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    <title>NISCAIR Online Periodicals Repository Community: Indian Journal of Radio &amp; Space Physics (IJRSP)</title>
    <link>http://nopr.niscair.res.in/handle/123456789/64</link>
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      <url>http://nopr.niscair.res.in/retrieve/143</url>
      <link>http://nopr.niscair.res.in/handle/123456789/64</link>
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      <title>Vertical profile variations of NO&lt;sub&gt;2&lt;/sub&gt;&lt;i&gt; &lt;/i&gt;and O&lt;sub&gt;3&lt;/sub&gt; using slant column density observations during twilight period</title>
      <link>http://nopr.niscair.res.in/handle/123456789/17463</link>
      <description>Title: Vertical profile variations of NO&lt;sub&gt;2&lt;/sub&gt;&lt;i&gt; &lt;/i&gt;and O&lt;sub&gt;3&lt;/sub&gt; using slant column density observations during twilight period
&lt;br/&gt;
&lt;br/&gt;Authors: Londhe, A L; Bhosale, C S; Meena, G S; Jadhav, D B; Gil, M; Puentedura, O; Yela, M
&lt;br/&gt;
&lt;br/&gt;Abstract: An algorithm developed to derive the&#xD;
vertical profiles of atmospheric species from their slant column density measurements&#xD;
using twilight spectroscopy is discussed. The algorithm has been tested by&#xD;
using the slant column density measurements at polar station, Reykjavik (64°N, 22.6°W)&#xD;
and tropical station, Pune (l8.53°N, 73.85°E). The vertical profiles of NO&lt;sub&gt;2&lt;/sub&gt;&#xD;
and O&lt;sub&gt;3&lt;/sub&gt; are retrieved by considering slant column densities for ten different&#xD;
solar zenith angles and ten different atmospheric layers of equal thickness. These&#xD;
vertical profiles are&#xD;
&#xD;
used to differentiate the tropospheric and&#xD;
stratospheric contribution of NO&lt;sub&gt;2&lt;/sub&gt; and O&lt;sub&gt;3&lt;/sub&gt; . The&#xD;
observations of &amp;nbsp;NO&lt;sub&gt;2&lt;/sub&gt; at polar station&#xD;
and at tropical station showed frequent higher values of tropospheric concentrations&#xD;
due to pollution episodes and are not correlated with stratospheric NO&lt;sub&gt;2&lt;/sub&gt;&#xD;
and O&lt;sub&gt;3.&lt;/sub&gt; The correlation between total column density variations of NO&lt;sub&gt;2&lt;/sub&gt;&#xD;
and O&lt;sub&gt;3&lt;/sub&gt; is not observed; however, the stratospheric variations of NO&lt;sub&gt;2&lt;/sub&gt;&#xD;
and O&lt;sub&gt;3&lt;/sub&gt; showed good correlation.
&lt;br/&gt;
&lt;br/&gt;Page(s): 291-301</description>
      <pubDate>Sun, 28 Nov 1999 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Determination of photolysis frequency of O&lt;sup&gt;1&lt;/sup&gt;D in the tropical region</title>
      <link>http://nopr.niscair.res.in/handle/123456789/17462</link>
      <description>Title: Determination of photolysis frequency of O&lt;sup&gt;1&lt;/sup&gt;D in the tropical region
&lt;br/&gt;
&lt;br/&gt;Authors: Paul, R; Mitra, A P; Mandal, T K; Srivastava, S K
&lt;br/&gt;
&lt;br/&gt;Abstract: An attempt has been made to estimate the photolysis&#xD;
frequency of O&lt;sup&gt;1&lt;/sup&gt;D in troposphere and stratosphere of the Indian region.&#xD;
The radiation code Lowtran 7 is used to estimate actinic flux at these altitudes.&#xD;
An accurate and efficient multiple scattering parametrization along with &lt;i&gt;k&lt;/i&gt;-distribution&#xD;
method has been used in this model. For ozone, observed averaged profile for the&#xD;
year 1976 as well as 1994 is used for Delhi,&#xD;
Pune and Thiruvananthapuram. Values as recommended by DeMore &lt;i&gt;et al. [JPL Publication,&#xD;
&lt;/i&gt;1994, p.94] and Michelsen &lt;i&gt;et al. [Geophys Res Lett (USA). &lt;/i&gt;21&#xD;
(1994) 2227.] have been taken for ozone quantum yield. The values of photolysis&#xD;
frequency of O&lt;sup&gt;1&lt;/sup&gt;D are found to be significantly higher for the quantum&#xD;
yield given by Michelsen &lt;i&gt;et al. &lt;/i&gt;A decrease in these values is also observed&#xD;
in the year 1994 as compared to that in&#xD;
&#xD;
preceding years up to 1976.
&lt;br/&gt;
&lt;br/&gt;Page(s): 286-290</description>
      <pubDate>Sun, 28 Nov 1999 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Solar beam radiation estimate’s correlation for Bangladesh</title>
      <link>http://nopr.niscair.res.in/handle/123456789/17461</link>
      <description>Title: Solar beam radiation estimate’s correlation for Bangladesh
&lt;br/&gt;
&lt;br/&gt;Authors: Rahman, M M; Uddin, M A; Islam, M W
&lt;br/&gt;
&lt;br/&gt;Abstract: An empirical&#xD;
correlation has been developed which correlates the monthly average daily solar beam&#xD;
radiation with the maximum possible number of bright sunshine&#xD;
hours. Airmass exponential correlation is also established. The applicability&#xD;
of these models in climatic conditions of Bangladesh is also&#xD;
studied. Measured beam radiation and the bright sunshine hour data are&#xD;
analyzed to find out the regression co-efficient of these correlations&#xD;
using computer simulation programme by Gaussian elimination&#xD;
technique. Applying&#xD;
these correlations, solar beam radiation is computed for&#xD;
different locations in&#xD;
&#xD;
Bangladesh. Predicted&#xD;
results are compared statistically with the experimental observations&#xD;
considering different statistical errors. The &lt;i&gt;t&lt;/i&gt;-statistics is also&#xD;
applied to test whether or not a model is statistically significant&#xD;
at a particular confidence level. On the basis of the&#xD;
analysis, a model has been recommended which is found to be best suited to the&#xD;
climatic conditions of Bangladesh.
&lt;br/&gt;
&lt;br/&gt;Page(s): 277-285</description>
      <pubDate>Sun, 28 Nov 1999 22:58:59 GMT</pubDate>
    </item>
    <item>
      <title>Feasibility study of extended range atmospheric prediction through time average Lorenz attractor</title>
      <link>http://nopr.niscair.res.in/handle/123456789/17460</link>
      <description>Title: Feasibility study of extended range atmospheric prediction through time average Lorenz attractor
&lt;br/&gt;
&lt;br/&gt;Authors: Pal, Pradip K; Shah, Shivani
&lt;br/&gt;
&lt;br/&gt;Abstract: Though the theoretical limit of&#xD;
atmospheric predictability is only up to 1-2 weeks, temporal and spatial averages&#xD;
may be predictable up to certain extent for extended range. It is not known&#xD;
what should be the length of time for averaging to have certain predictability of&#xD;
time average values. The time average behaviour of Lorenz attractor with and&#xD;
without forcing shows that there are upper and lower limits of such length of time&#xD;
for averaging, beyond which the system remains chaotic.
&lt;br/&gt;
&lt;br/&gt;Page(s): 271-276</description>
      <pubDate>Sun, 28 Nov 1999 22:58:59 GMT</pubDate>
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