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    <title>NOPR Community:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/25568</link>
    <description />
    <pubDate>Sat, 10 Oct 2026 09:42:33 GMT</pubDate>
    <dc:date>2026-10-10T09:42:33Z</dc:date>
    <item>
      <title>On the stability of atmospheric surface layer along the monsoon rough region over India</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/30597</link>
      <description>Title: On the stability of atmospheric surface layer along the monsoon rough region over India
Authors: Patil, M N; Parasnis, S S
Abstract: &lt;span style="mso-bidi-language:HI"&gt;Stability characteristics in the atmospheric&#xD;
surface layer over dry convection, moist convection and alternate deep moist/unsaturated&#xD;
convection zones of the monsoon trough have been explored using the tower data&#xD;
of wind and temperature obtained during monsoon trough boundary layer&#xD;
experiment (MONTBLEX). In general, different characteristics in three&#xD;
sub-layers of a 1-30 m layer were observed before, during and after the onset&#xD;
of monsoon. Before onset of the monsoon, 1-4 m layer was stably stratified over&#xD;
dry convection (western end) and moist convection (eastern&#xD;
&#xD;
&lt;span style="mso-bidi-language:HI"&gt;end) zones of the monsoon trough. After the onset&#xD;
of monsoon, inversion in this layer was not noticed. These results may possibly&#xD;
be attributed to the local effect.&#xD;
&#xD;
&lt;/span&gt;&lt;/span&gt;
Page(s): 266-272</description>
      <pubDate>Mon, 01 Oct 2001 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/30597</guid>
      <dc:date>2001-10-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Characteristics of turbulence in the atmospheric surface layer over a complex terrain</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/30596</link>
      <description>Title: Characteristics of turbulence in the atmospheric surface layer over a complex terrain
Authors: Murthy, B S; Dharmaraj, T
Abstract: &lt;span style="mso-bidi-language:HI"&gt;Measurements of fluctuating wind components and&#xD;
temperature have been made in the atmospheric surface layer over a complex&#xD;
terrain in the campus of the Indian Institute of Tropical Meteorology, Pune,&#xD;
using sonic anemorneter at 5.2 m above the surface. Characteristics of&#xD;
turbulence, i.e. spectra of wind velocity components and turbulence statistics&#xD;
of wind are presented. The peak of normalized &lt;i&gt;w&lt;/i&gt;-spectrum over a complex&#xD;
terrain for near-neutral condition was found to be ~ 0.6 as compared to ~ 0.4&#xD;
over homogeneous terrain. The non-dimensional frequency maximum for &lt;i&gt;w&lt;/i&gt;-component&#xD;
spectrum was observed to be 0.9 as compared to ~ 0.5 over homogeneous terrain.&#xD;
Empirical formulae for standard deviation of velocity components have been&#xD;
tested against observations over hilly terrain. Vertical flux of turbulence&#xD;
kinetic energy as a function of stability is also discussed.&#xD;
&#xD;
&lt;/span&gt;
Page(s): 260-265</description>
      <pubDate>Mon, 01 Oct 2001 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/30596</guid>
      <dc:date>2001-10-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>&lt;span style="mso-bidi-language:HI"&gt;A model study of the atmospheric heating rates due to O&lt;sub&gt;3&lt;/sub&gt;, H&lt;sub&gt;2&lt;/sub&gt;O and O&lt;sub&gt;2&lt;/sub&gt; &lt;/span&gt;</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/30595</link>
      <description>Title: &lt;span style="mso-bidi-language:HI"&gt;A model study of the atmospheric heating rates due to O&lt;sub&gt;3&lt;/sub&gt;, H&lt;sub&gt;2&lt;/sub&gt;O and O&lt;sub&gt;2&lt;/sub&gt; &lt;/span&gt;
Authors: Lal, M
Abstract: &lt;span style="mso-bidi-language:HI"&gt;The height distribution of solar heating rate due&#xD;
to ozone, water vapour and oxygen molecule from ground to 100 km altitude has&#xD;
been examined in this study. The cooling rate due to infrared emission of CO&lt;sub&gt;2&lt;/sub&gt;,&#xD;
O&lt;sub&gt;3&lt;/sub&gt; and water vapour molecules&#xD;
&#xD;
&lt;span style="mso-bidi-language:HI"&gt;has also been studied for middle atmospheric&#xD;
region. The heating and cooling rates have been calculated for midlatitude and equinox&#xD;
condition. The diurnal variation of net radiative temperature change in&#xD;
tropospheric and stratospheric region causes &lt;span style="mso-bidi-font-family:&#xD;
Arial;mso-bidi-language:HI"&gt;I&#xD;
&#xD;
&lt;span style="mso-bidi-language:HI"&gt;generation of waves, which propagate in the&#xD;
mesospheric region and affects the climatology of the upper atmosphere. The heating&#xD;
rate due to water vapour is found to be important in the troposphere, ozone&#xD;
heating is Significant in the stratosphere,&#xD;
&#xD;
&lt;span style="mso-bidi-language:HI"&gt;and oxygen heating rate is found to be important&#xD;
in the mesospheric region. The maximum ozone heating rate in the stratospheric&#xD;
region is found to be ~ 15 K/day. The cooling rate is due to CO&lt;sub&gt;2&lt;/sub&gt; is&#xD;
very significant in the stratospheric region and its found to be about -12&#xD;
K/day. The net radiative temperature change due to heating and cooling has been&#xD;
obtained to be similar to the atmospheric temperature profile.&#xD;
&#xD;
&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 254-259</description>
      <pubDate>Mon, 01 Oct 2001 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/30595</guid>
      <dc:date>2001-10-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Study of travelling ionospheric disturbances using IPS array at Rajkot</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/30594</link>
      <description>Title: Study of travelling ionospheric disturbances using IPS array at Rajkot
Authors: Jadeja, A K; Jadav, R M; Vats, Hari Om; Iyer, K N
Abstract: &lt;span style="mso-bidi-language:HI"&gt;Using a novel radio astronomical technique, the&#xD;
presence of travelling ionospheric disturbances (TIDs) are detected from&#xD;
observations of radio star signals by the interplanetary scintillation (IPS)&#xD;
system at Rajkot for the first time in India.&#xD;
&#xD;
&lt;span style="mso-bidi-language:HI"&gt;The periods of the TIDs (20-24 min) and&#xD;
north-south component of their velocity (66-273 m/s)&lt;i&gt; &lt;/i&gt;indicate that they&#xD;
belong to the medium scale category. The results are discussed in the light of&#xD;
a model of atmospheric gravity waves (AGWs) originating in auroral electrojet&#xD;
region and propagating meridionally equatorward.&#xD;
&#xD;
&lt;/span&gt;&lt;/span&gt;
Page(s): 249-253</description>
      <pubDate>Mon, 01 Oct 2001 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/30594</guid>
      <dc:date>2001-10-01T00:00:00Z</dc:date>
    </item>
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