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  <channel rdf:about="http://nopr.niscpr.res.in/handle/123456789/16021">
    <title>NOPR Collection:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/16021</link>
    <description />
    <items>
      <rdf:Seq>
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/16082" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/16081" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/16080" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/16079" />
      </rdf:Seq>
    </items>
    <dc:date>2026-10-10T23:55:19Z</dc:date>
  </channel>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/16082">
    <title>Emission and scattering behaviour of bare and vegetative soil surfaces of different moist states by microwave remote sensing</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/16082</link>
    <description>Title: Emission and scattering behaviour of bare and vegetative soil surfaces of different moist states by microwave remote sensing
Authors: Gupta, V K; Sharma, Neeta; Jangid, R A
Abstract: Dielectric&#xD;
constant (&lt;i&gt;ε&lt;/i&gt;′) and dielectric loss (ε′′) of artificially moistened soil&#xD;
of Alwar have been determined at microwave frequency 9.78 GHz and at&#xD;
temperature 32.5°C using wave guide cell method. In view of the active and&#xD;
passive microwave remote sensing, the horizontal-horizontal radar&#xD;
backscattering coefficient (&lt;img src='http://www.niscair.res.in/jinfo/sigmasuper.gif' border=0&gt;) for bare and vegetative soil surface have been estimated by&#xD;
Integral Equation Model (IEM) and Water Cloud Model (WCM), respectively using &lt;i&gt;ε&lt;/i&gt;′&#xD;
and ε′′ of soil and view angle as input parameters. The horizontal component of&#xD;
microwave emissivity (&lt;i&gt;e&lt;sub&gt;h&lt;/sub&gt;&lt;/i&gt;) for bare soil surfaces have been&#xD;
determined by emissivity model. The &lt;i&gt;e&lt;sub&gt;h&lt;/sub&gt;&lt;/i&gt;&lt;sub&gt; &lt;/sub&gt;for&#xD;
vegetative soil surfaces determined by radiative transfer equation using&#xD;
suitable vegetation dependent parameters, like&lt;span style="mso-bidi-font-style:&#xD;
italic"&gt; single way vegetation transmissivity &lt;img src='http://www.niscair.res.in/jinfo/sigmasuper.gif' border=0&gt; and single scattering&#xD;
albedo (ω) for agricultural vegetation, respectively. The present study reveals&#xD;
that the  &lt;span style="font-size:12.0pt;mso-bidi-font-size:&#xD;
16.0pt;font-family:"Arial Unicode MS";mso-ansi-language:NL;mso-fareast-language:&#xD;
EN-US;mso-bidi-language:AR-SA" lang="NL"&gt; for&#xD;
bare and vegetative soil surface exhibit a positive correlation with&#xD;
soil moisture content (&lt;span style="mso-bidi-font-style:italic"&gt;SMC).&#xD;
Vegetative soil surface &lt;span style="mso-bidi-font-style:italic"&gt; is lower than that of bare soil surface for&#xD;
the same values of SMC and view angle. Further, &lt;i&gt;e&lt;sub&gt;h&lt;/sub&gt;&lt;/i&gt; &lt;span style="mso-bidi-font-style:italic"&gt;for bare and vegetative soil surfaces&#xD;
decreases with an increase in SMC. Vegetative soil surface &lt;img src='http://www.niscair.res.in/jinfo/sigmasuper.gif' border=0&gt; emissivity is higher&#xD;
than that of bare surface for the same values of SMC and observation angle.&#xD;
Further, backscattering coefficient and emissivity for bare and&#xD;
vegetative soil surfaces decrease as the angle of observation increases due to&#xD;
contribution of diminished coherent component.&#xD;
&#xD;
&#xD;
&#xD;
&#xD;
&#xD;
&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 42-51</description>
    <dc:date>2013-02-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/16081">
    <title>Ionospheric electron and ion temperatures response to seismic activity</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/16081</link>
    <description>Title: Ionospheric electron and ion temperatures response to seismic activity
Authors: Sharma, D K; Bardhan, A; Rai, Jagdish
Abstract: A connection between earthquake and&#xD;
ionosphere has been proposed in the last few decades. A number of hypotheses&#xD;
have been suggested as the earthquake precursory to reduce the hazard of life&#xD;
and property but could not succeed. In the present study, effort has been made&#xD;
to correlate the ionospheric temperature anomalies to seismic activities. The&#xD;
ionospheric electron and ion temperatures were measured with the help of&#xD;
Retarding Potential Analyzer (RPA) payload aboard the Indian SROSS-C2&#xD;
satellite. The data is used for the period 1995-1998 in the altitude range&#xD;
430-630 km over the Indian region. The details of seismic events during this&#xD;
period were downloaded from the United State Geological Survey (USGS) website.&#xD;
The normal day ion and electron temperatures have been compared to the&#xD;
temperatures recorded during the seismic event. It has been observed that there&#xD;
is significant enhancement in the electron and ion temperatures. The electron&#xD;
temperature was enhanced by 1.2 - 1.5 times compared to the average normal day&#xD;
electron temperature. However, the ion temperature was 1.1 - 1.3 times over the&#xD;
average normal day ion temperature. The satellite data was analysed for&#xD;
corresponding seismic event duration in such way that the other possible&#xD;
effects are eliminated.
Page(s): 18-26</description>
    <dc:date>2013-02-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/16080">
    <title>Ionospheric TEC variations during the ascending solar activity phase at an equatorial station, Uganda</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/16080</link>
    <description>Title: Ionospheric TEC variations during the ascending solar activity phase at an equatorial station, Uganda
Authors: Oron, S; D’ujanga, F M; Ssenyonga, T J
Abstract: The total electron content (TEC) is a vital&#xD;
and most dominant ionospheric parameter that can cause Global Positioning&#xD;
System (GPS) signal delays, signal degradation and in extreme cases loss of&#xD;
lock. This results into inefficient operations of ground and space based Global&#xD;
Navigation Satellite System (GNSS) applications. The study of TEC variability&#xD;
is, therefore, useful for GNSS users in order to minimize errors where high&#xD;
levels of accuracy in measurements are required. This paper presents the&#xD;
diurnal, seasonal and solar activity dependence of TEC at the GPS-SCINDA&#xD;
(SCIntillation Network Decision Aid) station in Kampala, Uganda (geographic coordinates:&#xD;
latitude 0.3°N, longitude 32.6°S; and geomagnetic coordinates: latitude -9.3°,&#xD;
longitude 104.2°) for the years 2010 and 2011. The results obtained show that&#xD;
the diurnal variability in TEC at this station has a pre-dawn minimum followed&#xD;
by an early morning steady increase, an afternoon maximum and then a post&#xD;
sunset gradual reduction in TEC, with the equinoctial months depicting&#xD;
nighttime enhancements more prominently at around 2000 hrs UT (2300 hrs LT).&#xD;
Scintillation occurrence, a consequence of TEC fluctuations, was observed from&#xD;
about 1800 hrs UT (2100 hrs LT) to local midnight giving S&lt;sub&gt;4&lt;/sub&gt; index&#xD;
values above 0.4, with the equinox months recording higher occurrences than&#xD;
other seasons. TEC variations were also seen to exhibit solar activity dependence.&#xD;
The sunspot numbers and the F10.7 solar flux exhibited a good correlation with&#xD;
TEC recorded over the two years.
Page(s): 7-17</description>
    <dc:date>2013-02-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/16079">
    <title>&lt;span style="font-size:11.0pt;mso-bidi-font-size: 10.0pt;font-family:"Times New Roman";mso-fareast-font-family:"Times New Roman"; mso-ansi-language:EN-US;mso-fareast-language:EN-US;mso-bidi-language:AR-SA" lang="EN-US"&gt;Oil spill detection using SSM/I satellite data over Bombay High location in Arabian Sea&lt;/span&gt;</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/16079</link>
    <description>Title: &lt;span style="font-size:11.0pt;mso-bidi-font-size: 10.0pt;font-family:"Times New Roman";mso-fareast-font-family:"Times New Roman"; mso-ansi-language:EN-US;mso-fareast-language:EN-US;mso-bidi-language:AR-SA" lang="EN-US"&gt;Oil spill detection using SSM/I satellite data over Bombay High location in Arabian Sea&lt;/span&gt;
Authors: Calla, O P N; Dadhich, Harendra Kumar; Singhal, Shruti
Abstract: &lt;span style="mso-bidi-font-size:&#xD;
9.0pt;letter-spacing:-.1pt" lang="EN-US"&gt;Oil spill pollution is a severe environmental&#xD;
problem, which persists in marine environment or in inland water across the&#xD;
world. It has grown to an alarming magnitude with increased levels of oil&#xD;
production and transport. Thus, it is important to study and analyze this&#xD;
environmental pollution.&lt;span style="font-size:10.0pt;&#xD;
mso-bidi-font-size:9.0pt;letter-spacing:-.1pt" lang="EN-US"&gt; &lt;span style="mso-bidi-font-size:9.0pt;letter-spacing:-.1pt" lang="EN-US"&gt;The study and detection&#xD;
of oil spills can only be accomplished by satellite microwave remote sensing&#xD;
techniques. As microwaves have unique all weather penetration capability and&#xD;
can be used both in day and night, it does not require illumination of target&#xD;
from the sun. Two types of microwave sensors [Ulaby F T&#xD;
&lt;i style="mso-bidi-font-style:normal"&gt;et al&lt;/i&gt;. &lt;i style="mso-bidi-font-style:&#xD;
normal"&gt;Microwave remote sensing – Active and passive, &lt;/i&gt;Vol 1 and 3, 1981] &lt;span style="mso-bidi-font-size:9.0pt;letter-spacing:-.1pt" lang="EN-US"&gt;exist: one is&#xD;
passive sensor and other active sensor. Passive microwave sensor is radiometer&#xD;
that operates in the microwave region and detects microwave radiation emitted&#xD;
by the earth surface in addition to passively sensing emissions coming from&#xD;
objects on Earth. Active microwave sensor emits microwaves toward the earth's&#xD;
surface. These microwaves are reflected back from earth's surface and return&#xD;
back to the sensor. In this paper, for the detection of oil spills, data of&#xD;
passive microwave sensors onboard Special Sensor Microwave/Imager (SSM/I) [Hollinger J &lt;i style="mso-bidi-font-style:normal"&gt;et al&lt;/i&gt;. &lt;i style="mso-bidi-font-style:normal"&gt;Special Sensor Microwave/Imager user’s guide&lt;/i&gt;,&#xD;
1987, 120&lt;span style="mso-bidi-font-size:9.0pt;letter-spacing:&#xD;
-.1pt" lang="EN-US"&gt;] satellite at 19.3 GHz frequency is used and analyzed. The analyses&#xD;
shows sudden decrease of brightness temperature values in both horizontal and&#xD;
vertical polarization over the oil spill area (Bombay High Area, Arabian Sea)&#xD;
when compared to the brightness temperature values over oil free area in the&#xD;
Arabian sea.&#xD;
&#xD;
&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 52-59</description>
    <dc:date>2013-02-01T00:00:00Z</dc:date>
  </item>
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