# Temperature Measurement Using Optical Fiber Methods: Overview and Evaluation

Authors: Martin Mikolajek; Radek Martinek; Jiri Koziorek; Stanislav Hejduk; Jan Vitasek; Ales Vanderka; Radek Poboril; Vladimir Vasinek; Radim Hercik
Journal: Journal of Sensors
 (2020)

---

## Abstract

The paper deals with the overview of fiber optic methods suitable for temperature measurement and monitoring. The aim is to evaluate the current research of temperature measurements in the interval from temperature close to 0 up to 1000°C. Since the measuring chain is a functional combination of optical methods, optical fiber properties, and other photonic elements together with control electronic circuits, it is necessary to find a suitable compromise between the chosen measurement method, measuring range, accuracy, and resolution. Optical fiber sensors can be used in cases where standard electrical measurement methods cannot be used. These may be areas with high electrical and magnetic interference or critical areas. Therefore, there is intensive development of optical and fiber optic methods based on blackbody and greybody radiation, luminescence, fiber Bragg gratings (FBGs), and interferometers.


---

## Body

## 1. Introduction

At present, many fundamentally different ways of measuring high temperatures are used. One of the primary users of temperature measurements is the automotive industry. There are a number of areas where it is necessary to measure or at least monitor this high temperature directly. An overview of some key locations in which the temperature is measured is given in Figure1. These are, in particular, points in the exhaust pipe, near catalytic converters, or turbochargers. An example of temperature measurement using optical methods is dealt with in the article from Bock et al. [1]. Another article from Jiang et al. is about a temperature fiber sensor for the aviation industry [2].Figure 1
High-temperature measurement points in vehicles.There are noncontact measurement methods [3] using emitted radiation of the observed body [4], known as temperature measurement by thermal cameras [5–8]. These methods require knowledge of the surface emissivity of the measured bodies. By these methods, surface temperatures of bodies can easily be determined [5, 6]. In a standard way, however, metallically attached thermocouple or resistive sensors, bimetallic, extensible in volume, and other principles which are connected to the measured object so that they touch it or are located in a space where a given ambient or general fluid temperature is measured, are commonly used in measuring applications. Their typical property is low levels of electrical current or voltage. When designing the measuring chain, account must be taken of the adverse effects of electrical and magnetic disturbances [9, 10] on metallic conductors between the actual temperature sensor and the evaluation unit that converts the signal from the sensor to the amplifier or analogue digital converter [10]. In applications where such electrical interference can be expected, it is advisable to use other nonelectrical temperature measurement methods. It is possible to use optical methods using optical fibers and the principles of blackbody radiation [11–14], luminescence in crystals [15–22], refractive index phenomenon in the fiber Bragg gratings [23–28], or phase shift of two coherent beams in interferometric sensors [29–33].The use of fiber sensors also offers the possibility of galvanic isolation, which brings the possibility of use in the chemical industry and various explosive environments. The use of fiber sensors for temperature measurement is possible using several physical principles which are described in the individual chapters of this text.The individual principles of temperature measurement using optical sensors also require their own ways of converting the optical signal to the measured temperature in degrees Celsius. One of the tasks of the paper is to present possible ways of evaluating temperature data. The paper focuses only on optical fiber methods of temperature measurement. The contribution does not include comparison of other optical methods of temperature measurement, such as thermovision.


## 2. Types of Temperature Measurement Using Optical Methods

The method of measurement using optical fiber techniques is based on several fundamental principles. Each measurement method has its specific uses in the range of measuring temperatures, accuracy, etc. (see Table1). The table shows basic advantages and disadvantages of individual fiber methods.Table 1
The method of measurement using optical techniques.
MethodAdvantagesDisadvantagesMeasuring rangeBlackbodyHigh-temperature measurementLow temperatures cannot be measured300°C and aboveSimple design of the sensorCrystal luminescenceMeasure temperatures below 300°CComplicated sensor design-40 to 400°CTwo measurement principlesFiber Bragg gratingLow-temperature measurement, mechanical baseUnsuitable for high temperatures in conventional solutions, grating structure distortion due to high temperatureNormally using 0-320°C, 1200°C in case of sapphire fibersInterferometerHigh-temperature range, simple and relatively cheap probe manufacturingSpectrometer needed for measurementOver 1200°CDepends on mechanical construction of the sensorPossible interferences caused by mechanical stressThis article goes on to describe all of the above methods. The blackbody (greybody) radiation method uses optical fiber, one part of which leads to a blackbody at the temperature measurement point. The light output generated by the radiation of the heated blackbody is led from the end of the fiber to the photodetector. According to Donati [11], the detected optical power intensity or spectrum of light received by the photodetector corresponds to the measured temperature according to the recalculations below. This measurement principle is only suitable for high temperatures of approximately 500°C, for the use of special types of photodetectors and optical fibers, and even for lower temperatures of approximately 300°C. This can be the case of evaluation using a spectrometer or a silicon, InGaAs diode, or PbSe photodiode [11].The second way of measuring the temperature mentioned in this article is the method using the principle of crystal luminescence [15–20]. The subject deals with the description of individual crystals and analysis of individual results for the tested materials. The fundamental difference from the first method is that this method is not passive but requires a light flux generator. The light from one end of the fiber must fall on the selected luminescent crystal. At the other end of the fiber, the photodetector receives the light signal from the crystal depending on the light generated and the temperature at the desired point of measurement [18]. The dependence of the received light output on the temperature is given in the chapter temperature-dependent crystals. The method described later uses the fiber Bragg gratings [23–25]. The range of applications is considerable today; some textbooks describe the principles of FBG [34] and their applications [35]. The principle of this measurement method lies in the passage of light through the periodically modified optical fiber to produce a periodic or quasiperiodic change in the refractive index of the optical fiber. The last part describes interferometric measurements. These methods measure phase shift between two coherent beams that have travelled the same path in one or two optical fibers. This type of sensor can simultaneously measure different physical quantities, including temperature, since the mechanical parameters of the optical fiber changes with the temperature.The individual chapters deal with the description of general problems of selected methods and with individual features and possibilities of used parts employed in the described manner. The article presents a comprehensive overview of methods for temperature measurement by optical fiber.


## 3. Temperature Measurement Using Blackbody Radiation Method

This method is one of the easiest ways to measure temperature using optical fibers. Only an optical fiber and a suitable photodetector are essential for realization. With minimal financial costs, we are able to assemble a photodetector with a temperature range of approximately 500 to 1200°C.Higher temperatures can be measured using a sapphire fiber. For these cases, temperatures up to the melting point of the sapphire fiber can be considered. This means the temperature 2040°C [36, 37]. These boundaries can then be expanded using special components up to the physical limits of fibers and photodetectors.Each body with nonzero surface temperature emits a certain amount of radiant energy. Most energy is radiated by the so-called black (blackbody radiation, abbreviated as BBR) [38]. The amount of energy and the spectrum of emitted radiation depend only on the surface temperature of the body. Both of these parameters can also be described mathematically by the Planck blackbody emission law, where we can describe the spectral density of the radiation intensity using the following Equation (1), where “v” is given by Equation (2) [11], h=6.626×10−34Js is the Planck constant, k=1.38×10−23J/K is the Boltzmann constant, “λ” is the wavelength, “T” is the temperature, and “c” is the speed of light in vacuum (c=3×108m/s).
(1)rλ=hv2λ3ehv/kT−1,(2)v=cλ.This emitted radiation can easily be used for the optical measurement of the body temperature, where the total radiated energy according to the Stefan-Boltzmann law increases, depending on the absolute temperature with the fourth power (see Equation (3) [11]), where σ is the Stefan-Boltzmann constant according to Equation (4).
(3)E=σT4,(4)σ=2π5·k415c2·h4=5.670400·10−8Js−1m−2K−4.The Rayleigh-Jeans law can also be used to measure temperatures if the shortwave spectral region is applied (see Figure2), from which it is clear that for a suitably chosen wavelength, the radiated energy density at the wavelength interval will be dλ as seen below:
(5)rλdλ=8πkTdλλ4.Figure 2
Spectral radiance of the blackbody versusλ.The second relationship that can be used for the evaluation is Wien’s displacement law which says that with the increasing temperature, maximum radiation shifts to shorter wavelengths. In mathematical writing, this fact is expressed by(6)λmaxT=hc4.965k.


### 3.1. Measurement Principle Using Optical Fiber

Information about measured temperature might be transferred through different environments. Vacuum, atmosphere, or other gases are suitable only for Line-Of-Sight (LOS) measurements of blackbody, but for more flexible access to the measured temperature, we can use optical fibers. However, the range of the measured temperatures depends on the spectral sensitivity of the used photodetector and the properties of the transfer medium. When using the optical fiber, the transmission medium is glass, which is quite restrictive in the transmission spectrum. Conventional optical fibers (even low-OH versions) are designed for applications with wavelengths used for communication (i.e., from the visible spectrum to the near infrared range area as shown in Figure3) [39].Figure 3
Spectral characteristics of optical fibers.The spectral limit of low-OH optical fibers (2400 nm) can be extended with special fluoride-doped optical fibers (InF3) [39] or chalcogenide glass. So the spectral limit can be shifted to wavelengths over 5000 nm.By comparing Figures2 and 3, theoretically, we can transmit information about temperatures below 0°C by an optical fiber. However, in the case of detecting such a signal by a photodetector, we will probably observe few problems in the form of the spectral characteristics of the photodetector (see Figure 6 [11]) and possible external noise. For low temperatures, blackbody radiation is applied not only to the fiber optic signal but also to the optical fiber itself, case, and vicinity of the photodetector. For the successful blackbody measurement of low temperature, the temperature of the measurement optical fiber and photodetector case must be thermally stable; ideally it should be cooler then the measured signal, so the measured energy could be easily detected.If the measured body does not behave as an absolutely black radiator, its radiation density will be smaller. This reduced proportion is expressed either by the emissivity or by the degree of greyness of the particular body. The degree of greyness indicates how large the percentage of greybody radiation is compared to an absolutely blackbody at the same temperature. During the actual measurement, it is necessary to take into account that emissivity is a wavelength-dependent parameter.The temperature measurement system using the blackbody consists of three parts: optical radiation source approaching the blackbody, optical fiber for signal transmission, and evaluation electronics, shown in Figure4. The basis for the measurement is to adjust the end of the optical fiber so that its end is as similar to the blackbody as possible. In most cases, this is achieved by means of a metallic coating [13, 14] or by inserting a fiber into the measuring pit [12]. The fiber thus captures the blackbody emissions and transmits them to the detector end.Figure 4
Optical fiber deployment for measurement using the blackbody principles.


### 3.2. Implementation of High-Temperature Measurement Point (Coating or Cavity)

Two basic approaches are used to construct the temperature sensor. Using the coating, the end of the fiber becomes a sensor, and it is thus directly exposed to the measured temperatures during measurement. The coating materials must withstand high temperatures and must not change their emissivity value during repeated cycles.At higher temperatures, however, we cannot leave primary protection on the fiber as the fiber becomes brittle. The sensor produced this way either is not suitable for demanding conditions or must be suitably placed in another temperature-resistant shield.The cavity provides the fiber with the possibility of protection against adverse environmental influences because the fiber, in this case, does not have to be exposed directly to the measured temperatures. Depending on the shape of the cavity, measurements continue from the end of the fiber. This is given by the value of the acceptance angle at which the fiber collects ambient light and is defined by the numerical aperture (NA) value and the ambient refractive index; see Equation (7) where for air n=1, where Φ is the maximal half-angle of the cone of light that can enter or exit from the optical fiber.
(7)NA=n·sinΦ.Figure5 [12] shows the effect on the measured area where the energy at the distances x and l1 is not connected to the fiber. The measurement is thus mainly focused on the l2 area. In principle, the optical fiber in the cavity functions as a noncontact thermometer and retains this property until the fiber optic front is contaminated. Therefore, it is essential that the cavity does not cause evaporation of material due to high temperatures. The situation where the end of the fiber behaves like a grey (black) emitter and it is a source of radiation itself is more common. In this case, the fiber end contamination is not a significant problem.Figure 5
Configuration of the fiber and the blackbody element.


### 3.3. Optical Fiber for Blackbody Radiation Method

For measurement, we need to use the fiber to transfer as much optical signal as possible to the detector. Therefore, the optical fiber must have the greatest possible diameter of the core. While keeping the costs low, we can use the 62.5μm MM fiber; however, it is much better to deploy fibers with larger core diameters (e.g., 200 or 300 μm).The fiber material also directly determines the maximum measurable temperature. As soon as we come close to the melting point, the fiber becomes deformed. Fiber deformations result in a change of the sensor parameters. The melting point of pure SiO2 glass is 1610°C. This temperature varies depending on the addition agents used. For higher temperatures, it is possible to use sapphire [40] fibers that combine the properties of the sapphire crystal Al2O3 and optical fiber flexibility. With the melting point of 2045°C and chemical properties, they are suitable also for aggressive environments because they are almost chemically neutral.


### 3.4. Signal Detection for Blackbody Radiation Method

To evaluate the measured temperature, we can use the signal amplitude measurement on the photodiode [40] or evaluate the spectrum of the radiation with a spectrometer [4].The signal amplitude measurement is simple and inexpensive; however, it provides room for measurement deviations caused, for example, by mechanical and thermal stresses of the fiber.The lower part of the temperature range is determined in this case by the material of the photodiode used, as can be seen in Figure6 [11].Figure 6
Spectral characteristics of photodetectors depending on the composition.When using a silicon (Si) photodiode, the IR portion of the spectrum is limited to about 1000 nm, and at temperatures below 500°C, the signal amplitude is very small. Another option is the use of InGaAs-based photodiodes, capable of working up to 1800 nm. The applicable temperature range is thus moved up to 300°C.The theoretical option is to use InAs [41], a PbSe photoconductive photodetector [42, 43] which is capable of detecting wavelengths at the 4800 nm line, which will allow for further reduction of the working temperature.However, the measurement procedure differs in this case because this type of detector can process direct current (DC) signals but suffers from a large dark current value that is approximately three orders larger than the InGaAs detectors. To increase the resolving power of the detector, it is necessary to place a mechanical breaker (chopper) as shown in Figure7 between the detector and the measured signal [44].Figure 7
PbSe photoconductor measurement scheme.


### 3.5. Measurement Deviations of Blackbody Radiation Method

BBR measurement results in deviations due to its own emission of radiation from the inside of the optical fiber. If the fiber heats up, its material becomes a source of radiation. The longer the heated portion of the fiber, the greater the manifestations. For signal amplitude evaluation, this deviation can be eliminated, for example, by using the two-fiber method shown in Figure8 [13].Figure 8
Two-fiber optical thermometer.Both fibers are exposed to the same temperature; one is equipped with a blackbody cavity and the other one is covered with reflective coating. As a result, we can eliminate fiber-caused deviations by subtracting individual signals.


### 3.6. Partial Conclusion for the Blackbody Measurement Methods

The blackbody (greybody) measurement method is particularly suitable because of its simplicity since it requires only a fiber and a suitable photodetector. However, the pitfall of this method lies in the measuring range and accuracy that can be measured by this method; it is particularly suitable for measuring temperatures from 300°C to temperatures which depend on the softening or melting temperature of the deployed optical fiber, which may be up to 2000°C. For lower temperatures, it is possible to use optical fibers in primary or secondary protection and only bare fibers for high temperatures. The disadvantage of this method, however, lies in the complicated measurement of temperatures below the temperatures lower than 600°C. The measuring areas can be influenced by the type of photodetector used, especially for the lower temperature limit. In these cases, it is always necessary to use special photodetectors, then the price of the overall measuring chain increases. For still decreasing temperature ranges, the instability and inaccuracy of the measuring chain are increasing. This is due to the fact that when the temperature at the measuring point approaches the temperature of the photodetector, the received signal begins to be “drowned” in noise.


## 3.1. Measurement Principle Using Optical Fiber

Information about measured temperature might be transferred through different environments. Vacuum, atmosphere, or other gases are suitable only for Line-Of-Sight (LOS) measurements of blackbody, but for more flexible access to the measured temperature, we can use optical fibers. However, the range of the measured temperatures depends on the spectral sensitivity of the used photodetector and the properties of the transfer medium. When using the optical fiber, the transmission medium is glass, which is quite restrictive in the transmission spectrum. Conventional optical fibers (even low-OH versions) are designed for applications with wavelengths used for communication (i.e., from the visible spectrum to the near infrared range area as shown in Figure3) [39].Figure 3
Spectral characteristics of optical fibers.The spectral limit of low-OH optical fibers (2400 nm) can be extended with special fluoride-doped optical fibers (InF3) [39] or chalcogenide glass. So the spectral limit can be shifted to wavelengths over 5000 nm.By comparing Figures2 and 3, theoretically, we can transmit information about temperatures below 0°C by an optical fiber. However, in the case of detecting such a signal by a photodetector, we will probably observe few problems in the form of the spectral characteristics of the photodetector (see Figure 6 [11]) and possible external noise. For low temperatures, blackbody radiation is applied not only to the fiber optic signal but also to the optical fiber itself, case, and vicinity of the photodetector. For the successful blackbody measurement of low temperature, the temperature of the measurement optical fiber and photodetector case must be thermally stable; ideally it should be cooler then the measured signal, so the measured energy could be easily detected.If the measured body does not behave as an absolutely black radiator, its radiation density will be smaller. This reduced proportion is expressed either by the emissivity or by the degree of greyness of the particular body. The degree of greyness indicates how large the percentage of greybody radiation is compared to an absolutely blackbody at the same temperature. During the actual measurement, it is necessary to take into account that emissivity is a wavelength-dependent parameter.The temperature measurement system using the blackbody consists of three parts: optical radiation source approaching the blackbody, optical fiber for signal transmission, and evaluation electronics, shown in Figure4. The basis for the measurement is to adjust the end of the optical fiber so that its end is as similar to the blackbody as possible. In most cases, this is achieved by means of a metallic coating [13, 14] or by inserting a fiber into the measuring pit [12]. The fiber thus captures the blackbody emissions and transmits them to the detector end.Figure 4
Optical fiber deployment for measurement using the blackbody principles.


## 3.2. Implementation of High-Temperature Measurement Point (Coating or Cavity)

Two basic approaches are used to construct the temperature sensor. Using the coating, the end of the fiber becomes a sensor, and it is thus directly exposed to the measured temperatures during measurement. The coating materials must withstand high temperatures and must not change their emissivity value during repeated cycles.At higher temperatures, however, we cannot leave primary protection on the fiber as the fiber becomes brittle. The sensor produced this way either is not suitable for demanding conditions or must be suitably placed in another temperature-resistant shield.The cavity provides the fiber with the possibility of protection against adverse environmental influences because the fiber, in this case, does not have to be exposed directly to the measured temperatures. Depending on the shape of the cavity, measurements continue from the end of the fiber. This is given by the value of the acceptance angle at which the fiber collects ambient light and is defined by the numerical aperture (NA) value and the ambient refractive index; see Equation (7) where for air n=1, where Φ is the maximal half-angle of the cone of light that can enter or exit from the optical fiber.
(7)NA=n·sinΦ.Figure5 [12] shows the effect on the measured area where the energy at the distances x and l1 is not connected to the fiber. The measurement is thus mainly focused on the l2 area. In principle, the optical fiber in the cavity functions as a noncontact thermometer and retains this property until the fiber optic front is contaminated. Therefore, it is essential that the cavity does not cause evaporation of material due to high temperatures. The situation where the end of the fiber behaves like a grey (black) emitter and it is a source of radiation itself is more common. In this case, the fiber end contamination is not a significant problem.Figure 5
Configuration of the fiber and the blackbody element.


## 3.3. Optical Fiber for Blackbody Radiation Method

For measurement, we need to use the fiber to transfer as much optical signal as possible to the detector. Therefore, the optical fiber must have the greatest possible diameter of the core. While keeping the costs low, we can use the 62.5μm MM fiber; however, it is much better to deploy fibers with larger core diameters (e.g., 200 or 300 μm).The fiber material also directly determines the maximum measurable temperature. As soon as we come close to the melting point, the fiber becomes deformed. Fiber deformations result in a change of the sensor parameters. The melting point of pure SiO2 glass is 1610°C. This temperature varies depending on the addition agents used. For higher temperatures, it is possible to use sapphire [40] fibers that combine the properties of the sapphire crystal Al2O3 and optical fiber flexibility. With the melting point of 2045°C and chemical properties, they are suitable also for aggressive environments because they are almost chemically neutral.


## 3.4. Signal Detection for Blackbody Radiation Method

To evaluate the measured temperature, we can use the signal amplitude measurement on the photodiode [40] or evaluate the spectrum of the radiation with a spectrometer [4].The signal amplitude measurement is simple and inexpensive; however, it provides room for measurement deviations caused, for example, by mechanical and thermal stresses of the fiber.The lower part of the temperature range is determined in this case by the material of the photodiode used, as can be seen in Figure6 [11].Figure 6
Spectral characteristics of photodetectors depending on the composition.When using a silicon (Si) photodiode, the IR portion of the spectrum is limited to about 1000 nm, and at temperatures below 500°C, the signal amplitude is very small. Another option is the use of InGaAs-based photodiodes, capable of working up to 1800 nm. The applicable temperature range is thus moved up to 300°C.The theoretical option is to use InAs [41], a PbSe photoconductive photodetector [42, 43] which is capable of detecting wavelengths at the 4800 nm line, which will allow for further reduction of the working temperature.However, the measurement procedure differs in this case because this type of detector can process direct current (DC) signals but suffers from a large dark current value that is approximately three orders larger than the InGaAs detectors. To increase the resolving power of the detector, it is necessary to place a mechanical breaker (chopper) as shown in Figure7 between the detector and the measured signal [44].Figure 7
PbSe photoconductor measurement scheme.


## 3.5. Measurement Deviations of Blackbody Radiation Method

BBR measurement results in deviations due to its own emission of radiation from the inside of the optical fiber. If the fiber heats up, its material becomes a source of radiation. The longer the heated portion of the fiber, the greater the manifestations. For signal amplitude evaluation, this deviation can be eliminated, for example, by using the two-fiber method shown in Figure8 [13].Figure 8
Two-fiber optical thermometer.Both fibers are exposed to the same temperature; one is equipped with a blackbody cavity and the other one is covered with reflective coating. As a result, we can eliminate fiber-caused deviations by subtracting individual signals.


## 3.6. Partial Conclusion for the Blackbody Measurement Methods

The blackbody (greybody) measurement method is particularly suitable because of its simplicity since it requires only a fiber and a suitable photodetector. However, the pitfall of this method lies in the measuring range and accuracy that can be measured by this method; it is particularly suitable for measuring temperatures from 300°C to temperatures which depend on the softening or melting temperature of the deployed optical fiber, which may be up to 2000°C. For lower temperatures, it is possible to use optical fibers in primary or secondary protection and only bare fibers for high temperatures. The disadvantage of this method, however, lies in the complicated measurement of temperatures below the temperatures lower than 600°C. The measuring areas can be influenced by the type of photodetector used, especially for the lower temperature limit. In these cases, it is always necessary to use special photodetectors, then the price of the overall measuring chain increases. For still decreasing temperature ranges, the instability and inaccuracy of the measuring chain are increasing. This is due to the fact that when the temperature at the measuring point approaches the temperature of the photodetector, the received signal begins to be “drowned” in noise.


## 4. Luminescent Crystals with Temperature Dependence

Some crystal parameters show dependence on ambient temperature due to their composition. The parameter showing the temperature dependence is primarily luminescence. In luminescence, we can measure the excited spectrum, excited light intensity, or the lifetime of electrons in the excited state. Luminescence time response measurement is the most commonly used method because it is relatively simple and intensely independent of the amount of excited light [15, 45]. Crystals showing the temperature dependence of the lifetime of excited light-generating electrons are ruby (chromium-doped sapphire) [15–20], alexandrite [15, 16, 19, 46, 47], Cr:LiSAF [15, 16, 19, 48, 49], Cr:YAG, or Nd3+:YAG [15, 16, 19, 21, 50]. Ruby is a chromium-doped aluminium oxide (Cr3+:Al2O3). Chromium atoms, due to the similar size, can replace the aluminium atoms in the Al2O3 crystal lattice. Due to the presence of chromium, a phenomenon known as fluorescence occurs after absorbing the excitation light.


### 4.1. Description of Fluorescence

After delivery of the excitation light, the electrons move to the energy level of4T2, where they, however, do not hold and pass to the metastable level of 2E. Thanks to spin-orbit coupling [51], the metastable level of 2E is divided into two levels of −E and 2−A with the energy difference ΔE. This division of the metastable level causes the formation of two emission spectral lines. The first emission spectral line R1 is due to the transition of −E≥4A2 (694.3 nm); the second emission spectral line R2 is due to the transition of 2−A ≥ 4A2 (692.9 nm). The second emission spectral line R2 is slightly weaker than the first R1 [18, 52]. A simplified diagram of the energy levels of ruby is shown in Figure 9.Figure 9
Simplified diagram of ruby energy levels.Fluorescence is time-dependent, and after switching off the excitation light after a certain period of time called the lifetime, it disappears.For this reason, the excitation light source must be modulated by a rectangular pulse, thus alternately turning the excitation light on and off. The lifetime of the emission spectral lineR2 is ~3-3.5 ms and R1 is ~0.6 ms [15, 18].Changing the temperature leads to a change in the coupling (tension) in the crystal lattice and the distribution of phonons and energy, and consequently, it influences the fluorescence lifetime of ruby. The relatively short lifetime at the4T2 level causes the fluorescence of R lines to dominate due to the long-lasting 2E level at low temperatures (transition 2E→4A2 determines the temperature dependency of the lifetime). At room temperature (about 300 K) the lifetime is about ~3.5 ms [15, 18]. With increasing temperature, some Cr3+ ions are propped up to revert to the 4T2 level from the 2E level rapidly. With further increases in the temperature, more and more ions are propped up to this reversion, thereby emptying the 2E level and the nonradiant transitions 4T2→4A2 start to dominate. Significant loss of radiant transitions thus reduces the lifetime of fluorescence to ~1 μs at a temperature of about 600°C [15]. At the same time, the fluorescence-emitted light intensity decreases.Figure10 describes the radiant transitions of Cr3+ ions from the 2E→4A2 level at low temperatures where the nonradiant transitions from the 4T2 level are negligible due to the preferred occupancy of the 2E level. With an increasing temperature, the nonradiant transitions 4T2→4A2 start to dominate, the level 2E becomes a temporary level for the excitation of ions at the 4T2 level. The transition time 2E→4T2 is around ~7 ps. The temperature dependence of the fluorescence lifetime can be expressed by [53]
(8)τ=τS1+Cde−ΔE/kT1+τS/τie−ΔE/kT=τS1+3e−ΔE/kT1+αe−ΔE/kT,where τ is the fluorescence lifetime, ΔE is the energy difference between the levels 4T2 and 2E, τi and τs are the lives of transitions from the 4T2 and 2E levels, k is the Boltzmann constant, T is the temperature, and Cd is the ratio of degeneration 4T2/2E [54].Figure 10
Two-level ruby model.This model provides good results compared to measurements for temperatures ranging from 300 to 570 K [54].From the room temperature to about ~550 K, the lifetime is decreasing. Beyond the ~600 K limit, the4T2→4A2 transitions start to dominate, resulting in a rapid drop in the lifetime with an increasing temperature, which Equation (6) already cannot describe accurately enough.The selected article describes a simplified model for ruby that predicts changes in lifetime with changing temperatures, as shown in Figure11 [18]. This model includes the radiant 2E→4A2 and nonradiant 4T2→4A2 transitions. The schematic diagram of this model is shown in Figure 10. The lifetime of fluorescence is described by
(9)τ=τS1+3e−ΔE/kT1+αe−ΔE/kT+βe−ΔEq+ΔE,where τq is the nonradiant transition, ΔEq is the energy difference between 4T2 and 4A2, α=τs/τi, and β=τs/τq. This model is accurate from 300 to 800 K with a tolerance of ~1% over the given temperature range.Figure 11
A simplified model for ruby.


### 4.2. Absorption Spectrum

Although the absorption spectrum of ruby is strongly dependent on the polarization of the excitation light [18, 55], there are relatively small differences between the intensities R1 and R2.The absorption spectrum of ruby is spectrally broad, as shown in Figure12 [15, 18]. There are two absorption peaks around 410 and 550 nm. The emission spectrum has the main peaks, 694.3 nm (R1) and 692.9 nm (R2).Figure 12
Ruby absorption spectrum.


### 4.3. Dimensions of Crystals

Hu et al. [16] compare the lifetime of ruby luminescence for two sizes, for a smaller and a larger crystal. Measurements were conducted at temperatures ranging from 77 to 800 K. At the initial temperature, the lifetime of the small crystal fluorescence was 4.2 ms, while the lifetime of the large crystal fluorescence was 7.1 ms. This phenomenon occurs because the fluorescence light is reabsorbed in the large crystal and reexcitation occurs, thus extending the lifetime of fluorescence as the crystal radiates longer. This phenomenon, however, applies to low temperatures; from the temperature of about 0°C, the fluorescence lives balance out for small and large crystals. However, for practical applications, it is recommended that the ruby crystal size be as small as possible, just to minimize the redistribution of fluorescent light [16].


### 4.4. Concentration of Chromium in the Crystal

The fluorescence lifetime is independent of the concentration of chromium in ruby up to the critical level of about ~0.3 wt.% [56]. Higher chromium concentrations lead to a decrease in the fluorescence intensity. Additionally, over the concentration of ~1 wt.%, the lifetime is no longer simply exponential, as shown in Figure 12 [19].


### 4.5. Luminescent Experiments

Seat et al. [15] excited ruby using a laser diode with a modulated rectangular signal with a wavelength of 635 nm that flashed through the fiber optic (100/140 μm) through a 1×2 fiber coupler. The optical fiber was coupled to a ruby crystal using a silica glass tubing, both ends of which were melted, thus combining the fiber with the crystal. The sensor thus created was placed in a temperature-controlled furnace with a type K control thermocouple. The radiated fluorescence light was captured with the same optical fiber and passed through the coupler to the photodiode (APD:Si). A bandfilter>670nm was placed before the photodetector, which filtered the excitation light. The phase-locked detection (PLD) technique [57] was used to measure the ruby crystal fluorescence lifetime. The detected signal was processed to produce a recurring signal whose period was directly proportional to the time of the lifetime. This reduces the effect of the excitation light, allowing high-resolution measurements over a wide temperature range. The lifetime of ruby fluorescence was measured in the temperature range from 0 to 600°C. Around the temperature of 400°C, there was a strong drop in fluorescence. The measurement time interval was 1 s, with a resolution of 0.2°C. The results are shown in Figure 13 [15]. The following Figure 14 shows ruby fluorescence.Figure 13
Chromium concentration in ruby.Figure 14
Ruby fluorescence.Hu et al. [16] created two ruby temperature sensors, one large (0.5×0.5×2 mm) and the other small (0.3×0.3×0.05 mm). These crystals were excited with a He-Ne laser (5 mW) with a wavelength of 543.5 nm, which emitted continuous light; subsequently, this light was modulated by an acoustic-optical modulator (AOM) to rectangular pulses. As in the previous case, a 1×2 fiber coupler was used. In addition, an optical fiber with a diameter of 0.4 mm for a large sensor and a fiber with a diameter of 0.1 mm for a small sensor were used. Both threads had protection made of gold to withstand low temperatures. The crystals were also protected by the gold shield. The fibers and crystals were joined by a high-temperature adhesive. Fluorescent light was fed to an avalanche photodetector (APD). An optical filter (>690 nm) was placed before the photodetector to remove the excitation light. Measurements took place in the temperature range of 77 to 800 K (-196 to 527°C) with both sensors, so the effect of ruby crystal size on the fluorescence lifetime can be observed [16]. Figure 15 shows ruby fluorescence with two crystals of a different size.Figure 15
Ruby fluorescence with two crystals of a different size.Seat and Sharp [18] used a ruby crystal at a concentration of 0.1 wt.%. This crystal was connected to an optical fiber having a core diameter of 0.2 mm. The fiber and crystal were connected by means of a conical glass roller, at both ends of which a high-temperature ceramic adhesive was used, which joined a glass roller with a ruby at one end and an optical fiber at the other end. This sensor was inserted into a temperature-controlled furnace. The excitation light emanating from the Ar+ laser (514.5 nm) was modulated before entering the 1×2 fiber coupler. The excited light was fed to an avalanche photodiode in front of which there was an optical narrowband interference filter (694 nm, full width at half maximum FWHM±2nm) to remove the excitation light. Fluorescence lifetime measurements were carried out within the temperature range from 292 to 923 K (19 to 650°C) with a step of 50 K. Very good results were achieved up to a temperature of 773 K (500°C) when the standard deviation for this temperature was 0.32%, providing an ~2.4 K resolution. The accuracy of measurements at higher temperatures (>500°C) deteriorates due to the low fluorescence signal from ruby. The maximum deviation of the measurement was recorded at a maximum temperature of 923 K, namely, ~4.6%. The expected relatively long lifetime of fluorescence (~2-3 ms) was measured at low temperatures up to 600 K (327°C), then the lifetime decreased below 1 ms due to the increasing dominance of nonradiant transitions and heat extinction. The measured results of the fluorescence lifetime at different temperatures are shown in Table 2 [18]. Ruby fluorescence is shown in Figure 16.Table 2
The method of measurement using optical techniques.
T (K)292295323373374375423473523τ (ms)3.4203.4203.1602.6802.6702.6602.1201.5901.160T (K)573574623673723773823873923τ (ms)0.8420.8390.6150.4350.2890.1530.0820.0500.045Figure 16
Ruby fluorescence.Similar measurements can also be found in another publication [19]. For measurement, gold-coated quartz fiber with a core diameter of 400 μm was used. This sensor has been tested from 30 to 550°C. As expected, the fluorescence lifetimes were decreasing with an increasing temperature. Beyond 500°C, the fluorescence lifetime was essentially stabilized. The measurement results are shown in Figures 17 and 18.Figure 17
Ruby fluorescence lifetime.Figure 18
Intensity of ruby fluorescence.Obviously, the individual measurements are related to the types of crystals that are used for the measurements. The following part of the article deals with the analysis of crystalline materials using luminescence measurements.


### 4.6. Luminescent Material Alexandrite

Similar properties are shown by alexandrite which is hence used as a ruby. Alexandrite has a different absorption spectrum (see Figure18 [47] with respect to ruby); therefore, it is excited by another light source. To excite alexandrite, a 670 nm [46] or 633 nm He-Ne laser was deployed. Zhang et al. [47] set up a temperature sensor based on the fluorescence lifetime measurement like in the case of ruby. They performed measurements from 0 to 700°C, the results of which are shown in Figure 19 [19]. The lifetime of alexandrite fluorescence is shorter at room temperatures (300 μs) than in the case of ruby (~3.5 ms).Figure 19
Alexandrite absorption spectrum [47].Alexandrite can be produced artificially, as well as ruby, using the Czochralski method [58]. Additionally, alexandrite can be found in nature; it is mined in Brazil, Ural, Tanzania, Madagascar, and India [59].


### 4.7. Luminescent Material Cr:LiSAF

The material Cr:LiSAF is useful for temperature measurement in biomedical applications (30-50°C). Again, the fluorescence lifetime measurement is used. Zhang et al. [48] used a Cr:LiSAF laser with a wavelength of 670 nm for exciting. The excitation light was coupled to a quartz optical fiber (core 200 μm) through a 1×2 fiber coupler. At the end of the optical fiber, a Cr:LiSAF sample was attached using an adhesive. In front of the photodetector, the optical filter was deployed to suppress the excitation light. The measured results are shown in Figure 20 [19, 48]. Fluorescence lifetime at 0°C is about 64 μs and further decreases with an increasing temperature. Cr:LiSAF is usable approximately up to a temperature of about 100°C. The graph is shown in Figure 21.Figure 20
Alexandrite fluorescence [19].Figure 21
Cr:LiSAF fluorescence [8, 10].Fernicola and Crovini [21] used a Cr:YAG crystal to measure temperatures from -25 to 500°C. The graph is shown in Figure 22. Their experiment was also based on the measurement of the fluorescence lifetime. For excitation, they used a laser diode with a wavelength of 635 nm, the emission wavelength was 689 nm. They also deployed a quartz fiber with a diameter of 400 μm. The result of their measurement is shown in Figure 23 [21]. The fluorescence lifetime begins at 35 ms and decreases with an increasing temperature. The measurement was performed up to a temperature of 500°C.Figure 22
Cr:YAG fluorescence lifetime [21].Figure 23
Fluorescence lifetime cycle Cr:YAG [50].A similar measurement with the same material Cr:YAG was performed by Hehir et al. with results in Figure23 [50]. The temperature range was shifted to lower temperatures from 77 K to 420 K (−196~150°C).


### 4.8. Luminescent Material Nd3+:YAG

Another suitable material for measuring temperature is Nd3+:YAG. Grattan et al. [60] used a LED diode with a wavelength of 810 nm for excitation of the Nd3+:YAG crystal. They used 6 quartz fibers (core diameter 600 μm) for the excitation light and the emission light. The principle of the experiment is again based on the fluorescence lifetime measurement. The lifetime increases with an increasing temperature with a peak of about 700°C. With a further rise in temperature, the lifetime is decreasing. It is possible to measure temperatures up to about 1000°C. The measurement results are shown in Figure 24 [19].Figure 24
Nd3+:YAG fluorescence [19].


### 4.9. Partial Conclusion for Measurements Using Crystal Materials

The fluorescence lifetime measurement is a more convenient method of measuring the temperature, as the intensity of the emission light can vary greatly. Most commonly, ruby crystals are used. The fluorescence lifetime in ruby is measurable up to approximately 600°C. The lifetime fluorescence is also affected by the concentration of chromium in ruby and the dimensions of the crystal. The recommended concentration is about ~0.3 wt.%. Crystal dimensions should be as small as possible to avoid reabsorption and excitation, which prolongs the fluorescence lifetime. Either red or green lasers are often used for exciting ruby.Other materials capable of measuring the temperature are alexandrite, Cr:LiSAF, Cr:YAG, or Nd3+:YAG. For all measurements with these materials, a method of measuring the fluorescence lifetime was used. Alexandrite is able to react to temperatures up to 700°C. The initial lifetime is 10 times lower than the initial fluorescence lifetime in ruby. Cr:LiSAF is usable up to relatively low temperatures of around 100°C. It is applied primarily in medical applications. Cr:YAG is usable up to temperatures of around 500°C; the initial lifetime is long. Nd3+:YAG is usable at temperatures up to about 1000°C, but the problem may be an increase in the lifetime with an increasing temperature, a peak of about 700°C and a subsequent drop.Chen et al. and Wu et al. [61, 62] show the possibilities of measuring temperatures on the basis of luminescence using doped ceramic glass. Another contribution is about the sensitivity of temperature measurement using crystalline materials [63]. The construction of a measuring chain for measuring temperature using a fluorescent material is shown in the article “Small and Practical Optical Fiber Fluorescence Temperature Sensor” [22]. The article writes about a practical use of phosphorus for temperature measurement on the principle of extinction time of light luminescence. A scanning probe with a diameter of 1.8 mm was designed for the described measurement. The paper describes the measurement of temperatures using the time luminescence method, but only up to 90°C. The results of the described experimental measurement show that the measurement error can reach 0.4°C in the measured range of 0–90°C. Three types of fluorescence sensitive materials were selected for this experiment are described in the article. These are zinc-doped Mn2+ sulfide (ZnS:Mn2+), Eu3+-doped yttrium oxide (Y2O3:Eu3+), and Mn4+-doped oxyfluoride germanate. Another experiment published in the article “Low Temperature Measurement Using Fluorescence Thermometry” [64] shows a practical measurement and presents a luminescence measurement for measuring negative temperatures. A chrome-doped sapphire crystal (ruby) was used as the luminescent material. In the studied cases, the issue of the optical temperature measurement was, except for the practical examples of temperature sensors, mostly only the laboratory use of such an optical temperature sensor.


## 4.1. Description of Fluorescence

After delivery of the excitation light, the electrons move to the energy level of4T2, where they, however, do not hold and pass to the metastable level of 2E. Thanks to spin-orbit coupling [51], the metastable level of 2E is divided into two levels of −E and 2−A with the energy difference ΔE. This division of the metastable level causes the formation of two emission spectral lines. The first emission spectral line R1 is due to the transition of −E≥4A2 (694.3 nm); the second emission spectral line R2 is due to the transition of 2−A ≥ 4A2 (692.9 nm). The second emission spectral line R2 is slightly weaker than the first R1 [18, 52]. A simplified diagram of the energy levels of ruby is shown in Figure 9.Figure 9
Simplified diagram of ruby energy levels.Fluorescence is time-dependent, and after switching off the excitation light after a certain period of time called the lifetime, it disappears.For this reason, the excitation light source must be modulated by a rectangular pulse, thus alternately turning the excitation light on and off. The lifetime of the emission spectral lineR2 is ~3-3.5 ms and R1 is ~0.6 ms [15, 18].Changing the temperature leads to a change in the coupling (tension) in the crystal lattice and the distribution of phonons and energy, and consequently, it influences the fluorescence lifetime of ruby. The relatively short lifetime at the4T2 level causes the fluorescence of R lines to dominate due to the long-lasting 2E level at low temperatures (transition 2E→4A2 determines the temperature dependency of the lifetime). At room temperature (about 300 K) the lifetime is about ~3.5 ms [15, 18]. With increasing temperature, some Cr3+ ions are propped up to revert to the 4T2 level from the 2E level rapidly. With further increases in the temperature, more and more ions are propped up to this reversion, thereby emptying the 2E level and the nonradiant transitions 4T2→4A2 start to dominate. Significant loss of radiant transitions thus reduces the lifetime of fluorescence to ~1 μs at a temperature of about 600°C [15]. At the same time, the fluorescence-emitted light intensity decreases.Figure10 describes the radiant transitions of Cr3+ ions from the 2E→4A2 level at low temperatures where the nonradiant transitions from the 4T2 level are negligible due to the preferred occupancy of the 2E level. With an increasing temperature, the nonradiant transitions 4T2→4A2 start to dominate, the level 2E becomes a temporary level for the excitation of ions at the 4T2 level. The transition time 2E→4T2 is around ~7 ps. The temperature dependence of the fluorescence lifetime can be expressed by [53]
(8)τ=τS1+Cde−ΔE/kT1+τS/τie−ΔE/kT=τS1+3e−ΔE/kT1+αe−ΔE/kT,where τ is the fluorescence lifetime, ΔE is the energy difference between the levels 4T2 and 2E, τi and τs are the lives of transitions from the 4T2 and 2E levels, k is the Boltzmann constant, T is the temperature, and Cd is the ratio of degeneration 4T2/2E [54].Figure 10
Two-level ruby model.This model provides good results compared to measurements for temperatures ranging from 300 to 570 K [54].From the room temperature to about ~550 K, the lifetime is decreasing. Beyond the ~600 K limit, the4T2→4A2 transitions start to dominate, resulting in a rapid drop in the lifetime with an increasing temperature, which Equation (6) already cannot describe accurately enough.The selected article describes a simplified model for ruby that predicts changes in lifetime with changing temperatures, as shown in Figure11 [18]. This model includes the radiant 2E→4A2 and nonradiant 4T2→4A2 transitions. The schematic diagram of this model is shown in Figure 10. The lifetime of fluorescence is described by
(9)τ=τS1+3e−ΔE/kT1+αe−ΔE/kT+βe−ΔEq+ΔE,where τq is the nonradiant transition, ΔEq is the energy difference between 4T2 and 4A2, α=τs/τi, and β=τs/τq. This model is accurate from 300 to 800 K with a tolerance of ~1% over the given temperature range.Figure 11
A simplified model for ruby.


## 4.2. Absorption Spectrum

Although the absorption spectrum of ruby is strongly dependent on the polarization of the excitation light [18, 55], there are relatively small differences between the intensities R1 and R2.The absorption spectrum of ruby is spectrally broad, as shown in Figure12 [15, 18]. There are two absorption peaks around 410 and 550 nm. The emission spectrum has the main peaks, 694.3 nm (R1) and 692.9 nm (R2).Figure 12
Ruby absorption spectrum.


## 4.3. Dimensions of Crystals

Hu et al. [16] compare the lifetime of ruby luminescence for two sizes, for a smaller and a larger crystal. Measurements were conducted at temperatures ranging from 77 to 800 K. At the initial temperature, the lifetime of the small crystal fluorescence was 4.2 ms, while the lifetime of the large crystal fluorescence was 7.1 ms. This phenomenon occurs because the fluorescence light is reabsorbed in the large crystal and reexcitation occurs, thus extending the lifetime of fluorescence as the crystal radiates longer. This phenomenon, however, applies to low temperatures; from the temperature of about 0°C, the fluorescence lives balance out for small and large crystals. However, for practical applications, it is recommended that the ruby crystal size be as small as possible, just to minimize the redistribution of fluorescent light [16].


## 4.4. Concentration of Chromium in the Crystal

The fluorescence lifetime is independent of the concentration of chromium in ruby up to the critical level of about ~0.3 wt.% [56]. Higher chromium concentrations lead to a decrease in the fluorescence intensity. Additionally, over the concentration of ~1 wt.%, the lifetime is no longer simply exponential, as shown in Figure 12 [19].


## 4.5. Luminescent Experiments

Seat et al. [15] excited ruby using a laser diode with a modulated rectangular signal with a wavelength of 635 nm that flashed through the fiber optic (100/140 μm) through a 1×2 fiber coupler. The optical fiber was coupled to a ruby crystal using a silica glass tubing, both ends of which were melted, thus combining the fiber with the crystal. The sensor thus created was placed in a temperature-controlled furnace with a type K control thermocouple. The radiated fluorescence light was captured with the same optical fiber and passed through the coupler to the photodiode (APD:Si). A bandfilter>670nm was placed before the photodetector, which filtered the excitation light. The phase-locked detection (PLD) technique [57] was used to measure the ruby crystal fluorescence lifetime. The detected signal was processed to produce a recurring signal whose period was directly proportional to the time of the lifetime. This reduces the effect of the excitation light, allowing high-resolution measurements over a wide temperature range. The lifetime of ruby fluorescence was measured in the temperature range from 0 to 600°C. Around the temperature of 400°C, there was a strong drop in fluorescence. The measurement time interval was 1 s, with a resolution of 0.2°C. The results are shown in Figure 13 [15]. The following Figure 14 shows ruby fluorescence.Figure 13
Chromium concentration in ruby.Figure 14
Ruby fluorescence.Hu et al. [16] created two ruby temperature sensors, one large (0.5×0.5×2 mm) and the other small (0.3×0.3×0.05 mm). These crystals were excited with a He-Ne laser (5 mW) with a wavelength of 543.5 nm, which emitted continuous light; subsequently, this light was modulated by an acoustic-optical modulator (AOM) to rectangular pulses. As in the previous case, a 1×2 fiber coupler was used. In addition, an optical fiber with a diameter of 0.4 mm for a large sensor and a fiber with a diameter of 0.1 mm for a small sensor were used. Both threads had protection made of gold to withstand low temperatures. The crystals were also protected by the gold shield. The fibers and crystals were joined by a high-temperature adhesive. Fluorescent light was fed to an avalanche photodetector (APD). An optical filter (>690 nm) was placed before the photodetector to remove the excitation light. Measurements took place in the temperature range of 77 to 800 K (-196 to 527°C) with both sensors, so the effect of ruby crystal size on the fluorescence lifetime can be observed [16]. Figure 15 shows ruby fluorescence with two crystals of a different size.Figure 15
Ruby fluorescence with two crystals of a different size.Seat and Sharp [18] used a ruby crystal at a concentration of 0.1 wt.%. This crystal was connected to an optical fiber having a core diameter of 0.2 mm. The fiber and crystal were connected by means of a conical glass roller, at both ends of which a high-temperature ceramic adhesive was used, which joined a glass roller with a ruby at one end and an optical fiber at the other end. This sensor was inserted into a temperature-controlled furnace. The excitation light emanating from the Ar+ laser (514.5 nm) was modulated before entering the 1×2 fiber coupler. The excited light was fed to an avalanche photodiode in front of which there was an optical narrowband interference filter (694 nm, full width at half maximum FWHM±2nm) to remove the excitation light. Fluorescence lifetime measurements were carried out within the temperature range from 292 to 923 K (19 to 650°C) with a step of 50 K. Very good results were achieved up to a temperature of 773 K (500°C) when the standard deviation for this temperature was 0.32%, providing an ~2.4 K resolution. The accuracy of measurements at higher temperatures (>500°C) deteriorates due to the low fluorescence signal from ruby. The maximum deviation of the measurement was recorded at a maximum temperature of 923 K, namely, ~4.6%. The expected relatively long lifetime of fluorescence (~2-3 ms) was measured at low temperatures up to 600 K (327°C), then the lifetime decreased below 1 ms due to the increasing dominance of nonradiant transitions and heat extinction. The measured results of the fluorescence lifetime at different temperatures are shown in Table 2 [18]. Ruby fluorescence is shown in Figure 16.Table 2
The method of measurement using optical techniques.
T (K)292295323373374375423473523τ (ms)3.4203.4203.1602.6802.6702.6602.1201.5901.160T (K)573574623673723773823873923τ (ms)0.8420.8390.6150.4350.2890.1530.0820.0500.045Figure 16
Ruby fluorescence.Similar measurements can also be found in another publication [19]. For measurement, gold-coated quartz fiber with a core diameter of 400 μm was used. This sensor has been tested from 30 to 550°C. As expected, the fluorescence lifetimes were decreasing with an increasing temperature. Beyond 500°C, the fluorescence lifetime was essentially stabilized. The measurement results are shown in Figures 17 and 18.Figure 17
Ruby fluorescence lifetime.Figure 18
Intensity of ruby fluorescence.Obviously, the individual measurements are related to the types of crystals that are used for the measurements. The following part of the article deals with the analysis of crystalline materials using luminescence measurements.


## 4.6. Luminescent Material Alexandrite

Similar properties are shown by alexandrite which is hence used as a ruby. Alexandrite has a different absorption spectrum (see Figure18 [47] with respect to ruby); therefore, it is excited by another light source. To excite alexandrite, a 670 nm [46] or 633 nm He-Ne laser was deployed. Zhang et al. [47] set up a temperature sensor based on the fluorescence lifetime measurement like in the case of ruby. They performed measurements from 0 to 700°C, the results of which are shown in Figure 19 [19]. The lifetime of alexandrite fluorescence is shorter at room temperatures (300 μs) than in the case of ruby (~3.5 ms).Figure 19
Alexandrite absorption spectrum [47].Alexandrite can be produced artificially, as well as ruby, using the Czochralski method [58]. Additionally, alexandrite can be found in nature; it is mined in Brazil, Ural, Tanzania, Madagascar, and India [59].


## 4.7. Luminescent Material Cr:LiSAF

The material Cr:LiSAF is useful for temperature measurement in biomedical applications (30-50°C). Again, the fluorescence lifetime measurement is used. Zhang et al. [48] used a Cr:LiSAF laser with a wavelength of 670 nm for exciting. The excitation light was coupled to a quartz optical fiber (core 200 μm) through a 1×2 fiber coupler. At the end of the optical fiber, a Cr:LiSAF sample was attached using an adhesive. In front of the photodetector, the optical filter was deployed to suppress the excitation light. The measured results are shown in Figure 20 [19, 48]. Fluorescence lifetime at 0°C is about 64 μs and further decreases with an increasing temperature. Cr:LiSAF is usable approximately up to a temperature of about 100°C. The graph is shown in Figure 21.Figure 20
Alexandrite fluorescence [19].Figure 21
Cr:LiSAF fluorescence [8, 10].Fernicola and Crovini [21] used a Cr:YAG crystal to measure temperatures from -25 to 500°C. The graph is shown in Figure 22. Their experiment was also based on the measurement of the fluorescence lifetime. For excitation, they used a laser diode with a wavelength of 635 nm, the emission wavelength was 689 nm. They also deployed a quartz fiber with a diameter of 400 μm. The result of their measurement is shown in Figure 23 [21]. The fluorescence lifetime begins at 35 ms and decreases with an increasing temperature. The measurement was performed up to a temperature of 500°C.Figure 22
Cr:YAG fluorescence lifetime [21].Figure 23
Fluorescence lifetime cycle Cr:YAG [50].A similar measurement with the same material Cr:YAG was performed by Hehir et al. with results in Figure23 [50]. The temperature range was shifted to lower temperatures from 77 K to 420 K (−196~150°C).


## 4.8. Luminescent Material Nd3+:YAG

Another suitable material for measuring temperature is Nd3+:YAG. Grattan et al. [60] used a LED diode with a wavelength of 810 nm for excitation of the Nd3+:YAG crystal. They used 6 quartz fibers (core diameter 600 μm) for the excitation light and the emission light. The principle of the experiment is again based on the fluorescence lifetime measurement. The lifetime increases with an increasing temperature with a peak of about 700°C. With a further rise in temperature, the lifetime is decreasing. It is possible to measure temperatures up to about 1000°C. The measurement results are shown in Figure 24 [19].Figure 24
Nd3+:YAG fluorescence [19].


## 4.9. Partial Conclusion for Measurements Using Crystal Materials

The fluorescence lifetime measurement is a more convenient method of measuring the temperature, as the intensity of the emission light can vary greatly. Most commonly, ruby crystals are used. The fluorescence lifetime in ruby is measurable up to approximately 600°C. The lifetime fluorescence is also affected by the concentration of chromium in ruby and the dimensions of the crystal. The recommended concentration is about ~0.3 wt.%. Crystal dimensions should be as small as possible to avoid reabsorption and excitation, which prolongs the fluorescence lifetime. Either red or green lasers are often used for exciting ruby.Other materials capable of measuring the temperature are alexandrite, Cr:LiSAF, Cr:YAG, or Nd3+:YAG. For all measurements with these materials, a method of measuring the fluorescence lifetime was used. Alexandrite is able to react to temperatures up to 700°C. The initial lifetime is 10 times lower than the initial fluorescence lifetime in ruby. Cr:LiSAF is usable up to relatively low temperatures of around 100°C. It is applied primarily in medical applications. Cr:YAG is usable up to temperatures of around 500°C; the initial lifetime is long. Nd3+:YAG is usable at temperatures up to about 1000°C, but the problem may be an increase in the lifetime with an increasing temperature, a peak of about 700°C and a subsequent drop.Chen et al. and Wu et al. [61, 62] show the possibilities of measuring temperatures on the basis of luminescence using doped ceramic glass. Another contribution is about the sensitivity of temperature measurement using crystalline materials [63]. The construction of a measuring chain for measuring temperature using a fluorescent material is shown in the article “Small and Practical Optical Fiber Fluorescence Temperature Sensor” [22]. The article writes about a practical use of phosphorus for temperature measurement on the principle of extinction time of light luminescence. A scanning probe with a diameter of 1.8 mm was designed for the described measurement. The paper describes the measurement of temperatures using the time luminescence method, but only up to 90°C. The results of the described experimental measurement show that the measurement error can reach 0.4°C in the measured range of 0–90°C. Three types of fluorescence sensitive materials were selected for this experiment are described in the article. These are zinc-doped Mn2+ sulfide (ZnS:Mn2+), Eu3+-doped yttrium oxide (Y2O3:Eu3+), and Mn4+-doped oxyfluoride germanate. Another experiment published in the article “Low Temperature Measurement Using Fluorescence Thermometry” [64] shows a practical measurement and presents a luminescence measurement for measuring negative temperatures. A chrome-doped sapphire crystal (ruby) was used as the luminescent material. In the studied cases, the issue of the optical temperature measurement was, except for the practical examples of temperature sensors, mostly only the laboratory use of such an optical temperature sensor.


## 5. Measurement Using Fiber Bragg Gratings

Fiber Bragg gratings (FBGs) are formed in optical fibers by changes in the core refractive index. These are periodic or quasiperiodic changes in the refractive index of the optical fiber. These changes must meet the Bragg condition when the period of change in the core refractive index is equal to half wavelength or its whole multiples (long period). To ensure high efficiency, a sufficient difference between fraction indices and the core structure length is required. If a broad-scale light spectrum is fed to the FBG, the central wavelength of the FBG is reflected back and the remaining light passes through the FBG unchanged. The Bragg wavelength is calculated according to Equation (10), where λb is the Bragg wavelength, n is the refractive index of the core of the optical fiber, and Λ is the distance between the individual gratings [65–67]. Figure 25 shows the FBG in the optical fiber core. The advantages of the fiber Bragg gratings include small insertion attenuation, small dimensions, high reliability, and immunity to electromagnetic interference [28, 65, 66, 68–72].
(10)λb=2nΛ.Figure 25
FBG in a fiber [71].Changes in pressure and temperature affect the refractive index of the distance of the individual gratings, resulting in a change in the reflected wavelength. This can be roughly described by(11)Δλλ0=1−pe·ε+αΛ+αn∙ΔT,where Δλ is a wavelength change, λ0 is the initial wavelength, pe is the optical-strain coefficient, and ε is the strain acting on the FBG. The second part describes the influence of temperature on the wavelength shift, where αΛ is the coefficient of thermal expansion, which describes the grid extension due to the temperature; αn is the thermooptical coefficient describing the change of the refractive index; and ΔT is temperature change in K.Fiber Bragg gratings are highly suitable for accurate measurements of both low and high temperatures. For very high-temperature ranges, it is necessary to use high-temperature-resistant materials for the production of optical fibers and to choose a durable method for permanent FBG registration. The FBG temperature sensor solution is very simple and compact. The connection consists only of an optical source, spectrometer, divider, and the FBG—see Figure26. With the use of one optical source and spectrometer, a large number of the fiber Bragg gratings can be monitored, but the ranges of individual gratings cannot interfere with each other. The disadvantage of this solution is the thermal stabilization of the light source and the spectrometer [65–70, 73, 74].Figure 26
FBG connecting the light source and spectrometer to the FBG [75].The fiber Bragg grating is very sensitive to temperature changes. As the temperature increases, distances between the fiber Bragg gratings are widened, thus moving the central wavelength of the FBG. If it is necessary to increase the sensitivity, the FBG can be combined with a material that has a higher thermal expansion than glass.


### 5.1. Types of Bragg Gratings

We distinguish three basic types of gratings: Type I, Type II, and regenerated ones. The common type is Type I, which can be formed in many types of a germanium-doped fiber. They are very sensitive to UV light. Low-power UV lamps are used as sources which affect germanium dioxide by side-lighting of the fiber. These methods include interferometric, phase mask, and point-by-point production. These gratings are capable of measuring temperatures up to 320°C with a response of 10 pm/°C; above this temperature, they are no longer stable and degrade. The radiated part of the core has a higher index than the nonradiated core. In addition, we can use the IH type where germanium is replaced by hydrogen that absorbs UV photons or a combination of hydrogen dopants and germanium IHp, where the temperature stability is shifted up to 500°C with a response of 7 pm/°C. The last type is Id, where changes in the density of the undoped quartz core are induced by the laser (just before damaging the quartz structure) that is created. This type has higher dissipation losses than Type I but lower than Type II. In this type, the temperature stability is in the range of 500–800°C; the response is 11 pm/°C [76].Athermal gratings (Type II) can be created using powerful lasers, chemical production, and thermal regeneration. Using a high-power laser, microscopic damage is produced in the core. Due to permanent damage to the core structure without dopants, they have an increased temperature stability of over 1000°C [25].The last type is represented by the regenerated fiber Bragg gratings, which are made by annealing of the first type gratings (at temperatures above 1000°C). This makes it possible to obtain gratings with extreme stability without further degradation but at the expense of low reflectivity.The FBG can be created on a conventional SMF using a femtosecond laser. However, this structure is stable up to 1050°C, after exceeding this value, the grating is irreversibly transmitted. In this method, the fiber is markedly stressed by the temperature, and reliability and geometry are affected.Another type is a femtosecond pulse of Type II where residual stress is released due to long annealing, thus achieving the stability up to 1200°C. However, the fiber is fragile after several hours of annealing, which limits the range of its application.Other improvements came with the use of rapid air cooling when the FBG is created using a femtosecond laser, and consequently, the fiber is quickly cooled by cold air. This will stabilize the grating up to 1200°C while increasing its mechanical resistance. The grating remains unchanged for a minimum of 26 hours at 1200°C [23].The fiber Bragg gratings that are resistant even above 1500°C can be produced using sapphire fibers. The structure is written into these fibers by means of the femtosecond laser. The sapphire fiber is multimode; therefore, it has a larger reflecting bandwidth compared to the FBG in SMF [77, 78].Another option is the production of the FBG using a 193 nm ArF laser into a preheated germanium-doped quartz fiber [25].


### 5.2. Partial Conclusion for Measurement Methods Using the Fiber Bragg Gratings

There are several ways of measuring using the fiber Bragg gratings; the main advantage is always the resistance to magnetic and electrical interference. Compared to the optical methods described above, the FBG can be used not only for temperature measurements but also for measuring deformations and torques [28]. These methods can also be used in the biomedical area, for example, [26, 27] provide possibilities for monitoring the basic human functions. The article by Matveenko et al. [28] deals with the implementation of measurements in plastic materials. There is a disadvantage in some measurement applications, because of the narrow-spectrum laser source that should be thermally compensated. This disadvantage can be overcome by using wider spectrum sources, where the magnitude of the spectral shift of light reflected by the FBG is usually evaluated. Another disadvantage of the FBG is the inability to use it for high temperatures, with a higher measuring range requiring other types of gratings; lower accuracy is achieved, or the cost of these gratings increases. As standard, the FBGs are used approximately to measure temperatures up to 320°C. In special cases, resistance can be achieved up to 1500°C.


## 5.1. Types of Bragg Gratings

We distinguish three basic types of gratings: Type I, Type II, and regenerated ones. The common type is Type I, which can be formed in many types of a germanium-doped fiber. They are very sensitive to UV light. Low-power UV lamps are used as sources which affect germanium dioxide by side-lighting of the fiber. These methods include interferometric, phase mask, and point-by-point production. These gratings are capable of measuring temperatures up to 320°C with a response of 10 pm/°C; above this temperature, they are no longer stable and degrade. The radiated part of the core has a higher index than the nonradiated core. In addition, we can use the IH type where germanium is replaced by hydrogen that absorbs UV photons or a combination of hydrogen dopants and germanium IHp, where the temperature stability is shifted up to 500°C with a response of 7 pm/°C. The last type is Id, where changes in the density of the undoped quartz core are induced by the laser (just before damaging the quartz structure) that is created. This type has higher dissipation losses than Type I but lower than Type II. In this type, the temperature stability is in the range of 500–800°C; the response is 11 pm/°C [76].Athermal gratings (Type II) can be created using powerful lasers, chemical production, and thermal regeneration. Using a high-power laser, microscopic damage is produced in the core. Due to permanent damage to the core structure without dopants, they have an increased temperature stability of over 1000°C [25].The last type is represented by the regenerated fiber Bragg gratings, which are made by annealing of the first type gratings (at temperatures above 1000°C). This makes it possible to obtain gratings with extreme stability without further degradation but at the expense of low reflectivity.The FBG can be created on a conventional SMF using a femtosecond laser. However, this structure is stable up to 1050°C, after exceeding this value, the grating is irreversibly transmitted. In this method, the fiber is markedly stressed by the temperature, and reliability and geometry are affected.Another type is a femtosecond pulse of Type II where residual stress is released due to long annealing, thus achieving the stability up to 1200°C. However, the fiber is fragile after several hours of annealing, which limits the range of its application.Other improvements came with the use of rapid air cooling when the FBG is created using a femtosecond laser, and consequently, the fiber is quickly cooled by cold air. This will stabilize the grating up to 1200°C while increasing its mechanical resistance. The grating remains unchanged for a minimum of 26 hours at 1200°C [23].The fiber Bragg gratings that are resistant even above 1500°C can be produced using sapphire fibers. The structure is written into these fibers by means of the femtosecond laser. The sapphire fiber is multimode; therefore, it has a larger reflecting bandwidth compared to the FBG in SMF [77, 78].Another option is the production of the FBG using a 193 nm ArF laser into a preheated germanium-doped quartz fiber [25].


## 5.2. Partial Conclusion for Measurement Methods Using the Fiber Bragg Gratings

There are several ways of measuring using the fiber Bragg gratings; the main advantage is always the resistance to magnetic and electrical interference. Compared to the optical methods described above, the FBG can be used not only for temperature measurements but also for measuring deformations and torques [28]. These methods can also be used in the biomedical area, for example, [26, 27] provide possibilities for monitoring the basic human functions. The article by Matveenko et al. [28] deals with the implementation of measurements in plastic materials. There is a disadvantage in some measurement applications, because of the narrow-spectrum laser source that should be thermally compensated. This disadvantage can be overcome by using wider spectrum sources, where the magnitude of the spectral shift of light reflected by the FBG is usually evaluated. Another disadvantage of the FBG is the inability to use it for high temperatures, with a higher measuring range requiring other types of gratings; lower accuracy is achieved, or the cost of these gratings increases. As standard, the FBGs are used approximately to measure temperatures up to 320°C. In special cases, resistance can be achieved up to 1500°C.


## 6. Interferometric Temperature Sensors

These interferometric methods measure phase shift between two coherent beams that have travelled the same path in one or two optical fibers. In conditions when the length of both arms and their refractive index of the core is the same or in multiples of wavelengths2π rad, the resulting interference is constructive and the output of the interferometer is at a maximum. If the difference is in odd multiples of the wavelengths 2m−1π rad, the output is at a minimum. In the case of a general double-arm interferometer, the phase response increases linearly with arm length.Interferometers are able to detect 3 mechanisms that affect the optical beam: change in path length, wavelength, and change in the speed of light propagation (refractive index).A change in any of these quantities will result in a change in the phase of the wave. This depends on the path lengthL, the refractive index n, and the working wavelength λ. The phase delay of the light is given by
(12)Φ=2πnLλ.To measure the temperature, it is necessary to know information about the current value of the phase delay and wavelength shift. So, we need information about the amplitude and spectrum.The design of interferometers for temperature measurement can use different types of interferometers. A review article on interferometers is presented by Lee et al. [30] where the possibilities and uses of different types of fiber optic sensors were summarized.


### 6.1. Mach-Zehnder Interferometer (MZI)

Various types of fiber in-line MZI structures have been developed, such as tapered fiber structures in single-mode fibers [29, 79, 80].The in-line Mach-Zehnder interferometer is shown in Figure27.Figure 27
In-line Mach-Zehnder interferometer [79].Other MZI can be based on inner air microcavity [81, 82] and core-offset structures [83, 84]. The mentioned MZI are based on the difference of the effective refractive index between the core and cladding, so the temperature sensitivity is relatively low. A solution can be the use of graded index fibers as a collimator, which can achieve spectral temperature sensitivity around 12.37 nm/°C [85]. Even some hybrid solutions can be found [86, 87].With cascade connection of MZI, the temperature response of each MZI was 0.063 nm/°C from 30°C to 1000°C, 0.071 nm/°C from 30°C to 500°C, and 0.059 nm/°C from 30°C to 1000°C [31].


### 6.2. Michelson Interferometer

The Michelson interferometer comes up with the possibility of a single-ended measurement probe, so we can measure temperature at the end of the fiber [88–90]. Other configurations can employ a high birefringence fiber [91]. An advantage is that it is possible to make this interferometer easily with an ordinary optical fiber and splicer. And since silica fiber can sustain high temperatures, there is a possibility to measure in high temperatures. The maximum temperature sensitivity of 115.34 pm/°C at 550°C was achieved [92].


### 6.3. Sagnac Interferometer

This method of measurement compares two light waves that are transmitted against each other [93, 94]. If the frequencies of electromagnetic waves are different, the phase shift between them is changing with the time. As a result, we can detect interferences (periodic changes at minimum and maximum).A schematic of this type of measurement is shown in Figure28.Figure 28
Sagnac interferometer for temperature measurement [93].The light is emitted from SLED and goes through a 3 dB optocoupler. Single-mode optical fibers transfer light to the measurement part with a polarization maintaining fiber. As a result, we can measure the shift of the interference spectrum of the PMF. The sensitivity of 1.38 nm/°C was achieved within the temperature range 21–50°C [93] or even 18.27 nm/°C within the range 0–40°C [95]. However, a wide spectrum of research around this type of temperature measurement seems to be limited to temperatures of around 120°C [96]. The main reason for such limitation is the periodic nature of this measurement, also mentioned by Domínguez-Cruz et al. [97] or Cui et al. [98]. Figure 29 shows that measured waveforms have more than one spike, so we cannot perform measurements outside this limit.Figure 29
Temperature and spectrum measurement for Sagnac interferometer [97].As a result, the Sagnac interferometer is more suitable for a close range of temperatures, while offering high sensitivity. The only possibilities are decreasing the sensitivity or making the periodic effect in the waveform wider.


### 6.4. Modal Interferometer

This method is based on the reflective single-mode–multimode–single-mode fiber structure. The measurement is achieved via monitoring the spectral shift of the modal interference between the core and the cladding modes in the ended single-mode fiber. The achieved sensitivity was −92.6 pm/°C in the range of 28 to 51°C [99].Another type is a fiber optic modal interferometer fabricated by a segment of a low elliptical hollow-core photonic bandgap fiber (EHC-PBGF), where 12.99 pm/°C was achieved within the range from 30 to 110°C [100].With regard to high-temperature measurements, we can mention a thin-core fiber (TCF) modal interferometer for temperatures up to 850°C with 18.3 pm/°C sensitivity [101].Figure30 shows a schematic of a thin-core modal interferometer, where the thin-core fiber is placed between two standard single-mode fibers (SMF).Figure 30
Thin-core fiber interferometer scheme [101].Another high-temperature modal interferometer is based on a hollow-core fiber (HCF) where temperatures up to 1000°C were achieved with sensitivity up to 33.4 pm/°C [32].


### 6.5. Fabry-Perrot Interferometer

Figure31 shows a hybrid-structured Fabry-Perot interferometer (HSFPI) based on large lateral offset splicing for simultaneous measurement of the strain and temperature. An advantage of this structure is price and easy fabrication; however, spectrum measurement is not always convenient for real low-cost deployment. In this case, sensitivity of 12.71 pm/°C was achieved within the temperature range of 100–700°C [102].Figure 31
Fabry-Perrot interferometer setup [102].In articles from Wang et al. [103–105], the proposals of intrinsic and extrinsic fiber optic sensors based on the Fabry-Perot interferometer were able to measure up to 1600°C.A proposal of a fiber optic Fabry-Perot interferometric (FFPI) sensor by using PFC (photonic crystal fiber) as a high-temperature sensor was achieved by Ding et al. [33]. The measurement shows that sensitivity of 10 pm/°C can be achieved together with the temperature range over 1200°C.


### 6.6. Partial Conclusion for the Interferometric Measurement Methods

Interferometric sensors are capable of measuring high temperatures, especially with the Mach-Zehnder or Fabry-Perrot configurations. Physical limitations are given by optical fiber endurance, so there is also possibility to measure with special fibers up to 1600°C. There are also low-temperature configurations like the Sagnac interferometer which can offer much higher resolution. The resolution reaches values 18.27 nm/°C [95] in comparison with only 10 pm/°C for the Fabry-Perrot interferometer [33]. So the measurement is more precise, but the temperature range is low. A compromise between range and sensitivity is offered by MZI or Michelson.However, interferometric measurements can also be quite sensitive to ambient vibrations or other mechanical changes.


## 6.1. Mach-Zehnder Interferometer (MZI)

Various types of fiber in-line MZI structures have been developed, such as tapered fiber structures in single-mode fibers [29, 79, 80].The in-line Mach-Zehnder interferometer is shown in Figure27.Figure 27
In-line Mach-Zehnder interferometer [79].Other MZI can be based on inner air microcavity [81, 82] and core-offset structures [83, 84]. The mentioned MZI are based on the difference of the effective refractive index between the core and cladding, so the temperature sensitivity is relatively low. A solution can be the use of graded index fibers as a collimator, which can achieve spectral temperature sensitivity around 12.37 nm/°C [85]. Even some hybrid solutions can be found [86, 87].With cascade connection of MZI, the temperature response of each MZI was 0.063 nm/°C from 30°C to 1000°C, 0.071 nm/°C from 30°C to 500°C, and 0.059 nm/°C from 30°C to 1000°C [31].


## 6.2. Michelson Interferometer

The Michelson interferometer comes up with the possibility of a single-ended measurement probe, so we can measure temperature at the end of the fiber [88–90]. Other configurations can employ a high birefringence fiber [91]. An advantage is that it is possible to make this interferometer easily with an ordinary optical fiber and splicer. And since silica fiber can sustain high temperatures, there is a possibility to measure in high temperatures. The maximum temperature sensitivity of 115.34 pm/°C at 550°C was achieved [92].


## 6.3. Sagnac Interferometer

This method of measurement compares two light waves that are transmitted against each other [93, 94]. If the frequencies of electromagnetic waves are different, the phase shift between them is changing with the time. As a result, we can detect interferences (periodic changes at minimum and maximum).A schematic of this type of measurement is shown in Figure28.Figure 28
Sagnac interferometer for temperature measurement [93].The light is emitted from SLED and goes through a 3 dB optocoupler. Single-mode optical fibers transfer light to the measurement part with a polarization maintaining fiber. As a result, we can measure the shift of the interference spectrum of the PMF. The sensitivity of 1.38 nm/°C was achieved within the temperature range 21–50°C [93] or even 18.27 nm/°C within the range 0–40°C [95]. However, a wide spectrum of research around this type of temperature measurement seems to be limited to temperatures of around 120°C [96]. The main reason for such limitation is the periodic nature of this measurement, also mentioned by Domínguez-Cruz et al. [97] or Cui et al. [98]. Figure 29 shows that measured waveforms have more than one spike, so we cannot perform measurements outside this limit.Figure 29
Temperature and spectrum measurement for Sagnac interferometer [97].As a result, the Sagnac interferometer is more suitable for a close range of temperatures, while offering high sensitivity. The only possibilities are decreasing the sensitivity or making the periodic effect in the waveform wider.


## 6.4. Modal Interferometer

This method is based on the reflective single-mode–multimode–single-mode fiber structure. The measurement is achieved via monitoring the spectral shift of the modal interference between the core and the cladding modes in the ended single-mode fiber. The achieved sensitivity was −92.6 pm/°C in the range of 28 to 51°C [99].Another type is a fiber optic modal interferometer fabricated by a segment of a low elliptical hollow-core photonic bandgap fiber (EHC-PBGF), where 12.99 pm/°C was achieved within the range from 30 to 110°C [100].With regard to high-temperature measurements, we can mention a thin-core fiber (TCF) modal interferometer for temperatures up to 850°C with 18.3 pm/°C sensitivity [101].Figure30 shows a schematic of a thin-core modal interferometer, where the thin-core fiber is placed between two standard single-mode fibers (SMF).Figure 30
Thin-core fiber interferometer scheme [101].Another high-temperature modal interferometer is based on a hollow-core fiber (HCF) where temperatures up to 1000°C were achieved with sensitivity up to 33.4 pm/°C [32].


## 6.5. Fabry-Perrot Interferometer

Figure31 shows a hybrid-structured Fabry-Perot interferometer (HSFPI) based on large lateral offset splicing for simultaneous measurement of the strain and temperature. An advantage of this structure is price and easy fabrication; however, spectrum measurement is not always convenient for real low-cost deployment. In this case, sensitivity of 12.71 pm/°C was achieved within the temperature range of 100–700°C [102].Figure 31
Fabry-Perrot interferometer setup [102].In articles from Wang et al. [103–105], the proposals of intrinsic and extrinsic fiber optic sensors based on the Fabry-Perot interferometer were able to measure up to 1600°C.A proposal of a fiber optic Fabry-Perot interferometric (FFPI) sensor by using PFC (photonic crystal fiber) as a high-temperature sensor was achieved by Ding et al. [33]. The measurement shows that sensitivity of 10 pm/°C can be achieved together with the temperature range over 1200°C.


## 6.6. Partial Conclusion for the Interferometric Measurement Methods

Interferometric sensors are capable of measuring high temperatures, especially with the Mach-Zehnder or Fabry-Perrot configurations. Physical limitations are given by optical fiber endurance, so there is also possibility to measure with special fibers up to 1600°C. There are also low-temperature configurations like the Sagnac interferometer which can offer much higher resolution. The resolution reaches values 18.27 nm/°C [95] in comparison with only 10 pm/°C for the Fabry-Perrot interferometer [33]. So the measurement is more precise, but the temperature range is low. A compromise between range and sensitivity is offered by MZI or Michelson.However, interferometric measurements can also be quite sensitive to ambient vibrations or other mechanical changes.


## 7. Real Deployment and the Future

Nowadays, some manufacturers already started to focus on fiber-based sensors. Optical sensors can be specially designed to allow measurements in extreme environments including automotive [106], where temperature of the brake and the clutch can be measured in the 200–1200°C range. The advantage of this measurement is that we do not need information about low temperatures, so the blackbody measurement and IR sensor can be used. Another type of sensor is specified by the manufacturer Anton Paar [107]. This type of optical temperature sensor uses the principle of measuring with a ruby crystal. The sensor uses the principle described in the chapter on luminescence measurement. The principle of the measurement is based on measuring the temperature-dependent decay time of the ruby crystal luminescence. The sensor manufacturer provides information on temperature measurements up to 300°C. Advantages of this sensor are the calibration-free design and low-temperature measurement, which is not possible with blackbody. And a nonmetallic design also meets immunity for use in electromagnetic interference environments.The future of every method is connected to its low-cost version. So the spectrum-based sensors have a major disadvantage even if they cover the required temperature range. However, there is possibility to combine individual optical methods that are cheaper but usually suitable only for measuring a narrow temperature range. Figure32 shows the possible combination of luminescence and blackbody measurement. A suitable luminescent material can survive high temperatures during blackbody measurement together with the measurement possibility at low temperatures. Accuracy of the amplitude-based measurement could be affected during the manufacturing, so any optical sensor constructed in this manner will require calibration before being used for measuring temperatures. But the detection part of the system could be a simple photodetector, so it is still an interesting way.Figure 32
Expected signal from the photodetector using a combination of optical methods.The principle of possible connection for this method by a combination of measuring methods can be performed according to Figure33. This method of optical connection is also mentioned in the article “Temperature Monitoring System of Electric Apparatus Based On Optical Fiber Fluorescence” [108]. It can be assumed that such a sensor allows measurements from low temperatures (use of luminescence) to temperatures around 1000°C (use of blackbody radiation). This type of sensor finds application in many industrial areas in which it is necessary to resist electromagnetic interference and galvanic separation of the thermometer from the measured object for measuring high temperatures, for example, in the field of metal welding.Figure 33
A temperature measurement system for combination of measuring methods [108].


## 8. Discussion and Summary of the Pitfalls of the Individual Optical Measuring Methods Described

Several methods of temperature measurement based on optical measurement methods were presented in this article. If fiber Bragg gratings are used, this method can also be applied to measure deformations, bends, or vibrations. Generally, each method has its own pitfalls. At present, the problem of temperature measurement for most applications can be solved using the mastered and calibrated methodology using resistance or thermocouple methods. The purpose of this article was not to determine a method that would replace a specific temperature measurement using a nonelectric fiber optic probe in cases where electrical measuring probes can be unreliable due to the effects of electrical and magnetic interference. The answer to this question cannot be easily obtained. This is mainly because each system requires specific temperature ranges, the dynamics of the measuring system, the working environment, the impact of vibrations, and so on. However, the following findings can be summarized from this article. The blackbody- (greybody-) based method is suitable for temperatures operating from 500°C to 2000°C using commonly available optical fibers. In terms of mechanical design, this method appears to be the most robust one, mainly due to the fact that only the end of the glass fiber with the blackbody is brought into the measured area. This method is suitable for the use in measurement areas for measuring temperatures of 500°C and above, for simplicity; a rapid response of the measuring system can be achieved because of the good dynamics of changing the temperature of the blackbody negligible mass. However, when designing a measuring system, it is always necessary to consider the instability of this measuring chain when changing the temperature on the part of the evaluation side and the photodetector. Therefore, it is necessary to place a high emphasis on the temperature stability of the evaluation electronics or to consider these temperature changes of the photodetector and the evaluation unit when evaluating the received light power at the conversion to the measured temperature. In cases where we would like to apply the measurement methods using crystal luminescence, it is also necessary to consider the need for thermal compensation of the photodetector when evaluating the received light output. Moreover, in cases where this method is used in a real measuring chain, it is also necessary to know its temperature due to the nonlinearity of the excitation light source and to include it in the overall result evaluation. For the luminescent measurement method, the correct crystal must be selected for the measured temperature range. The dynamics of the measuring system will also depend on the size of the crystal used and the type and size of the protective shield. The method always requires an external excitation, for example, with a photodiode. The individual measuring ranges are listed in the article, and they always depend on the excitation light and crystal used. Using this crystal method, the basic advantage is the possibility to perform measurements in the temperature range 0–400°C. However, the disadvantage may be the need to use a crystal and to establish a mechanical and optical connection between the fiber and the crystal; in this case, a nonlinear transmission of optical power between the individual parts may occur due to mechanical and thermal instability. The method of the fiber Bragg gratings also provides an alternative to measuring temperatures in lower temperature ranges. When using this method, it is also necessary to take into account the temperature calibration and compensation for the excitation source and photodetector. We have a choice of several types of gratings described in this article to realize the thermal or mechanical measurements using this method. The method is particularly suitable for lower measuring ranges of up to 320°C when we achieve the required accuracy of about 10 pm/°C. For higher temperatures, the special and more expensive gratings mentioned in this article are used. The last mentioned methods are interferometric measurements. The achieved temperature range depends on the chosen configuration, and it is able to cover temperatures over 1200°C. However, interferometric measurement is able to interact with mechanical changes in the system, especially vibrations. Signal measurement also requires spectrum analysis, which creates an expensive part of the system. As a result, we can achieve fiber optic measurement in wide range of temperatures but with the limitation of sensitivity to mechanical interferences (also depends on configuration). It is possible to implement this type of measurement in laboratory conditions, but its implementation in harsh industrial environments can be difficult.


## 9. Conclusion

This article contains information and partial evaluation of various optical fiber methods in temperature measurement. It is advisable to consider measurements using optical methods in cases where the electrical and magnetic interference can be taken into account in the temperature measuring range or in cases where we need to remove the galvanic connection between the measured object and the evaluation unit. For example, optical methods can measure the temperature of electrical wires used for high-voltage and microwave applications. The article describes individual optical principles and presents the benefits and applicability of the methods mentioned. When designing the measuring chain, it is always necessary to take into account the dynamic range, the sensitivity, and the resistance to mechanical and electrical influences. It is also important to recall the necessary thermal compensation of optical receivers and transmitters in cases where it would be decided to replace the existing purely electrical modes of temperature measurement by optical methods. These optical semiconductor transmitters and receivers are usually more temperature dependent than those used to process the signal from thermocouples and resistive temperature sensors. However, in designing the temperature measuring chain using these optical methods, in addition to removing the effect of the above-mentioned magnetic interference, a long nonelectrical connection between the measured point and the evaluation unit is obtained. Designing such a measurement system is always a compromise between the price and utility value of such a system and choosing the appropriate method with the individual options described in this article.



---

*Source: 8831332-2020-10-12.xml*