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  <channel rdf:about="http://nopr.niscpr.res.in/handle/123456789/17297">
    <title>NOPR Collection:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/17297</link>
    <description />
    <items>
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        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/17342" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/17341" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/17340" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/17339" />
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    <dc:date>2026-10-11T22:17:10Z</dc:date>
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  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/17342">
    <title>Strong diffusion of protons by Pc1 waves</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/17342</link>
    <description>Title: Strong diffusion of protons by Pc1 waves
Authors: Singh, D P; Singh, U P
Abstract: &lt;span style="font-size:14.0pt;line-height:&#xD;
115%;font-family:" times="" new="" roman";mso-fareast-font-family:"times="" roman";="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN"&gt;Diffusion of energetic protons by &lt;i&gt;L &lt;/i&gt;mode electromagnetic ion&#xD;
cyclotron (EMIC) waves in the Pc1 range is studied. It is found that &lt;i&gt;L=&lt;/i&gt;4&lt;i&gt;&#xD;
&lt;/i&gt;(which is strong diffusion region for energetic electrons by VLF whistler&#xD;
mode waves)&lt;i&gt; &lt;/i&gt;is a weak diffusion region and &lt;i&gt;L &lt;/i&gt;&lt;span style="font-size:14.0pt;line-height:115%;font-family:" times="" new="" roman";="" mso-fareast-font-family:hiddenhorzocr;color:black;mso-ansi-language:en-in;="" mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN"&gt;≥ &lt;span style="font-size:14.0pt;line-height:115%;font-family:" times="" new="" roman";="" mso-fareast-font-family:"times="" roman";color:black;mso-ansi-language:en-in;="" mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN"&gt;5.5 is a strong diffusion&#xD;
region for energetic protons. Different criteria to measure diffusion strength&#xD;
support this result. The result is in agreement with various theoretical and &lt;i&gt;in&lt;/i&gt;&#xD;
&lt;i&gt;situ &lt;/i&gt;observations.&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 148-152</description>
    <dc:date>1999-06-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/17341">
    <title>Role of oblique whistler-mode waves in energetic electron precipitation at the lower edge of inner radiation belt</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/17341</link>
    <description>Title: Role of oblique whistler-mode waves in energetic electron precipitation at the lower edge of inner radiation belt
Authors: Prakash, Ram; Agrawal, Bal Mukund
Abstract: &lt;span style="font-size:14.0pt;line-height:&#xD;
115%;font-family:" times="" new="" roman";mso-fareast-font-family:"times="" roman";="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN"&gt;An attempt has been made to study the precipitation of energetic (keV and&#xD;
MeV) electrons at the lower edge of inner radiation belt in terms of their&#xD;
quasi-linear gyro-resonant interaction with oblique whistler-mode waves. The&#xD;
calculated average pitch angle scattering (~10&lt;sup&gt;-1&lt;/sup&gt; degree) and&#xD;
lifetimes (~ days and hours only) indicate a significant electron precipitation&#xD;
by these waves into the lower latitude atmosphere. The low calculated lifetimes&#xD;
of energetic electrons and sufficiently high calculated flux of precipitated&#xD;
electrons caused due to gyro-resonant interaction involving oblique&#xD;
whistler-mode waves show that these non-ducted waves are likely to be an effective&#xD;
electron precipitator at the lower edge of inner radiation belt.&lt;/span&gt;
Page(s): 141-147</description>
    <dc:date>1999-06-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/17340">
    <title>A bit synchronizer for telecommunication with a balloon-borne experiment</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/17340</link>
    <description>Title: A bit synchronizer for telecommunication with a balloon-borne experiment
Authors: Chalke, S A; Costa, S L D; Ghosh, S K; Patkar, D M
Abstract: &lt;span style="font-size:14.0pt;line-height:&#xD;
115%;font-family:" times="" new="" roman";mso-fareast-font-family:"times="" roman";="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN"&gt;The bit synchronizer forms &lt;span style="font-size:14.0pt;&#xD;
line-height:115%;font-family:" times="" new="" roman";mso-fareast-font-family:hiddenhorzocr;="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN"&gt;an important &lt;span style="font-size:14.0pt;line-height:&#xD;
115%;font-family:" times="" new="" roman";mso-fareast-font-family:"times="" roman";="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN"&gt;component of a telemetry ground station for receiving on-line information&#xD;
from a s&lt;span style="font-size:14.0pt;line-height:115%;&#xD;
font-family:" times="" new="" roman";mso-fareast-font-family:hiddenhorzocr;color:black;="" mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN"&gt;pace&#xD;
borne &lt;span style="font-size:14.0pt;line-height:115%;&#xD;
font-family:" times="" new="" roman";mso-fareast-font-family:"times="" roman";="" color:black;mso-ansi-language:en-in;mso-fareast-language:en-in;mso-bidi-language:="" hi"="" lang="EN-IN"&gt;experiment. A new bit synchronizer for a pulse code modulation (PCM)&#xD;
telemetry system which was developed use with the TIFR 100 cm balloon-borne&#xD;
far-infrared telescope payload has been described. This system performed &lt;span style="font-size:14.0pt;line-height:115%;font-family:" times="" new="" roman";="" mso-fareast-font-family:hiddenhorzocr;color:black;mso-ansi-language:en-in;="" mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN"&gt;satisfactorily&lt;span style="font-size:14.0pt;line-height:115%;font-family:" times="" new="" roman";="" mso-fareast-font-family:"times="" roman";color:black;mso-ansi-language:en-in;="" mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN"&gt; during recent balloon flight&#xD;
experiments.&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 134-140</description>
    <dc:date>1999-06-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/17339">
    <title>Modelling of tropospheric ozone in the equatorial region</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/17339</link>
    <description>Title: Modelling of tropospheric ozone in the equatorial region
Authors: Jain, Meena; Kundu, Namita
Abstract: The averaged&#xD;
ozone profile at the Indian station Trivandrum&#xD;
(8° N) is analyzed to get its characteristics in the tropical region. The&#xD;
vertical profile derived from rocket and balloonsonde data shows low&#xD;
concentration of ozone in the 8-12 km&#xD;
&#xD;
&lt;span style="font-size:14.0pt;line-height:115%;font-family:" times="" new="" roman";="" mso-fareast-font-family:"times="" roman";color:black;mso-ansi-language:en-in;="" mso-fareast-language:en-in;mso-bidi-language:hi"="" lang="EN-IN"&gt;altitude range. A&#xD;
photochemical-diffusive model has been developed to explain this phenomenon.&#xD;
The calculated profile obtained from the model does not give the knee in the&#xD;
above mentioned height range, but the shape produced by the model tallies with&#xD;
the observed profiles.&lt;/span&gt;
Page(s): 127-133</description>
    <dc:date>1999-06-01T00:00:00Z</dc:date>
  </item>
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