A Low-Cost Wireless Temperature Sensor: Evaluation for Use in Environmental Monitoring Applications

Duick T. Young School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham, United Kingdom

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Lee Chapman School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham, United Kingdom

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Catherine L. Muller School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham, United Kingdom

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Xiao-Ming Cai School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham, United Kingdom

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C. S. B. Grimmond Department of Meteorology, University of Reading, Reading, United Kingdom

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Abstract

A wide range of environmental applications would benefit from a dense network of air temperature observations. However, with limitations of costs, existing siting guidelines, and risk of damage, new methods are required to gain a high-resolution understanding of spatiotemporal patterns of temperature for agricultural and urban meteorological phenomena such as the urban heat island. With the launch of a new generation of low-cost sensors, it is possible to deploy a network to monitor air temperature at finer spatial resolutions. This study investigates the Aginova Sentinel Micro (ASM) sensor with a custom radiation shield (together less than USD$150) that can provide secure near-real-time air temperature data to a server utilizing existing (or user deployed) Wi-Fi networks. This makes it ideally suited for deployment where wireless communications readily exist, notably urban areas. Assessment of the performance of the ASM relative to traceable standards in a water bath and atmospheric chamber show it to have good measurement accuracy with mean errors <±0.22°C between −25° and 30°C, with a time constant in ambient air of 110 ±15 s. Subsequent field tests also showed the ASM (in the custom shield) had excellent performance (RMSE = 0.13°C) over a range of meteorological conditions relative to a traceable operational Met Office platinum resistance thermometer. These results indicate that the ASM and radiation shield are more than fit for purpose for dense network deployment in environmental monitoring applications at relatively low cost compared to existing observation techniques.

Corresponding author address: Lee Chapman, School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom. E-mail: l.chapman@bham.ac.uk

Abstract

A wide range of environmental applications would benefit from a dense network of air temperature observations. However, with limitations of costs, existing siting guidelines, and risk of damage, new methods are required to gain a high-resolution understanding of spatiotemporal patterns of temperature for agricultural and urban meteorological phenomena such as the urban heat island. With the launch of a new generation of low-cost sensors, it is possible to deploy a network to monitor air temperature at finer spatial resolutions. This study investigates the Aginova Sentinel Micro (ASM) sensor with a custom radiation shield (together less than USD$150) that can provide secure near-real-time air temperature data to a server utilizing existing (or user deployed) Wi-Fi networks. This makes it ideally suited for deployment where wireless communications readily exist, notably urban areas. Assessment of the performance of the ASM relative to traceable standards in a water bath and atmospheric chamber show it to have good measurement accuracy with mean errors <±0.22°C between −25° and 30°C, with a time constant in ambient air of 110 ±15 s. Subsequent field tests also showed the ASM (in the custom shield) had excellent performance (RMSE = 0.13°C) over a range of meteorological conditions relative to a traceable operational Met Office platinum resistance thermometer. These results indicate that the ASM and radiation shield are more than fit for purpose for dense network deployment in environmental monitoring applications at relatively low cost compared to existing observation techniques.

Corresponding author address: Lee Chapman, School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom. E-mail: l.chapman@bham.ac.uk

1. Introduction

Near-surface air temperature is of interest for a wide range of applications, such as frost protection in agriculture (Beckwith et al. 2004) or within urban areas, where the well-documented urban heat island (UHI) effect (e.g., Stewart and Oke 2012) has implications for the health and well-being of residents. However, there is a paucity of routine observations due to a multitude of factors, including the cost of instrumentation, security concerns, and siting requirements (Muller et al. 2013a). Thus, observations are often limited to one or two meteorological stations that may neither be collocated with nor truly representative of the surrounding environs in respect to the application, and are certain not to capture smaller-scale variability, which may be of significant importance. With lower-cost meteorological sensors becoming available, of accuracy claimed to be comparable to existing instrumentation, there is scope to deploy high-density networks of sensors to identify spatiotemporal patterns of meteorological variables across environments of interest, such as cities (Muller et al. 2013b) or vineyards (Matese et al. 2009). This potentially transformative approach would enable observation of the dynamic nature of temperature patterns in more detail than previously possible and could be used to aid real-time decision making (e.g., building energy usage, frost protection), data assimilation to improve and evaluate model performance (Chen et al. 2012), ground-truth remote sensing (Tomlinson et al. 2012), and verify crowd-sourced data quality (Overeem et al. 2013) at an unprecedented scale. However, confidence in the quality of measurements made by lower-cost sensors needs further investigation.

This paper investigates the performance of a low-cost sensor with custom radiation shield (purchased together for approximately USD$150): the Aginova Sentinel Micro (ASM, Aginova Inc., Mason, Ohio). Although this sensor was developed specifically for deployment within HiTemp (high-resolution temperature measurements within the urban environment) (Muller et al. 2013b), it is applicable to other situations that may benefit from a dense network (e.g., source area studies, atmospheric profiles) and those that require a rapid response to changing temperature conditions (e.g., ripening and frost detection for high-value crops in orchards and vineyards; Beckwith et al. 2004; Matese et al. 2009). An advantage of this sensor over existing low-cost air temperature sensors is inbuilt Wi-Fi communications that allow transmission of data from sensor to server (either through existing wireless Internet infrastructure or via ad hoc networks formed of a computer and a wireless router), in near–real time.

2. Wireless temperature sensor

The ASM (Fig. 1) is a 10-kΩ negative temperature coefficient thermistor connected to a low-powered wireless communications card contained within a weatherproof enclosure (further specification given in Table 1). Power is provided by a single-cell AA 3.6-V lithium-thionyl chloride battery that is capable of providing the peak current (150 mA) required for radio transmission and, under good wireless network conditions, is reported to last up to 3 years (Aginova Inc. 2013).

Fig. 1.
Fig. 1.

Annotated photograph of the ASM sensor and radiation shield (with cut away section) developed with and parts provided by Aginova Inc.: A: additional shielding above sensing volume, B: black matte paint on underside of shield plates, C: nylon nut and bolt (M10) and probe sheathing (40 mm), D: ASM sensor housing and thermistor probe with 120-mm cable (different lengths available on request), E: plastic spacer (45 mm) to reduce antenna interference, and F: aluminum base plate (shield base: 110 mm × 110 mm; mounting face: 110 mm × 30 mm).

Citation: Journal of Atmospheric and Oceanic Technology 31, 4; 10.1175/JTECH-D-13-00217.1

Table 1.

Manufacturer specifications plus test results for three low-cost temperature sensors (Aginova Inc. 2013; Hubbart et al. 2005); Maxim Integrated (2014); Onset Computer Corporation (2014); Whiteman et al. 2000).

Table 1.

Data communication uses standard Institute of Electrical and Electronics Engineers (IEEE) 802.11 b/g 2.4-GHz Wi-Fi at bit rates of up to 11 Mbps. When located on existing Wi-Fi hotspots/networks, the sensor utilizes limited bandwidth (user datagram protocol packets ≈2 kB) and poses minimal risk to security, as sensor to Internet data packets are secured using the latest encryption and all communications are sensor initiated. Data packets are transmitted periodically (user definable) through the Internet (or local ad hoc network) to a server with Aginova WiBox software. The software manages sensor-to-server communication and enables sensor configuration and the viewing/downloading of data. Figure 2 provides an overview of communication pathways, sensor settings, and software.

Fig. 2.
Fig. 2.

Schematic of ASM communication pathways, user-definable settings, and server software features.

Citation: Journal of Atmospheric and Oceanic Technology 31, 4; 10.1175/JTECH-D-13-00217.1

The sensor has limited flash memory (1440 data points = 24 h with 60-s sampling); therefore, raw data are not stored on the sensor long term but are transmitted periodically to the server. To ensure continuity of data collection, data are kept until receipt confirmation is returned by the server. In locations with intermittent Wi-Fi, further safeguards can be applied via a conditional storage mode, so that data are only logged when there is a temperature change ≥±0.1°C between samples and server communication has been lost.

Thus, the self-contained ASM sensor requiring no additional power or communications, coupled with its lower-cost enables deployment of large numbers at a range of spatial scales, provided an accessible wireless network is available (e.g., Muller et al. 2013b).

3. Radiation shield

An initial assessment of existing commercially available radiation shields revealed that many were more expensive than low-cost sensors, requiring a large capital outlay for network deployment. To address this, a custom nonaspirated radiation shield was designed for the ASM.

Following a review of the radiation shield literature (e.g., Anderson and Baumgartner 1998; Richardson et al. 1999; Nakamura and Mahrt 2005; Thomas and Smoot 2013) and a number of design iterations and field tests, a custom shield formed of 10 UV-resistant pressure-molded plastic plates was produced (Fig. 1). The design incorporates a fixing for the sensor housing and a nylon bolt to hold the probe within the sensing volume; this coupled with additional rubber sheathing around the probe base minimizes conduction. Plastic spacers located above the base reduce signal interference to the antenna. The underside of the middle plates are painted matte black, which is now standard in Met Office (UKMO) plastic Stevenson screens (Perry et al. 2007), to reduce error due to reflected solar radiation. Testing of an unpainted design with a SKS1110 pyranometer (Skye Instruments, Llandrindod Wells, United Kingdom) mounted within the radiation shield (after Hubbard et al. 2001) found between 50% and 75% of reflected solar radiation in the sensing volume. After application of the paint, this was reduced to <5%. The shield plates are held together by four metal threaded bars screwed into the top plate and secured to the base plate, which can be customized to meet site mounting requirements (51-mm stainless steel U-bolts used in field testing).

4. Methods

a. Time constant

The time constant, the time taken to reach 63.2% of a prescribed step change (e.g., Whiteman et al. 2000), for operational air temperature sensors is required to be <20 s to meet World Meteorological Organization (WMO) specifications (WMO 2008). Typically low-cost temperature sensors do not meet this requirement due to their construction. This deficiency can be overcome by selecting an appropriate sampling rate that is representative of the process observed (1 and 60 s for laboratory and field, respectively, in this study) before being averaged over a longer (15 min) period (Kurzeja 2010).

The time constant of five randomly selected ASMs were measured in a naturally ventilated laboratory following a step change of −10° to 25°C, generated by removal from a freezer into a warm room (after Whiteman et al. 2000). The ASMs were tied together, so the tips of the probes were reasonably close to each other but not touching. The process was repeated three times with a sensor sampling rate of 1 Hz.

b. Accuracy

The accuracy of four ASMs was tested over a temperature range of −25° to 40°C as part of an academic collaboration with the UKMO in their Instrumentation Laboratory. Two sensors were placed in a Vötsch Industrietechnik VT4011 atmospheric chamber (Balingen, Germany) and compared against a Thermocoax Air Platinum Resistance Thermometer (Flers, France); the other two sensors were submerged in a PSL Scientific System 1 water bath (Clausthal-Zellerfeld, Germany) and compared with a Tinsley SPRT “C” (serial number 238 701; Redhill, United Kingdom) connected to an AΣA Automatic Systems Laboratories resistance bridge (model F17A; Redhill, United Kingdom). Both systems have a certified National Physical Laboratory (NPL) calibration uncertainty of ±0.1°C (calibrated 2012).

c. Field tests

Three ASMs were deployed (60-s sampling) within the custom radiation shield over eight test periods (of varying lengths) between January and July 2013, at the UKMO Winterbourne No. 2 meteorological observation site (52.456°N, −1.927°W; elevation 140 m; metadata at http://www.bucl.bham.ac.uk/data/WinterbourneNo2_metadata.pdf; Muller et al. 2013c). Sensors were mounted onto a test bed frame at a height of 1.25 m over grass (no snow occurred during the tests), between 2 and 3 m to the west of the station Stevenson screen that housed the UKMO platinum resistance thermometer (PRT) (1-min average data). The screen PRT was selected as the reference due to its operational usage, traceability against national standards due to annual calibration, and the absence of an aspirated radiation shield at the site.

Additional observations for analysis of shield performance included incoming shortwave solar radiation using a Kipp & Zonen CMP 3 (Delft, Netherlands) and wind speed (1.25 m) using a Gill WindSonic (Lymington, United Kingdom) sampling at 1 Hz.

d. Data analysis techniques

For analysis, raw 60-s air temperature data from each ASM were corrected based on temperature offsets determined from the accuracy tests (section 4b) before being averaged over 15-min periods to account for differences in sensor and PRT time constants and sampling frequency (Kurzeja 2010).

Exploratory autocorrelation analyses of the 15-min ASM and PRT (Met Office 2013) mean data highlighted statistically significant serial dependence. To assess goodness of fit between each sensor and the PRT, generalized additive models (GAMs) were used, as they are suitable for serially autocorrelated data. GAMs, which use nonparametric functions to maximize the quality of fit to the data (Hastie and Tibshirani 1990; Wood 2004), were fit using the mixed GAM computation vehicle (mgcv) package in R (Wood 2013). The PRT observations were used as the independent variable.

5. Results

a. Time constant

The time constant, calculated from the 15 samples, of the time taken for sensors to reach 12.1°C (63.2% of −10° to 25°C step change) in ambient air was 110 s with a standard deviation of ±15 s. Although this time constant is slower than that recommended (WMO 2008) for operational instrumentation (sampling rates <60 s), it is of similar magnitude to other low-cost thermistor probes currently available (e.g., HOBO H8 Pro; Table 1; Whiteman et al. 2000).

b. Sensor accuracy

Tests undertaken at the UKMO Instrumentation Laboratory indicated that all four sensors observed temperatures were within ±0.22°C (over the range −25° to 30°C) of that of the water bath and chamber (Fig. 3). This is smaller than the error ranges obtained by Aginova (Table 1) in their laboratory sensor resistance testing (K. Baumgartner 2011, personal communication). When the sensors were within the water bath, they were within ±0.1°C across the same temperature range. At 40°C the difference was found to be slightly greater (±0.27°C) in both media, in part due to the nonlinear relation between resistance and temperature of thermistor probes (McGee 1988).

Fig. 3.
Fig. 3.

Observed temperature errors of four ASM probes (serial numbers given in key) relative to a reference temperature (UKMO PRT, traceable to national standards) of a water bath (superscript W) and atmospheric chamber (superscript C) during experiments undertaken within the UKMO Instrumentation Laboratory. Dashed line represents the probe accuracy as reported by Aginova.

Citation: Journal of Atmospheric and Oceanic Technology 31, 4; 10.1175/JTECH-D-13-00217.1

c. Field tests

The general field performance of three ASMs was assessed using 15-min averaged data from the UKMO Winterbourne No. 2 meteorological observation site. A GAM was fit to data from 6006 periods, during which screen temperatures were between −3.9° and 29.3°C. Temperature errors (TError = TASMTGAM) ranged from −0.76° to 2.56°C, with the largest errors typically occurring around sunrise, although such errors were not seen consistently (Fig. 4). This could be a result of low sun angles increasing radiation error (Anderson and Baumgartner 1998) or more probably when there is limited mixing, resulting in poor ventilation through the shield because conditions are stable with low friction velocity (Richardson et al. 1999; Harrison 2010). As the larger errors [TError > ±3 × interquartile range (IQR); 2.0% of data] occurred at low wind speeds (<1 m s−1; Fig. 4), poor ventilation is the most likely reason. However, PRT observation errors are likely large at these times, as it is housed in an unventilated screen (Harrison 2010). Despite these few large errors, the root-mean-square error (RMSE) for the whole period was 0.13°C. This is marginally larger than the measurement uncertainty of the PRT.

Fig. 4.
Fig. 4.

Temperature errors (°C) determined using a GAM analysis of 15-min average air temperature from three ASM sensors (serial numbers 12 681, 12 682, and 12 672), in custom radiation shields, relative to screen UKMO PRT temperature during field trials conducted over eight periods (of varying lengths) between January and July 2013. The hourly IQR (25th and 75th percentile) boxplots have ±1.5 IQR whiskers plus horizontal lines at ±3.0 IQR. Points above/below these points are considered outliers. The 15-min average sonic anemometer wind speed (U, m s−1) observed at 1.25 m for each TError is represented by the symbols given in the figure legend.

Citation: Journal of Atmospheric and Oceanic Technology 31, 4; 10.1175/JTECH-D-13-00217.1

Analysis of day (1000–1500 UTC, 1214 periods) and night (2200–0400 UTC, 1534 periods) TError showed RMSEs of 0.10° and 0.11°C, respectively. It is encouraging that 95% of temperature errors had a magnitude of <0.27°C during night periods when wind was <1.0 m s−1, with no errors exceeding 0.61°C. The application of a black coating on the underside of the radiation shield appears justified, as temperature error magnitude did not exceed 0.42°C during the day hours when solar irradiance was at its maximum (observed range: 8.5–1031 W m−2), even at wind speeds <1 m s−1, where the magnitude of 95% of errors did not exceed 0.22°C.

The overall performance of the custom radiation shield is particularly promising due to the magnitude of temperature errors (95% of data) being <±0.24°C for all conditions (Fig. 4). The daytime RMSE (0.10°C) exceeds the performance of other field tests of low-cost sensors in unaspirated shields (e.g., Whiteman et al. 2000: 0.2°C; Nakamura and Mahrt 2005: 0.39°C) albeit under differing meteorological conditions. Further reduction in measurement uncertainty may be achieved by determining a radiation correction for the shield using a combination of modeling and observation (e.g., Nakamura and Mahrt 2005; Mauder et al. 2008) and increasing ventilation of the sensing volume (Harrison 2010).

6. Conclusions

Testing of the low-cost ASM sensor shows it to perform very well relative to national standards in the laboratory [accuracy <±0.22°C (−25° to 30°C)] and traditional traceable operational observing techniques (PRT) in the field (daytime RMSE = 0.10°C), as well as relative to existing lower-cost sensors on the market (Table 1). This performance coupled with Wi-Fi connectivity enables sensors to collect and provide raw sampled data in near–real time to end users. This has the potential benefit of allowing deployment in large numbers of locations that may include those where current operational observation methods are impractical, coupled with being able to provide the data rapidly to a wide range of end users who are eager to have data in such places for decision making and real-time operations (Grimmond 2013).

The custom shield shows promising performance in initial field tests with very few large temperature errors relative to the screen PRT during periods of high solar insolation even when wind speeds were low (<1 m s−1). During periods of low wind speed despite errors being slightly larger, the majority (95%) of observations were within ±0.24°C of an UKMO PRT.

Ongoing work is underway to test sensor–shield performance over a wider range of meteorological conditions, to determine if sensor calibration drift is a problem after extended deployment in the field, and to gain a better understanding of the radiation error (both longwave and shortwave) within the sensing volume, so that an appropriate correction factor could be determined. Notwithstanding these ongoing tests, it is concluded that the low-cost ASM sensor and radiation shield are more than fit for purpose for network deployment in environmental monitoring applications.

Acknowledgments

This work is funded by the U.K. Natural Environment Research Council (NERC)’s “Network of Sensors” project HiTemp (Grants NE/I006915/1 and NE/I007032/1; further information at www.bucl.org.uk). The authors thank Mike Molyneux and Paula Taylor for use of UKMO’s testing laboratory; Aginova Inc. for their collaboration in the development of the sensor and radiation shield; and from the University of Birmingham, Elliott Warren, Grace Garner, Sophie Bland, and Richard Johnson.

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Save
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    • Search Google Scholar
    • Export Citation
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  • Fig. 1.

    Annotated photograph of the ASM sensor and radiation shield (with cut away section) developed with and parts provided by Aginova Inc.: A: additional shielding above sensing volume, B: black matte paint on underside of shield plates, C: nylon nut and bolt (M10) and probe sheathing (40 mm), D: ASM sensor housing and thermistor probe with 120-mm cable (different lengths available on request), E: plastic spacer (45 mm) to reduce antenna interference, and F: aluminum base plate (shield base: 110 mm × 110 mm; mounting face: 110 mm × 30 mm).

  • Fig. 2.

    Schematic of ASM communication pathways, user-definable settings, and server software features.

  • Fig. 3.

    Observed temperature errors of four ASM probes (serial numbers given in key) relative to a reference temperature (UKMO PRT, traceable to national standards) of a water bath (superscript W) and atmospheric chamber (superscript C) during experiments undertaken within the UKMO Instrumentation Laboratory. Dashed line represents the probe accuracy as reported by Aginova.

  • Fig. 4.

    Temperature errors (°C) determined using a GAM analysis of 15-min average air temperature from three ASM sensors (serial numbers 12 681, 12 682, and 12 672), in custom radiation shields, relative to screen UKMO PRT temperature during field trials conducted over eight periods (of varying lengths) between January and July 2013. The hourly IQR (25th and 75th percentile) boxplots have ±1.5 IQR whiskers plus horizontal lines at ±3.0 IQR. Points above/below these points are considered outliers. The 15-min average sonic anemometer wind speed (U, m s−1) observed at 1.25 m for each TError is represented by the symbols given in the figure legend.

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