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Article

Visible Light Communication System Based on Software Defined Radio: Performance Study of Intelligent Transportation and Indoor Applications

Department of Cybernetics and Biomedical Engineering, Faculty of Electrical Engineering and Computer Science, VSB–Technical University of Ostrava, 17. listopadu 15, 708 33 Ostrava, Czech Republic
*
Authors to whom correspondence should be addressed.
These authors contributed equally to this work.
Electronics 2019, 8(4), 433; https://doi.org/10.3390/electronics8040433
Submission received: 28 February 2019 / Revised: 31 March 2019 / Accepted: 10 April 2019 / Published: 15 April 2019
(This article belongs to the Special Issue Visible Light Communication and Positioning)

Abstract

:
In this paper, our first attempt at visible light communication system, based on software defined radio (SDR) and implemented in LabVIEW is introduced. This paper mainly focuses on two most commonly used types of LED lights, ceiling lights and LED car lamps/tail-lights. The primary focus of this study is to determine the basic parameters of real implementation of visible light communication (VLC) system, such as transmit speed, communication errors (bit-error ratio, error vector magnitude, energy per bit to noise power spectral density ratio) and highest reachable distance. This work focuses on testing various multistate quadrature amplitude modulation (M-QAM). We have used Skoda Octavia III tail-light and Phillips indoor ceiling light as transmitters and SI PIN Thorlabs photodetector as receiver. Testing method for each light was different. When testing ceiling light, we have focused on reachable distance for each M-QAM variant. On the other side, Octavia tail-light was tested in variable nature conditions (such as thermal turbulence, rain, fog) simulated in special testing box. This work will present our solution, measured parameters and possible weak spots, which will be adjusted in the future.

1. Introduction

In recent years, visible light communication (VLC) surfaced as an alternative to classical radio frequency (RF) technology [1,2,3]. Current communication bands often lack free channels, which is notable particularly in Wi-Fi or in industrial, scientific and medical bands. VLC is an optical wireless standard which operates from 380 to 780 nm, using a visible light source as a signal transmitter, free space environment as transmission medium and the appropriate photodiode/photodetector as a receiver. VLC seems to be capable technology for short-range or possibly in the future even long-range communications. Future appliances vary greatly, spanning from vehicle-to-vehicle [4,5,6,7,8,9] communications, infrastructure-to-vehicle communications or simply as an alternative to typical local area networks (LAN) [10,11].
A number of papers focused on multiple VLC technologies [12]. Light-fidelity (Li-Fi) [13,14,15,16,17,18,19,20] is slowly surfacing as commercially available alternative to Wi-Fi [21]. Orthogonal frequency division multiplexing in car-to-car was tested in real-world driving scenarios by Shen et al. [22].
VLC on software defined radio (SDR) [23,24] is evolving quickly. In 2011, a 1 Mbps video stream was achievable over 3 meters, when deployed on custom LED matrixes [25]. In 2015, Hussain et al. tested the implementation of IEEE 802.15.7, they achieved results according to this standard, however transmission distance was limited to 1 m [26]. Nowadays, we are testing longer distances and mainly higher data rates, even on commercial light sources.
Rapid expansion of LED is crucial for this technology, as it offers multiple advantages such as long lifespan, low power consumption, high tolerance to humidity, high efficiency, and fast switching. However the main advantage of VLC based on LED is the use of the visible spectrum (380–780 nm). For this reason LED can perform communication functionality while maintaining the original function as illumination lighting. In this paper, we used commercially available and currently used light sources. For this purpose, a Skoda Octavia III tail-light without any modifications was chosen. To test indoor deployment, we have also used Phillips Fortimo DLM 300 44 W/840 Gen3 [27]. Avalanche photodiodes (APD) and positive-intrinsic-negative (PIN) detectors are commonly used as receivers. We used Thorlabs PDA36A-EC PIN [28] photodetector with 13 mm 2 of active area as receiver, since it was the most suitable candidate from available portfolio.
Our work is aimed at implementation of a vehicle-to-everything (V2X) system with highly modular design [29,30,31]. For this reason, we have developed a system, based on SDR. Each individual component can be swiftly exchanged, without any necessary adjustments to original code. Concept of V2X is based on the passing of information from a vehicle to any appropriate entity and vice versa. It is also often divided into different subsections, such as vehicle-to-infrastructure (V2I) [32,33], vehicle-to-network (V2N) [34,35], vehicle-to-vehicle (V2V) [36,37], vehicle-to-pedestrian (V2P) [35,38], vehicle-to-device (V2D) [39,40] and vehicle-to-grid (V2G) [41,42], vehicle-to-home (V2H) [43,44]. To test these concepts, we have also built our own testing polygon named BroadBAND light. As Skoda cars are the most widespread vehicles in the Czech Republic, we have picked Skoda Octavia III tail-light as the transmitter in V2X scenarios. So far, the partnership with manufacturers of these lights have yielded results, as we have received multiple samples of planned or already available products for testing. Philips Fortimo DLM300 is the most deployed LED indoor ceiling light in Czech Republic, so we used it in indoor experiments. Most Czech public institutions deploy exactly this type–testing it is the most logical step, as we can use every ceiling light at our university as transmitters.
Figure 1 describes different ways of V2X communication [30,45,46], mentioned earlier. V2V is a system, which enables car to communicate with each other. Its main goal is to reduce vehicle collisions and crashes. It will be a backbone of multiple levels of autonomy, delivering assisted driver services like collision warnings [32,47,48]. One key issue with V2V is that to be most effective, it should reside in all cars on the road. However, this technology has to start somewhere, so car manufacturers are slowly introducing their solutions. V2D is a system, that links cars to many external receiving devices and will be particularly useful to bikers. Vehicles can communicate with V2D device on cycle to alert rider to potential danger or to avoid accidents [39,40,49]. V2P is a system which should be particularly useful to elderly persons, school kids and physically challenged persons. V2P maintains a link between pedestrian’s smart devices and vehicles to act as an advisory to avoid collisions [50,51]. V2H communications involve a link between a vehicle and the owner’s home, sharing the task of providing energy [52,53]. During power outages, a vehicles battery can be used as a critical power source. V2G is a system which can communicate with the power grid to adjust the vehicle’s charging rate [54,55]. It will be an element in some electric vehicles and is used as a power grid modulator to dynamically adjust to the energy demand [56].
Figure 2 describes proposed different ways of indoor visible light communication (VLC) communication. Smart lighting inside smart buildings provides the infrastructure for illumination, control and communications and will greatly reduce energy consumption within a building. Smart appliances, meters or factory applications, especially in dangerous conditions are all possible target devices. Direct connection between mobile devices might be possible as well, since modern smartphones have illumination LEDs which might be used as transmitters and cameras, which could work as receivers. There are advantages of using VLC in hospitals and healthcare [57,58,59,60]. RF technologies are mostly undesirable in certain parts of hospitals, especially around MRI scanners and in operating theatres. VLC deployment in aviation is also desirable. Radio is undesirable in passenger compartments of aircrafts. Modern aircrafts already use LEDs for illumination, so VLC might replace wiring to passenger seats. This might reduce aircraft construction costs and weight [61,62].
Factory applications are especially interesting. There are multiple benefits to machine to machine VLC solutions (machine-to-machine communication - M2M [20,63,64,65,66]). Smart factories could be built upon enhanced industrial instrumentation, such as advanced sensors or meters. VLC can be also used to coordinate the movement and timing of robots in manufacturing settings, such as automobile factories. It can provide location-based communications to automated guided carts and “smart cart” robots or provide drone-to-station communications for precise, interference-free movement, drop zones and landing sites [67,68].
Vehicular visible light communication (V-VLC) [46,69,70,71,72,73] is often described as supplementary or “sister” technology to planned 5G [31]. There is also a concept of social internet of vehicles (SIOV) [74,75,76], which is based on LTE/4G network, consisted of multiple road side units (RSU) based on eNodeB base stations and on-board units (OBU) with LTE/4G capabilities. SIOV consists of multiple entities, which are treated as nodes connected to each other via links. However this concept can be further expanded by VLC implementation. Daytime running lamps (DRL) are often mandatory in European countries and optional VLC capabilities would possibly save energy needed to maintain continual 4G/5G connection [77,78].
Multiple teams implemented VLC using SDR and LabVIEW, with different success. A turkish team successfully carried out a number of experiments, using simpler on-off keying (OOK) and variable pulse position modulation (VPPM) modulations [79]. Another team from Chile managed to implement their own system using similar hardware [7]. However, there are two main concerns. Both teams do not mention their maximal reached transmit speed and the used photodetector (PDA36A) is certainly a limiting factor, as we have run a number of tests on it as well. According to manufacturer’s datasheet, increasing gain of its trans-impedance amplifier significantly limits useable bandwidth. According to the state of art study, universal software radio peripherals(USRPs) are more than capable of being used in VLC experiments [80]. They also mention the necessary adjustments and possible limitations of lower end (USRP 292X) models. That’s why we switched to much more powerful and newer models which will be used in future experiments [7,79,80,81,82].
As mentioned before, the described system is our team’s first attempt at SDR VLC quadrature amplitude modulation(QAM) system. Different teams have already delved into different problematics, such as adaptive modulation schemes [83]. Multiple input multiple output design described by Deng et al. 2017 [84] is already implementing higher state QAM modulation schemes capable of adaptive switching. Designing similar systems based on orthogonal frequency division multiplexing (OFDM) will be a topic of imminent research, as we are already switching to more capable hardware components [85,86]. Khalid et al. investigated the implementation of a VLC system based on DAQ hardware [87]. This system is however very limited performance-wise. The second iteration of our prototype will be also based on LabVIEW, but we are focusing on field programmable gate array (FPGA) implementation, as it will increase performance dramatically.
There are multiple advantages to practical implementation of VLC. Each of presented solution has its own use and advantages. When approaching the problems of V2V communication, the natural conditions are major concerning factor, as they significantly vary throughout the year. Carrying out a number of experiments in this area is a logical first step in implementation of channel equalization, as we estimate it will significantly improve transmit speeds or reachable distance. Also we tested our modular platform in previously mentioned conditions, as it will become a basic platform, which will be modified and improved in the future. Currently, we are exploring outdoor car lamps, tail-lights, and indoor ceiling lights, as these light sources that are the most perspective. In the future we will also include street lamps, as V2I and V2V outdoor experiments will be carried out in previously mentioned testing polygon, which is already running on LEDs, so every lamp is prepared for VLC.
Tsiropoulou et al. [88] have investigated problematics of non-orthogonal multiple acces (NOMA) vs. orthogonal frequency division multiple access (OFDMA) approach [89,90,91]. According to her, NOMA offers us multiple advantages, such as considerable interference mitigation or simultaneous bandwidth utilization. Also due to the absence of resource block per user, NOMA can sufficiently accommodate more users than OFDMA. Modern mobile networks based on LTE use the OFDMA approach, as it is a basis of LTE standardization. Car manufacturers are currently enrolling LTE modules into vehicles and are preparing for 5G transfer. Currently, 5G is surfacing technology, which was deployed in only a limited number of countries. However 5G is based on NOMA, so its implementation in VLC is necessary if both technologies should coexist or work in conjunction. Lin et al. also tested hybrid NOMA/OFDMA approach with partial success [92].
Tsiropoulou et al. [93] propose a concept of visible light communication local area networks (VLC-LANs), where users are served by optical access points (OAPs). In this scenario, VLC-LANs [94] are presented as alternative to macrocell area coverage. Two-tier VLC topology is considered, mostly for indoor and outdoor coverage. The system is based on OFDMA, basically to be ready for LTE incorporation. Each user communicates directly with a single OAP via communication link. OAPs total bandwidth is divided into subcarriers, which are organized in resource block (RB). Each RB is occupied exclusively by one user. This concept could be easily adapted for 5G by introduction of NOMA, as discussed earlier.

2. Experimental Setup

Experimental setup is based upon application created in LabVIEW, which was used for input/output signal processing and measurement. Application output was fed into NI USRP-2921 [95], which stands for transmitting element. Signal was then amplified by a 1.6 W amplifier, effectively working from 1 to 200 MHz. The amplified signal went through bias tee into the transmitting light source, which can be exchanged at will. A photodetector was located at a variable distance from the transmitting element. It was also possible to insert special measuring box, used for simulation of multiple nature conditions, such as fog, rain or thermal turbulence. Received signal was fed into NI USRP-2921 whose output is connected to the same computer running LabVIEW application. Signal was then evaluated, and parameters were displayed accordingly. This whole setup was designed with the highest possible modularity in mind. We wanted to switch each component at will and observe their direct impact on whole prototype.
We had to swap NI USRP-2921 transmitting and receiving boards with Ettus LFRX/LFTX Daughterboards, which were operating at 0-30 MHz. This band was approximately what we had in mind when designing whole prototype, as USRP capabilities were one of the biggest limiting factors. Original boards from 2921 were designed for 2.4–2.5 GHz and 4.9–5.9 GHz, which was completely unsuitable for our needs. We had also adjusted connectors on the Octavia tail-light, as they were designed for car engine control unit. To further improve RSL when transmitting using tail-light, we had mounted a planoconvex lens on a photodetector to focus received light into the converging beam with lens focus at the active area of photodiode. However, since we measured RSL at variable receiving angle when using stationary ceiling light as source, it was undesirable to use lens in this different scenario. We have chosen ZX85-12G+ bias tee [96], which operates from 0.2 MHz to 12 GHz, its maximal current is 0.4 A and maximal input voltage is 25 V. There are multiple parameters, that can be configured in LabVIEW application, such as:
  • Carrier frequency: max 30 MHz
  • Bandwidth
  • Sample width
  • Number of states: max 4096-QAM
  • Message symbols
  • Used TX filter
  • TX gain
  • RX gain
  • TX device IP address
  • RX device IP address
Tests wre carried out using static modulation formats. Long term measurements were essential to specify threshold for successful modulation switching in adaptive modulation. We were aiming for a similar system, which is used in case of microwave point-to-point links, where both units are capable of quickly changing modulation scheme according to natural conditions and measured parameters. Sacrificing part of the transmission speed in favor of link robustness is the main concept of this system.

Evaluation Parameters

Received signal level (RSL), which signalize signal strength received at second, or receiver, USRP. It is the sum of all losses and gains on the receiver input.
Our LabVIEW application use channel coding with hard decision forward error correction (FEC) threshold of 3.8 × 10 3 . Data with bit-error ratio (BER) below this threshold can be repaired by FEC codes. This threshold was appropriate for our M-QAM modulation. LabVIEW Modulation Tookit [97] also includes multiple different types of channel coding [98]. The influence of these techniques on transmission quality will be a topic of further research. As FEC was not the main topic of this paper, we used predetermined threshold and functions already present in LabVIEW libraries. Problematics of FEC in QAM VLC was investigated by team in Edinburg [99].
Modulation error ratio (MER) [100] is defined as a relationship between error vector magnitude (EVM) and signal-to-noise ratio (SNR). It was used to quantify the performance of transmitter/receiver in the system, which used digital modulations (in this case QAM). It is influenced by various imperfections in the implementation (such as noise, phase noise, distortion, right focusing) and characteristics of signal path which cause the actual constellation point to deviate from ideal locations.
EVM [101] is a measurement of demodulator performance in the presence of impairments (Figure 3, where v is the ideal symbol vector, w is the measured symbol vector, w v is the magnitude error, Φ is the phase error, and e = w v is the error vector). The soft symbol decisions obtained after decimating the recovered waveform at the demodulator output were compared against ideal symbol locations. The root mean square error vector magnitude and phase error were then used in determining the EVM measurement over a window of N demodulated symbols. EVM was related to the modulation error ratio. There is one-to-one relationship between EVM and MER.
Energy per bit to noise power spectral density ratio (E b /N 0 ) was an important parameter in digital communications. It is a normalized SNR measure, also known as SNR per bit. It is useful when comparing BER performance of different digital modulation schemes without taking bandwidth into account. To calculate this value, SNR must be periodically obtained at receiver USRP. E b /N 0 was calculated at the receiver from the estimation of the SNR, the relationship between them is the following:
E b N 0 | dB = S N R | dB + 10 l o g 10 ( n ) 10 l o g 10 ( s p s ) ,
where n is the amount of information bits per symbol. Both modulation order and the code rate (in case that channel coding is employed) have an influence on this value. E b /N 0 measurement on USRP is further expanded in paper by Alonso et al. [102].

3. A Feasibility Study on Indoor Visible Light Communication

Measurements using ceiling light were carried out under laboratory conditions (calm wind, 24 C). Figure 4 describes tested setup. Our tested light source is capable to cover a conical area with radius of approximately 350 cm, as is described on Figure 5. We began our measurements at a right center of this covered area, directly under light source. Then, we periodically repeated measurements but moved to the edge of covered area with a step of 25 cm. The distance between receiver and transmitter was 202 cm.
The following configuration was used in this scenario:
  • Carrier frequency: 3 MHz
  • Bandwidth: 1–4 MHz
  • Modulation type: M-QAM
  • TX/RX gain: 0 dB
  • Message symbols: 10,000
  • Tx filter: root raised cosine
  • Sample width: 16-bit
  • Receiver-transmitter distance: 202 cm
  • Measured distance: 0–350 cm (step of 25 cm)
  • Photodetector without planoconvex lens → more suitable for this scenario
  • Measured parameters: E b /N 0 , BER, EVM and MER
In Table 1 you can see parameters of light of Fortimo LED DLM 3000 44 W/840 Gen3 and in Table 2 you can see chosen parameters of photodetector PDA36A-EC.
Before proceeding with the main part, we measured attenuation characteristics of our prototype by using the vector network analyzer. Figure 6 represents measured data. It is visible that attenuation quickly increased with longer distances. Even the sample with the best conditions (directly under light source) showed an increase in attenuation by 47 dB relative to the reference of 0 dB. By increasing distance to 3 m, attenuation reached 68 dB, which negatively impacted prototype capabilities, mainly the constellation decoding. We have chosen carrier frequency of 3 MHz, so that we can increase bandwidth up to 4 MHz without getting into sub 1 MHz band. However, increasing bandwidth also increases the difference in attenuation between highest and lowest frequency. This fact negatively impacted constellation decoding as well. The resulting theoretical transmit speed was influenced by many factors, such as modulation scheme, used bandwidth and mainly by the distance of photodetector from center of measurements, which affected attenuation. We were able to reach 2 Mbps at 325 cm, by using 4-QAM with bandwidth of 1 MHz. The highest achieved transmit speed was 20 Mbps (32-QAM, 4 MHz), which could be maintained up to 90 cm from the center. Figure 7 represent possible maximal reachable transmission speeds for different M-QAM and bandwidths. Further implementation of adaptive modulation seems like a good way to further push this prototype forward. By defining strict rules for modulation switching, we could seamlessly maintain the highest possible transmit speed while having reliable connection. For our testing, we have used BER = 10 5 as a threshold value.
The valubble in Figure 7 are theoretically achievable transmit speeds. They were calculated in LabVIEW software, but a number of measurements were carried out to verify them. Effective transmit speed varied a bit (by approximately hundreds of kbps), because it was practically impossible to design an ideal channel. However deviations were so small, it was possible to neglect them.
Figure 8 represents a constellation diagrams of 4-QAM modulation measured at different distances and channel widths. It is noticeable that constellation points of the 4 MHz channel width measurements were more spread from their ideal position. These diagrams did not exceed the BER threshold mentioned earlier, but implementation of higher state modulation at limiting distance would result in rapid increase of BER and might even end in complete link degradation.
Figure 9 describes BER values of multiple channel widths and M-QAM modulation combinations. The graph itself also shows highest possible communication distance for measured modulation, which did not exceed BER threshold. The red line represents the FEC limit, so values exceeding it are beyond capabilities of fast error correction algorithms. Values located next to the arrows are BER.
Figure 10 and Figure 11 represent a comparison of 1 MHz and 4 MHz channel widths, the highest and lowest measured variants. It is visible that E b /N 0 values slowly decreased with increasing measured distance. In comparison, EVM values shows opposite trend. Wider channels were also much more limited in maximal reachable operation distance, which is also visible on Figure 7 as well. Simpler modulation schemes in combination with narrow channel are much more robust, which is visible on Figure 9.

4. A Feasibility Study on Outdoor Visible Light Communication: Car Tail-Light

Measurements using car tail-light were carried out in multiple meteorological conditions. We approached this problem differently, as in real-life scenarios, meteorological conditions tend to often vary. These conditions were simulated in a plastic box made of plexiglass with dimensions of 50 × 50 × 500 cm. Maximal measured distance in this scenario was 550 cm, which was effective threshold for functional communication. The first step was to measure the empty box as reference values for future comparisons. After that, three scenarios were simulated: fog, thermal turbulence and rain. These scenarios will be discussed further in this paper.
Figure 12 describes the tested setup, modified for Octavia tail-light. The whole experimental setup was very similar to the one used in ceiling light measurements. However, to carry out different scenarios the simulation box was inserted between transmitting light and receiving photodetector. Also using plano-convex lens was suitable for reaching higher RSL values and thus better transmit speed.
The following configuration was used in this scenario:
  • Carrier frequency: 3 MHz
  • Bandwidth: 1–4 MHz
  • Modulation type: M-QAM
  • TX/RX gain: 0 dB
  • Message symbols: 10,000
  • Tx filter: root raised cosine
  • Sample width: 16-bit
  • Receiver-transmitter distance: 550 cm
  • Measured distance: 0–350 cm (step of 25 cm)
  • Photodetector with planoconvex lens → more suitable for this scenario
  • Measured parameters: E b /N 0 , BER, EVM, MER
Table 3 shows parameters of LED - LA G6SP. A matrix of these LEDs is used in Octavia tail-lights.
Each measurement consisted of attenuation characteristics, which were measured by a vector network analyzer. By comparing every scenario, it was visible that fog had the highest impact, followed by rain and thermal turbulence, as seen on Figure 13. Also, we have included a reference power level of laser needed for functional 4-QAM transmission in the fog scenario.
Following measurements should cover most situations, which might happen in infrastructure-to-vehicle (I2V), V2V, V2I, V2N, V2P, V2D, V2G and V2H scenarios.

4.1. Scenario 1-Empty Box

As mentioned earlier, these measurements were used as reference values for further comparisons. To ensure conformity of measured data, these conditions were set as referential: 24 C, direct visibility, windless. Setup can be seen in Figure 14.
Comparison of BER values with different bandwidths can be seen on Figure 15. It is noticeable that up to 64-QAM, BER values tended to stay below 10 5 threshold set earlier. On the contrary, 128-QAM and higher modulations suffered from much higher BER values. Bit error ratio of 256-QAM was even below 10 2 in every bandwidth combination. These values were too high for FEC and communication is impossible in these conditions. Figure 16 and Figure 17 describe E b /N 0 and EVM values for every M-QAM and bandwidth combination. It is noticeable that starting from 256-QAM modulation, the difference between each bandwidth tended to increase rapidly.

4.2. Scenario 2-Thermal Turbulence

Measurements with thermal turbulence were carried out with modified box. The bottom part was removed, and multiple hot-air blowers were mounted instead. The top part of box was perforated to ensure sufficient air flow. Each blower heated the air to 50 C. Heated air then steadily flowed through box and slowly cooled to 44 C, which were measured directly at perforations. The horizontal airflow was 0.3 m/s and vertical was 2.5 m/s. Whole measurement was carried out multiple times until temperature inside box stabilized. Setup can be seen in Figure 18.
Comparison of BER values with different bandwidths can be seen in Figure 19. It is noticeable that up to 32-QAM, BER values tended to stay below 10 5 . On the contrary, 64-QAM and higher modulations suffered from much higher BER. Figure 20 and Figure 21 describe E b /N 0 and EVM values for every M-QAM and bandwidth combination. By comparing these values to the reference, we can notice a slight decrease of E b /N 0 and increase of EVM values. The most significant changes began at 128-QAM and progressed further. Communication ceased to work, so 2048-QAM was not measurable.

4.3. Scenario 3-Rain 42 L/min

The first part of measurements with rain were carried out in modified box as well. In this scenario, we have removed the top part of the box and exchanged it with three water nozzles. The box was equipped with compressor which pumped water from the bottom of the box back into nozzles. The transmitter and receiver were located outside the box, which was opened from both sides. In this scenario, the water flow was set to 42 L/min. Setup can be seen on Figure 22. Figure 23 shows a photo of this setup.
Measurements were carried out in a room at 22–25 C. Water temperature was stabilized at 22–25 C before each measurement. Both transmitter and receiver were located 25 cm from open side of the box. This way, it was impossible for them to get fogged up. To investigate the influence of walls or partitions a series of tests without a box and in a completely dark room were carried out before. The box had minimal influence, as its construction was adjusted to prevent it. Transmitting light was precisely focused into the box to avoid interference, which could be caused by possible reflections. Incoming light was also focused into photodetector by planoconvex lens, as mentioned earlier. Box construction was spacious enough to avoid unnecessary reflections on running water. However, the influence of water particles on detector/transmitter itself will definitely be a topic of further research.
Comparison of BER values with different bandwidths can be seen on Figure 24. This time, up to 8-QAM, BER stayed below 10e 5 . On the contrary, 16-QAM and higher modulations suffer from much higher BER.
E b /N 0 and EVM values are displayed on Figure 25 and Figure 26. By comparing these values to reference setup, there was a significant drop in signal quality. For example, in case of 4-QAM modulation and 1 MHz bandwidth, SNR was nearly 10 dB lower than the reference. Significant decrease in signal quality was observed, which also led to lower maximal reachable modulation/bandwidth combination, which was 128-QAM/1 MHz.
This setup was also influenced by the drops of water on the sides of the box. Mainly the “separation wall” between box sections caused concerns. To analyze this concerning issue, we have carried out several measurements with different box setups, which can be seen on Figure 27. The first curve corresponds to the empty box, second one to the box with rain but without partition and the last one was the original measured setup. By comparing these values, there is a noticeable 3 dB increase in attenuation between second and third curve.

4.4. Scenario 4 -Rain 22 L/min

The second part of measurements with rain were carried out in the modified setup from scenario 3. The main difference was a different water flow of 22 L/min. Setup can be seen on Figure 28.
Comparison of BER values with different bandwidths can be seen on Figure 29. This time, up to 16-QAM, BER stayed below 10e 5 . On the contrary, 32-QAM and higher modulations suffer from much higher BER.
E b /N 0 and EVM values (Figure 30 and Figure 31) tended to follow the trend from previous scenario. This time, in case of 4-QAM modulation and 1 MHz bandwidth, SNR is nearly 7 dB lower than the reference scenario 1. Significant decrease in signal quality was observed, which also led to lower maximal reachable modulation/bandwidth combination, which was 256-QAM/1 MHz.
Scenario 4 was also influenced by water drops. By carrying out the same test as in scenario 3, we have measured a 4 dB difference in attenuation, which was caused by “partition bar”’. Measured values are displayed on Figure 32.

4.5. Scenario 5-Fog

The last scenario consisted of a sealed box connected to the fog machine. This measurement differed from the others in that we did not always have the same conditions in the box, as fog inside gradually evaporated. That is why we had to add a 4 mW laser and optical power meter to our experiment (Figure 33). Figure 34 shows a photo of this setup. During measurements, we have monitored and gathered optical power levels to use them as reference values. Due to the slow fog evaporation, higher modulations gradually reached the desired BER threshold of 10 3 . As soon as it happened, we carried out our main measurements. In this case we have measured all bandwidths at once, to preserve credibility. Figure 35 describes a slow dissipation of fog inside box with gathered laser optical power levels and BER values for 1 MHz bandwidth.
The Laser itself was mainly used to exactly determine how fast the fog dissipated (concentration) and if it dissipated similarly in multiple measurements, which proved to be true. High directionality of laser beam and planoconvex lens on photodetector helped us to avoid any unnecessary effects of second light source. As mentioned the box was big enough to host both devices, which can work independently. In this case, the laser was the available device which we already had and could be used.
Table 4 consists of measured optical power level thresholds, after passing through fog. It is visible that at least a quarter of transmitted optical power is needed for higher modulation formats (128-QAM+) to work. That is why following the figures display minimal values for successful initiation of communication between transmitter and receiver for multiple modulation formats.
Measured BER values are displayed on Figure 36. This figure consists of all modulation formats, where BER values were better than 1. However, it is necessary to compare these values to Table 4, as different optical power levels were needed for every modulation scheme. For example, at least a quarter of transmitted optical power had to be received for 128-QAM/2MHz combination to work. E b /N 0 and EVM values displayed on Figure 37 and Figure 38 also must be compared to Table 4.
From all the meteorological phenomena, fog had the greatest influence on visible light communication and will be the hardest to overcome. Figure 39 displays attenuation characteristics for different laser power levels. For example, at 1 mW output power, attenuation increased by 63 dB in comparison with reference values.

5. Future Research and Discussion

During testing we have encountered several shortcomings, we will try to overcome in the future. As our prototype is designed with the highest possible modularity in mind, we want to aim for better parts especially tailored for our needs. We have identified amplifier nonlinearity and photodetector as our biggest limitation. We were able to acquire two APD modules from Hamamatsu Photonics Japan, which will be tested, evaluated and possibly incorporated into our prototype [103,104]. There are also multiple companies we are currently in contact with to manufacture custom amplifiers such as Mini Circuits and Ophir RF.
Figure 6 and Figure 13 show trend of increasing attenuation below 1 MHz and above 5 MHz. It is caused either by insufficient optimization of inbuild pre or post equalizers or by an amplifier in combination with insufficient impedance matching. Nonlinearity at 1 MHz to 5 MHz did not cause any significant changes to transmission quality. However we are currently working on optimization and have ordered a number of specialized parts.
We would like to propose a new concept of software defined optics (SDO). SDO is a visible light communication system, in which the critical part of signal processing is implemented by software programmable circuits. As a result, a variety of software changes can be used to swiftly modify the communication system, such as used modulation, channel coding etc. The transmitter consists of D/A converter and appropriate transmitter (LED or laser diode), which is modulated by a bias-tee. The receiver consists of a photodiode or camera and A/D converter.
The main advantage of our experiment was deployment of commercially available lights as transmitters. We avoided excessive modifications of original designs and tested them to their thresholds. However, we estimate, that modification of an Octavia tail-light LED cluster might increase effective maximal communication distance by 20%, as original LED matrixes tend to be of lower quality.
Implementation of adaptive modulation and/or channel width would allow our setup to dynamically react to different conditions. We have also estimated that channel equalization would improve whole prototype significantly. Channel equalization implementation will be a topic of our immediate research, which will follow this paper shortly.
Next revision of our software will replace simpler QAM with full-fledged OFDM, which will also significantly improve our prototype. The next generation of our LabVIEW SDR VLC implementation is currently under development and will be a topic of further papers.
Another advantage of our prototype is its software based on virtual instrumentation. LabVIEW SDR offers us a reliable and highly modular platform, which we can easily modify, adjust or move. Whole software was frequently moved between stationary desktop computer and powerful laptop, so we were able to test it in different labs with custom equipment, such as special box mentioned earlier. Main advantage lays in LabVIEW modularity. We can implement multiple functions very fast, such as addition of channel coding or equalization, which is a huge advantage in debug phase. The final implementation of our prototype will be minimalized and optimized. We estimate, that third generation of our software (second generation of OFDM) will run natively on FPGA.
Each measurements/tests were carried out multiple times and mainly independently. Each scenario was specially designed to represent the most pressing problems in VLC. Variable natural conditions and their compensation are a topic for multiple teams and their research [6,9,37,105]. As fog is the most concerning problem, several teams tried to compensate its impact [47,106,107]. A sandstorm, which was not tested in our paper, is considered as another concerning topic, however according to simulations, its characteristics is very similar to fog and rain [108].
We have also acquired a number of blue-light filters from Thorlabs. According to some papers, a system which uses these filters will have wider useable bandwidth but might suffer from shorter communication distance. Analysis of these parameters will be a topic of further research. As mentioned earlier, our Octavia taillight setup used plano-convex lens, which were already available at our university. We have also acquired another set of plano-convex and Fresnel lens which will be also a topic of further research.
Setup with indoor ceiling light could be enhanced with VLC positioning system, as there are a number of proposed implementations [109]. However primary purpose is data transmissions, so positioning would be only a supplementary function, which should not interfere with primary purpose or limit measured parameters. Some teams even reached up to 95 % accuracy in their experiments. OFDM, or more specifically OFDMA can be used for data transmissions as well as positioning. Positioning methods are usually based on trilateration model, which needs at least three transmitters with known location. However, we have used only one ceiling light for prototyping, so positioning would not be possible. This area will be a topic of further research [110,111,112,113,114].
In case of VLC, most teams are mainly focused on achieving longer communication distances or higher transmit speeds. Security was pushed sideways in favor of other areas. However we agree with colleagues, that non-line-of-sight (NLoS) or even line-of-sight (LoS) eavesdropping is possible without sturdy security, which is not covered enough in IEEE standardization. Possible NLoS eavesdropping will be a topic for further research, as we are just entering this area [115].
Many teams tend to use their own LED matrixes or custom designed lights. However, that is concerning, as quality of deployed LEDs in commercially available products tend to vary significantly. Manufacturers often use lower quality LEDs, because even a small difference in price will make a huge impact in higher quantities. That’s why we split our research into two branches. We begun our research on commercially available lights, as they are “target hardware”. However we are also running a number of test on multiple LEDs of different qualities, and are looking for best price/performance ratio. This area will be also a topic of further research [7,79,80,81,82].
Technical University of Ostrava has its own newly developed testing polygon called ”BroadbandLIGHT”. BroadbandLIGHT is situated next to faculty of electrical engineering and computer science. It consists of 20 lamp posts and central management located in laboratory EB418 (see Figure 40). The whole system is prepared for future implementation of VLC technology. It is a unique polygon that is oriented at potential customers, demonstrations of functionality or long-term measurements. It is a next step for incorporation of smart technologies (smart city, IoT, Industry 4.0) into lighting and can be used for either indoor or outdoor setups. Detailed description and possible implementation will be discussed in further papers.
A new kind of hybrid system is currently in development by our team. It is based on powerline, which will be connected directly to ceiling light. The return channel is based on power efficient Bluetooth technology. It Is estimated that whole system should be much more energy efficient. It is based on the premise that most of the users download much more than they upload, which will result in lower battery drain.
Table 5 summarizes multiple tests with different configurations, including ours. We have included information about modulation, detector, maximal reachable transmit speed and even maximal reachable distance.
Next version of our prototype will feature advanced signal processing methods, which we already investigated multiple times in different areas [116,117,118,119,120,121].

6. Conclusions

In this paper, we have presented results of our ongoing research. Our VLC prototype based on NI LabVIEW SDR and commercially available lights is introduced. First part of our experiment was carried out on Phillips indoor ceiling light. We have analyzed maximal possible transmit speeds at different distances from center, located directly below transmitter. The maximal reachable distance was 325 m, when using 4-QAM and 1 MHz bandwidth. Transmit speed was at least 2 Mbps. With wider channels and higher modulations (8-QAM to 256-QAM), maximal reachable distance decreased rapidly.
The second part was based on Octavia tail-light, which was tested under different natural conditions. A maximal measuring distance was constant 550 cm. A special box was inserted between transmitter (tail-light) and receiver (photodetector), which simulated different conditions such as: thermal turbulence, rain and fog. A number of figures with real measured data was presented and commented accordingly. We have also identified weak spots, which will be adjusted and possibly researched in future publications. From measured data, fog has the greatest impact on communication, as it caused. On the other side, thermal turbulence had the lowest impact. The highest reachable transmit speed was 28 Mbps for combination of 256-QAM and 4MHz, which was reachable only in the empty box.
Weak spots were identified and thoroughly discussed. A number of possible upgrades were mentioned, focusing on custom parts, which will significantly improve whole setup.

Author Contributions

Conceptualization, R.M. and L.D.; Methodology, R.M.; Software, L.D. and R.M.; Validation, R.M., L.D. and R.J.; Formal Analysis, R.M. and L.D.; Investigation, R.M. and R.J.; Resources, R.M.; Data Curation, L.D.; Writing—Original Draft Preparation, L.D.; Writing—Review & Editing, R.M. and R.J.; Visualization, R.J.; Supervision, R.M.; Project Administration, R.M.; Funding Acquisition, R.M.

Funding

This article was supported by the Ministry of Education of the Czech Republic (Project No. SP2019/85). This work was supported by the European Regional Development Fund in the Research Centre of Advanced Mechatronic Systems project, project number CZ.02.1.01/0.0/0.0/16_019/0000867 within the Operational Programme Research, Development and Education. This work was supported by the European Regional Development Fund in A Research Platform focused on Industry 4.0 and Robotics in Ostrava project, CZ.02.1.01/0.0/0.0/17_049/0008425 within the Operational Programme Research, Development and Education.

Conflicts of Interest

The authors declare no conflicts of interest.

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Figure 1. Vehicle-to-everything scenarios communication.
Figure 1. Vehicle-to-everything scenarios communication.
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Figure 2. Indoor VLC scenarios.
Figure 2. Indoor VLC scenarios.
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Figure 3. Error vector magnitude.
Figure 3. Error vector magnitude.
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Figure 4. Ceiling light setup.
Figure 4. Ceiling light setup.
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Figure 5. Setup with measured distance.
Figure 5. Setup with measured distance.
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Figure 6. Attenuation characteristics of ceiling setup.
Figure 6. Attenuation characteristics of ceiling setup.
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Figure 7. Transmit speed/distance from center relationship for ceiling light with different M-QAM and bandwidths.
Figure 7. Transmit speed/distance from center relationship for ceiling light with different M-QAM and bandwidths.
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Figure 8. 4-QAM constellation diagrams of ceiling light and different bandwidths: (a) 4-QAM, BW = 1 MHz, (b) 4-QAM, BW = 2 MHz, (c) 4-QAM, BW = 3 MHz, (d) 4-QAM, BW = 4 MHz.
Figure 8. 4-QAM constellation diagrams of ceiling light and different bandwidths: (a) 4-QAM, BW = 1 MHz, (b) 4-QAM, BW = 2 MHz, (c) 4-QAM, BW = 3 MHz, (d) 4-QAM, BW = 4 MHz.
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Figure 9. BER/distance from center relationship for ceiling light with different M-QAM and bandwidths.
Figure 9. BER/distance from center relationship for ceiling light with different M-QAM and bandwidths.
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Figure 10. E b /N 0 / distance from center relationship for ceiling light with different M-QAM and bandwidths.
Figure 10. E b /N 0 / distance from center relationship for ceiling light with different M-QAM and bandwidths.
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Figure 11. EVM/distance from center relationship for ceiling light with different M-QAM and bandwidths.
Figure 11. EVM/distance from center relationship for ceiling light with different M-QAM and bandwidths.
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Figure 12. Octavia tail-light setup.
Figure 12. Octavia tail-light setup.
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Figure 13. Attenuation characteristics of the Octavia tail-light.
Figure 13. Attenuation characteristics of the Octavia tail-light.
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Figure 14. Octavia taillight setup adjusted for scenario 1—empty box.
Figure 14. Octavia taillight setup adjusted for scenario 1—empty box.
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Figure 15. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 1—empty box.
Figure 15. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 1—empty box.
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Figure 16. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 1—empty box.
Figure 16. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 1—empty box.
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Figure 17. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 1—empty box.
Figure 17. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 1—empty box.
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Figure 18. Octavia tail-light setup adjusted for scenario 2-thermal turbulence.
Figure 18. Octavia tail-light setup adjusted for scenario 2-thermal turbulence.
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Figure 19. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 2—thermal turbulence.
Figure 19. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 2—thermal turbulence.
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Figure 20. E b /N 0 /distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 2—thermal turbulence.
Figure 20. E b /N 0 /distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 2—thermal turbulence.
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Figure 21. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 2—thermal turbulence.
Figure 21. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 2—thermal turbulence.
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Figure 22. Octavia tail-light setup adjusted for scenario 3—Rain 42 L/min.
Figure 22. Octavia tail-light setup adjusted for scenario 3—Rain 42 L/min.
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Figure 23. Photo of setup for scenario 3 and 4—rain.
Figure 23. Photo of setup for scenario 3 and 4—rain.
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Figure 24. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 3—Rain 42 L/min.
Figure 24. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 3—Rain 42 L/min.
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Figure 25. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 3—Rain 42 L/min.
Figure 25. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 3—Rain 42 L/min.
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Figure 26. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 3—Rain 42 L/min.
Figure 26. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 3—Rain 42 L/min.
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Figure 27. Attenuation characteristics of Octavia tail-light for scenario 3—Rain 42 L/min—comparison of intended setup and adjusted setup without partition.
Figure 27. Attenuation characteristics of Octavia tail-light for scenario 3—Rain 42 L/min—comparison of intended setup and adjusted setup without partition.
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Figure 28. Octavia tail-light setup adjusted for scenario 4-Rain 22 L/min.
Figure 28. Octavia tail-light setup adjusted for scenario 4-Rain 22 L/min.
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Figure 29. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 4-Rain 22 L/min.
Figure 29. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 4-Rain 22 L/min.
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Figure 30. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 4—Rain 22 L/min.
Figure 30. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 4—Rain 22 L/min.
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Figure 31. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 4—Rain 22 L/min.
Figure 31. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 4—Rain 22 L/min.
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Figure 32. Attenuation characteristics of Octavia tail-light for scenario 4-Rain 22 L/min—comparison of intended setup and adjusted setup without partition.
Figure 32. Attenuation characteristics of Octavia tail-light for scenario 4-Rain 22 L/min—comparison of intended setup and adjusted setup without partition.
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Figure 33. Octavia tail-light setup adjusted for scenario 5–fog.
Figure 33. Octavia tail-light setup adjusted for scenario 5–fog.
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Figure 34. Photo of setup for scenario 5-fog.
Figure 34. Photo of setup for scenario 5-fog.
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Figure 35. Fog dissipation with laser power levels and modulations with appropriate BER values.
Figure 35. Fog dissipation with laser power levels and modulations with appropriate BER values.
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Figure 36. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 5—fog.
Figure 36. BER/distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 5—fog.
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Figure 37. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 5—fog.
Figure 37. E b /N 0 / distance relationship for Octavia tail-light with different M-QAM and bandwidths—in scenario 5—fog.
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Figure 38. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 5—fog.
Figure 38. EVM/distance relationship for Octavia tail-light with different M-QAM and bandwidths—scenario 5—fog.
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Figure 39. Attenuation characteristics of Octavia tail-light during fog dissipation –in scenario 5 - fog.
Figure 39. Attenuation characteristics of Octavia tail-light during fog dissipation –in scenario 5 - fog.
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Figure 40. BroadbandLIGHT testing polygon implementation and management center.
Figure 40. BroadbandLIGHT testing polygon implementation and management center.
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Table 1. Parameters of light of Fortimo LED DLM 3000 44 W/840 Gen3.
Table 1. Parameters of light of Fortimo LED DLM 3000 44 W/840 Gen3.
Initial lumens3000 lm
Color rendering index80
Correlated color temperature4000 K
System input power46.0 W
System efficiency68.0 Lm/W
Input voltage220–240 V
Max. vitality5000 h
U max dc80 V
Max operating temperature65 C
P max 40 W
Table 2. Chosen parameters of photodetector PDA36A-EC.
Table 2. Chosen parameters of photodetector PDA36A-EC.
Type of detectorSi PIN
Active area3.6 × 3.6 mm (13 mm 2 )
Wavelength range350–1100 nm
Gain adjustment range70 dB
Gain step8 × 10 dB
Operating temperature0–40 C
Max output current100 mA
Table 3. Parameters of LED - LA G6SP.
Table 3. Parameters of LED - LA G6SP.
TechnologyInGaAlP Thinfilm
Viewing angle at 50 % IV120 (Lambertian Emitter)
ColorRed (623 nm)
Optical efficiency56 lm/W
Operating temperaturefrom –40 to 110 C
Max surge current1000 mA
Max current140 mA
Typical voltage2.1 V
Table 4. Minimal optical power levels of laser for multiple bandwidth and modulations measured after passing through fog.
Table 4. Minimal optical power levels of laser for multiple bandwidth and modulations measured after passing through fog.
M-QAMBandwidth
-1 MHz2 MHz3 MHz4 MHz
4-QAM101 μ W95 μ W97 μ W93 μ W
8-QAM112 μ W135 μ W175 μ W189 μ W
16-QAM154 μ W205 μ W250 μ W276 μ W
32-QAM275 μ W308 μ W463 μ W550 μ W
64-QAM525 μ W780 μ W930 μ W951 μ W
128-QAM905 μ W1.095 mW1.399 mW1.550 mW
256-QAM2.180 mW2.394 mW2.545 mW2.585 mW
512-QAM2.475 mW2.522 mW2.735 mW2.930 mW
1024-QAM2.640 mW2.955 mW3.120 mW3.172 mW
Table 5. Comparison of different VLC experiments.
Table 5. Comparison of different VLC experiments.
YearMain AuthorSourceDistanceDetectorModulation TypeTransmit Speed
2016Wen-Hsuan Shen [22]Tail-light 1157
(12 V, red LED)
45 mPhotodiode Thorlabs
PDA100A
(10 mm × 10 mm)
PWM (OFDM)45–55 Mbps
2016Yuki Goto [30]Red LED matrix
(4 × 5; 0.72 V, 14.5 MHz)
1.5 mOCI camera
(Focal distance
of the lens 50 mm)
4-256 QAM (OFDM)45 Mbps
50 Mbps
55 Mbps
2014Isamu Takai [122]Red LED matrix
(10 × 10; 4 W, 55 MHz)
7.78 mHigh-speed camera
(Focal distance
of the lens 12.5 mm)
Pulse Width
modulation (PWM)
10 Mpbs
2014Takaya Yamazato [122]Red LED matrix
(32 × 32)
45 mHigh-speed camera
(CMOS sensor)
Pulse Width
modulation (PWM)
10 Mpbs
2016Yoshihito Imai [123]Red LED
(OS5RKA5B61P)
1–8 mHigh-speed camera
XCG-V60E, SONY
(Focal distance
of the lens 8–48 mm)
Pulse Width
modulation (PWM)
84 bps
2017Takaya Yamazato [124]Red LED matrix
(32 × 32)
30–70 mHigh-speed image
sensor and OCI sensor
Pulse Width
modulation (PWM)
55 Mbps
2019Radek MartinekPhillips Fortimo
DLM 300 44 W/840 Gen3
3.25 m from centerThorlabs PDA-36AQAM modulation2 Mbps
2019Radek MartinekSkoda Octavila
Tail-light
5.5 mThorlabs PDA-36AQAM modulation28 Mbps

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Martinek, R.; Danys, L.; Jaros, R. Visible Light Communication System Based on Software Defined Radio: Performance Study of Intelligent Transportation and Indoor Applications. Electronics 2019, 8, 433. https://doi.org/10.3390/electronics8040433

AMA Style

Martinek R, Danys L, Jaros R. Visible Light Communication System Based on Software Defined Radio: Performance Study of Intelligent Transportation and Indoor Applications. Electronics. 2019; 8(4):433. https://doi.org/10.3390/electronics8040433

Chicago/Turabian Style

Martinek, Radek, Lukas Danys, and Rene Jaros. 2019. "Visible Light Communication System Based on Software Defined Radio: Performance Study of Intelligent Transportation and Indoor Applications" Electronics 8, no. 4: 433. https://doi.org/10.3390/electronics8040433

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