<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JEP</journal-id><journal-title-group><journal-title>Journal of Environmental Protection</journal-title></journal-title-group><issn pub-type="epub">2152-2197</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jep.2015.611113</article-id><article-id pub-id-type="publisher-id">JEP-61544</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Spatial and Temporal Variations of the Particulate Matter in Riyadh City, Saudi Arabia
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>bdullah</surname><given-names>S. Modaihsh</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fahd</surname><given-names>N. Al-Barakah</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mahmoud</surname><given-names>E. A. Nadeem</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mohamed</surname><given-names>O. Mahjoub</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Soil Science, College of Food and Agricultural Sciences, King Saud University, Riyadh, 
Kingdom of Saudi Arabia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>osmanmahjoub@gmail.com(MOM)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>12</day><month>11</month><year>2015</year></pub-date><volume>06</volume><issue>11</issue><fpage>1293</fpage><lpage>1307</lpage><history><date date-type="received"><day>22</day>	<month>October</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>24</month>	<year>November</year>	</date><date date-type="accepted"><day>27</day>	<month>November</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Mass concentrations of PM
  <sub>10</sub> and PM
  <sub>2.5</sub> for January 2012 up to October 2013 were measured at two sites; a suburban area, Riyadh airport (AP) and an urban area, King Fahd road district (KF) (densely trafficked site). Daily concentrations of both PM
  <sub>10</sub> and PM
  <sub>2.5</sub> measured at these two sites were highly variable. The temporal variation observed either for PM
  <sub>10</sub> or PM
  <sub>2.5</sub> was associated mainly with the dust events. The annual pattern of PM
  <sub>10</sub> and PM
  <sub>2.5</sub> at the AP station shows a significant increase in spring and summer (dusty seasons) where monthly mean concentrations of up to 696 μg&#183;m
  <sup>-3</sup> PM
  <sub>10</sub> were recorded in March. PM
  <sub>10</sub> concentrations during winter months are significantly lower, with 65 μg&#183;m
  <sup>-3</sup> measured in November and 78 μg&#183;m
  <sup>-3</sup> measured in December. January exhibits PM
  <sub>10</sub> concentrations little above 100 μg&#183;m
  <sup>-3</sup>. Both PM
  <sub>10</sub> and PM
  <sub>2.5</sub> showed substantial variations at these two monitoring stations during the study period. In the ur-ban station (King Fahd), average annual PM
  <sub>10</sub> varied by up to roughly a factor of two. This variation implies that local emission sources in this site often contribute much (i.e. greater than half) of the PM
  <sub>10</sub> mass on annual average. The variation of monthly (temporal) mean PM
  <sub>10</sub> at KF station showed more or less similar results to the AP station. Higher concentrations were observed during spring and summer (12%, 17% and 13% in Feb., March and April respectively and 17, 15% during June and July). Starting from September and October, PM
  <sub>10</sub> concentrations started to drop to 7% and 8% respectively. The relationships between the mean values of suspended particle concentrations and meteorological variables (relative humidity ambient temperature and wind speed) were analyzed. The results demonstrate that the influence of weather factors upon dust particulates is largely inconclusive. However, At KF station a moderate positive correlation was observed between wind speed and PM.
 
</p></abstract><kwd-group><kwd>PM&lt;SUB&gt;10&lt;/SUB&gt;</kwd><kwd> PM&lt;SUB&gt;2.5&lt;/SUB&gt;</kwd><kwd> Meteorological Data</kwd><kwd> Saudi Arabia</kwd><kwd> Riyadh</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Increased knowledge of the impact of suspended particulate matter on human health has significantly resulted in growing concern over the so-called particulate matter, in recent years. Since 1997, researches on air pollution have considered aerosols as one of the six major air pollutants [<xref ref-type="bibr" rid="scirp.61544-ref1">1</xref>] . Elevated particle concentration is strongly linked to increased mortality and morbidity [<xref ref-type="bibr" rid="scirp.61544-ref2">2</xref>] . According to their origin, particulate matters have been divided into natural and anthropogenic aerosols [<xref ref-type="bibr" rid="scirp.61544-ref3">3</xref>] . The major sources of anthropogenic aerosols include fuel combustion from automobiles, power plants, wood burning, industrial processes, and diesel powered vehicles such as buses and trucks. Soil-derived (mineral) dust particles can be a major part of the atmospheric PM<sub>2.5</sub> and PM<sub>10</sub> concentrations [<xref ref-type="bibr" rid="scirp.61544-ref4">4</xref>] . In the Kingdom of Saudi Arabia, studies of PM concentrations were extensively studied in Makkah, especially during the Hajj period when usually more than two million people visited the city to perform Hajj [<xref ref-type="bibr" rid="scirp.61544-ref5">5</xref>] -[<xref ref-type="bibr" rid="scirp.61544-ref7">7</xref>] . Recently, a brief review of the studies conducted in Saudi Arabia was presented [<xref ref-type="bibr" rid="scirp.61544-ref8">8</xref>] . To address the issue of atmospheric particulate matter in Riyadh city, El-Shobokshy [<xref ref-type="bibr" rid="scirp.61544-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.61544-ref10">10</xref>] conducted his pioneering study on particulate pollution in Saudi Arabia, but his studies concentrated only on atmospheric lead-pollution in the city of Riyadh. In 1990, investigation on the influence of meteorology on the concentration of inhalable particulate which was usually observed in the atmosphere of Riyadh at high concentrations was undertaken [<xref ref-type="bibr" rid="scirp.61544-ref11">11</xref>] . However, the studies mentioned above were based on limited number of samples. A relatively detailed study on PM samples collected from June 2006 to May 2007 showed that the PM concentrations were higher for PM<sub>10</sub> compared to PM<sub>2.5</sub>, indicating that the major PM source was local dust [<xref ref-type="bibr" rid="scirp.61544-ref12">12</xref>] . A recent study showed that PM concentration was approximately 3 times higher than the country’s ambient air quality standards respectively. In addition, this study demonstrated that summer vs. winter comparison showed that PM concentrations were approximately 84% higher in summer [<xref ref-type="bibr" rid="scirp.61544-ref13">13</xref>] .</p><p>The primary goal of this study was to carry out a comprehensive characterization of PM<sub>1</sub>, and PM<sub>2.5</sub> and provide the scientific background for further control of air pollution at Riyadh and to develop effective strategies to reduce the ambient deposition and concentrations of those pollutants to the city.</p></sec><sec id="s2"><title>2 Methods</title><p>Traditional method of PM<sub>10</sub> dust measurement is based on a weight to volume measurement, where by the dust is collected on a filer and subsequently weighed. This method requires a rigid adherence to time consuming procedures. With the finer dust size fraction introduction (PM<sub>2.5</sub>, PM<sub>1</sub>) the problem is negligible mass compared to the large numbers of these particles. For these reason a newly developed Aerosol Spectrometer will be introduced for measurement of various PM particulates.</p><p>In this study, the concentrations of coarse (PM<sub>10</sub>), and fine (PM<sub>2.5</sub>), particulate matter were measured using a Grimm model EDM 365 aerosol spectrometer (Grimm Aerosol Technique GmbH, Airing, Germany). The device, an optical particle counter (OPC), is an instrument for real-time measurement of particulate matter. The particle size analyzer/dust monitor determines the dust-concentration (counts/liter) through the optical-light- scattering method directly; however, the mass concentration is determined by extrapolation. The calculated mass concentration may be corrected to the specific aerosol measured with the gravimetric-correction factor (C-Factor). The advantages of this instrument over other real-time measurement instruments, such as TEOM or DMA devices, are its convenience, its low maintenance requirements, and its ability to run for long periods without specific supervision. The ability to measure particulate matter concentrations in time intervals ranging from 1 s to 60 min is considered to be another advantage offered by the instrument. The validity of the measurements performed by the instrument has been evaluated by several studies [<xref ref-type="bibr" rid="scirp.61544-ref14">14</xref>] . The dust monitor was installed on the roof of the Meteorology and Environmental building near Riyadh airport. The dust monitor runs 24 hours a day continuously.</p></sec><sec id="s3"><title>3 Results and Discussion</title><sec id="s3_1"><title>3.1. Seasonal and Monthly Variability in PM Concentrations</title><sec id="s3_1_1"><title>3.1.1. Airport Station</title><p>The monthly variation of PM<sub>10</sub> concentrations as obtained from the daily mean recordings across the whole study period (February 2012 to January 2013) is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>. Results indicate that the highest PM concentrations occurs mainly in February, March and April, which is the period with the most frequent dust-storm</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Average monthly PM<sub>10</sub> mass concentration during Feb. 2012-January 2013 (A.P)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x7.png"/></fig><p>events [<xref ref-type="bibr" rid="scirp.61544-ref15">15</xref>] . The highest PM<sub>10</sub> concentration (2234 &#181;g・m<sup>−3</sup>) is recorded during March 18<sup>th</sup>, closely associated with a severe dust event. One can, therefore, conclude that the intense dust storms taking place on specific days during spring and early summer are predominantly responsible for the large month-to month variations at all PM concentrations. The annual pattern of PM<sub>10</sub> shows a significant increase in spring and summer where monthly mean concentrations of up to 696 μg・m<sup>−3</sup> were recorded in March. PM<sub>10</sub> concentrations during winter months are significantly lower, with 65 μg・m<sup>−3</sup> measured in November and 79 μg・m<sup>−3</sup> measured in December. January exhibits PM<sub>10</sub> concentrations of little above 100 μg・m<sup>−3</sup>, which persists until February when PM<sub>10</sub> levels increase as a result of dust events.</p><p>The PM<sub>10</sub> data when grouped by month (<xref ref-type="fig" rid="fig2">Figure 2</xref>), indicated a consistent and systematic pattern decreasing in the order: spring (February-April, 53%) followed by summer (May-July, 30%) and fall and winter (September- January, 18%). The spring Peak of PM<sub>10</sub> is coinciding with dust events that commonly occur during spring in Riyadh. In contrast, the lowest PM concentration in winter can be attributed to the absence of dust events during winter. The variation of monthly mean PM<sub>2.5</sub> (<xref ref-type="fig" rid="fig3">Figure 3</xref>, <xref ref-type="fig" rid="fig4">Figure 4</xref>) is quite similar to PM<sub>10</sub>; (March maximum). The similarity in the annual variation between PM<sub>10</sub> and PM<sub>2.5</sub> suggests some similarities in source regions for these aerosol sizes.</p><p>Some studies conducted in other urban environments, in Turkey [<xref ref-type="bibr" rid="scirp.61544-ref16">16</xref>] and in Athens, Greece [<xref ref-type="bibr" rid="scirp.61544-ref17">17</xref>] found, contrary to our results, that in winter both PM concentrations were higher, which was attributed to larger use of fossil fuels in winter. A monthly mean PM<sub>10</sub> concentrations in Athens ranging from 60.3 μg・m<sup>−3</sup> (January) to 88.9 μg・m<sup>−3</sup> (December), with an annual mean value of 75.5μg・m<sup>−3</sup> was reported [<xref ref-type="bibr" rid="scirp.61544-ref17">17</xref>] . In Barcelona, Spain, the ambient PM<sub>10</sub> and PM<sub>2.5</sub> were in the range of 39 to 42 μg・m<sup>−3</sup> and 25 to 29 μg・m<sup>−3</sup>, respectively over the period 2003-2006 with 97 daily values exceeding 50 μg・m<sup>−3</sup> [<xref ref-type="bibr" rid="scirp.61544-ref18">18</xref>] while the mean annual PM10 concentration ranges from 20 to 37 μg・m<sup>−3</sup> in Rio de Janeiro, Brazil [<xref ref-type="bibr" rid="scirp.61544-ref19">19</xref>] . Comparing the present results with those of the above- mentioned studies, it is concluded that the city of Riyadh is exposed to much higher PM concentration levels. This is not only the case for summer, when the area is affected by natural phenomena, but also for winter. This highlights the fact that PM concentrations over Riyadh can be regarded as a genuine environmental problem that poses a real risk to quality of life and threatens human health.</p></sec><sec id="s3_1_2"><title>3.1.2. King Fahd Station (2012)</title><p>The monthly mean values of PM<sub>10</sub>, PM<sub>2.5</sub>, and PM<sub>1</sub> in 2012-2013 are shown in <xref ref-type="fig" rid="fig5">Figure 5</xref>-7, and the month wise percentage share of PM<sub>10</sub> in 2012 is shown in a pie chart (<xref ref-type="fig" rid="fig8">Figure 8</xref>). The concentrations of PM<sub>10</sub> are highest in summer (June-July 23% and 24% respectively). The concentration decreases in September and October (14%) and reaches its minimum in November (10%). The monthly variability of PM<sub>2.5</sub> (<xref ref-type="fig" rid="fig9">Figure 9</xref>) followed the same trend except the relatively higher percentage which was registered in December (20%). On the other hand it is noticeable that the monthly variability of PM<sub>1</sub> (<xref ref-type="fig" rid="fig1">Figure 1</xref>0) reflected higher percentage in winter months, (December, November and October, 21%, 17% and 17% respectively). The difference in the monthly variation</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Monthly variation of PM<sub>10</sub> represented as pie chart (A.P)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x8.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Average monthly PM<sub>2.5</sub> mass concentration during Feb. 2012-January 2013 (A.P)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x9.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Monthly variation of PM<sub>2.5</sub> represented as pie chart (A.P)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x10.png"/></fig><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Average monthly (King Fahd) PM<sub>10</sub> mass concentration during June 2012-October 2013 (A.P)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x11.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Average monthly (King Fahd) PM<sub>2.5</sub> mass concentration during June 2012-October 2013</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x12.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Average monthly (King Fahd) PM<sub>1</sub> mass concentration during June 2012-October 2013</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x13.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Monthly variation of PM<sub>10</sub> represented as pie chart (King Fahd 2012)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x14.png"/></fig><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Monthly variation of PM<sub>2.5</sub> represented as pie chart (King Fahd 2012)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x15.png"/></fig><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>0</label><caption><title> Monthly variation of PM<sub>1.0</sub> represented as pie chart (King Fahd 2012)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x16.png"/></fig><p>between PM<sub>10</sub> on one hand and PM <sub>2.5</sub> and PM<sub>1.0</sub> on the other hand, may suggests differences in source regions for these aerosol sizes. The main anthropogenic source of PM<sub>2.5-1</sub> in Riyadh urban environment can be confined to vehicular traffic, fossil-fuel combustion, been observed within urban environments in other cities [<xref ref-type="bibr" rid="scirp.61544-ref20">20</xref>] - [<xref ref-type="bibr" rid="scirp.61544-ref22">22</xref>] . In addition, the boundary layer mixing height is lower in winter and traps the pollutants near the ground as a result of temperature inversions. This may explain the relatively higher concentration of small-sized particles (PM<sub>1.0</sub>) in winter. In contrast, during summer months thermal heating at the surface and the increase of the mixing layer height favors buoyancy and the dilution of anthropogenic aerosols (PM<sub>1.0</sub>). Apart from desert dust, a natural contribution to the total PM (mainly to PM<sub>2.5</sub> and PM<sub>10</sub>) is also expected to originate from eolian and traffic- driven re-suspension of dust, since the scarce rainfall favors the accumulation of road dust in summer.</p></sec><sec id="s3_1_3"><title>3.1.3. King Fahd Station (2013)</title><p>The variation of monthly mean PM<sub>10</sub> in 2013 showed more or less similar results to 2012 during month June, July, September and October. Higher concentrations were observed during spring and summer (12%, 17% and 13% in Feb., March and April respectively and 17, 15% during June and July,). Starting from September and October PM<sub>10</sub> concentrations started to drop to 7% and 8% respectively (<xref ref-type="fig" rid="fig1">Figure 1</xref>1). Data of November and December is expected to drop further as was demonstrated in 2012 at both KF and AP stations. As described above, a characteristic seasonal variation can be observed during 2013 with relatively elevated PM concentrations observed in the warmer seasons peaking in March, June and July (<xref ref-type="fig" rid="fig1">Figure 1</xref>1). This is consistent with the earlier results at the airport station. Higher summertime PM concentrations can be attributed to elevated wind speed that enhances wind induced re-suspended PM concentrations. Wind speeds are higher in the summer. A somewhat similar pattern―if reduced in magnitude was observed during 2012</p><p>In contrast, the variation of monthly mean PM<sub>2.5</sub> and PM<sub>1</sub> concentrations vary less seasonally compared to PM<sub>10</sub> mass concentrations (<xref ref-type="fig" rid="fig1">Figure 1</xref>2, <xref ref-type="fig" rid="fig1">Figure 1</xref>3) This has been observed previously during 2012. This could be due to the fact that a major source for PM<sub>2.5</sub> and PM<sub>1</sub> which is motor-vehicle emissions is not directly affected by seasons. In contrast, secondary atmospheric formation of fine particles through photochemical processes is higher during the summer (relatively higher concentrations are observed from May?October). Stronger source strength in the summer however is counterbalanced by the lower mixing height in winter months thus reducing seasonal variability.</p><p>In general, the results of PM<sub>10</sub>, PM<sub>2.5,</sub> and, PM<sub>1</sub> concentrations, obtained during the current work were little higher than those found in other studies. Results obtained by studies of PM<sub>2.5</sub> concentrations conducted in China [<xref ref-type="bibr" rid="scirp.61544-ref23">23</xref>] reported a mean PM<sub>2.5</sub> concentration of 67.6 &#181;g/m<sup>3</sup>. Also [<xref ref-type="bibr" rid="scirp.61544-ref24">24</xref>] reported 89 &#181;g/m<sup>3</sup> during the spring. These values are little less than the values reported in this study. On the other hand, some other studies reported more or less similar results. For an example, PM<sub>10</sub> concentrations higher than 3000 and produced by dust events were</p><fig id="fig11"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>1</label><caption><title> Monthly variation of PM<sub>10</sub> represented as pie chart (King Fahd 2013)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x17.png"/></fig><fig id="fig12"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>2</label><caption><title> Monthly variation of PM<sub>2.5</sub> represented as pie chart (King Fahd 2013)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x18.png"/></fig><fig id="fig13"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>3</label><caption><title> Monthly variation of PM<sub>1.0</sub> represented as pie chart (King Fahd 2013)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x19.png"/></fig><p>observed in a study conducted in Iraq, Kuwait and Saudi Arabia [<xref ref-type="bibr" rid="scirp.61544-ref25">25</xref>] . In contrast, Meng and Lu [<xref ref-type="bibr" rid="scirp.61544-ref26">26</xref>] observed mean PM<sub>2.5</sub> concentrations of up to 216.7 &#181;g/m<sup>3</sup>, which was higher than the results presented in this study (almost double). The explanation for this substantial difference is that the PM<sub>2.5</sub> is measured during winter months where fossil fuel combustions which considered as the primary source of fine particulate are highest.</p></sec></sec><sec id="s3_2"><title>3.2. Frequency Distribution of PM<sub>10</sub> and PM<sub>2.5</sub> Concentrations</title><sec id="s3_2_1"><title>3.2.1. Airport</title><p>The frequency of occurrence for PM<sub>10</sub> and PM<sub>2.5</sub> concentrations for the studied period in A.P station showed that 4.5% of the PM10 values were more than 1000 μg・m<sup>−3</sup> occurring all in spring. Approximately 9.5%, 9% and 16% occurred at 500 - 1000, 340 - 500 and 200 - 340 μg・m<sup>−3</sup> interval, respectively. A peak in the distribution of PM<sub>10</sub> concentrations occurred at 100 - 200 μg・m<sup>−3</sup>, (32%). The percentage of occurrence of values 50 - 100 μg・m<sup>−3</sup> and less than 50 μg・m<sup>−3</sup> were 19% and 9% respectively. PM<sub>10</sub> values &lt;50 μg・m<sup>−3</sup> is observed in winter months (<xref ref-type="table" rid="table1">Table 1</xref>, <xref ref-type="table" rid="table2">Table 2</xref>).</p><p>Regarding the frequency distributions of PM<sub>2.5</sub> in all seasons the largest frequency is observed for values between 35 and 100 μg・m<sup>−3</sup>, (52%), while in spring the largest frequency shifts towards higher values (100 - 600 μg・m<sup>−3</sup>, 18%. Similarly to PM10, spring presents a broader distribution for PM<sub>2.5</sub>, with values &gt;100 μg・m<sup>−3</sup></p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Frequency of occurrence of PM<sub>10</sub> concentrations (King Fahad)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Season</th><th align="center" valign="middle" >PM<sub>10</sub> concentration</th><th align="center" valign="middle" >% Frequency</th></tr></thead><tr><td align="center" valign="middle"  rowspan="5"  >June-September 2012</td><td align="center" valign="middle" >&gt;1000</td><td align="center" valign="middle" >2</td></tr><tr><td align="center" valign="middle" >500 - 1000</td><td align="center" valign="middle" >23</td></tr><tr><td align="center" valign="middle" >340 - 500</td><td align="center" valign="middle" >19</td></tr><tr><td align="center" valign="middle" >180 - 340</td><td align="center" valign="middle" >55</td></tr><tr><td align="center" valign="middle" >&lt;180</td><td align="center" valign="middle" >0</td></tr><tr><td align="center" valign="middle"  rowspan="6"  >October-January</td><td align="center" valign="middle" >&gt;1000</td><td align="center" valign="middle" >1</td></tr><tr><td align="center" valign="middle" >500 - 1000</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle" >340 - 500</td><td align="center" valign="middle" >15</td></tr><tr><td align="center" valign="middle" >200 - 340</td><td align="center" valign="middle" >40</td></tr><tr><td align="center" valign="middle" >100 - 200</td><td align="center" valign="middle" >31</td></tr><tr><td align="center" valign="middle" >50 - 100</td><td align="center" valign="middle" >7</td></tr><tr><td align="center" valign="middle"  rowspan="6"  >Feb-March</td><td align="center" valign="middle" >&gt;1000</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle" >500 - 1000</td><td align="center" valign="middle" >17</td></tr><tr><td align="center" valign="middle" >340 - 500</td><td align="center" valign="middle" >18.5</td></tr><tr><td align="center" valign="middle" >200 - 340</td><td align="center" valign="middle" >47.5</td></tr><tr><td align="center" valign="middle" >100 - 200</td><td align="center" valign="middle" >12</td></tr><tr><td align="center" valign="middle" >50 - 100</td><td align="center" valign="middle" >0</td></tr><tr><td align="center" valign="middle"  rowspan="5"  >June-October</td><td align="center" valign="middle" >&gt;1000</td><td align="center" valign="middle" >3</td></tr><tr><td align="center" valign="middle" >500 - 1000</td><td align="center" valign="middle" >12</td></tr><tr><td align="center" valign="middle" >340 - 500</td><td align="center" valign="middle" >11</td></tr><tr><td align="center" valign="middle" >200 - 340</td><td align="center" valign="middle" >30</td></tr><tr><td align="center" valign="middle" >100 - 200</td><td align="center" valign="middle" >43</td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Frequency of occurrence of PM<sub>2.5</sub> concentrations (King Fahad)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Season</th><th align="center" valign="middle" >PM<sub>10</sub> concentration</th><th align="center" valign="middle" >% Frequency</th></tr></thead><tr><td align="center" valign="middle"  rowspan="3"  >June-September 2012</td><td align="center" valign="middle" >&gt;100</td><td align="center" valign="middle" >27</td></tr><tr><td align="center" valign="middle" >50 - 100</td><td align="center" valign="middle" >50</td></tr><tr><td align="center" valign="middle" >Less than 50</td><td align="center" valign="middle" >23</td></tr><tr><td align="center" valign="middle"  rowspan="6"  >October-January</td><td align="center" valign="middle" >More 500</td><td align="center" valign="middle" >1.5</td></tr><tr><td align="center" valign="middle" >200 - 500</td><td align="center" valign="middle" >3</td></tr><tr><td align="center" valign="middle" >100 - 200</td><td align="center" valign="middle" >6</td></tr><tr><td align="center" valign="middle" >50 - 100</td><td align="center" valign="middle" >57.5</td></tr><tr><td align="center" valign="middle" >Less than 50</td><td align="center" valign="middle" >33</td></tr><tr><td align="center" valign="middle" >More 200</td><td align="center" valign="middle" >8.5</td></tr><tr><td align="center" valign="middle"  rowspan="4"  >Feb-March</td><td align="center" valign="middle" >100 - 200</td><td align="center" valign="middle" >18.5</td></tr><tr><td align="center" valign="middle" >50 - 100</td><td align="center" valign="middle" >46</td></tr><tr><td align="center" valign="middle" >Less than 50</td><td align="center" valign="middle" >27</td></tr><tr><td align="center" valign="middle" >More 200</td><td align="center" valign="middle" >4</td></tr><tr><td align="center" valign="middle"  rowspan="3"  >June-October</td><td align="center" valign="middle" >100 - 200</td><td align="center" valign="middle" >16</td></tr><tr><td align="center" valign="middle" >50 - 100</td><td align="center" valign="middle" >37</td></tr><tr><td align="center" valign="middle" >Less than 50</td><td align="center" valign="middle" >42</td></tr></tbody></table></table-wrap><p>range. Apart from these similarities in the PM<sub>10</sub> and PM<sub>2.5</sub> frequency distributions, some differences in winter and summer reveal a possible different source of aerosols in these seasons (natural or anthropogenic). For example, the intense dust storms during summer do not have such a pronounced signal in PM<sub>2.5</sub> concentrations as in PM<sub>10</sub> ones, while the larger contribution of anthropogenic aerosols in winter rather increases the PM<sub>2.5</sub> levels. However, it should be noted that dust events may also affect significantly the PM<sub>2.5</sub> levels, as observed during a severe dusty day in March.</p></sec><sec id="s3_2_2"><title>3.2.2. King Fahd</title><p>The frequency of occurrence for PM<sub>10</sub> and PM<sub>2.5 </sub>concentrations for each season is depicted in table, respectively. In summer 2012 (June-September), 55% of the PM<sub>10</sub> values were between 180 and 340 μg・m<sup>−3</sup>; 25% of the PM<sub>10</sub> values were more than 500 μg・m<sup>−3</sup>. In October 2012 to January 2013, the frequency distribution shifts towards lower values, with values above 500 μg・m<sup>−3</sup> only 6% and the peak frequency occurred for values between 200 - 340 μg・m<sup>−3</sup> (40%). On the other hand, a considerable fraction (24%) of PM<sub>10</sub> values &lt;500 μg・m<sup>−3</sup> is observed in spring (Feb.-March). The frequency of occurrence for PM10 during June to October is some who resembles the values of the summer months. Peak concentrations occurred for values between 100 - 200 μg・m<sup>−3</sup> (43%), 15% of the values were above 500 μg・m<sup>−3</sup>. Regarding the frequency distributions of PM<sub>2.5</sub> in all seasons except June- October, the largest frequency is observed for values between 50 and 100 μg・m<sup>−3</sup>, while in June-October the largest frequency shifts towards lower values (&lt;50 μg・m<sup>−3</sup>), which is opposite to that observed for PM<sub>10</sub>. However, similarly to PM<sub>10</sub>, summer presents a broader distribution for PM<sub>2.5</sub>, with values &gt; a 100 μg・m<sup>−3</sup> range. Apart from these similarities in the PM<sub>10</sub> and PM<sub>2.5</sub> frequency distributions, some differences in winter and summer reveal a possible different source of aerosols in these seasons (natural or anthropogenic). For example, the intense dust storms during summer do not have such a pronounced signal in PM<sub>2.5</sub> concentrations as in PM<sub>10</sub> ones, while the larger contribution of anthropogenic aerosols in winter rather increases the PM<sub>2.5</sub> levels. Also note that the mean PM<sub>2.5</sub> in winter (32 μg・m<sup>−3</sup>) is similar to that of spring and larger than that of autumn, despite the fact that winter PM<sub>10</sub> is the lowest. However, it should be noted that dust events may also affect significantly the PM<sub>2.5</sub> levels, as observed during a severe dusty day in June (PM<sub>2.5</sub> daily value of 182 μg・m<sup>−3</sup>) (<xref ref-type="table" rid="table1">Table 1</xref>, <xref ref-type="table" rid="table2">Table 2</xref>).</p><p>During this study period, we observed that PM<sub>10</sub> and PM<sub>2.5</sub> concentrations mainly depend on dust storms occasions and increased significantly during dust storms; however, there is no universally accepted definition of dust storms in terms of hourly dust concentrations. Previous researchers have classified dust storms by their intensities on the basis of hourly mean PM<sub>10</sub> concentrations together with wind speed and visibility. The classification system proposed by Hoffmann et al., [<xref ref-type="bibr" rid="scirp.61544-ref27">27</xref>] is based on the hourly mean PM<sub>10</sub> concentration in combination with visibility and wind speed as follows: “dusty air” (haze) means hourly mean PM<sub>10</sub> concentrations higher than 50 μg・m<sup>−3</sup>; “light dust storm”, &gt;200 μg・m<sup>−3</sup>; “dust storm”, &gt;500 μg・m<sup>−3</sup>; “strong dust storm”, &gt;2000 μg・m<sup>−3</sup>; and “serious strong dust storm”, &gt;5000 μg・m<sup>−3</sup>.Wang et al. [<xref ref-type="bibr" rid="scirp.61544-ref28">28</xref>] used hourly mean PM<sub>10</sub> concentrations of &lt;200 μg・m<sup>−3</sup> for “suspended dust,” 200 - 5500 μg・m<sup>−3</sup> for “blowing dust,” 5500 - 15,000 μg<sup>?3</sup> for “sand and dust storm”, and &gt;15,000 μg<sup>−3</sup> for “severe sand and dust storm”. <sup> </sup></p><p>In Taiwan an Asian dust storm event is defined each day that hourly mean PM<sub>10</sub> concentrations observed at the Yangmingshan station exceed the air quality standard (125 μg・m<sup>−3</sup>) for a period of at least 3 h [<xref ref-type="bibr" rid="scirp.61544-ref29">29</xref>] . Dust storms are defined in Korea when the measured PM<sub>10</sub> concentration exceeds 190 μg・m<sup>−3</sup> for at least 2 h [<xref ref-type="bibr" rid="scirp.61544-ref30">30</xref>] . The KMA has developed an Asian Dust Warning System with alarm, advisory, and warning levels depending on the dust concentration. Alarms, advisories, and warnings are issued when the hourly mean dust concentrations (PM<sub>10</sub>) are expected to exceed 300 μg・m<sup>−3</sup>, 400 μg・m<sup>−3</sup>, or 800 μg・m<sup>−3</sup>, respectively, for over 2 h [<xref ref-type="bibr" rid="scirp.61544-ref30">30</xref>] . Park et al. (2010) [<xref ref-type="bibr" rid="scirp.61544-ref31">31</xref>] identified dust events as the peak PM10 concentration exceeding one standard deviation of the annual mean concentration. We arbitrary choose this criterion. Our criterion for dust storm events was an hourly mean PM<sub>10</sub> concentration exceeding one standard deviation of the mean concentration at the airport station during February 2012 to January 2013 months (mean = 282.11.34 &#181;g/m<sup>3</sup> and standard deviation = 372). Based on this criterion, we identified 16, 21, 10, 6, 5, 6 and 1 dust events at February, March, April, May, June, July and December 2013. Based on the same criterion, we identified 8, 17, 7, 7, 3, and 6 dust events at June, July, September, October, November and December 2012 and 14, 11, 20, 16, 7, 9, and 4 at January, February, March, June, July September and October 2013 respectively.</p></sec></sec><sec id="s3_3"><title>3.3. Influence of Meteorological Parameters on Particulate Matter</title><p>Air quality strongly depends on the dynamics of the atmosphere and meteorological conditions play a vital role in governing the fate of air pollutants. During the monitoring period in the AP station, the hottest day of 2012 was July 17, with a high temperature of 47˚C. The longest warm spell was from July 14 to August 5, constituting 23 consecutive days with warmer than average high temperatures. The month of May had the largest fraction of warmer than average days with 84% days with higher than average high temperatures.</p><p>The highest sustained wind speed was 15 m/s, occurring on February 2; the highest daily mean wind speed was 10 m/s (June 3); and the highest wind gust speed was 23 m/s (February 25). The windiest month was May, with an average wind speed of 4 m/s. The least windy month was October, with an average wind speed of 2 m/s.</p><p>The average daily temperature in KF was found to be very similar to that of the AP. The relative humidity had also rather a low spatial variability (Correlation coefficients for temperature and relative humidity for these two sites was r = 0.899 and 0.974 respectively</p><p>The relationships between the mean values of suspended particle concentrations and meteorological variables (relative humidity and ambient temperature for these two locations and wind speed, temperature and relative humidity for KF station , were analyzed using Pearson’s correlation analysis, the analyses results are represented in <xref ref-type="table" rid="table3">Table 3</xref> for the AP and <xref ref-type="table" rid="table4">Table 4</xref> for KF.</p><p>The results indicated that, the PM<sub>10</sub> and PM<sub>2.5</sub> were strongly correlated with each other and inversely correlated with temperature and relative humidity with correlation coefficient of −0.11 and −0.15 respectively at the AP station. The resulting t-value is not statistically significant at the 0.05 level. This may be due to the fact that means of the whole day of PM on one hand and the average temperature humidity on the other hand might cancel the variation between night and day. In this regard, Shao [<xref ref-type="bibr" rid="scirp.61544-ref32">32</xref>] , stated that the influence of weather factors upon repairable dust particulates is largely inconclusive. Never the less, several studies have confirmed the influence of meteorological conditions on PM concentrations [<xref ref-type="bibr" rid="scirp.61544-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.61544-ref34">34</xref>] . Atmospheric pressure, wind velocity temperature and humidity were found to be significant factors in influencing PM.</p><p>On the other hand, at KF station a moderate positive correlation was observed between wind speed and PM (r = 0.48, 0.45 and 0.38 for PM<sub>10</sub>, PM<sub>2.5</sub>, and PM<sub>1</sub> respectively) due to their suspension effect of wind. The best correlation was observed with wind speeds and PM<sub>10</sub> (r = 0.48). It seems that the wind has the potential to transport particulates between areas around the studied site. Contrary to our results Oren [<xref ref-type="bibr" rid="scirp.61544-ref35">35</xref>] , found that wind speed yielded negative correlation with PM<sub>10</sub> but positive and statistically significant at 0.01 confidence level with PM<sub>2.5-10</sub>. Wind speed plays a leading role in cleansing atmosphere of fine particulates compare to course. Wind speed affects the turbulence near the ground. The greater the wind speed, the greater the dispersion of particulates, the greater the dilution effects and transport of the particulate hence the lower the mass concentration [<xref ref-type="bibr" rid="scirp.61544-ref36">36</xref>] .</p><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Correlation coefficient of particulate data and meteorological factors AP station</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >PM<sub>10</sub></th><th align="center" valign="middle" >PM<sub>2.5</sub></th><th align="center" valign="middle" >TEMP</th><th align="center" valign="middle" >RH</th><th align="center" valign="middle" >Dew point</th></tr></thead><tr><td align="center" valign="middle" >PM<sub>10</sub></td><td align="center" valign="middle" >1.000</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >PM<sub>2.5</sub></td><td align="center" valign="middle" >0.986**<sup> </sup></td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >TEMP</td><td align="center" valign="middle" >−0.108</td><td align="center" valign="middle" >−0.105</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >RH</td><td align="center" valign="middle" >−0.147</td><td align="center" valign="middle" >−0.090</td><td align="center" valign="middle" >−0.708</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Dew point</td><td align="center" valign="middle" >−0.398</td><td align="center" valign="middle" >−0.338</td><td align="center" valign="middle" >0.082</td><td align="center" valign="middle" >0.6454</td><td align="center" valign="middle" >1.00</td></tr></tbody></table></table-wrap><p>** Highly significant.</p><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Correlation coefficient of particulate data and meteorological factors KF station</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >PM<sub>10</sub></th><th align="center" valign="middle" >PM<sub>2.5</sub></th><th align="center" valign="middle" >PM<sub>1</sub></th><th align="center" valign="middle" >TEMP</th><th align="center" valign="middle" >RH</th><th align="center" valign="middle" >Wind speed</th><th align="center" valign="middle" >Dew point</th></tr></thead><tr><td align="center" valign="middle" >PM<sub>10</sub></td><td align="center" valign="middle" >1.000</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >PM<sub>2.5</sub></td><td align="center" valign="middle" >0.967<sup> </sup></td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >PM<sub>1</sub></td><td align="center" valign="middle" >0.792</td><td align="center" valign="middle" >0.871</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >TEMP</td><td align="center" valign="middle" >0.074</td><td align="center" valign="middle" >−0.009</td><td align="center" valign="middle" >−0.0922</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >RH</td><td align="center" valign="middle" >−0.127</td><td align="center" valign="middle" >−0.090</td><td align="center" valign="middle" >0.203</td><td align="center" valign="middle" >−0.772</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Wind speed</td><td align="center" valign="middle" >0.479</td><td align="center" valign="middle" >0.453</td><td align="center" valign="middle" >0.380</td><td align="center" valign="middle" >0.182</td><td align="center" valign="middle" >−0.107</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Dew point</td><td align="center" valign="middle" >−0.147</td><td align="center" valign="middle" >-0.334</td><td align="center" valign="middle" >0.222</td><td align="center" valign="middle" >−0.101</td><td align="center" valign="middle" >0.6454</td><td align="center" valign="middle" >−0.0306</td><td align="center" valign="middle" >1.00</td></tr></tbody></table></table-wrap></sec><sec id="s3_4"><title>3.4. Spatial Variations of PM<sub>10</sub> and PM<sub>2.5</sub></title><p><xref ref-type="fig" rid="fig1">Figure 1</xref>4 shows the average concentrations of PM<sub>10</sub> and PM<sub>2.5</sub> at these two monitoring stations during the study period. Both PM<sub>10</sub> and PM<sub>2.5</sub> showed substantial variations. In the urban station (King Fahd) average annual PM<sub>10</sub> varied by up to roughly a factor of two. This variation imply that local emission sources often contribute much (i.e. greater than half) of the PM<sub>10</sub> mass on annual average. This may be attributed to the strengths of the related anthropogenic sources, as reflected by population size and traffic density. The observation of high PM<sub>10</sub> levels in highly trafficked areas has been reported extensively. Based on the measurements at six locations of Kathmandu Valley, Nepal, Aryal et al. [<xref ref-type="bibr" rid="scirp.61544-ref37">37</xref>] reported that the mean PM<sub>10</sub> values varied considerably from 42 (rural area) to 230 &#181;g/m<sup>3</sup> (urban roadside).</p><p>Similarly, based on the study from Seoul, Korea, Bae et al., [<xref ref-type="bibr" rid="scirp.61544-ref38">38</xref>] reported enhanced levels of PM<sub>10</sub> in roadside (URS) over urban background (U-BG), despite similarity in relative diurnal patterns at each site. Likewise, [<xref ref-type="bibr" rid="scirp.61544-ref39">39</xref>] also reported enhanced (24.5%) levels of PM<sub>10</sub> at roadside relative to background site in Seoul which is explained by the direct effect and proximity of vehicular sources [<xref ref-type="bibr" rid="scirp.61544-ref40">40</xref>] .</p><fig id="fig14"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>4</label><caption><title> Concentrations of PM<sub>10</sub> and PM<sub>2.5</sub> at these two monitoring stations</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-6702783x20.png"/></fig></sec></sec><sec id="s4"><title>4. Conclusions</title><p>This study provides a valuable and complementary baseline data on PM. It is the first of its kind in which such data are collected in Riyadh city. However, Readers should be cautioned that the data presented in this report represent only one year of data (twelve months), and that patterns may vary and may not be conclusive at this stage. Since many studies have demonstrated a close relationship between particulate matter (PM) pollution and deterioration in human health, as such, there is a need for constantly monitoring the air quality and PM concentrations throughout Riyadh city to find out if different areas meet national ambient air quality standards. These standards require to be reviewed every 5 years to make sure the standards protect human health and the environment. The standards must protect groups of people who are most at risk from the pollution.</p><p>The following conclusions were reached:</p><p>1) The results show that the PM concentrations are considerably higher than the corresponding European Union air quality annual standard.</p><p>2) PM<sub>2.5</sub> data appear to be a constant fraction of the PM<sub>10</sub> at all the sites, indicating common influences of meteorology and sources.</p><p>3) Statistical analysis of air quality data shows that PM<sub>10</sub> and PM<sub>2.5</sub> are showing poor correlation with temperature and relative humidity. Wind speed is moderately correlated with PM.</p><p>4) There are clear associations between PM<sub>10</sub> and PM<sub>2.5</sub> data sets throughout the study period.</p></sec><sec id="s5"><title>Acknowledgements</title><p>This study was funded by the National Plan for Science, Technology and Innovation (MAARIFAH), King Abdulaziz City for Science and Technology, Kingdom of Saudi Arabia, Project #8 ENV319-02 under the title “Characteristics and Composition of the Falling Dust and Particulate Matter and Its Health Hazards in Riyadh City, Saudi Arabia”.</p></sec><sec id="s6"><title>Cite this paper</title><p>Abdullah S.Modaihsh,Fahd N.Al-Barakah,Mahmoud E. A.Nadeem,Mohamed O.Mahjoub, (2015) Spatial and Temporal Variations of the Particulate Matter in Riyadh City, Saudi Arabia. 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