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    <title>NISCAIR Online Periodicals Repository Collection: IJRSP Vol.39(4) [August 2010]</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10161</link>
    <description />
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        <rdf:li resource="http://nopr.niscair.res.in/handle/123456789/10168" />
        <rdf:li resource="http://nopr.niscair.res.in/handle/123456789/10167" />
        <rdf:li resource="http://nopr.niscair.res.in/handle/123456789/10166" />
        <rdf:li resource="http://nopr.niscair.res.in/handle/123456789/10165" />
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    <title>The Collection's search engine</title>
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  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10168">
    <title>Carbonaceous aerosols at a suburban site in Indo-Gangetic plain</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10168</link>
    <description>Title: Carbonaceous aerosols at a suburban site in Indo-Gangetic plain
&lt;br/&gt;
&lt;br/&gt;Authors: Satsangi, Aparna; Pachauri, Tripti; Singla, Vyoma; Lakhani, Anita; Kumari, K Maharaj
&lt;br/&gt;
&lt;br/&gt;Abstract: Carbonaceous&#xD;
aerosols are emitted by combustion sources and may influence the climate by&#xD;
altering the radiation balance of the atmosphere. The carbonaceous component of&#xD;
the atmospheric aerosols is composed of two main fractions, viz. organic carbon&#xD;
(OC) and black carbon (BC). BC is emitted from the incomplete combustion while&#xD;
OC comes from the primary emission such as traffic exhaust and biomass burning&#xD;
and is also formed through atmospheric chemical conversion processes.&#xD;
Carbonaceous aerosols were monitored at a suburban site, Dayalbagh, Agra from&#xD;
January to October 2009 in the present study. It was found that total suspended&#xD;
particulate mass (TSPM) varied from 79 to 658&#xD;
&lt;img src='/image/spc_char/micro.gif' border=0&gt;g m&lt;sup&gt;-3 &lt;/sup&gt;with an average of 273±179.9 &lt;img src='/image/spc_char/micro.gif' border=0&gt;g m&lt;sup&gt;-3&lt;/sup&gt;. Also, daily&#xD;
concentrations of OC and BC ranged from 20.4 to 147.4 &lt;img src='/image/spc_char/micro.gif' border=0&gt;g m&lt;sup&gt;-3 &lt;/sup&gt;and&#xD;
from 1.4 to 20.3 &lt;img src='/image/spc_char/micro.gif' border=0&gt;g m&lt;sup&gt;-3&lt;/sup&gt; with the overall average concentrations of&#xD;
60.9±40.5 &lt;img src='/image/spc_char/micro.gif' border=0&gt;g m&lt;sup&gt;-3 &lt;/sup&gt;and 7.5±4.6 &lt;img src='/image/spc_char/micro.gif' border=0&gt;g m&lt;sup&gt;-3&lt;/sup&gt;, respectively. OC/BC&#xD;
ratios indicate the emission sources of carbonaceous aerosols. When the OC/BC&#xD;
ratio exceeds 2.0, it indicates that carbonaceous aerosols mainly originate&#xD;
from secondary organic transformation. Daily average OC/BC ratio varied between&#xD;
5.2 and 16.2 with an average of 8.1. To give an insight into the source&#xD;
contribution of OC and BC, correlation coefficient was determined. The&#xD;
correlation coefficient is found to be 0.79. This indicates that major fraction&#xD;
of OC and BC originates from a common source. Distinct monthly variation was&#xD;
observed in their concentrations.
&lt;br/&gt;
&lt;br/&gt;Page(s): 218-222</description>
  </item>
  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10167">
    <title>Measurement of atmospheric aerosols during monsoon and winter seasons at Roorkee, India</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10167</link>
    <description>Title: Measurement of atmospheric aerosols during monsoon and winter seasons at Roorkee, India
&lt;br/&gt;
&lt;br/&gt;Authors: Saxena, Deepti; Yadav, R; Kumar, Adarsh; Rai, Jagdish
&lt;br/&gt;
&lt;br/&gt;Abstract: &lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="place"&gt;&lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="country-region"&gt;&lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="City"&gt;&#xD;
&#xD;
Measurement of aerosol concentration has been carried out&#xD;
in view of some meteorological parameters like wind speed, temperature,&#xD;
relative humidity and rainfall during south-east (SE) monsoon (June-September&#xD;
2006) and winter (November 2006-February 2007) at Roorkee, India.&#xD;
The measurements were done with the help of laser beam scatterometer for wide&#xD;
range of aerosols (0.05-3.0 μm). The present study reveals the fact that the&#xD;
number density of aerosols is very much affected by meteorological parameters.&#xD;
The aerosol concentration was minimum in August, September and November 2006&#xD;
and remained around maximum during June-July 2006 and January-February 2007.&#xD;
During monsoon period, the rain plays important role in characterizing aerosol&#xD;
density. The aerosol concentration and size were found to be decreased during&#xD;
September 2006 although relative humidity was found to be very high due to scavenging&#xD;
of aerosol particles.&lt;/smarttagtype&gt;&lt;/smarttagtype&gt;&lt;/smarttagtype&gt;
&lt;br/&gt;
&lt;br/&gt;Page(s): 208-217</description>
  </item>
  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10166">
    <title>Preliminary reverse impulse in SC (Y) at off - equatorial stations in India</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10166</link>
    <description>Title: Preliminary reverse impulse in SC (Y) at off - equatorial stations in India
&lt;br/&gt;
&lt;br/&gt;Authors: Rastogi, R G; Ahmed, K
&lt;br/&gt;
&lt;br/&gt;Abstract: &lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="City"&gt;&lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="place"&gt;&#xD;
&#xD;
&#xD;
&#xD;
The&#xD;
storm sudden commencement (SSC) at 2345 hrs UT on 24 September 1998, occurring&#xD;
at around local sunrise for Indian stations had produced uniquely two–step&#xD;
impulses on the H magnetogram at all stations. The amplitude ∆H had increased&#xD;
progressively from Trivandrum&#xD;
to Gulmarg, unlike the characteristic of the day time equatorial enhancement of&#xD;
SC (H). The solar wind parameters too showed abnormal variations during the&#xD;
period of SC.&#xD;
&#xD;
The magnetogram trace for&#xD;
declination (or eastward field Y) recorded a preliminary reverse impulse (PRI)&#xD;
close to the latitude of Sq focus at stations Gulmarg, Ujjain, Nagpur and&#xD;
Shillong. The PRI was absent in SC (Y) at equatorial stations Trivandrum and&#xD;
Pondicherry. This observations show a new complex relationship between the&#xD;
ionospheric dynamo and magnetospheric dawn / dusk electric field with the&#xD;
equatorial geomagnetic field around sunrise.&lt;/smarttagtype&gt;&lt;/smarttagtype&gt;
&lt;br/&gt;
&lt;br/&gt;Page(s): 203-207</description>
  </item>
  <item rdf:about="http://nopr.niscair.res.in/handle/123456789/10165">
    <title>Diurnal and seasonal variation of fading rates of E- and F- region echoes during IGY and IQSY at the equatorial station of Ibadan</title>
    <link>http://nopr.niscair.res.in/handle/123456789/10165</link>
    <description>Title: Diurnal and seasonal variation of fading rates of E- and F- region echoes during IGY and IQSY at the equatorial station of Ibadan
&lt;br/&gt;
&lt;br/&gt;Authors: Somoye, E O
&lt;br/&gt;
&lt;br/&gt;Abstract: &lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="City"&gt;&lt;smarttagtype namespaceuri="urn:schemas-microsoft-com:office:smarttags" name="place"&gt;&#xD;
&#xD;
Fading rates of E- and F-region echoes observed at Ibadan (7.4°N, 3.9°E, 6°S dip) during the&#xD;
International Geophysical Year (IGY) 1958 and the International Quiet Year of&#xD;
the Sun (IQSY) 1964 are investigated for diurnal and seasonal variations. The&#xD;
fading rates of E- and F-region echoes are found to be of the same order of&#xD;
magnitude during the IQSY. However, the same is not true during IGY indicating&#xD;
that fading of F-region echoes is dependent on solar activity while that of&#xD;
E-region echoes is not as fading rate of E-region echoes are about the same&#xD;
during both epochs. The fading rate is found to be maximum at noon and minimum&#xD;
at sunrise and sunset for E-region echoes during both epochs and for F-region&#xD;
echoes during IQSY. During IGY, fading rate is maximum at noon; and minimum at&#xD;
sunrise and 2000 hrs LT (i.e. post sunset) at both epochs and for the two&#xD;
regions about same times of reversal of F-region East-West (EW) and E×B&#xD;
vertical drift during solar maximum. The maximum at noon appears to be due to:&#xD;
(i) continuous daytime rise in hmF2 which enhances irregularities and (ii)&#xD;
spread F irregularities generated by sudden increase in E×B plasma uplift not&#xD;
seen by the close-spaced antenna technique used in the present study. F-region&#xD;
fading rate is maximum during December solstice while E-region fading rates&#xD;
show no seasonal variation.&lt;/smarttagtype&gt;&lt;/smarttagtype&gt;
&lt;br/&gt;
&lt;br/&gt;Page(s): 194-202</description>
  </item>
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