This paper proposes a novel combined optical-electronic simulation in an indoor environment consisting of four luminaires with tunable LEDs of different Correlated Color Temperatures (CCT). This paper investigates the ability to perform Visible Light Positioning (VLP) to identify the receiver positions in such a scenario with tunable LEDs. In this regard, the ray-tracing simulation, generating a list of rays consisting of optical power, CCT, and the corresponding wavelength of each ray, impinging on the receiver's surface, is combined with the simulation of an electronic receiver with wavelength depending sensitivity in Simulink/Simscape. This configuration allows us to evaluate the impact of tunable CCT on the electronic design, especially regarding optimizing certain parameters. In this work, we show how the number of unique values in an offline-fingerprinting map can be optimized, which is a crucial requirement for indoor positioning utilizing the fingerprinting method. With our outlined solution approach, a system-level tool is formed based on a precise and comprehensive optical-electronic simulation that allows for assessing VLP scenarios.
By enabling Free Space Optics (FSO) technology as complementary solution to RF systems, the next generation satellite communication that relies on optical links is on the verge. Even though the transition to wireless optical communication is a fact, the space domain is very conservative to such critical changes that call for close evaluation of each system aspect. Since trade-off between costs and efficiency is required, a state-of-the-art laboratory testbed for verification of satellite-to-ground APD-based (Avalanche Photodiode) FSO links subject to atmospheric turbulence-induced fading is proposed in the current paper. In particular, the self-developed hardware channel emulator represents an FSO channel by means of fiber-coupled Variable Optical Attenuator (VOA) controlled by driver board and software. Having addressed real atmospheric Radiosonde Observation (RAOB) databases for Vienna, Austria, highly precise optical attenuation data due to atmospheric turbulence fading are generated and applied into the considered software. The used approach relies on complex analysis simulating atmospheric vertical profile of refractive index structure parameter as well as Gamma- Gamma and Log-Normal scintillation models considering both parameters the telescope aperture and the elevation angle. Along with the FSO channel emulator, the receiver under-test is high-speed 10 Gbps APD photodetector with integrated Transimpedance Amplifier (TIA) that is typically installed in future OGSs (Optical Ground Stations) for LEO/GEO satellite communication. Having considered On-Off Keying (OOK) Intensity Modulation/Direct Detection architecture, the emulated optical downlink is evaluated based on two different data throughputs while atmospheric turbulence induced-scintillations are also taken into account. The overall testbed performance is addressed by a BER tester and a digital oscilloscope, providing high-quality BER graphs and eye diagrams that prove the applied approach for testing APD-TIA in the presence of scintillations. Furthermore, the accuracy of the hardware channel emulator is evaluated by means of calibration measurements as well as beam camera providing measured proof of the propagated high-quality laser beam.
Free Space Optical (FSO) systems offer tremendous channel capacity, which can significantly contribute to the bandwidthhungry next generation networks. FSO technology is certainly highly vulnerable to atmospheric Mie scattering, which leads to severe degradation of the established optical communication link. To address this key-issue, the current paper is focused on detailed investigation of the fog effect using artificially built fog environment. Low-visibility conditions are adjusted within a 50 m long corridor covered with PVC and including two artificial fog machines and a signal flare. The Particle Size Distributions (PSDs) of the simulated fog are measured with a sophisticated and so-called “Spraytec” device provided by Malvern Instruments Company. Once the main characteristics of the artificial fog are assessed, the measurements are compared with an empirical estimated fog model using modified gamma function. The comparison is accomplished in terms of theoretically defined PSDs where both radiation as well as advection fog modelling are taken into account. In order to calculate the relevant FSO channel attenuation only based on our measured fog PSDs, Mie theory is applied. For this purpose, Mie scattering efficiencies of a fog water sphere with arbitrary radius and refractive index are shown and examined. Respectively, apart from the presented figures with comparison of various PSDs, also the specific attenuation in dependence on fog particles size is introduced and discussed. Taking into account that particle density of the artificial fog can be manually setup in accordance with the applied theoretical models, our simulations offer attenuation up to 210 dB/km in the presence of continental moderate and dense fog effects. Consequently, we have the possibility to simulate significantly well various fog conditions in artificially simulated environment.
Optical Wireless Communication (OWC) systems rapidly increase their importance in very long-distance deep space communication scenarios. However, the high performance requirements of deep space OWC systems demand preliminary experiments which are unmanageable in real conditions. Regarding this issue, an innovative approach for testing deep space optical communication links in controlled laboratory environment is developed. The proposed testbed is based on fibre optics technology and combines various modules which represent a real deep space OWC link. Similar to already demonstrated deep space missions, the implemented optical receiver is Superconducting Nanowire Single- Photon Detector (SNSPD) characterized with single photon sensitivity and high detection efficiency. Consequently, in this paper an authentic deep space Poisson channel is emulated and examined. The given theoretical description of the Poisson process is supported by real SNSPD measurements in terms of high efficient single photon detection. The provided measured graphs clearly show the operation of SNSPD. In addition, a variable optical attenuator (VOA) is applied as a main device emulating the tropospheric part of a deep space optical Poisson channel characterized predominantly by Mie scattering (fog and clouds) and turbulence effects. This OWC channel emulator also contains self-developed software and attenuator control unit based on external Digital Analog Converter (DAC). Moreover, the response time parameter of channel emulator is examined in detail. Two different times in terms of reaching the lowest and the highest allowed attenuation are measured and shown. Finally, the developed channel emulator is tested and evaluated under real attenuation data. The experimental results show that the proposed method can evaluate various deep space optical scenarios.
Visible light communication (VLC) has been extensively studied for car-to-car (C2C) communication due to its inherent benefits. It is the idea of using light-emitting diodes for both illumination and data communications. The main motivations are longer lifetime of high-brightness light emitting diodes (LED) and growing popularity of the solid state of lighting sources compared to other sources of artificial light. These two features have made a whole range of developing applications such as C2C communication since the level of reliability and power efficiency offered by LED are excellent compared to the traditional incandescent light sources used for lightning. Car industry and automobile lighting market are more and more motivated also to use Laser diodes instead of LED because of higher intensity (Power). Fiber Laser and Glass Photonics could be the next generation components for carto-car VLC. This paper presents the main features of physical layer for VLC based on the IEEE 802.15.7 standard including useful Modulations, Forward Error Correction Coding for single light source also a comparison to wireless RF-Technology and different weather influences are considered. These aspects would also be of main interest for safety, availability and security for autonomous driving in the future applications
For the verification of Free Space Optics (FSO) systems it is common to determine optical power measured depending on illuminated area at a certain wavelength. In the context of this work a new measurement system was developed, which is able to measure not only the optical power but also the complete spectral distribution of the light beam. FSO is becoming more and more important, because of the high usable bandwidth (leading to high data-rates) in optics compared to radio frequency (RF).
The measurement system consists of a mechanical structure, where a collimator is mounted on. This collimator can be moved in two dimensions to enable the measurement of predefined points. It is connected with a spectrum analyzer using an optical fiber. A computer controls the position of the collimator and initiates the spectrum analyzer to record the spectral curves, the maximum peak of power, the 3dB bandwidth and the total power of spectrum. The obtained data covers a measurement area of 0.91 m by 0.77 m which can be surveyed at a high local resolution of 0.7 mm. Collimated beams in the range between 600 and 1750 nm are analyzed. The measurement results discussed in this contribution are shown on the example of light sources, used in at TU Graz developed FSO-systems.
KEYWORDS: Fiber optic gyroscopes, Signal attenuation, Data modeling, Free space optics, Visibility through fog, Visibility, Received signal strength, Optical engineering, Statistical analysis, Clouds
Recent measurement campaigns in Prague, Czech Republic have recorded the specific attenuation caused by fog in terrestrial free-space optical (FSO) links along with visibility, liquid water content (LWC), and integrated particle surface area for operational wavelengths of 1550 and 830 nm. Data recorded during 5 months of measurements has been analyzed in an attempt to validate and improve the empirical models for LWC and visibility-based attenuation and the probability density function (PDF) estimation of the received signal strength (RSS). The results strongly suggest that further attempts in refinement of the empirical modeling for visibility-based attenuation or LWC-based attenuation shall move towards the establishment of a global data bank of fog attenuation measurements in different climatic regions. This data bank can then help develop generic models which could lead to better system design of future terrestrial FSO links. The PDF estimation of RSS puts forth the Kumaraswamy distribution as the best fit for settled continental fog conditions.
The Satellite Laser Ranging (SLR) Station Graz is measuring routinely distances to satellites with a 2 kHz laser,
achieving an accuracy of 2-3 mm. Using this available equipment, we developed - and added as a byproduct - a kHz SLR
LIDAR for the Graz station: Photons of each transmitted laser pulse are backscattered from clouds, atmospheric layers,
aircraft vapor trails etc. An additional 10 cm diameter telescope - installed on our main telescope mount - and a Single-
Photon Counting Module (SPCM) detect these photons. Using an ISA-Bus based FPGA card - developed in Graz for the
kHz SLR operation - these detection times are stored with 100 ns resolution (15 m slots in distance). Event times of any
number of laser shots can be accumulated in up to 4096 counters (according to > 60 km distance).
The LIDAR distances are stored together with epoch time and telescope pointing information; any reflection point is
therefore determined with 3D coordinates, with 15 m resolution in distance, and with the angular precision of the laser
telescope pointing.
First test results to clouds in full daylight conditions - accumulating up to several 100 laser shots per measurement -
yielded high LIDAR data rates (> 100 points per second) and excellent detection of clouds (up to 10 km distance at the
moment). Our ultimate goal is to operate the LIDAR automatically and in parallel with the standard SLR measurements,
during day and night, collecting LIDAR data as a byproduct, and without any additional expenses.
Using our Satellite Laser Ranging (SLR) facility, our experience and our available equipment for Single Photon
detection, we installed a Single Photon Counting Module (SPCM) to measure the photon flux of variable stars, and of
stars with transiting exoplanets; these observations are intended as a complementary application to our standard SLR
activities, to contribute observations to already known - and also to candidate - variable stars and stars with transiting
exoplanets. While it is relatively easy to detect the large - in some cases up to 50% - variations of some stars, it is a
challenge to detect the transiting exoplanets with this method; the decrease in photon flux here is only in the order of a
few percent. In this paper, we present first results.
Free-space optics (FSO) has gained considerable importance in this decade of demand for high-bandwidth transmission capabilities. FSO can provide the last mile solution, but the availability and reliability issues concerned with it have received increasing attention and need thorough investigation. In this work, we present our results on fog attenuation measurement and prediction at wavelengths 650, 850, and 950 nm with peak values up to 500 dB/km. For the attenuation measurement, optical wavelengths are transmitted over the same path of fog in free air to a receiver, measuring the power at every wavelength. The measurement of fog attenuation was performed at the France Telecom R&D test facility at La Turbie (in the south of France). We compare our measurement data with the commonly used light attenuation models (Kruse and Kim models) and with a new proposed model allowing the prediction of fog attenuation for the 0.69- to 1.55-µm spectral band. We present some interesting insights and discuss the wavelength dependence. The practical measurements described promise to validate the models and therefore should lead to more accurate availability prediction for FSO links.
KEYWORDS: Fiber optic gyroscopes, Signal attenuation, Free space optics, Visibility through fog, Visibility, Particles, Data modeling, Modulation, Light scattering, Aerosols
Terrestrial free space optical (FSO) links are based on the simple concept of a light beam carrying information, thus facilitating very high data rates. Fog remains the major hurdle in increasing the availability and reliability of terrestrial FSO links, as fog particles scatter the propagating light, causing nonnegligible attenuation. We present measurement results from our campaigns carried out at the continental city of Graz and at La Turbie near Nice, the southern coast of France. We perform a detailed analysis of the measurement results providing time-series analysis of these fog measurements and a comparison between maritime and continental fogs. Based on our measurement analysis, we provide insight into designing efficient FSO systems, with better performance and enhanced resilience.
Free Space Optics (FSO) has gained considerable importance in this decade of demand for high bandwidth transmission capabilities. FSO can provide the last mile solution, but the availability and reliability issues concerned with it can not be ignored, and requires thorough investigations. In this work, we present our results about light attenuation at 950 and 850 nm wavelengths in continental city fog conditions with peak values up to 130 dB/km and compare them with attenuation under dense maritime conditions with peak values up to 480 dB/km. Dense fog is the most severe limiting factor in terrestrial optical wireless applications and light propagation in fog has properties in the spatial, spectral and the time domain, which are of importance to free-space optic data communication. In 2004 (within a short term scientific mission of COST 270) measurements of very dense maritime fog and low clouds were made in the mountains of La Turbie, close to the coast of southern France. Using the same equipment, the measurements were continued for the conditions of the continental city of Graz, Austria. This campaign was done in the winter months from 2004 to 2005 and 2005 to 2006 and allows us to compare fog properties for different environments, and the impact of snow fall. We provide detail analysis of a fog and a snow event for better understanding of their attenuation behavior.
Free Space Optics (FSO) has gained considerable importance in this decade of demand for high bandwidth transmission capabilities. FSO can provide the last mile solution, but the availability and reliability issues concerned with it have acquired more attention, and a need for thorough investigations. In this work, we present our results about fog attenuation at the 950 and 850 nm wavelengths in heavy maritime fog with peak values up to 500 dB/km. For the attenuation measurement, optical wavelengths are transmitted over the same path of fog in free air to a receiver, measuring the power of every wavelength. The RF marker technology employed takes advantage of modulating every optical wavelength with an individual carrier frequency, allowing to use one optical front end for the receiver and to separate individual wavelengths by electrical signal filters. The measurement of fog attenuation at different wavelengths was performed at the France Telecom R & D test facility at La Turbie. Maritime or advection fog, which caused the light attenuation consists of water droplets of larger diameter in the order of 20 μm and can cause visibilities as low as 30 meters. The visibility was measured using a transmissiometer at 550 nm. We compare our measurement data with the commonly used light attenuation models of Kruse and Kim, and present some interesting insights. The practical measurements described try to validate the models and therefore should lead to a more accurate availability prediction for FSO links.
In this paper Free Space Optics (FSO) in combination with Wireless LAN and Satellite Communications in Civil-Military-Cooperation (CIMIC) is presented. At first a modular communication system developed at the TU Graz is shown, which allows worldwide access to the Internet or other networks by combining Satellite Communications, FSO and Wireless LAN. Wireless LAN offers connectivity to mobile users in a network cell, Free Space Optics allows quick installation of broadband fixed wireless links instead of cables and Satellite Communications provides a backbone between distant locations in the world.
In the second part results of Free Space Optics- and Satellite applications installed at a civil-military exercise in Spring 2004 in Styria (southern part of Austria) are presented. In this civil-military cooperation a mobile Satellite Earth Station (equipped with FSO and Wireless LAN) was used for Videoconferencing between military and civil organisations.
Free Space Optical (FSO) links offer high bandwidth and the flexibility of wireless communication links. However, the availability of FSO links is limited by weather patterns like fog and heavy snowfall. Microwave based communication links operating at high frequencies (40 - 43 GHz) have similar characteristics like high data rates and needed line-of-sight. Link availability for microwave systems is limited by heavy rain. Combining FSO links with microwave links within a hybrid FSO/microwave communication network has the advantage of added redundancy and higher link availability. Measurements over a period of one year show a combined availability of 99.93% for the climatic region of Graz (Austria) which proves that the combination of both technologies leads to a highly available wireless connection offering high bandwidth.
KEYWORDS: Free space optics, Data storage, Video, Signal attenuation, Visibility, Internet, Visibility through fog, Atmospheric optics, Fiber optic gyroscopes, Receivers
The satisfaction of all communication needs from single households and business companies over a single access infrastructure is probably the most challenging topic in communications technology today. But even though the so-called "Last Mile Access Bottleneck" is well known since more than ten years and many distribution technologies have been tried out, the optimal solution has not yet been found and paying commercial access networks offering all service classes are still rare today. Conventional services like telephone, radio and TV, as well as new and emerging services like email, web browsing, online-gaming, video conferences, business data transfer or external data storage can all be transmitted over the well known and cost effective Ethernet networking protocol standard. Key requirements for the deployment technology driven by the different services are high data rates to the single customer, security, moderate deployment costs and good scalability to number and density of users, quick and flexible deployment without legal impediments and high availability, referring to the properties of optical and wireless communication. We demonstrate all elements of an Ethernet Access Network based on Free Space Optic distribution technology. Main physical parts are Central Office, Distribution Network and Customer Equipment. Transmission of different services, as well as configuration, service upgrades and remote control of the network are handled by networking features over one FSO connection. All parts of the network are proven, the latest commercially available technology. The set up is flexible and can be adapted to any more specific need if required.
The impact of nonlinear optical effects, the optimization of the dispersion, the bandwidth of the filters and the optical signal powers play a major role in an optical network and even more the higher the data rates are.
This work deals with the simulation of dispersion in order to determine its impact on the performance of high-capacity WDM-transmission systems. By consideration of nonlinear optical effects and suitable dispersion management, it is shown that the system performance can partly be improved. A 10 Gbps or 40 Gbps external modulated laser signal is transmitted through a standard single mode fiber (SSMF) followed by a dispersion compensation fiber (DCF) (postcompensation). Due to cross-phase modulation, four-wave mixing and self-phase modulation crosstalk which influences the optimum length of the DCF can be detected. The filter bandwidth and length of the DCF have been optimized for various signal powers and two different data-rates.
It turned out that the influence of different non-linear effects on the system performance can be partly reduced by optimized dispersion management (undercompensation). It is shown that the optimum length of the DCF is independent of the signal bandwidth. The simulation reasons the maximum launched power per channel and the optimum filter bandwidth for 40 Gbps transmission systems. Real measurements on optical components and networks agree with our simulation results.
Free Space Optics (FSO) is an excellent supplement to conventional radio links and fiber optics. It is the broadband wireless solution for closing the "Last Mile" connectivity gap throughout metropolitan networks. FSO is useful in dense urban and urban applications. The realiabilty and availability of the FSO-link is mainly determined by the local atmospheric condition. In this paper the results of the investigations of the research group "OptiKon" on different installed common network-architectures (ring, mesh and star) are presented. An "Optical Repeater" was used, if there was no line of sight between transmitter and receiver. The usage of optical free space propagation wthi Light Emitting Diodes are source instead of conventionally broadband transmission systems like optical fibers or radio links was also investigated at the Department of Communications and Wave Propagation. Using extended light sources like LEDs and/or multiple transmitter optics due to new laser safety regulations allows multiple output power within the same laser class, increasing the power link budget especially for short range FSO systems. In a first step two families of cost-effective systems were developed and realized. One is based on a modular concept using available standard components, allowing demonstrates at 2×10 Mbps data rae. Another is used for the larger distnaces of about 300 m at a specific power margin of 25 dB/km. Systems for higher data rate are under development. Additionally some ideas and their possible realization for point-to-multipoint configuration are considered. In the last chapter a short overivew about the main results of the work of "OptiKom" is discussed.
This paper describes a novel and efficient method for parameter extraction and characterization of Erbium-doped fiber amplifiers (EDFA). In DWDM systems gain and noise behavior of EDFAs depend on the number and distribution of transmission channels. Hence, characterization of EDFAs for reliability evaluations requires a costly measurement setup of up to 80 or even more wavelength selected laser sources. Our novel method uses photonic transmission simulation to drastically reduce the measuring efforts. Using only a few characteristic measurements with one tunable laser, the gain and noise behavior of amplifiers can be simulated for any number and distribution of transmission channels in DWDM systems. The simulation of the photonic transmission is based on the commercial simulation package WDMTransmissionMaker by VPI systems. We utilize black-box models for fiber amplifiers which can take into account all linear optical effects like e.g. gain-flattening filters or dynamic gain equalizers. The predictions of the simulations for different single-stage as well as double-stage amplifiers comply with the experiments within the measurement accuracies and help to understand new up-coming optical amplifier technologies and to ensure more reliable optical system designs. The measuring effort for qualification and reliability evaluations can be significantly reduced by using the novel characterization method.
The coherent wave propagation is affected by the atmosphere in many ways. Several theoretical models for propagation of light through the atmosphere are well known. To predict link availability in different climate zones it is necessary to do field tests for data acquisition. Therefore we have done reliability- and availability-tests on commercial available and also on self-developed optical point-to-point and point-to-multipoint systems. We sent test data at 155 Mbps (STM-1) from one FSO-unit to a distant (2.7 km) FSO-unit. The received data were sent back (loop) to the first unit. Our primary interest in this long-time investigation was the time of link failure, because it turned out that BERs be low in general, less than 10-8 at very bad weather conditions in winter and less than 10-12 at clear sky. In a second measurement campaign we investigated the influence of turbulences in the air. The measurements clearly show variations in the fluctuation of the incoming optical power during a day. In principle there are two periods with strong variations, during the day and during the night, and two periods of rather stable air, these are around sunset and sunrise. The power variations have the highest amplitude and show the fastest changes at noon and they are less distinct and show slower changes in the night. As a medium value we got power variations of 4 dB over the distance of 2.7 km in summer. The duration of fades/scintillations was in the order of 4 to 60 milliseconds at daytime and about 10 to 150 ms in the night.
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