limitations. The lattice [disambiguation needed] absorption characteristics observed at the lower frequency regions (mid IR to far-infrared wavelength range) define the long-wavelength transparency limit of the material. They are the result of the interactive coupling between the motions of thermally induced vibrations of the constituent atoms and molecules of the solid lattice and the incident light wave radiation. Hence, all materials are bounded by limiting regions of absorption caused by atomic and molecular vibrations (bond-stretching)in the far-infrared (>10 µm).

Normal modes of vibration in a crystalline solid.

Thus, multi-phonon absorption occurs when two or more phonons simultaneously interact to produce electric dipole moments with which the incident radiation may couple. These dipoles can absorb energy from the incident radiation, reaching a maximum coupling with the radiation when the frequency is equal to the fundamental vibrational mode of the molecular dipole (e.g. Si-O bond) in the far-infrared, or one of its harmonics.

The selective absorption of infrared (IR) light by a particular material occurs because the selected frequency of the light wave matches the frequency (or an integer multiple of the frequency) at which the particles of that material vibrate. Since different atoms and molecules have different natural frequencies of vibration, they will selectively absorb different frequencies (or portions of the spectrum) of infrared (IR) light.

Reflection and transmission of light waves occur because the frequencies of the light waves do not match the natural resonant frequencies of vibration of the objects. When IR light of these frequencies strikes an object, the energy is either reflected or transmitted.

Manufacturing

Materials

Glass optical fibers are almost always made from silica, but some other materials, such as fluorozirconate, fluoroaluminate, and chalcogenide glasses as well as crystalline materials like sapphire, are used for longer-wavelength infrared or other specialized applications. Silica and fluoride glasses usually have refractive indices of about 1.5, but some materials such as the chalcogenides can have indices as high as 3. Typically the index difference between core and cladding is less than one percent.

Plastic optical fibers (POF) are commonly step-index multi-mode fibers with a core diameter of 0.5 millimeters or larger. POF typically have higher attenuation coefficients than glass fibers, 1 dB/m or higher, and this high attenuation limits the range of POF-based systems.

Silica

Tetrahedral structural unit of silica (SiO2).
The amorphous structure of glassy silica (SiO2). No long-range order is present, however there is local ordering with respect to the tetrahedral arrangement of oxygen (O) atoms around the silicon (Si) atoms.

Silica exhibits fairly good optical transmission over a wide range of wavelengths. In the near-infrared (near IR) portion of the spectrum, particularly around 1.5 μm, silica can have extremely low absorption and scattering losses of the order of 0.2 dB/km. A high transparency in the 1.4-μm region is achieved by maintaining a low concentration of hydroxyl groups (OH). Alternatively, a high OH concentration is better for transmission in the ultraviolet (UV) region.

Silica can be drawn into fibers at reasonably high temperatures, and has a fairly broad glass transformation range. One other advantage is that fusion splicing and cleaving of silica fibers is relatively effective. Silica fiber also has high mechanical strength against both pulling and even bending, provided that the fiber is not too thick and that the surfaces have been well prepared during processing. Even simple cleaving (breaking) of the ends of the fiber can provide nicely flat surfaces with acceptable optical quality. Silica is also relatively chemically inert. In particular, it is not hygroscopic (does not absorb water).

Silica glass can be doped with various materials. One purpose of doping is to raise the refractive index (e.g. with Germanium dioxide (GeO2) or Aluminium oxide (Al2O3)) or to lower it (e.g. with fluorine or Boron trioxide (B2O3)). Doping is also possible with laser-active ions (for example, rare earth-doped fibers) in order to obtain active fibers to be used, for example, in fiber amplifiers or laser applications. Both the fiber core and cladding are typically doped, so that the entire assembly (core and cladding) is effectively the same compound (e.g. an aluminosilicate, germanosilicate, phosphosilicate or borosilicate glass).

Particularly for active fibers, pure silica is usually not a very suitable host glass, because it exhibits a low solubility for rare earth ions. This can lead to quenching effects due to clustering of dopant ions. Aluminosilicates are much more effective in this respect.

Silica fiber also exhibits a high threshold for optical damage. This property ensures a low tendency for laser-induced breakdown. This is important for fiber amplifiers when utilized for the amplification of short pulses.

Because of these properties silica fibers are the material of choice in many optical applications, such as communications (except for very short distances with plastic optical fiber), fiber lasers, fiber amplifiers, and fiber-optic sensors. The large efforts which have been put forth in the development of various types of silica fibers have further increased the performance of such fibers over other materials.[30][31][32][33][34][35][36][37]

Fluorides

Fluoride glass is a class of non-oxide optical quality glasses composed of fluorides of various metals. Because of their low viscosity, it is very difficult to completely avoid crystallization while processing it through the glass transition (or drawing the fiber from the melt). Thus, although heavy metal fluoride glasses (HMFG) exhibit very low optical attenuation, they are not only difficult to manufacture, but are quite fragile, and have poor resistance to moisture and other environmental attacks. Their best attribute is that they lack the absorption band associated with the hydroxyl (OH) group (3200–3600 cm−1), which is present in nearly all oxide-based glasses.

An example of a heavy metal fluoride glass is the ZBLAN glass group, composed of zirconium, barium, lanthanum, aluminium, and sodium fluorides. Their main technological application is as optical waveguides in both planar and fiber form. They are advantageous especially in the mid-infrared (2000–5000 nm) range.

HMFGs were initially slated for optical fiber applications, because the intrinsic losses of a mid-IR fiber could in principle be lower than those of silica fibers, which are transparent only up to about 2 μm. However, such low losses were never realized in practice, and the fragility and high cost of fluoride fibers made them less than ideal as primary candidates. Later, the utility of fluoride fibers for various other applications was discovered. These include mid-IR spectroscopy, fiber optic sensors, thermometry, and imaging. Also, fluoride fibers can be used to for guided lightwave transmission in media such as YAG (yttria-alumina garnet) lasers at 2.9 μm, as required for medical applications (e.g. ophthalmology and dentistry).[38][39]

Phosphates

The P4O10 cagelike structure—the basic building block for phosphate glass.

Phosphate glass constitutes a class of optical glasses composed of metaphosphates of various metals. Instead of the SiO4 tetrahedra observed in silicate glasses, the building block for this glass former is Phosphorus pentoxide (P2O5), which crystallizes in at least four different forms. The most familiar polymorph (see figure) comprises molecules of P4O10.

Phosphate glasses can be advantageous over silica glasses for optical fibers with a high concentration of doping rare earth ions. A mix of fluoride glass and phosphate glass is fluorophosphate glass.[40][41]

[edit] Chalcogenides

The chalcogens—the elements in group 16 of the periodic table—particularly sulfur (S), selenium (Se) and tellurium (Te)—react with more electropositive elements, such as silver, to form chalcogenides. These are extremely versatile compounds, in that they can be crystalline or amorphous, metallic or semiconducting, and conductors of ions or electrons.

Process

Illustration of the modified chemical vapor deposition (inside) process

Standard optical fibers are made by first constructing a large-diameter preform, with a carefully controlled refractive index profile, and then pulling the preform to form the long, thin optical fiber. The preform is commonly made by three chemical vapor deposition methods: inside vapor deposition, outside vapor deposition, and vapor axial deposition.[42]

With inside vapor deposition, the preform starts as a hollow glass tube approximately 40 centimeters (16 in) long, which is placed horizontally and rotated slowly on a lathe. Gases such as silicon tetrachloride (SiCl4) or germanium tetrachloride (GeCl4) are injected with oxygen in the end of the tube. The gases are then heated by means of an external hydrogen burner, bringing the temperature of the gas up to 1900 K (1600 °C, 3000 °F), where the tetrachlorides react with oxygen to produce silica or germania (germanium dioxide) particles. When the reaction conditions are chosen to allow this reaction to occur in the gas phase throughout the tube volume, in contrast to earlier techniques where the reaction occurred only on the glass surface, this technique is called modified chemical vapor deposition.

The oxide particles then agglomerate to form large particle chains, which subsequently deposit on the walls of the tube as soot. The deposition is due to the large difference in temperature between the gas core and the wall causing the gas to push the particles outwards (this is known as thermophoresis). The torch is then traversed up and down the length of the tube to deposit the material evenly. After the torch has reached the end of the tube, it is then brought back to the beginning of the tube and the deposited particles are then melted to form a solid layer. This process is repeated until a sufficient amount of material has been deposited. For each layer the composition can be modified by varying the gas composition, resulting in precise control of the finished fiber's optical properties.

In outside vapor deposition or vapor axial deposition, the glass is formed by flame hydrolysis, a reaction in which silicon tetrachloride and germanium tetrachloride are oxidized by reaction with water (H2O) in an oxyhydrogen flame. In outside vapor deposition the glass is deposited onto a solid rod, which is removed before further processing. In vapor axial deposition, a short seed rod is used, and a porous preform, whose length is not limited by the size of the source rod, is built up on its end. The porous preform is consolidated into a transparent, solid preform by heating to about 1800 K (1500 °C, 2800 °F).

The preform, however constructed, is then placed in a device known as a drawing tower, where the preform tip is heated and the optic fiber is pulled out as a string. By measuring the resultant fiber width, the tension on the fiber can be controlled to maintain the fiber thickness.

Coatings

The light is "guided" down the core of the fibre by an optical "cladding" with a lower refractive index that traps light in the core through "total internal reflection."

The cladding is coated by a "buffer" that protects it from moisture and physical damage. The buffer is what gets stripped off the fibre for termination or splicing. These coatings are UV-cured urethane acrylate composite materials applied to the outside of the fiber during the drawing process. The coatings protect the very delicate strands of glass fiber—about the size of a human hair—and allow it to survive the rigors of manufacturing, proof testing, cabling and installation.

Today’s glass optical fiber draw processes employ a dual-layer coating approach. An inner primary coating is designed to act as a shock absorber to minimize attenuation caused by microbending. An outer secondary coating protects the primary coating against mechanical damage and acts as a barrier to lateral forces. Sometimes a metallic armour layer is added to provide extra protection.

These fiber optic coating layers are applied during the fiber draw, at speeds approaching 100 kilometers per hour (60 mph). Fiber optic coatings are applied using one of two methods: wet-on-dry, in which the fiber passes through a primary coating application, which is then UV cured, then through the secondary coating application which is subsequently cured; and wet-on-wet, in which the fiber passes through both the primary and secondary coating applications and then goes to UV curing.

Fiber optic coatings are applied in concentric layers to prevent damage to the fiber during the drawing application and to maximize fiber strength and microbend resistance. Unevenly coated fiber will experience non-uniform forces when the coating expands or contracts, and is susceptible to greater signal attenuation. Under proper drawing and coating processes, the coatings are concentric around the fiber, continuous over the length of the application and have constant thickness.

Fiber optic coatings protect the glass fibers from scratches that could lead to strength degradation. The combination of moisture and scratches accelerates the aging and deterioration of fiber strength. When fiber is subjected to low stresses over a long period, fiber fatigue can occur. Over time or in extreme conditions, these factors combine to cause microscopic flaws in the glass fiber to propagate, which can ultimately result in fiber failure.

Three key characteristics of fiber optic waveguides can be affected by environmental conditions: strength, attenuation and resistance to losses caused by microbending. External fiber optic coatings protect glass optical fiber from environmental conditions that can affect the fiber’s performance and long-term durability. On the inside, coatings ensure the reliability of the signal being carried and help minimize attenuation due to microbending..

Practical issues

Optical fiber cables

In practical fibers, the cladding is usually coated with a tough resin buffer layer, which may be further surrounded by a jacket layer, usually plastic. These layers add strength to the fiber but do not contribute to its optical wave guide properties. Rigid fiber assemblies sometimes put light-absorbing ("dark") glass between the fibers, to prevent light that leaks out of one fiber from entering another. This reduces cross-talk between the fibers, or reduces flare in fiber bundle imaging applications.[43][44]

Modern cables come in a wide variety of sheathings and armor, designed for applications such as direct burial in trenches, high voltage isolation, dual use as power lines,[45][not in citation given] installation in conduit, lashing to aerial telephone poles, submarine installation, and insertion in paved streets. The cost of small fiber-count pole-mounted cables has greatly decreased due to the high demand for fiber to the home (FTTH) installations in Japan and South Korea.

Fiber cable can be very flexible, but traditional fiber's loss increases greatly if the fiber is bent with a radius smaller than around 30 mm. This creates a problem when the cable is bent around corners or wound around a spool, making FTTX installations more complicated. "Bendable fibers", targeted towards easier installation in home environments, have been standardized as ITU-T G.657. This type of fiber can be bent with a radius as low as 7.5 mm without adverse impact. Even more bendable fibers have been developed.[46] Bendable fiber may also be resistant to fiber hacking, in which the signal in a fiber is surreptitiously monitored by bending the fiber and detecting the leakage.[47]

Another important feature of cable is cable withstanding against the horizontally applied force. It is technically called max tensile strength defining how much force can applied to the cable during the installation of a period.

Telecom Anatolia fiber optic cable versions are reinforced with aramid yarns or glass yarns as intermediary strength member. In commercial terms, usage of the glass yarns are more cost effective while no loss in mechanical durability of the cable. Glass yarns also protect the cable core against rodents and termites.

Termination and splicing

ST connectors on multi-mode fiber.

Optical fibers are connected to terminal equipment by optical fiber connectors. These connectors are usually of a standard type such as FC, SC, ST, LC, or MTRJ.

Optical fibers may be connected to each other by connectors or by splicing, that is, joining two fibers together to form a continuous optical waveguide. The generally accepted splicing method is arc fusion splicing, which melts the fiber ends together with an electric arc. For quicker fastening jobs, a "mechanical splice" is used.

Fusion splicing is done with a specialized instrument that typically operates as follows: The two cable ends are fastened inside a splice enclosure that will protect the splices, and the fiber ends are stripped of their protective polymer coating (as well as the more sturdy outer jacket, if present). The ends are cleaved (cut) with a precision cleaver to make them perpendicular, and are placed into special holders in the splicer. The splice is usually inspected via a magnified viewing screen to check the cleaves before and after the splice. The splicer uses small motors to align the end faces together, and emits a small spark between electrodes at the gap to burn off dust and moisture. Then the splicer generates a larger spark that raises the temperature above the melting point of the glass, fusing the ends together permanently. The location and energy of the spark is carefully controlled so that the molten core and cladding do not mix, and this minimizes optical loss. A splice loss estimate is measured by the splicer, by directing light through the cladding on one side and measuring the light leaking from the cladding on the other side. A splice loss under 0.1 dB is typical. The complexity of this process makes fiber splicing much more difficult than splicing copper wire.

Mechanical fiber splices are designed to be quicker and easier to install, but there is still the need for stripping, careful cleaning and precision cleaving. The fiber ends are aligned and held together by a precision-made sleeve, often using a clear index-matching gel that enhances the transmission of light across the joint. Such joints typically have higher optical loss and are less robust than fusion splices, especially if the gel is used. All splicing techniques involve the use of an enclosure into which the splice is placed for protection afterward.

Fibers are terminated in connectors so that the fiber end is held at the end face precisely and securely. A fiber-optic connector is basically a rigid cylindrical barrel surrounded by a sleeve that holds the barrel in its mating socket. The mating mechanism can be "push and click", "turn and latch" ("bayonet"), or screw-in (threaded). A typical connector is installed by preparing the fiber end and inserting it into the rear of the connector body. Quick-set adhesive is usually used so the fiber is held securely, and a strain relief is secured to the rear. Once the adhesive has set, the fiber's end is polished to a mirror finish. Various polish profiles are used, depending on the type of fiber and the application. For single-mode fiber, the fiber ends are typically polished with a slight curvature, such that when the connectors are mated the fibers touch only at their cores. This is known as a "physical contact" (PC) polish. The curved surface may be polished at an angle, to make an "angled physical contact" (APC) connection. Such connections have higher loss than PC connections, but greatly reduced back reflection, because light that reflects from the angled surface leaks out of the fiber core; the resulting loss in signal strength is known as gap loss. APC fiber ends have low back reflection even when disconnected.

In the 1990s, terminating fiber optic cables was very labor intensive. The number of parts per connector, polishing of the fibers, and the need to oven-bake the epoxy in each connector made terminating fiber optic cables very difficult. Today, many different connectors are on the market and offer an easier, less labor intensive way of terminating the cables. Some of the most popular connectors have already been polished from the factory and include a gel inside the connector and those two steps help save money on labor especially on large projects. A cleave is made at a required length in order to get as close to the polished piece already inside the connector, with the gel surrounding the point where the two piece meet inside the connector very little light loss is exposed.[citation needed]

Free-space coupling

It is often necessary to align an optical fiber with another optical fiber, or with an optoelectronic device such as a light-emitting diode, a laser diode, or a modulator. This can involve either carefully aligning the fiber and placing it in contact with the device, or can use a lens to allow coupling over an air gap. In some cases the end of the fiber is polished into a curved form that is designed to allow it to act as a lens.

In a laboratory environment, a bare fiber end is coupled using a fiber launch system, which uses a microscope objective lens to focus the light down to a fine point. A precision translation stage (micro-positioning table) is used to move the lens, fiber, or device to allow the coupling efficiency to be optimized. Fibers with a connector on the end make this process much simpler: the connector is simply plugged into a pre-aligned fiberoptic collimator, which contains a lens that is either accurately positioned with respect to the fiber, or is adjustable. To achieve the best injection efficiency into single-mode fiber, the direction, position, size and divergence of the beam must all be optimized. With good beams, 70 to 90% coupling efficiency can be achieved.

With properly polished single-mode fibers, the emitted beam has an almost perfect Gaussian shape—even in the far field—if a good lens is used. The lens needs to be large enough to support the full numerical aperture of the fiber, and must not introduce aberrations in the beam. Aspheric lenses are typically used.

Fiber fuse

At high optical intensities, above 2 megawatts per square centimeter, when a fiber is subjected to a shock or is otherwise suddenly damaged, a fiber fuse can occur. The reflection from the damage vaporizes the fiber immediately before the break, and this new defect remains reflective so that the damage propagates back toward the transmitter at 1–3 meters per second (4−11 km/h, 2–8 mph).[48][49] The open fiber control system, which ensures laser eye safety in the event of a broken fiber, can also effectively halt propagation of the fiber fuse.[50] In situations, such as undersea cables, where high power levels might be used without the need for open fiber control, a "fiber fuse" protection device at the transmitter can break the circuit to prevent any damage.

Example

Fiber connections can be used for various types of connections. For example, most high definition televisions offer a digital audio optical connection. This allows the streaming of audio over light, using the TOSLink protocol.

Electric power transmission

Optical fiber can be used to transmit electricity.[51] While the efficiency is not nearly that of traditional copper wire, it is especially useful in situations where it is desirable to not have a metallic conductor as in the case of use near MRI machines which produce strong magnetic currents.[52]

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