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  <title>NOPR Collection:</title>
  <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/29039" />
  <subtitle />
  <id>http://nopr.niscpr.res.in/handle/123456789/29039</id>
  <updated>2026-10-10T06:22:26Z</updated>
  <dc:date>2026-10-10T06:22:26Z</dc:date>
  <entry>
    <title>FDTD based SAR analysis in human head using irregular volume averaging techniques of different resolutions at GSM 900 band</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/29056" />
    <author>
      <name>Ali, Md Faruk</name>
    </author>
    <author>
      <name>Ray, Sudhabindu</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/29056</id>
    <updated>2016-07-20T06:06:11Z</updated>
    <published>2014-06-01T00:00:00Z</published>
    <summary type="text">Title: FDTD based SAR analysis in human head using irregular volume averaging techniques of different resolutions at GSM 900 band
Authors: Ali, Md Faruk; Ray, Sudhabindu
Abstract: Specific absorption&#xD;
rate (SAR) induced inside human head in the near-field of a mobile phone&#xD;
antenna has been investigated for three different SAR resolutions using Finite&#xD;
Difference in Time Domain (FDTD) method at GSM 900 band. Voxel based&#xD;
anthropomorphic human head model, consisting of different anatomical tissues,&#xD;
is used to calculate the peak SAR values averaged over 10-g, 1-g and 0.1-g&#xD;
mass. It is observed that the maximum local SAR increases significantly for&#xD;
smaller mass averages.
Page(s): 235-242</summary>
    <dc:date>2014-06-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>0°C isotherm height distribution for Earth-space communication satellite links in Nigeria</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/29055" />
    <author>
      <name>Ojo, J S</name>
    </author>
    <author>
      <name>Falodun, S E</name>
    </author>
    <author>
      <name>Odiba, O</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/29055</id>
    <updated>2016-07-20T06:05:09Z</updated>
    <published>2014-06-01T00:00:00Z</published>
    <summary type="text">Title: 0°C isotherm height distribution for Earth-space communication satellite links in Nigeria
Authors: Ojo, J S; Falodun, S E; Odiba, O
Abstract: For an optimum performance of Earth-space satellite communication&#xD;
links, a number of meteorological parameters &#xD;
are needed to be considered along the Earth-space path for specific locations&#xD;
and the height of the 0°C isotherm (freezing level height) is among such parameters.&#xD;
Information regarding this parameter is always based on the recommendation of&#xD;
ITU-RP-839 in the form of contour maps. Since the meteorological parameters are&#xD;
location dependent, there is a need for the establishment of these parameters&#xD;
for specific locations. In addition, ITU-R model uses an yearly averaged&#xD;
constant rain height for the attenuation estimation, which may not be&#xD;
appropriate for tropical regions. In the present paper, the 0°C isotherm (ZDI)&#xD;
height has been established using two years of data collected on-board the&#xD;
precipitation radar of the Tropical Rain Measuring Mission (TRMM) satellite.&#xD;
The result shows the seasonal dependence of the 0°C isotherm height. It is&#xD;
observed, among other things, that the height is higher during the wet season&#xD;
as compared to the dry season. Rain induced attenuation at frequencies above 10&#xD;
GHz is also estimated using the 0°C isotherm height derived for each of the&#xD;
locations over the elevation angle of the NIGCOMSAT-1R in Nigeria.
Page(s): 225-234</summary>
    <dc:date>2014-06-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Estimation of global solar radiation in Nigeria using a modified Angstrom model and the trend analysis of the allied meteorological components</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/29054" />
    <author>
      <name>Ogolo, E O</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/29054</id>
    <updated>2016-07-20T06:03:57Z</updated>
    <published>2014-06-01T00:00:00Z</published>
    <summary type="text">Title: Estimation of global solar radiation in Nigeria using a modified Angstrom model and the trend analysis of the allied meteorological components
Authors: Ogolo, E O
Abstract: The trend of some&#xD;
common and related atmospheric variables were investigated in the light of&#xD;
climate change on annual time scale and a suitable scheme was further developed&#xD;
for the simulation of annual global solar radiation in Nigeria. In this&#xD;
connection, annual trends of global solar radiation, air temperature,&#xD;
precipitation, relative humidity and sunshine hours was carried out, covering&#xD;
about 13 tropical stations during 1975-2006 in Nigeria using F-test as the&#xD;
significance test technique. &#xD;
It was found that nine stations exhibited an upward trend in global solar&#xD;
radiation series, of which 6 passed F-test at &#xD;
1% significant level. At 11 stations, precipitation had shown an increasing&#xD;
trends but none passed F-test at 2.5% and hence, not significant. About 98.8%&#xD;
of the stations displayed an upward trend in sunshine hours of which 16% passed&#xD;
F-test at &#xD;
1% significant level. On trend analysis for relative humidity series, eight&#xD;
stations exhibited a positive trend and only one station passed F-test at 1%&#xD;
significant level. The trend of temperature series in Nigeria under the period&#xD;
under investigation was found to be increasing at 12 stations and eight&#xD;
stations passed the F-test at 1% significant level. The other objective of this&#xD;
study was to determine a more suitable empirical equation by modifying Angstrom&#xD;
model for the estimation of global solar radiation using all data for all 14&#xD;
stations pooled together to predict global solar radiation using linear and&#xD;
multiple linear regression. This was done to improve the low performance of the&#xD;
Angstrom model used for the annual estimation of global solar radiation. The&#xD;
model parameters ‘a’ and ‘b’ of Angstrom model were parameterized in terms of&#xD;
the geographical locations (latitude, longitude and elevation) and the&#xD;
meteorological variables (sunshine hour, precipitation, relative humidity and&#xD;
temperature), respectively. This scheme gave better simulation of the global&#xD;
solar radiation compared with other schemes and the original Angstrom models.&#xD;
In addition, the preferential consideration of relative humidity to&#xD;
precipitation as potent contributing factor in the estimation of global solar&#xD;
radiation was also established.
Page(s): 213-224</summary>
    <dc:date>2014-06-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Modelling of the equatorial ionospheric E-layer based on cos&lt;img src='/image/spc_char/lembda.gif' border=0&gt; index</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/29053" />
    <author>
      <name>Kazeem, A K</name>
    </author>
    <author>
      <name>Adeniyi, J O</name>
    </author>
    <author>
      <name>Adediji, A T</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/29053</id>
    <updated>2016-07-20T06:02:35Z</updated>
    <published>2014-06-01T00:00:00Z</published>
    <summary type="text">Title: Modelling of the equatorial ionospheric E-layer based on cos&lt;img src='/image/spc_char/lembda.gif' border=0&gt; index
Authors: Kazeem, A K; Adeniyi, J O; Adediji, A T
Abstract: Daytime hourly values of the critical&#xD;
frequency of the ionospheric E-layer, &lt;img src='http://www.niscair.res.in/jinfo/ff.gif' border=0&gt;oE,&#xD;
obtained at Ouagadougou Ionospheric Observatory (12.4°N, 1.5°W) in Burkina&#xD;
Faso, West Africa, an equatorial station, during the solar cycle 22 (1985 –&#xD;
1995) have been used to develop a model based on solar zenith angle through cos&lt;span style="font-family:Symbol;mso-ascii-font-family:" times="" new="" roman";="" mso-hansi-font-family:"times="" roman";mso-char-type:symbol;mso-symbol-font-family:="" symbol"="" lang="EN-GB"&gt;c index factor using the relation &lt;span style="font-family:Symbol;mso-ascii-font-family:" times="" new="" roman";mso-hansi-font-family:="" "times="" roman";mso-char-type:symbol;mso-symbol-font-family:symbol"="" lang="EN-GB"&gt;&lt;img src='http://www.niscair.res.in/jinfo/ff.gif' border=0&gt;oE = a (cos&lt;img src='/image/spc_char/lembda.gif' border=0&gt;)&lt;sup&gt;n&lt;/sup&gt;&lt;sub&gt;,&lt;/sub&gt;&#xD;
The average value of the diurnal cos&lt;img src='/image/spc_char/lembda.gif' border=0&gt; index, &lt;span style="mso-bidi-font-weight:bold"&gt;n, at Ouagadougou was found to be 0.30&#xD;
for both low and high solar activity. The model was tested with &lt;img src='http://www.niscair.res.in/jinfo/ff.gif' border=0&gt;oE data from Korhogo (9.3°N, 5.4°W) in Cote-d’Ivoire, another&#xD;
equatorial station, and there is good agreement between the model and&#xD;
observations. The validity of the &lt;img src='http://www.niscair.res.in/jinfo/ff.gif' border=0&gt;oE model&#xD;
was also compared with predicted values by IRI-2012 model and good agreement&#xD;
has been observed. The percentage difference, when &lt;img src='http://www.niscair.res.in/jinfo/ff.gif' border=0&gt;oE observed compared with IRI-2012 model, was found to be within &lt;img src='http://www.niscair.res.in/jinfo/ff.gif' border=0&gt;±10% for both equinoxes and solstices for the two levels of solar&#xD;
activity. &#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;
Page(s): 205-212</summary>
    <dc:date>2014-06-01T00:00:00Z</dc:date>
  </entry>
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