Abstract
Atmospheric remote sensing offers a unique opportunity to compute indirect estimates of air quality, which are critically important for the management and surveillance of air quality in megacities of developing countries, particularly in India and China, which have experienced elevated concentration of air pollution but lack adequate spatial–temporal coverage of air pollution monitoring. This article examines the relationship between aerosol optical depth (AOD) estimated from satellite data at 5 km spatial resolution and the mass of fine particles ≤2.5 μm in aerodynamic diameter (PM2.5) monitored on the ground in Delhi Metropolitan where a series of environmental laws have been instituted in recent years.
PM2.5 monitored at 113 sites were collocated by time and space with the AOD computed using the data from Moderate Resolution Imaging Spectroradiometer (MODIS onboard the Terra satellite). MODIS data were acquired from NASA’s Goddard Space Flight Center Earth Sciences Distributed Active Archive Center (DAAC). Our analysis shows a significant positive association between AOD and PM2.5. After controlling for weather conditions, a 1% change in AOD explains 0.52±0.202% and 0.39±0.15% change in PM2.5 monitored within ±45 and 150 min intervals of AOD data. This relationship will be used to estimate air quality surface for previous years, which will allow us to examine the time–space dynamics of air pollution in Delhi following recent air quality regulations, and to assess exposure to air pollution before and after the regulations and its impact on health.
Keywords: PM2.5, Aerosol optical depth (AOD), Air pollution, Remote sensing
1. Introduction
Elevated concentration of air pollution and its associated health effects in rapidly growing megacities of developing countries particularly that of India and China have drawn our attention in recent years. Therefore, it is critically important to monitor air quality at high spatial–temporal resolutions. But limited network of air pollution monitoring in developing countries restricts our ability to evaluate time–space dynamics of air pollution and its effect on human health. Nonetheless, advances in satellite remote sensing seem promising to compute indirect estimates of particle smaller than ≤2.5 and ≤10 μm in aerodynamic diameters (PM2.5 and PM10, respectively) over a large area frequently and inexpensively (Chu et al., 2003). Satellite imageries record electromagnetic radiation from the earth surface. When the radiation travels through the atmosphere, it interacts with aerosols—fine solid and/or liquid particles suspended in the air—prior to reaching the sensor mounted onto satellites. The distortion caused by this interaction can be estimated with the aid of radiative transfer model and converted into aerosol loading, also known as aerosol optical depth (AOD), which has shown a strong positive relationship with the PM2.5 and PM10 observed on the surface (Chu et al., 2002, 2005; Gupta et al., 2006).
Building on these innovative methods, this article has two main goals: (a) to establish an empirical relationship between satellite-based AOD, an indirect measure of air quality, and particulate matter (PM) monitored on the earth surface in Delhi Metropoitan and (b) to exmaine whether AOD can effectively predict PM2.5 and PM10 surfaces at high spatial-temporal resolutions. There are various measures of air quality. However, suspended particles, especially PM2.5 and PM10, have been a widely accepted measure of air quality (WHO, 2000). Therefore, the term air quality will refer to as the ambient concentration of PM2.5/PM10 in the remaining parts of this paper.
The need for this work emerged from our desire to model the effects of improvement in air quality on respiratory health in response to a series of recently instituted air quality regulations in Delhi, the capital of India and the only city that was subject to these regulations (Fig. 1a). Due to limited spatial–temporal coverage of air pollution data in Delhi, we began to explore the potential of satellite remote sensing to study the effect of these regulations on the time–space dynamics of air pollution, and the present article is an outcome of these explorations. This paper examines the relationship between AOD and PM2.5 in Delhi Metropolitan, and this relationship will formulate the basis to assess change in air quality and the burden of mortality and morbidity alleviated in response to these regulations. The next three sections present the data and methods, results and discussion.
Fig. 1.
(a) Location of megacities in India, 2001. (b) 113 sampling sites in Delhi and its environs, 2003.
2. Data and methods
2.1. Data
The data for this research come from four different sources: (a) air quality monitoring in Delhi and its surroundings, (b) Terra MODIS (Moderate Resolution Imaging Spectroradiometer), (c) the Indian Meteorological Department and (d) the National Climatic Data Center.
2.1.1. Air pollution data
Air pollution data on suspended particulates were collected at 113 sites in the study area from July 23 to December 3, 2003 (Fig. 1b). Since our major focus was on estimating spatial variability in air pollution, a spatially dispersed sampling design was adopted (Kumar, 2007). Sample sites were identified using a two-step process—first, a rectangular grid was overlaid onto the study area, which ensured coverage of the entire study area, and second, a random location was simulated within each cell (of the size 1 × 1.5 km2) to avoid bias in the site selection. The simulated locations were then transferred to a Garmin Global Positioning System (GPS) to navigate them and examine their suitability. Some sites, which were inaccessible, were re-simulated, and finally 113 sites were found to be suitable. At each site, air was sampled at two different times every third day. Although air was sampled at different times between 7:30 a.m. and 10:00 p.m. from July to December 2003, data for the present analysis were extracted using three conditions: (a) ±150 min of satellite crossing time, generally 10:30 a.m. local time, to minimize the effect of temporal noise in the ground measurements of PM; (b) for the months of October and November 2003 to minimize the effect of weather conditions on AOD, because AOD is very sensitive to weather conditions and only these months in Delhi observe relatively stable weather conditions; and (c) relative humidity ≤50%.
The Aerocet 531, a real-time photometric sampler (Met One Inc, 2003), was used to collect air pollution data. It is an automatic instrument that estimates PM in a range of 1, 2, 5, 7 and 10 μm in aerodynamic diameters in mass mode, and PM≤0.5 and PM≤10 in count mode. The instrument uses a right angle scattering method at 0.780 μm. The source light travels at a right angle to the collection system and detector, and the instrument uses the information from the scattered particles to calculate a mass per unit volume. A mean particle diameter is calculated for each of the five different sizes. This mean particle diameter is used to calculate a volume (cubic meters), which is then multiplied by the number of particles and then a generic density (μg m−3) that is a conglomeration of typical aerosols. The resulting mass is divided by the volume of air sampled for mass per unit volume measurement (μg m−3). Each sample (in mass) mode takes 2 min. Particle mass estimation using this technology can be influenced by increase in relative humidity (McMurry et al., 1996). However, this problem can be addressed by excluding observation with high relative humidity (≥50%) because the particle size and its mass inflates dramatically when relative humidity is greater than 50%, or by calibrating data with the aid of an empirical relationship between the distortion in PM mass and relative humidity developed by Lowenthal et al. (1995).
One sample site was established beside air pollution monitoring station run by the Central Pollution Control Board (CPCB). This station is equipped with gravimetric samplers and records PM10 and TSP regularly using high-volume samplers. At this site, we monitored PM10 and PM2.5 from July to November 2003, though PM2.5 data were not recorded at the CPCB facility. Unlike TEOM series 1400a, which measures PM2.5 mass in real time, no instrument was installed in Delhi and its environs for comparison purposes (Thermo Electron Corporation, 2006). Thus, the only choice left was to compare photometric estimate of PM10 mass from Aerocet 531 with the PM10 mass from gravimetric measurements by high-volume sampler (Fig. 2). The average PM10 mass by Aerocet 531 was 157±24 μg m−3 during July–November 2003 which was significantly lower than PM10 mass from gravimetric sampler 210±18.6 μg m−3. Given the differences in the method and duration of the sampling between gravimetric and real-time photometric samplers, the average difference (≤54 μg m−3) seems reasonable, because the Aerocet 531 estimates are based on 8 min of sampling—4 min each during peak and off peak hours every third day. Gravimetric measurements, however, were based on 8 h of sampling across three shifts in a day. In the absence of gravimetric measurements of PM2.5, it was not possible to validate PM2.5 with the gravimetric measurements. Nonetheless, our recent experiment in Delhi from September to November 2006 shows that the difference between gravimetric and photometric estimates of PM2.5 mass is significantly smaller than that of PM10.
Fig. 2.
Photometric and gravimetric estimate of PM10 at CPCB monitoring station at ITO, Delhi, August–November 2003.
Weather conditions, particularly relative humidity, can greatly affect mass of aerosol from photometric technology, because the concentration measurement of light-scattering devices increases with the increase in average particle size under the influence of humidity (McMurry et al., 1996). Ramachandran et al. (2003) have exploited the relative humidity correction curve developed by Lowenthal et al. (1995) to compute robust estimate of gravimetric standard PM2.5 mass from photometric samplers. Their analysis shows that the error increases from 6% at 40% relative humidity to 40% at 70% relative humidity. Thus, the bias of relative humidity was controlled by restricting the data to the less than 50% relative humidity and by introducing relative humidity as one of the confounders in the regression model.
2.1.2. Satellite data
Data from MODIS (onboard Terra satellite) were acquired from NASA’s Goddard Earth Sciences Distributed Active Archive Center (DAAC). Although air pollution data were recorded from July to December, satellite data were acquired for the months of October and November 2003 because of stable weather conditions during these 2 months. During this 2-month period, AOD values were retrieved at 5 km spatial resolution from cloud-free images, and the 10 km AOD for the same period were downloaded from DAAC.
2.1.3. Meteorological data
We used a probe with the Aerocet 531 instrument to record temperature and relative humidity in real time. Other meteorological data on sea-level atmospheric pressure, wind velocity, wind direction and rainfall were acquired from the Indian Meteorological Department at 3-h intervals, and daily meteorological data were downloaded from the National Climatic Data Center.
2.1.4. Data integration
PM data, collected at 113 sites, were point data, and AOD MODIS data were at 5 and 10 km pixel sizes (at nadir), which created the problem of geographic misalignment. For example, on a given day, two or more sample sites could be located in the same 5 km AOD pixel. Thus, data were integrated using one-to-many (same AOD value for all points within a pixel (Fig. 3)) and many-toone (average value of PM at many sample sites to the AOD pixel) relationships. Assigning one AOD value to all sample sites within the pixel allowed us to model PM2.5 as a function of AOD at point level, which is referred to as the disaggregate/point-level analysis in the subsequent sections. Although the intra-AOD pixel noise in PM2.5 was evident from the preliminary analysis, the disaggregate analysis allowed us to assess the association between AOD and PM2.5 without loosing the spatial resolution of point data. In the aggregate analysis, however, we averaged point measurements of PM2.5 data to match the spatial resolution of AOD data. This will be referred to as aggregate/pixel-level analysis in the subsequent sections.
Fig. 3.
Collocating 5 km AOD and PM2.5 estimate at point location.
2.2. Methods
Aerosols are solid and liquid particles suspended in the air, and AOD can be defined as will be the extinction of beam power due to the presence of aerosols in the atmosphere. AOD typically decreases with increasing wavelength for fine-mode dominated aerosols. Visible spectral bands of various remote sensing satellites have been used to estimate AOD over both water and land surfaces (Christopher et al., 2000; Chu et al., 2003, 2005; Holben et al., 1992; King et al., 1999; Wang and Christopher, 2003). In essence, AOD (τ) at a given site s is the log of the ratio of irradiance at the top of atmosphere (Io) to irradiance at the surface (Is). Scattering due to the presence of aerosol increases and decreases the beam power towards and against the direction of sensor Ω, respectively. The effect of aerosols loading (due to scattering and/or absorption) on radiances recorded by the sensor is computed using a radiative transfer model (Kaufman et al., 1997; King et al., 1999).
Aerosol retrieval over land is more complicated than over sea, because the land surface shows large variability, from dark vegetation to bright desert and snow/ice-covered regions. Owing to the competing processes of surface reflection and aerosol backscattering in radiative transfer, radiance measured with less surface interference results in a smaller uncertainty in the retrieved aerosol properties. The dark target approach is based on the correlation between the chlorophyll absorption of vegetation in the visible (0.47 and 0.66 μm) and liquid water absorption at 2.1 μm (reflectance <0.25). The fine-mode particles (urban/industrial and biomass-burning aerosols) are transparent at 2.1 μm (i.e., minimal aerosol effect), which allows direct observation of the earth’s surface, even through heavy pollution, to estimate the surface reflectance in the visible spectrum. The MODIS AOD is computed at 0.47 and 0.66 μm by matching the averaged reflectance (after screening for clouds, water and snow/ice pixels from a total of 100 pixels) at a 5 × 5 km2 grid to the value of a pre-calculated lookup table under the same Sun–satellite geometrical condition. The selection of 5 × 5 km2 is mainly due to large surface variability of concern at a global scale. It can be enhanced to meet different requirements of applications (e.g., urban air quality) under proper conditions. In general, the errors are within Δτa = ±0.05 and Δτa = ±0.20τa over vegetated and semi-vegetated regions, respectively (Chu et al., 2002).
The lookup table is constructed by Dave’s code (Dave and Gazdag, 1970), which assumes spherical particle shape, an “average” aerosol profile, and lognormal size distributions (Chu et al., 2003). Three general aerosol types have been considered: urban/industrial pollution, biomass-burning aerosols, and dust. The spectral aerosol path radiance is used to separate dust from the other two types, because dust particles are significantly larger than pollution or smoke particles. Mixture of dust and non-dust aerosols is taken into account by the fine-mode fraction obtained from the linear interpolation from the derived path radiance ratio and the assumed ratio of dust and pollution (or smoke) models. Since pollution and biomass-burning aerosols both are dominated by fine-mode particles, they are distinguished by a priori assumptions based on geography varying with season. Using this methodology, AOD values were computed for 40 days, and PM and AOD data were integrated for the matching days.
The link between AOD and PM2.5 observed at the surface is through the integration of layers of particles from the surface to the top of the atmosphere (more precisely the top of the tropopause if no stratospheric aerosols exist, or the top of the boundary layer if all particles reside within boundary layer). Good correlations between AOD and PM2.5 are generally found if particles are within the boundary layer (since they are well mixed). Aloft particles that are present in the atmosphere, such as smoke or dust from long-range transport, result in no (or poor) correlation with surface-measured PM.
Regression models were employed to examine the association between AOD estimates from satellite data and PM mass observed on the ground. We examined this association at two different geographic scales—at point level and 5 and 10 km AOD pixel levels. In the latter, also referred to as aggregate analysis, the average PM2.5 within 5 and 10 km AOD pixel (j) was modeled as a function of AOD at jth pixel and weather conditions as in Eq. (1):
(1) |
where PMj is the average PM (either PM2.5 or PM10) for jth pixel; τj the AOD value estimated from MODIS data at jth location; w′j the matrix of confounders, including relative humidity and temperature; the intra-pixel variance in PM, also referred to as intra-pixel noise; and εj the unobserved random error.
In the disaggregated analysis, PM at ith sample site located in jth pixel was modeled as a function of AOD (τ) for the pixel in which ith sample site is located and confounders (as in Eq. (2)). Since all sample sites (in a given day) within a pixel were assigned the same AOD value, resulting in an intra-pixel correlation structure in AOD, the pixel-level random effect was introduced to compute pixel-independent estimates, as in Eq. (2):
(2) |
where δj is the pixel-level random effect.
Direct evaluation of the predictive power of the model is complicated by the fact that the PM measures are effectively sampled at a different resolution than the AOD measures. In particular, one would like to know the predictive value of AOD in terms of average true PM at the level of an AOD pixel. The problem is that we only have a small sample of the PM measures at the pixel level, and thus the R-squared from Eq. (2) will underestimate the percentage of variation that could be explained for average PM (averaged across all possible locations in a given AOD pixel). Nonetheless, this estimate can be constructed from the estimated random-effect errors:
(3) |
3. Results
PM2.5 and AOD surfaces were generated using the data averaged for the months of October and November 2003 (Fig. 4). There are some similarities in PM2.5 and AOD surfaces and both observed high values in the areas near industrial clusters. The summary statistics of PM and AOD are reported in Table 1. While the concentration of PM varies greatly in Delhi, the AOD concentration varies significantly outside Delhi, albeit the AOD variance is much smaller than the variance of PM (Table 1), which is expected given the coarser spatial resolution (5 km) of AOD and PM data at the point location. The average concentrations of PM2.5 and PM10 between August and November 2003 in Delhi were recorded as 82.9±7.8 μg m−3 (at 95% confidence interval) and 304.2±29.8 μg m−3, respectively, which are significantly higher than the US EPA standards. The average AOD measurements in Delhi during the months of October and November 2003 were estimated as 0.64±0.023 and 0.65±0.025 at 5 and 10 km spatial resolutions, respectively. The average AOD values were also computed with reference to distance from the city’s center (Connaught Place). Table 2 shows a gradual decline in the average AOD with increasing distance from the city’s center; the AOD concentration drops from 0.664 within 0.1 decimal degree (about 9.17 km) to 0.545 within 0.5 decimal degree (about 48.5 km) distance from the city’s center. The gradient of decline in AOD is higher at 5 km spatial resolution than that at 10 km resolution.
Fig. 4.
Interpolated surfaces of PM2.5 and 5 km AOD, October–November 2003.
Table 1.
Descriptive statistics—PM2.5, PM10, AOD at 5 and 10 km spatial resolutions
Statistical parameter | PM2.5 (μg m−3)
|
PM10 (μg m−3)
|
AOD (5 km)a |
AOD (10 km)
|
||||
---|---|---|---|---|---|---|---|---|
Delhi | Outside Delhi | Delhi | Outside Delhi | Delhi | Outside Delhi | Delhi | Outside Delhi | |
Minimum | 30.5 | 70.0 | 117.7 | 172.1 | 0.548 | 0.549 | 0.611 | 0.603 |
Mean | 82.9 | 95.7 | 304.2 | 466.5 | 0.647 | 0.612 | 0.662 | 0.636 |
Maximum | 268.4 | 167.8 | 850.3 | 957.9 | 0.714 | 0.685 | 0.693 | 0.680 |
S.D. | 38.8 | 26.9 | 148.4 | 229.7 | 0.038 | 0.051 | 0.019 | 0.031 |
Skewness | 1.8 | 1.5 | 1.3 | 0.6 | −0.509 | 0.334 | −0.613 | 0.369 |
Kurtosis | 7.7 | 5.0 | 4.5 | 2.6 | 2.415 | 1.511 | 2.636 | 1.343 |
Coefficient of variation | 46.9 | 28.1 | 48.8 | 49.2 | 5.9 | 8.3 | 2.9 | 4.8 |
Aggregate AOD estimates were assigned to 113 monitoring sites.
Table 2.
Distance from the city center and the distribution of AOD and PM
Distance from the city center (decimal degree) | AOD
|
PM
|
|||||
---|---|---|---|---|---|---|---|
5 km spatial resolution
|
10 km spatial resolution
|
No. of sites | PM2.5 (μg m−3) | PM10 (μg m−3) | |||
N | Mean | n | Mean | ||||
0.1 | 13 | 0.664±0.040 | 3 | 0.687±0.169 | 47 | 75±7.5 | 263±40.4 |
0.2 | 39 | 0.649±0.028 | 10 | 0.673±0.048 | 59 | 99±16.8 | 391±61.5 |
0.3 | 63 | 0.600±0.020 | 16 | 0.634±0.029 | 7 | 103±37.6 | 380±143.5 |
0.4 | 89 | 0.576±0.018 | 22 | 0.633±0.025 | NA | NA | |
0.5 | 127 | 0.545±0.013 | 62 | 0.623±0.012 | NA | NA | |
Inside Delhi | 55 | 0.640±0.023 | 23 | 0.657±0.025 | 98 | 82.9±7.8 | 304.2±29.8 |
The scatter plots at both point (disaggregated) and pixel (aggregated) levels reveal a positive association between PM2.5 and AOD (Fig. 5a and b). From Fig. 5a it is evident PM2.5 varies significantly within a 5 km pixel, and hence the point-level estimates of PM2.5 are noisy for 5 km AOD pixel. Two different approaches were adopted to address this problem—first, R2 values for intra-pixel noise in PM2.5 were adjusted using Eq. (3), and second, point-level estimates of PM2.5 were aggregated to pixel level. Although the average PM2.5 plotted against AOD shows improvement in the PM2.5–AOD association, the points still deviate significantly from the line of best fit (Fig. 5b), which means that there are factors (including weather conditions) other than AOD that influence PM2.5.
Fig. 5.
(a) AOD–PM2.5 distribution disaggregate analysis—same AOD for all points within the same 5 km pixel. (b) 5 km AOD and average PM2.5 at 5 km pixel.
In the preliminary analysis, PM2.5 was regressed on AOD at both 5 and 10 km spatial resolutions. Given the substantial intra-pixel variability, the AOD did not emerge as an effective predictor of PM2.5 at 10 km spatial resolution. Thus, the final analysis was restricted to 5 km AOD only. The regression results of point- and pixel-level analyses are presented in Tables 3 and 4, respectively. The AOD was computed using the data from MODIS onboard Terra satellite, which records electromagnetic energy just once in a day in the morning, generally 10:30 a.m. local time. Thus, the AOD estimates are the true representatives of aerosol loading at the time electromagnetic energy was recorded. PM2.5 measurements on the ground (even with 2 min of sampling window), however, will not match the satellite overpass time very precisely. Therefore, the uncertainty in AOD–PM2.5 association is likely to increase as the time of PM2.5 observation deviates from the overpass time of satellites. To examine this effect, the analysis was conducted separately at 15 min time intervals within ± 150 min of the overpass time of the Terra satellite.
Table 3.
Regression of PM2.5 on AOD, mean sea-level pressure and relative humidity at 5 km pixel resolution: point/disaggregate-level analysis—same AOD value was assigned to all points within the 5 km AOD pixel
PM2.5 as a function of | Interval across satellite crossing time (h:min)
|
||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
0:15 | 0:30 | 0:45 | 1:00 | 1:15 | 1:30 | 1:45 | 2:00 | 2:15 | 2:30 | All | |
ln(AOD) | 0.43 (2.77)** | 0.449 (3.70)** | 0.521 (5.05)** | 0.491 (5.35)** | 0.497 (5.62)** | 0.451 (5.61)** | 0.427 (5.41)** | 0.419 (5.56)** | 0.401 (5.33)** | 0.398 (5.17)** | 0.398 (5.18)** |
Relative humidity (%) | 0.024 (1.97)* | 0.014 (−1.72) | 0.012 (−1.87) | 0.011 (−1.85) | 0.018 (3.31)** | 0.019 (4.51)** | 0.019 (4.92)** | 0.02 (5.48)** | 0.021 (6.05)** | 0.023 (6.59)** | 0.024 (6.65)** |
Mean sea-level pressure (hPa) | 0.075 (3.37)** | 0.072 (4.42)** | 0.07 (5.09)** | 0.063 (5.07)** | 0.066 (5.71)** | 0.067 (6.12)** | 0.065 (6.13)** | 0.067 (6.74)** | 0.066 (6.68)** | 0.07 (6.84)** | 0.07 (6.85)** |
Constant | −72.9 (3.21)** | −69.5 (4.18)** | −66.8 (4.80)** | −59.6 (4.75)** | −63.7 (5.39)** | −64.1 (5.79)** | −62.4 (5.79)** | −64.4 (6.39)** | −63.8 (6.34)** | −67.2 (6.51)** | −67.2 (6.52)** |
Observations | 129 | 231 | 347 | 423 | 515 | 589 | 652 | 708 | 745 | 760 | 762 |
Number of AOD pixels | 74 | 104 | 141 | 164 | 191 | 210 | 226 | 237 | 246 | 248 | 248 |
Pixel R2 | 0.76 | 0.76 | 0.71 | 0.74 | 0.73 | 0.72 | 0.72 | 0.74 | 0.75 | 0.70 | 0.70 |
Robust t statistics in parentheses.
Significant at 5%.
Significant at 1%.
Table 4.
Regression of PM2.5 on AOD, mean sea-level pressure and relative humidity at 5 km pixel resolution: aggregate/pixel-level analysis—PM2.5 data were averaged to match the spatial resolution of AOD data
PM2.5 as a function of | Interval across satellite crossing time (h:min)
|
||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
0:15 | 0:30 | 0:45 | 1:00 | 1:15 | 1:30 | 1:45 | 2:00 | 2:15 | 2:30 | All | |
ln(AOD) | 0.458 (3.23)** | 0.482 (3.66)** | 0.454 (4.24)** | 0.369 (4.29)** | 0.366 (4.46)** | 0.371 (4.85)** | 0.336 (4.77)** | 0.333 (4.61)** | 0.342 (4.93)** | 0.352 (4.98)** | 0.352 (4.99)** |
Relative humidity (%) | 0.037 (3.62)** | 0.012 (31.16) | 0.01 (31.32) | 0.012 (31.86) | 0.013 (2.09)* | 0.015 (2.72)** | 0.017(3.37)** | 0.019 (3.98)** | 0.016 (3.80)** | 0.016 (3.66)** | 0.016 (3.66)** |
Mean sea-level pressure (hPa) | 0.029 (31.57) | 0.054 (3.21)** | 0.054 (4.06)** | 0.052 (4.67)** | 0.051 (4.86)** | 0.051 (5.30)** | 0.046 (4.92)** | 0.047 (5.17)** | 0.046 (5.11)** | 0.047 (5.10)** | 0.047 (5.10)** |
Intra-pixel PM2.5 variance | 0.205 (10.77)** | 0.178 (8.30)** | 0.158 (9.40)** | 0.144 (9.99)** | 0.166 (11.27)** | 0.173 (12.12)** | 0.167 (12.36)** | 0.159 (12.53)** | 0.156 (12.65)** | 0.162 (13.17)** | 0.162 (13.15)** |
Constant | 327.198 (31.46) | 351.383 (3.02)** | 351.683 (3.82)** | 349.588 (4.39)** | 348.25 (4.58)** | 348.432 (5.01)** | 343.471 (4.63)** | 344.843 (4.88)** | 343.664 (4.80)** | 344.513 (4.80)** | 344.525 (4.80)** |
Observations | 37 | 58 | 94 | 109 | 126 | 142 | 155 | 167 | 174 | 175 | 175 |
R2 | 0.81 | 0.66 | 0.61 | 0.61 | 0.62 | 0.63 | 0.62 | 0.61 | 0.6 | 0.61 | 0.61 |
Robust t statistics in parentheses.
Significant at 5%.
Significant at 1%.
As mentioned above, weather conditions can greatly influence aerosol loading. Thus the effect of weather conditions, such as wind velocity, relative humidity, temperature and atmospheric pressure, can confound the AOD–PM2.5 association. Among these, relative humidity and sea-level atmospheric pressure, which also experienced significant association with the wind direction, were used in the final analysis. Both relative humidity and sea-level atmospheric pressure showed a statistically significant impact on PM2.5.
The 5 km AOD shows a statistically significant positive association with PM2.5 in both disaggregate (Table 3) and aggregate (Table 4) analyses. At the point level, 1% change in AOD explains 0.398% (±0.151 at 95% confidence level) change in PM2.5 ± 150 min of AOD data (i.e., the overpass time of EOS Terra satellite). The predictive power of AOD is stronger for shorter time intervals; for example, within a 45 min time interval, a 1% change in AOD (holding other variables constant) explains 0.52% and 0.45% change in PM2.5 at point and pixel levels, respectively. In the study area, the concentration of PM varies significantly. Consequently, the daily estimate of PM for a given pixel is expected to be noisy. But after controlling for this noise, the R2 value increases substantially; for example, within a ±15 min interval, the R2 values increased to 76% and 81% for PM2.5 at point and pixel levels, respectively (Tables 3 and 4).
Fig. 4 shows the average estimates of AOD and PM2.5 during the months of October–November 2003. There are some similarities in the spatial distributions of PM and AOD. One of the important findings that emerges from this figure is that the areas in and around industrial clusters show elevated concentrations of both PM and AOD, except in the southwestern parts. The average AOD gradually declines with increasing distance from the city’s center. The average concentration of AOD (τ) in the northeastern parts of Delhi was more than 0.6, and the figures outside Delhi boundaries are less than 0.5. The spatial variability in AOD does not perfectly matches with that of PM2.5 because of several reasons: (a) the spatial–temporal resolutions of AOD–PM2.5 data do not match perfectly—AOD were estimated at about 10:30 a.m. and their spatial resolution was 5 km; PM data, however, were spread ±150 min of AOD data and these data were recorded at 113 point locations; (b) AOD are column measurements and PM2.5 were recorded at 5 feet above the surface; (c) unlike daily match of AOD–PM2.5 for regression analysis, maps of AOD and PM2.5 are based on the averages for the entire 2 months; and (d) PM2.5 surface was interpolated using Kriging methods, while AOD surface is true to its spatial resolution and did not require any interpolation.
4. Discussion
As far as the association between the 5 km AOD and PM concentration is concerned, our results are consistent with the findings of the existing literature (Chu et al., 2003; Gupta et al., 2006). The AOD, in association with relative humidity and sea-level atmospheric pressure, explains more than 70% variability in PM2.5 within ±150 min of overpass time window of the ESO Terra satellite and these estimates account for intra-pixel noise in PM. The PM–AOD association in Delhi is weaker than that reported in other parts of the world (Chu et al., 2005). As described above, the concentration of PM varies significantly across space and time. Therefore, it is critically important to match the spatial–temporal resolutions of AOD and PM as closely as possible. Although the 5 km AOD data used in the analysis is the first ever attempt to compute AOD from MODIS data at such a fine spatial resolution and collocated with a large number of spatially dispersed sites in the study area, we have observed substantial variability in PM2.5 within 5 km pixel. Moreover, for research on health effects we will need geographically detailed information on air pollution to compute precise exposure to ambient air pollution. Our future research aims at improving algorithms for computing AOD at 2.5 and 1 km spatial resolutions.
The temporal variability can be addressed by collecting air pollution data at different time intervals. Our analysis reveals the best association between AOD and PM2.5 within ±45 min of the overpass window of the EOS Terra satellite, and ±75 min window for the association between AOD and PM10. These findings have important implications for research that examines the relationship between AOD and PM in different parts of the world and for air pollution monitoring strategies.
In the absence of air pollution data at high spatial–temporal resolutions, researchers have begun to explore the potential of AOD to predict air quality in megacities in developing countries. Given the regional variations in the nature and sources of aerosol, the association between PM and AOD can vary regionally as reported by Gupta et al. (2006). This will require a field experiment to collect air pollution data using real-time samplers, because the existing air pollution monitoring stations use gravimetric method, which requires a minimum of eight or more hours of sampling, and the PM concentration reported from these samplers is the average for this duration, which can be quite noisy for PM–AOD analysis. The use of photometric samplers is one of the potential solutions for real-time monitoring of PM, and based on the results of our analysis, we recommend monitoring PM data at sufficiently large number of sites within ±75 min of the overpass time of satellites (generally 10:30 a.m. local time). For AOD data from both Terra (morning) and Aqua (afternoon) satellites, 9:00 a.m.–3:00 p.m. will be an ideal time window for collecting PM data on the ground.
A host of factors, such as sources of air pollution, proximity to water bodies, vegetation, seasonality and weather conditions, all of which vary regionally, can influence aerosol loading and hence its relationship with PM. Future research should also aim at studying the AOD–PM association with reference to sources of air pollution, land-use type and aerosol characterization. This article demonstrates a visual association between sources of air pollution—namely industrial locations and main roads—and the concentration of AOD and PM. Another interesting finding of our research is the diminishing level of AOD with the increasing distance from the city’s center, which clearly shows that air pollution distribution in the study area is an inverse function of distance from the city’s center.
A myriad of studies have shown relationship between AOD from satellite data and ground measurements of PM (Chu et al., 2005; Kaufman et al., 2002; Li et al., 2005; Wang and Christopher, 2003). Satellites with MODIS have been in orbit since the year 2000 and the spatial–temporal trends of PM2.5 and PM10 can be imputed with the aid of AOD since the 2000. But the relationship between AOD and PM observed in one region cannot be extrapolated to other, because the type and sources of aerosols and air pollution vary regionally and hence the strength of the relationship between AOD and PM. Therefore, it is important to establish an empirical relationship between AOD and PM using the current data, and use this relationship to impute estimates for the back years. It will require a field campaign to monitor PM daily at sufficiently large number of sites for about a year and then collocate PM data with the AOD data at as fine spatial–temporal resolutions as possible. Real-time photometric samplers, as demonstrated in this article, can be deployed to collect PM data at a large number of sites frequently and inexpensively.
The methodology demonstrated in this article has important implications for air quality management in the megacities of developing countries, particularly in India and China, because these cities have experienced significant deterioration in air quality by increase in income through foreign direct investment, urbanization, industrialization and abated increase in the demand for automobiles (Bell et al., 2004; Mukherji, 2006). Although data from various satellites can be used to compute air quality estimates, data from MODIS onboard Terra and Aqua, which have a daily repetitive global coverage, are particularly useful to compute daily estimates of air pollution needed to study the health effects of the short-term exposure to ambient air pollution. The results reported in this research can be used to predict PM surfaces for previous years in the study area. Although 5 km spatial resolution is inadequate to compute exposure to ambient air pollution, it can certainly be valuable to examine the time–space dynamics of air pollution in response to recently enacted environmental laws in Delhi. Future research to compute PM surfaces from AOD at high spatial resolution is likely to pave the way to compute exposure to ambient air pollution for health research.
Acknowledgments
We greatly acknowledge the funding support provided by the Population Studies and Training Center, Brown University to collect air pollution data and NICHD and NIH (Grant-R21 HD046571-01A1) for data analysis. We are thankful to Mr. Vineet Kumar and Dr. O.P. Malik for coordinating air pollution data collection.
Contributor Information
Naresh Kumar, Email: naresh-kumar@uiowa.edu.
Allen Chu, Email: achu@climate.gsfc.nasa.gov.
Andrew Foster, Email: Andrew_Foster@Brown.edu.
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