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Using Cellular Communication Networks to Detect Air Pollution Noam David, and H. Oliver Gao Environ. Sci. Technol., Just Accepted Manuscript • DOI: 10.1021/acs.est.6b00681 • Publication Date (Web): 04 Aug 2016 Downloaded from http://pubs.acs.org on August 5, 2016
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Environmental Science & Technology
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Using Cellular Communication Networks to
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Detect Air Pollution
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Noam David† and H. Oliver Gao†‡*
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†
The School of Civil and Environmental Engineering, Cornell University, Ithaca, NY,
14853, United States. ‡
One-Hundred Talents Scholar, School of Hydraulics, Changsha University of
Science and Technology, Hunan Province, China
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ABSTRACT
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Accurate real time monitoring of atmospheric conditions at ground level is vital for
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hazard warning, meteorological forecasting and various environmental applications
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required for public health and safety. However, conventional monitoring facilities are
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costly and often insufficient, for example, since they are not representative of the
27
larger space, and are not deployed densely enough in the field.
28
There have been numerous scientific works showing the ability of commercial
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microwave links that comprise the data transmission infrastructure in cellular
30
communication networks to monitor hydrometeors as a potential complementary
31
solution. However, despite the large volume of research carried out in this emerging
32
field during the past decade, no study has shown the ability of the system to provide
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critical information regarding air quality.
34
Here we reveal the potential for identifying atmospheric conditions prone to air
35
pollution by detecting temperature inversions that trap pollutants at ground level. The
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technique is based on utilizing standard signal measurements from an existing cellular
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network during routine operation.
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INTRODUCTION
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A wide spectrum of severe and chronic health impacts are associated with air
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pollution. The US Environmental Protection Agency (EPA), for instance, is
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responsible for setting the national ambient air quality standards for six pollutants
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commonly found in the air: particulate matter (PM), ground-level ozone, carbon
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monoxide, nitrogen oxides - NOx (a generic term for NO and NO2), sulfur oxides, and
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lead. Of these contaminators, also known as “criteria pollutants”, PM that is 10
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micrometers in diameter or smaller (PM10), and particularly that of 2.5 micrometers
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and below (PM2.5) is of main concern, as these can generally pass through the human
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respiratory pathways and enter the lungs and bloodstream. Once inhaled, they can
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cause acute health damage, including lung cancer and other cardiopulmonary
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mortality.1 According to the World Health Organization (WHO), in the year of 2012,
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for example, 3.7 million premature deaths worldwide were attributable to ambient air
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pollution.2
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Notably, temperature inversion (TINV) within the boundary layer has been found to
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be a major contributor to events of poor air quality worldwide.3-11 In typical
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conditions in the lower atmosphere, temperature decreases as altitude increases.
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TINV, on the other hand, is a case where the temperature in a certain layer increases
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with an increase in altitude. 11-14 The resulting stagnation inhibits vertical motion in
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the atmosphere, creating ideal conditions for increased contaminant concentrations
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when formed close to the surface, since air pollutants released into the atmosphere's
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lowest layer are trapped near the ground beneath a warmer air stratum. As reviewed
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by Bailey et al.8, in European cities, for example, both elevated and ground-based
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TINVs have been found to coincide with events of excessive PM concentration.6
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Anthropogenic emission of particulates, or the suspension of dust are certainly the 3 ACS Paragon Plus Environment
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root causes of these periods of poor air quality. Still, regardless of whether the high
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pollution event was in a maritime or continental climate, over complex terrain or
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elsewhere, a temperature inversion was also present, intensifying the conditions of
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poor air quality, and preventing dissipation of polluted air. An additional example has
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often been cited from Logan, Utah, USA, where during the winter of 2004, a series of
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elevated PM events occurred, coinciding with strong winter TINVs.15 Moreover,
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TINVs have been linked with respiratory16 and cardiovascular 10, 17 diseases. Thus, the
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trapping of pollutants, and their precursors at ground level by inversions, has crucial
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public health implications.
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Beyond the adverse effects caused by TINVs intensifying air pollution and human
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health hazards, a combination of an inversion and high Relative Humidity (RH>95%)
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trapped at the bottom of the stable layer creates favorable conditions for the creation
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of fog18-20, which is in itself a natural hazard with potentially destructive
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repercussions.21-23
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Existing tools for inversion monitoring are based on limited in-situ measurements or
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remote sensing observations. Instrumented towers, which have temperature sensors
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installed on them at different altitudes and radiosondes, are the common instruments
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for direct in-situ monitoring. While these tools provide precise measurements, their
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spatial coverage and representativeness is poor due to the specific point
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measurements. Remote sensing systems24-25 are limited in many conditions. Lidar
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ceilometers, for example, have difficulty in detecting the inversion layer during fog.26
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Aside from the specific technical limitations of each method reviewed above, the
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instrument costs are high, and they require continuous maintenance and operation. 27
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Consequently, deployment of these tools is insufficient in terms of both coverage and
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resolution. Satellite systems produce measurements at a better spatial resolution,
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including from various surfaces, such as oceans and the Arctic, where it is difficult to
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measure.28 However, while the vertical resolution of these systems is good at higher
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altitudes, remote sensing from satellite systems is lacking for measurement of TINVs
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that are low to the ground level (e.g. McGrath‐Spangler and Denning 29), which
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happen to be the inversions that are critical in the creation of the conditions for
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extreme air pollution.
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In this study we show the potential for detecting low lying inversions using received
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signal level (RSL) measurements taken by cellular communication networks. Weather
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phenomena and variations in atmospheric conditions interfere with the
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electromagnetic waves transmitted by commercial microwave links (MLs) that
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comprise the infrastructure for data transport between cellular base stations. Thus,
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cellular network infrastructure provides, in essence, an already existing atmospheric
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monitoring facility, as was first demonstrated for rainfall measurements30,31 , although
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these networks were not originally intended for this purpose. MLs are deployed over a
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wide geographic expanse and close to ground level, typically at elevations of tens of
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meters above the surface. These links operate at frequencies of tens of GHz and are
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widely deployed around the world, including in many developing countries (e.g.
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Doumounia et al.41). Thus, this technology can provide a low cost monitoring solution
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in regions where conventional measurement tools are limited or non-existent. So far,
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most of the research projects on this topic have focused dominantly on the ability of
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this system to monitor and map rainfall since, comparing to other hydrometeors,
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raindrops induce predominant transmission losses to the microwave channel.30-42 Only
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few other works have pointed out the technology's potential for monitoring additional
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hydrometeors, including water vapor,43, 44 fog45, 46 and dew47. The common factor of
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all research carried out to this point is that they rely on the signal loss measured by the
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wireless network to detect and estimate the intensity of the weather phenomenon
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observed.
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Notably, low lying inversions induce a unique effect on the microwave beam. In cases
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of inversion a layering occurs that manifests in a change of the profile of the
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atmospheric refraction index as elevation increases. As a result, the atmosphere may
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operate as a waveguide, due to the channels or ducts that form in it. A scenario called
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multipath may also occur, in which, several waves arrive at the receiver due to
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reflections from the layers with the different refraction indices.48 These phenomena
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may lead to an amplification of the received signal when compared to the standard
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case. Consequently, detection of this effect using commercial microwave networks
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can be utilized to identify low lying inversions that are prone to hazardous conditions
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for public health and safety. We demonstrate the novel concept by analyzing extreme
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air pollution events using standard measurements of existing commercial microwave
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links. Additional proof of feasibility for detection of low lying inversions using the
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proposed technique is demonstrated during a heavy fog event.
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METHOD
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Atmospheric Refractivity
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Snell's law, given by Equation (1), describes the angle of refraction of a wave passing
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through a boundary between two different isotropic media:
n1 sin 1 n2 sin 2
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Where:
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n1 – The refractive index of the first medium.
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n2 – The refractive index of the second medium.
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ϕ1 – The angle of incidence.
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ϕ2 – The angle of refraction.
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Figure 1(A) shows the path of a wave according to this law. Note that the larger the
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refractive index of one medium is than the other, the greater the angle of refraction is
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in relation to the angle of incidence. Part of the beam is returned at an angle equal to
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the angle of incidence (the red trajectory).
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If the wave enters the boundary at an angle greater than the critical angle, total
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internal reflection will occur (the blue trajectory). The magnitude of the critical angle
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can be used as a measure of the intensity of guided propagation, i.e. of how much
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radiant energy is trapped within the duct.49
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The atmospheric refractive index can be expressed by the following relation:
n 1 N 106
157
(N-Units)
(2)
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Where N is the refractivity which can be computed according to the following
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formula:50, 51
N Ndry Nwet 77 .6
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e P + 3.732 105 2 T T
(N-units)
(3)
where:
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P-
total atmospheric pressure (hPa).
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T-
absolute temperature (K).
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e-
partial water vapour pressure (hPa).
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For frequencies up to 100 GHz, the expression above has an error of less than 0.5%.51
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Let the gradient of a given parameter X with altitude H, be denoted as- X'= dN/dH.
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Derivating Eq. (3) and substituting typical values of 1013 millibar, 15 C, and 15
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millibar for the pressure, temperature and water vapor pressure, respectively, we get
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the following expression describing the dependency of refractivity N on the
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atmospheric parameters:52
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N ' 0.27 P' 4.5e' 1.18T '
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(N-units/km)
(4)
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Note that temperature and moisture are the dominant factors functioning jointly to
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generate the meaningful variations in refraction. Typically, the inversion is
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accompanied by sufficient humidity gradient. The variations of refractivity N due to
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pressure fluctuations are negligible since wind gusts rebuild equilibrium.
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It can be shown53 that the gradient of N with altitude (dN/dH) is relatively equal to the
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radius of curvature of the microwave ray -
dN N dH H
:
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ML
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Atmospheric Microwave Propagation
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The propagation of a wave in lower troposphere can be categorized into four cases
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according to the changes in refractive index with altitude:52, 54
(N- units/km)
(5)
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I
N -76 to 0 (N-Units/km): Normal H
(6)
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II
N 0 (N-Units/km): Sub refraction H
(7)
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III -157
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IV
N - 76 (N-Units/km): Super refraction H
N - 157 (N-Units/km): Ducting H
(8) (9)
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Figure 1(B) schematically describes the beam propagation in the medium under each
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of these four cases.
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Normal Propagation – In standard conditions in the lower troposphere the typical
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gradient of N is around −40 N-units/km,53 and may vary somewhat51 from area to
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area, and from season to season. As a result of the moderate gradient of N with
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altitude in these conditions, a wave propagating through the medium is refracted
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downwards slightly, according to Snell's law, as shown by the curve signified as 8 ACS Paragon Plus Environment
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"Normal" in Fig. 1(B) that simulates the path of microwave radiation between the
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transmitter and receiver in standard atmospheric conditions. Commercial MLs are
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designed to take this effect into consideration.
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Cases where the gradient of N is different from the standard case (cases II through IV)
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cause anomalous propagation of waves in the atmosphere.
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Sub Refraction- A condition where the wave is refracted less (sub-normally) with
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respect to the standard condition, and in a manner that can often cause the upward
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bending of the wave causing it to move further away from the surface with distance
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from the transmitter.
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The generating factor of the following phenomena - super refraction and ducting, is
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typically a temperature inversion.49, 54
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Super Refraction –In this situation, the gradient of the refractive index with altitude
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in the layer is higher than the standard case, and will cause increased bending of the
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microwave radiation towards the Earth. As a result, a phenomenon called multipath
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may occur – the arrival of two or more waves at the receiver.48 This causes
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constructive and destructive interference which results in relative amplification, or
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attenuation of the received signal, respectively. A boundary case of super refraction is
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the case known as ducting.
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Ducting – Earth's radius is approximately 6,400 km and therefore Earth's curvature
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is: Earth 157 (km-1). Thus, by Eqs. (2) and (4) in a case where dN/dH = −157 (N-
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Units/km), the radio waves will travel parallel to Earth's curvature. When dN/dH
c ). The trajectory in red describes the refraction angle of the beam (Φ2), and the
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angle of reflection (which is equal to the angle of incidence). (B) Beam bending during standard, sub-refractive and super refractive conditions. Under ducting conditions, beam trapping occurs.
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RESULTS
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Using central Israel as an illustrative case, we investigated the potential of
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commercial microwave systems for detecting near-ground inversions that formed a
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basis for the development of extreme air pollution events and fog. The ML
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measurements were compared to lidar ceilometer measurements that detected the
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mixing layer height coupled to the altitude of the inversion.9 This height represented
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the upper bound of a ground inversion, or the elevation of the inversion base in cases
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where it occurred at higher altitudes (we also used the radiosonde measurements to
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assist in this determination).
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Additionally, comparisons were made to measurements of air pollutants (PM-10 and
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NOx) that were found in prior research to have increased concentrations during near-
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ground inversions.6,9,10,58 In their standard configuration, the microwave networks
Typical atmospheric stratification in cases of inversion. The refraction coefficient of the middle layer where the wave propagates (n2) is higher than those of the two layers confining it (n1, n3). According the Snell's law (Eq. 1), when the angle of incidence (Φ1) is greater than the critical angle (indicated as c ) total internal reflection occurs (the path indicated in blue
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used for this research are set up to log the minimum and maximum RSL measurement
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in intervals of 15 minutes. We used the maximum RSL measurements which, by
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definition, would capture cases where the RSL is increased when compared to the
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standard case. Accordingly, the proprietary sensor measurements are based on quarter
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hourly averages.
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Figure 2(A) shows the relative location of the research area on a map of Israel. Beside
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it, Fig. 2(B) maps the location of MLs, the air pollution measuring stations,59 and the
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meteorological ground stations60 from which data was taken. The monitoring stations
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and links shown for event 1 are indicated in red, those used in event 2 are indicated in
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green, and those used in event 3 are colored blue. The instruments used to detect the
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inversion layer were a Lidar ceilometer located at the Beit Dagan ground station (35
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m ASL), and a radiosonde released from that station twice every 24 hours at 00:00
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and 12:00 (All times in this paper are stated in Universal Time Coordinated).
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In cases where the inversion layer was not detected by the ceilometer due to
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obstruction by low level clouds, the level of the cloud base was taken as a reference
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altitude (these cases are indicated in the ceilometer figures with a blue line, see Figs.
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3F and 5D). The calculations of the refraction gradient with elevation (N/H) in the
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cases of inversion studied were based on the Beit Dagan radiosonde samples (the
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symbol indicates a discrete calculation). In the few cases where no specific
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measurements were taken by the proprietary instruments, an average of adjacent
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measurements was taken (these time periods were all shorter than or equal to half an
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hour).
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Figure 2. A) Israel map. The research area focused on the center of Israel. An enlarged insert map of this area is given in Fig, 2(B). B) Microwave network and atmospheric measurement stations. Each of the three colors (Red, Green, Blue) appearing in the figure indicates the MLs and measuring stations used in each of the three events described below. Red – Event 1, Green – Event 2, Blue – Event 3. Each line represents two links operating over the same propagation path at two different frequencies between 18 and 19 GHz. The line near Tel Itzhak represents a single ML operating at a frequency of 23 GHz. Link lengths are between 6.1 and 14.3 kilometers. The elevations of the MLs indicated in red and blue vary between 41 and 87 meters ASL. The elevations of the MLs indicated in green vary between 116 and 316 meters ASL. Additionally, the meteorological ground stations at Beit Dagan (35 m ASL) and the air quality monitoring station in Holon (24 m ASL), Road 4 (50 m ASL), and Yad Rambam (92 m ASL) are shown. The location of the city of Tel Aviv is indicated with a star.
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NOx Episode and ML Measurement: the Air Pollution Event on November 14,2010
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According to the Israeli environmental protection agency, two episodes of extreme air
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pollution took place in central Israel on November 14th, 2010. On that day several air
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monitoring stations measured NOx concentrations above the standard of 100
299
(ppb/hour) 1 between 05:00 and 06:00 in the morning, as well as in the evening hours,
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between 16:00 and 18:00. The radiosonde released at 00:00 between the 13th and 14th
301
of November measured a continuous increase in temperature (inversion) and a
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continuous decrease in RH as altitude increased, with values between 17.2 and 23.2
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°C and 88% to 31% for altitudes between 35 and 111 meters ASL, respectively. Using
304
Eq. (4), and given the radiosonde measurements, the change in refraction as a function
305
of altitude indicated a case of atmospheric ducting:
N 616 157 (N-units/km) H
306
(10)
307
For comparison, we reviewed the measurements of the different instruments on
308
November 11th and 11th, when these conditions did not occur and the radiosonde
309
measurements (from 00:00 between 35 and 135 meters ASL) showed:
N 39 H
310
(N-units/km)
(11)
311
Figure 3 shows the measurements of the MLs (indicated by a red line in Fig.2(B)),
312
NOx concentration values, and the ceilometer measurements taken over a period of 36
313
hours between November 13th and 14th when the air pollution episode was observed
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(left column), and during the same hours between November 11th and 12th (right
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column) taken as a reference day for comparison. The blue and red lines (Figs. 3(A)
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and 3(B)) show the maximum RSL measurements of the two different links deployed
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over the same propagation path. The green and black lines (Figs. 3(C) and 3(D)) show
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the concentration measurements at the Holon and Road 4 stations, respectively. The
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lines in Figs. 3(E) and 3(F) show the ceilometer measurements of the mixing layer
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height.
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Looking at the left column in Fig. 3, the anomaly resulting in relative amplification of
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the RSL during episodes of air pollution can be seen (Indicated in Fig. 3(A) in grey).
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The relative amplification was measured by both links simultaneously. During the
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three air pollution episodes where RSL measurement anomalies were observed, both
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simultaneously detected NOx levels above the standard value of 100 ppb,1 reaching
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up to 7 times the standard value at peak concentration (Fig. 3(C)). Additionally, note
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that the anomaly on the links occurred only at times when the upper boundary of the
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inversion (Fig. 3(E)) was at its minimal height, which is of the order of the link's
330
altitude, at around 100 meters Above Ground Level (AGL). On the other hand, by
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looking at the right column in Fig. 3, which represents a reference day, one sees no
332
RSL anomaly for the entire 36 hour period (Fig. 3(B)). The inversion base, in this
333
case, was consistently above 200 meters (Fig. 3(F)). An increase in NOx
334
measurements above standard levels was observed, though, particularly by the Road 4
335
station, between the hours of 17:00 and 22:00 on the evening of November 11th (Fig.
336
3(D)). The time interval when this increase was detected was during period with
337
highly congested traffic (the end of the work day).
338 339 340 341 342 343 344
Figure 3. The microwave network monitoring compared to specialized measurement systems. Maximum RSL measurements (A, B), NOx (C, D) and altitude of the boundary of the inversion (E, F) as measured during the high pollution day (left column), and the reference day (right column). The dashed horizontal line in figures (C, D) represents an hourly baseline level of 100 ppb above which the measured concentration is considered to exceed the standard1. The dashed line in figs. E and F represents an elevation of 100 meters AGL. The 15 ACS Paragon Plus Environment
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areas in grey broadly represent episodes where the links registered a relative increase in RSL
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measurements and the measurements taken by the other sensors during the same time period.
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However, these hours are also a high vehicular traffic period on the day discussed
348
(November 14), for the same reason. The possible explanation for the measurable
349
increase in NOx concentration on November 14 is thus the result of a strong near-
350
ground inversion, detected by the MLs and the proprietary instruments, compared to
351
November 11-12 where TINV and rapid lapse in humidity with altitude did not occur.
352
Accordingly, no anomalous propagation was observed by the MLs during November
353
11-12.
354
Figure 4 present scatter plots of the maximum RSL measured by the links (ML1 and
355
ML2) compared to the NOx concentration measurements taken by the Holon and
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Road 4 monitoring stations during the air pollution event (between 09:00 on
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November 13th, and 21:00 on November 14th, i.e. a scatter plot based on the
358
measurements presented in Figures 3(A) and 3(C)). The equation at the right bottom
359
of each panel shows the linear fit that was calculated. The Pearson correlation, R,
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between the link and the NOx measurements was found to be between 0.47 and 0.6
361
during the event (based on 145 data points in each panel, P-value< 0.01). An increase
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in the pollutant concentration can be seen in each of the figures when RSL
363
amplification is measured. A
B
C
D
364
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Figure 4: Maximum RSL measurements vs. NOx concentration measurements. Figures 4(A) and 4(B) show the measurements from ML1 compared to the Holon and Road 4 station measurements, respectively. Figures 4(C) and 4(D) show the measurements of ML2 compared with the Holon and Road 4 station measurements, respectively.
369
Note that there is a difference between the locations of the MLs and the locations of
370
the stations. Further, the method of measurement is different: a point measurement of
371
the air pollution sensors, compared to an areal measurement over several kilometers
372
taken by the MLs. Specifically, the phenomenon observed by each of the tools is
373
different. Air pollution sensors provide a direct measurement of NOx concentration,
374
whereas the MLs provide a measurement of received signal levels which are affected
375
by the TINV that exists in the area (and which induces an increase in pollutant
376
concentration). As a result, the figures indicate a correlation in direction, but
377
differences are expected.
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PM10 Episode and ML Measurement: The air pollution event of 11-12 May, 2009
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On the night between the 11th and 12th of May 2009, a holiday took place in Israel
380
("Lag Ba'Omer"61), during which, as is custom, thousands of bonfires are lit across the
381
country, starting from the evening hours of the holiday and continuing until the
382
following morning.
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Figure 5 presents PM10 vs. commercial ML measurements which were taken over a
384
time frame of 36 hours during this air pollution event. The Figure illustrates the
385
ability of commercial ML to detect situations where air quality decreases dramatically
386
as a result of PM10 being captured within a TINV that, combined with increased
387
particulate emissions, caused extreme air pollution (i.e. PM10 concentrations of 150
388
μg / m3 or above1).
389
Radiosonde measurements from 00:00 between the above dates indicated atmospheric
390
layering in the area, and anomalous propagation conditions at the elevations of the
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links that were examined. A temperature inversion existed in the first 140 meters ASL
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and between 470 and 530 meters ASL (with an average increase of 1.5ºC per 100
393
meters in both cases).
394
We calculated the refractivity index using a sample from a representative elevation for
395
each layer, and the refraction changes with elevation. These values were found to be:
396
Layer I - between 35 and 140 meters:
397
N 103 (N-Units/km) – subrefraction H
398
N1(35 m ASL)= 340 (N-units)
399
Layer II - between 140 and 470 meters:
400
N 52 (N-Units/km)- standard conditions H
401
N2(240 m ASL)= 345 (N-units)
402
(12)
(13)
Layer III - between 470 and 530 meters:
403
N 502 (N-Units/km) – ducting H
404
N3(470 m ASL)= 333 (N-units)
(14)
405
We note that similar to the description in theoretical Fig. 1(A), the profile of refraction
406
indices with elevation fulfilled the condition: N1N3, for these three layers such
407
that an air waveguide was formed. The resulting atmospheric layering can be
408
observed in the region indicated in grey in Fig. 5(C), according to the Beit Dagan
409
ceilometer measurements.
410
This instrument detected the upper boundary of the ground inversion that was
411
fluctuating between elevations of 140 and 200 meters AGL, between 21:20 and 03:40
412
of 11 and 12 May, respectively (brown graph). In conjunction, during part of this
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period, the ceilometer detected a cloud base (the graph in blue) at the elevation of the
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layer III inversion base (around 500 meters ASL).
415
Now let us focus on two MLs that span 14.3 kms in length and operate along a slant
416
path from 116 m to 316 m ASL (marked in green in Fig. 2). The propagation path
417
elevation of these links passes through layer I and is the same, for the most part, as the
418
air waveguide created in layer II.
419
These links measured a relative increase in RSL (Fig. 5 (A)) between the hours of
420
22:45 and 04:15 ( of 11 and 12 May, respectively), overlapping with the period when
421
the peak PM10 concentration was observed at Yad Rambam air monitoring station
422
between 21:45 and 03:30 (Fig. 5(B)).
423
Notably, Yad Rambam ground station is located 92m ASL, i.e. within the ground level
424
TINV. As a result, the increase in PM10 concentration is correlated with the
425
measurements of the microwave system (and ceilometer). When the layering
426
dissipated, the microwave propagation returned to normal (and the pollutant
427
concentration dropped measurably).
428
The Pearson correlation between the measurements of links 1 and 2, and the PM10
429
measurements from Yad Rambam station was found to be 0.56 and 0.59 respectively
430
(based on 145 samples, P-value< 0.01). Scatter plots created for this event in the
431
manner described in Fig. 4 showed similar results.
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A
B
C
432 433 434 435 436 437 438 439 440
Figure 5. Proprietary atmospheric instrument measurements compared to microwave network measurements. The observations were taken between 11-12 May 2009 (36 hours). ML measurements (A), PM10 measurements taken by the station at Yad Rambam (B), and Beit Dagan ceilometer measurements (C). Notably, an atmospheric layering state can be observed in the region indicated in grey in Fig. 5(C). A sharp increase in PM10 concentration can been seen at the Yad Rambam station as the top boundary of the inversion layer descends to 200 meters and below (as measured by the ceilometer). Accordingly, a correlation can be seen with the measurements of the MLs operating between 116 and 316 meters ASL.
441
Fog and ML Measurement: The fog event of 19- 20 November, 2010
442
According to the Israeli Meteorological Service, starting in the late evening of
443
November 19th, heavy fog began to develop over Southern and Central Israel,
444
reaching its peak in the early morning hours of November 20th, 2010. A Red Sea
445
Trough20 with a central axis moved Eastward over the ground, accompanied by a
446
barometric high to the south-west at altitude. The change to a westerly flow after a hot
447
dry day, with cold, humid air intruding under a strong, low marine inversion on the
448
shore, caused the event to develop.
449
Figure 6 presents RSL measurements taken by 3 MLs (Fig, 6 (A),(B)), a ceilometer
450
(Fig. 6(C)) and Meteorological Optical Range (MOR27) measurements – (Fig. 6(D)).
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451
The ceilometer detected the upper boundary of the inversion that was fluctuating
452
between altitudes of 90 and 170 meters AGL, between 17:30 and 07:30 of November
453
19- 20, respectively. The MLs (Fig. 2, blue) are deployed at elevations between 41-87
454
meters ASL. The measurements of the radiosonde released on the night of the event
455
(00:00) indicated conditions of anomalous propagation. At elevations between 35 and
456
200 meters sub-refraction conditions were measured (N/H = 137 (N-Units/km)),
457
while in the layer above, between 200 and 240 meters ducting was measured (N/H
458
= −792 (N-Units/km)). A temperature inversion at an average rate of 3.6ºC per 100
459
meters existed continuously in these elevations (between 35 and 240 meters ASL).
460
The Beit Dagan station (35 ASL) measured high RH values (96%-100%) during 20:00
461
and 08:00 of November 19-20, respectively.
462
According to the above, we calculated the refraction index according to the
463
radiosonde samples from three representative altitudes in the 240 meters above sea
464
level. The values were found to be:
465
N1 at ground level (35 meters ASL)= 352 (N-units)
466
N2 (170 meters ASL)= 375 (N-units )
467
N3 (240 meters ASL)= 340 (N-units)
468
Note that the atmospheric condition – N1< N2> N3 is fulfilled in this case as well.
469
An anomaly (relative amplification) can be seen simultaneously in the measurements
470
of the 3 links prior to the peak of the fog event. The beginning of the peak fog level is
471
indicated by the vertical dashed line in Fig. 6, and from that moment on the
472
ceilometer detected severe visibility limitations, and indicated conditions called “Sky
473
obscured” (according to the Synop code). This period is indicated by a dashed blue
474
line in Fig. 6(C). The effective meaning is that during this interval thick fog existed at
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475
ground level. The MOR, taken by a visibility sensor at Beit Dagan during the same
476
period, dropped to a few tens to hundreds of meters (Fig. 6(D)).
A
B
C
D
477 478 479 480 481 482 483
Figure 6. The fog event between 19- 20 November 2010 (36 hours): proprietary instrument measurements vs. microwave network measurements. The measurements from the two MLs which were operating over the same propagation path near Herzliya (Fig. 2(B), blue) are presented in Fig. 6(A). The measurements from the Tel Itzhak ML (Fig. 2(B), blue) are shown in Fig. 6(B). Ceilometer measurements (Fig. 6(C)) and MOR observations (Fig. 6(D)) were taken from Beit Dagan station.
484
We note that the anomalies in the link measurements ended simultaneously with the
485
beginning of the fog's peak. A plausible explanation for this observation is the
486
inversion layer sinking down to an altitude below the link's line of sight (as is
487
supported by the ceilometer measurements), and thus above the layer adjacent to the
488
ground, standard atmospheric conditions that allowed for normal propagation now
489
returned. Prior research54 has shown that conditions of anomalous propagation are
490
typical in precursor conditions to fog, and can provide a measure for early warning
491
against its occurrence.
492 493 494
The proof-of-concept results presented above point to the feasibility of using commercial microwave infrastructure as an environmental sensor network for 22 ACS Paragon Plus Environment
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495
detecting anomalies in the atmospheric refraction index near ground level. The
496
interest in detecting these cases derives from the fact that the phenomenon of
497
atmospheric layering is associated with TINVs, a leading cause to a plunge in air
498
quality, and to fog.
499
The validation of the concept presented here draws robust scientific rationale from
500
several different aspects. The verification was supported by observations during
501
different events, different episodes, in varying locations, and with different
502
microwave systems while, generally, in events where no ducting occurred, no
503
anomalies in link measurements were observed. More specifically, in cases where
504
these conditions were detected by the specialized instruments at elevations in the
505
order of magnitude of the propagation path, a relative increase in RSL was observed.
506
We note that, in particular, a relative increase in RSL is a unique effect which is linked
507
directly with ducting and multi-pathing, phenomena that occur during inversions.48, 54
508
From a different vantage point, previous research has shown marked increase in
509
specific air pollutant concentrations, similar to those observed here, during TINVs.6,
510
10, 58
511
the variance of the observed NO, NO2, PM10 (and benzene) concentrations was
512
caused by changes in the mixing layer height (which is bounded by the inversion
513
base). The results revealed here from the proposed novel method of using cellular
514
communication infrastructure as a sensor network are therefore corroborated by those
515
arrived at in prior research.
516
The extreme visibility limitations caused by fog can lead to tragic accidents and
517
widespread economic damages, such as disruption of schedules and flight
518
cancellations.21-23 However, the tools that exist today, do not always provide sufficient
A recent study conducted by Schäfer et al.9 concluded that an important part of
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519
response.45, 46 Thus the motivation to develop techniques to improve the ability to
520
monitor and forecast this phenomenon.
521
The third event discussed above provides additional proof of feasibility for the ability
522
of commercial MLs to identify low lying TINVs and more specifically the potential of
523
this technology to detect and forecast fog, a precondition of which is the existence of
524
this phenomenon.20
525
We note that the potential for monitoring fog using commercial microwave links was
526
revealed in recent works,45, 46 but the physical principle on which the measurements
527
were based was different. In these recent works fog was measured directly, based on
528
the attenuation of the microwave signal by the fog droplets suspended in the air, and
529
specifically, only after the phenomenon had already occurred. In the principle we
530
demonstrate here, what is detected is anomalous propagation caused by a low lying
531
TINV, which is one of the prerequisite conditions for the creation or strengthening of
532
fog.54 Thus, use of the method proposed here, can provide information crucial to
533
early warning about, hence proactive mitigation or preparation for the phenomenon.
534
During the second and third events studied here, proximity to the proprietary
535
instruments (radiosonde, ceilometer, visibility sensor) was slightly lower when
536
compared to the first case. However, the comparison between the different
537
instruments is reasonable, because ducting and inversions take place over a larger
538
spatial scale than the difference in locations between the instruments and links. The
539
typical spatial scale of the phenomenon can reach tens and even hundreds of
540
kilometers,62 and particularly in the test area where the climate and geographic
541
conditions are similar.19 Thus, the phenomenon was observed simultaneously by the
542
proprietary instruments and the MLs in events 2 and 3 as well. That being said, clearly
543
the altitude and thickness of the various layers differs from one place to the next (e.g.
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544
Bean63), and may contribute to the discrepancy in measurements between the different
545
methods.
546
While in case 1 ducting was observed directly at link elevation, in cases 2 and 3 sub-
547
refraction conditions were observed with ducting conditions occurring above. Sub-
548
refraction conditions cause an upwards bending of the wave, so in these cases it is
549
possible that the amplification was a result of an upward deflection of the beam and
550
its capture in the duct layer, or constructive interference due to multipath as a
551
consequence of the beam being subnormally bent upwards from the lower layer and
552
then reflecting downwards off the higher layer. Alternately, it is possible that the
553
atmospheric waveguide was at the elevation of the links in the area where they were
554
deployed thus, causing the amplification. However, due to the difference in locations
555
between the links and the proprietary measuring instruments the elevation detected at
556
the measuring station (Beit Dagan) did not correctly represent the elevation of the air
557
waveguide at the link location.
558
Overall, our results indicate the potential of commercial microwave systems to
559
provide indirect detection of air pollution and fog. The widely existing MLs, in a
560
unique manner with inherent advantages over the commonly used conventional
561
techniques, provide near-ground atmospheric measurements at a high tempo-spatial
562
resolution with simple implementation of minimal extra cost. The work reported in
563
this paper shows feasibility of this novel idea, and possible future research can be
564
conducted to fully investigate relevant practical details and societal implications along
565
the new path presented here.
566 567
25 ACS Paragon Plus Environment
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568
DISCUSSION
569
The novelty of this work stems from revealing the great potential of cellular
570
communication networks for detecting near-ground temperature inversions, and the
571
adverse atmospheric conditions that can exist during such occurrence. Due to their
572
deployment at ground level, and their wide geographic distribution and the type of
573
measurements they offer, commercial MLs are particularly suited for detection and for
574
provision of real time warning of air pollution episodes and fog. The microwave
575
network engineering literature refers to the phenomenon of atmospheric stratification
576
as interference that more intensively affects longer microwave links (e.g., 5km or
577
longer in length),48 and as a result, such longer links are the MLs with the highest
578
potential that can be exploited for detecting near-ground hazardous atmospheric
579
conditions. Future research can be done to analyze additional events in different
580
regions using ML networks in conjunction with ground truth instruments adjacent to
581
the link. Robust signal processing algorithms and comprehensive analysis methods for
582
the large volume of ML data can then be developed to support practical deployment of
583
ML-based high-resolution atmospheric sensor networks at near-ground level. The
584
proposed technique can provide benefit to many developing countries (e.g. India,
585
countries in Africa, etc.) where the percentage of ML facilities is high,41, 64 while on
586
the other hand, conventional monitoring resources are limited, if they exist at all. The
587
current paper concentrated on the signal amplification effect as a result of the
588
atmosphere behaving as a wave guide. However the multipath effect, as well as
589
ducting, that are identified with cases of TINV, may also cause signal attenuation.54-56
590
Furthermore, in some specific cases, signal amplification may be happening due to
591
other reasons, such as multipath due to terrestrial objects in the close vicinity of the
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592
propagation path, which can lead to misdetection. Further investigation, outside the
593
scope of the current paper, is required on these topics, in future research.
594
It appears that the field of wireless environmental sensor networks had progressed less
595
quickly than was expected about a decade ago, as a result of a multitude of obstacles,
596
including – deployment costs, communication and data processing requirements,
597
maintenance and reliability.67 The main characteristics of an efficient wireless sensor
598
network require: low cost, large spatial dispersion and autonomous sensing.68
599
Commercial MLs operate continuously by default, the system is routinely maintained
600
and monitored, the measuring instruments are already deployed in the field, and the
601
relevant data sent and collected efficiently, by many of the cellular providers, as part
602
of normal operation. Thus, this infrastructure can be considered as an "opportunistic
603
wireless sensor network"68 for environmental monitoring. The challenge, then, is the
604
alternative use of such resources. The possibilities arise from the diversity of the
605
opportunistic sensors, reflected in the different operating frequencies of the system,
606
the variation in signal polarization, different link lengths and varying link elevations
607
above ground. By definition, the system is a communication network, and thus,
608
naturally, the measurement quality of a single sensor (link) may at times not be
609
optimal, but the number of measurements is large and diverse – and thus compensates
610
for the measurement quality of each single link, or, alternatively, allows for the
611
selection of specific, suitable links from the large array available for monitoring the
612
phenomenon of interest.
613
We note that in addition to MLs, data transmission in the network can be carried out
614
by other means, such as fiber optic (or copper) cables. There are some locations where
615
MLs are replaced with fiber optic cables. However, the use of microwave
616
infrastructure is expected to continue to be widespread in the future.64
27 ACS Paragon Plus Environment
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617
Considering commercial microwave systems as an innovative method for monitoring
618
atmospheric conditions creates many opportunities to provide valuable information
619
regarding air quality. To this point, tools for the creation of 2D rainfall maps (e.g.
620
Overeem et al.42) and fog monitoring (David et al.45, 46) were developed. Thus, the
621
system can provide information about relatively clean air regions due to washout
622
effects as a result of rainfall65 in a known area mapped by the system or pollutant
623
scavenging processes due to fog66 – new capabilities that have yet to be demonstrated
624
using this technology. However, the goal of the current research was to take the whole
625
approach one step further, and to show proof of concept of the potential commercial
626
MLs may have to monitor air quality and precursors for fog.
627
AUTHOR INFORMATION
628
Corresponding Author
629
*Email:
[email protected], Phone: +1607-2548334.
630
Present Addresses
631
§School of Civil and Environmental Engineering, Cornell University, Ithaca, NY
632
14853.
633
ACKNOWLEDGMENTS
634
This work is dedicated to Ella David Helfman, the daughter of Adi and Noam (the
635
lead author), in celebration of her first birthday.
636
The microwave data were provided by Cellcom, Pelephone and PHI to the research
637
team of Tel Aviv University (TAU) to whom Dr. David was affiliated. The authors
638
are grateful to Y. Koriat, I. Alexandrovitz, E Levi and B. Bar (Cellcom), N. Dvela, A.
28 ACS Paragon Plus Environment
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639
Hival and Y. Shachar (Pelephone), Y. Bar Asher, O. Tzur, Y. Sebton, A. Polikar and
640
O. Borukhov (PHI). We extend our sincere acknowledgments to Prof. Hagit Messer,
641
Prof. Pinhas Alpert and their research team from TAU for fruitful and valuable
642
discussions. Finally, we deeply thank the Israeli Meteorological Service (IMS) and
643
the Israel Ministry of Environmental Protection for supplying meteorological and air
644
pollution data. This work was supported by Cornell University's David R. Atkinson
645
Center for a Sustainable Future (ACSF). The second author acknowledges partial
646
funding support from the Natural Science Foundation of China (NSFC) project #
647
71428001.
648 649 650 651 652 653 654 655 656 657 658 659 660 661 662 663 664 665 666 667 668 669 670 671 672 673 674 675 676 677
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