Free-space optical communication ( FSO) is an optical communication technology that uses light propagating in free space to transmit data for telecommunications or over long distances. "Free space" means air, outer space, vacuum, or something similar. This contrasts with using solids such as optical fiber cable. The technology is useful where the physical connections are impractical due to high costs or other considerations.
In 1880, Alexander Graham Bell and his assistant Charles Sumner Tainter created the photophone, at Bell's newly established Volta Laboratory in Washington, DC. Bell considered it his most important invention. The device allowed for the transmission of sound on a beam of light. On June 3, 1880, Bell conducted the world's first wireless telephone transmission between two buildings, some apart.
also published as "Selenium and the Photophone" in ''Nature'', September 1880.
Its first practical use came in military communication systems many decades later, first for optical telegraphy. German colonial troops used heliograph telegraphy transmitters during the Herero Wars starting in 1904, in German South-West Africa (today's Namibia) as did British, French, US or Ottoman signals.
During the trench warfare of World War I when wire communications were often cut, German signals used three types of optical Morse transmitters called Blinkgerät, the intermediate type for distances of up to at daylight and of up to at night, using red filters for undetected communications. Optical telephone communications were tested at the end of the war, but not introduced at troop level. In addition, special blinkgeräts were used for communication with airplanes, balloons, and tanks, with varying success.
A major technological step was to replace the Morse code by modulating optical waves in speech transmission. Carl Zeiss, Jena developed the Lichtsprechgerät 80/80 (literal translation: optical speaking device) that the German army used in their World War II anti-aircraft defense units, or in bunkers at the Atlantic Wall.
The invention of in the 1960s revolutionized free-space optics. Military organizations were particularly interested and boosted their development. In 1973, while prototyping the first laser printers at Xerox PARC, Gary Starkweather and others made a duplex 30 Mbit/s campus network optical link using astronomical telescopes and HeNe lasers to send data between offices; they chose the method due partly to less strict regulations (at the time) on free-space optical communication by the FCC. However, laser-based free-space optics lost market momentum when the installation of optical fiber networks for civilian uses was at its peak.
Many simple and inexpensive consumer use low-speed communication using infrared (IR) light. This is known as consumer IR technologies.
Military based studies consistently produce longer estimates for reliability, projecting the maximum range for terrestrial links is of the order of . All studies agree the stability and quality of the link is highly dependent on atmospheric factors such as rain, fog, dust and heat. Relays may be employed to extend the range for FSO communications.
TMEX USA ran two eight-mile links between Laredo, Texas and Nuevo Laredo from 1998 to 2002. The links operated at 155 Mbit/s and reliably carried phone calls and internet service.
Other non-government groups are fielding tests to evaluate different technologies that some claim have the ability to address key FSO adoption challenges. , none have fielded a working system that addresses the most common atmospheric events.
FSO research from 1998 to 2006 in the private sector totaled $407.1 million, divided primarily among four start-up companies. All four failed to deliver products that would meet telecommunications quality and distance standards:
One private company published a paper on November 20, 2014, claiming they had achieved commercial reliability (99.999% availability) in extreme fog. There is no indication this product is currently commercially available.
In December 2023, the Australian National University (ANU) demonstrated its Quantum Optical Ground Station at its Mount Stromlo Observatory. QOGS uses adaptive optics and lasers as part of a telescope, to create a bi-directional communications system capable of supporting the NASA Artemis program to the Moon. New Quantum Optical Ground Station allows Canberra to play starring role in space communications, Emmy Groves, ABC News Online, 2023-12-06
In January 2013, NASA used lasers to beam an image of the Mona Lisa to the Lunar Reconnaissance Orbiter roughly away. To compensate for atmospheric interference, an error correction code algorithm similar to that used in CDs was implemented.
In the early morning hours of October 18, 2013, NASA's Lunar Laser Communication Demonstration (LLCD) transmitted data from lunar orbit to Earth at a rate of 622 megabits per second (Mbit/s). LLCD was flown aboard the LADEE (LADEE) spacecraft, whose primary science mission was to investigate the tenuous and exotic atmosphere that exists around the Moon.
Between April and July 2014 NASA's OPALS instrument successfully uploaded 175 megabytes in 3.5 seconds and downloaded 200–300 MB in 20 s. Their system was also able to re-acquire tracking after the signal was lost due to cloud cover.
On December 7, 2021 NASA launched the Laser Communications Relay Demonstration (LCRD), which aims to relay data between spacecraft in geosynchronous orbit and ground stations. LCRD is NASA's first two-way, end-to-end optical relay. LCRD uses two , Optical Ground Station (OGS)-1 and -2, at Table Mountain Observatory in California, and Haleakalā, Hawaii. One of LCRD's first operational users is the Integrated LCRD Low-Earth Orbit User Modem and Amplifier Terminal (ILLUMA-T), on the International Space Station. The terminal will receive high-resolution science data from experiments and instruments on board the space station and then transfer this data to LCRD, which will then transmit it to a ground station. After the data arrives on Earth, it will be delivered to mission operation centers and mission scientists. The ILLUMA-T payload was sent to the ISS in late 2023 on SpaceX CRS-29, and achieved first light on December 5, 2023. NASA's First Two-way End-to-End Laser Communications System Oct 2023
On April 28, 2023, NASA and its partners achieved 200 gigabit per second (Gbit/s) throughput on a space-to-ground optical link between a satellite in orbit and Earth. This was achieved by the TeraByte InfraRed Delivery (TBIRD) system, mounted on NASA's Pathfinder Technology Demonstrator 3 (PTD-3) satellite.
In 2004, a visible light communication consortium was formed in Japan. This was based on work from researchers that used a white LED-based space lighting system for indoor local area network (LAN) communications. These systems present advantages over traditional UHF RF-based systems from improved isolation between systems, the size and cost of receivers/transmitters, RF licensing laws and by combining space lighting and communication into the same system. In January 2009, a task force for visible light communication was formed by the Institute of Electrical and Electronics Engineers working group for wireless personal area network standards known as . A trial was announced in 2010, in St. Cloud, Minnesota.
Amateur radio operators have achieved significantly farther distances using incoherent sources of light from high-intensity LEDs. One reported in 2007. However, physical limitations of the equipment used limited bandwidths to about 4 kHz. The high sensitivities required of the detector to cover such distances made the internal capacitance of the photodiode used a dominant factor in the high-impedance amplifier which followed it, thus naturally forming a low-pass filter with a cut-off frequency in the 4 kHz range. Lasers can reach very high data rates which are comparable to fiber communications.
Projected data rates and future data rate claims vary. A low-cost white LED (GaN-phosphor) which could be used for space lighting can typically be modulated up to 20 MHz. Data rates of over 100 Mbit/s can be achieved using efficient modulation schemes and Siemens claimed to have achieved over 500 Mbit/s in 2010. Research published in 2009, used a similar system for traffic control of automated vehicles with LED traffic lights.
In September 2013, pureLiFi, the Edinburgh start-up working on Li-Fi, also demonstrated high speed point-to-point connectivity using any off-the-shelf LED light bulb. In previous work, high bandwidth specialist LEDs have been used to achieve the high data rates. The new system, the Li-1st, maximizes the available optical bandwidth for any LED device, thereby reducing the cost and improving the performance of deploying indoor FSO systems.
The light beam can be very narrow, which makes FSO hard to intercept, improving security. Encryption can secure the data traversing the link. FSO provides vastly improved electromagnetic interference (EMI) behavior compared to using .
These factors cause an attenuated receiver signal and lead to higher bit error ratio (BER). To overcome these issues, vendors found some solutions, like multi-beam or multi-path architectures, which use more than one sender and more than one receiver. Some state-of-the-art devices also have larger fade margin (extra power, reserved for rain, smog, fog). To keep an eye-safe environment, good FSO systems have a limited laser power density and support laser safety 1 or 1M. Atmospheric and fog attenuation, which are exponential in nature, limit practical range of FSO devices to several kilometers. However, free-space optics based on infrared wavelength, have considerably lower optical loss than free-space optics using infrared wavelength, in dense fog conditions. FSO using wavelength 1550 nm system are capable of transmitting several times higher power than systems with Infrared and are safe to the human eye (1M class). Additionally, some free-space optics, such as EC SYSTEM, ensure higher connection reliability in bad weather conditions by constantly monitoring link quality to regulate laser diode transmission power with built-in automatic gain control.
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