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    <title>NOPR Collection:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/17290</link>
    <description />
    <pubDate>Tue, 13 Oct 2026 04:08:13 GMT</pubDate>
    <dc:date>2026-10-13T04:08:13Z</dc:date>
    <item>
      <title>Some anomalous behaviour of GPS/GLONASS constellations during meteor shower of 18 Nov. 1998</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/17326</link>
      <description>Title: Some anomalous behaviour of GPS/GLONASS constellations during meteor shower of 18 Nov. 1998
Authors: Banerjee, P; Mukherjee, Somik; Mathur, B S
Abstract: Anticipating&#xD;
that during the recent visit of the comet 55p(Temple-Tuttle), the overall&#xD;
system performance of GPS/GLONASS would be affected, the GPS/GLONASS signals&#xD;
were monitored during that time at National Physical Laboratory, New Delhi. Initial&#xD;
observation indicated a significant degradation&#xD;
&#xD;
of position&#xD;
accuracy in GPS/GLONASS mix mode. The accuracy had been found to reach its&#xD;
nominal value in about 25 h after the event. Anomalies were also found in&#xD;
residual errors of pseudoranges.
Page(s): 53-54</description>
      <pubDate>Mon, 01 Feb 1999 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/17326</guid>
      <dc:date>1999-02-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Simulation of secondary radiation pattern of MSMR antenna</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/17325</link>
      <description>Title: Simulation of secondary radiation pattern of MSMR antenna
Authors: Sharma, S B; Sriharsha, C
Abstract: Simulation&#xD;
of secondary radiation pattern of the multi frequency scanning microwave&#xD;
radiometer (MSMR) has been presented in this paper. Simulated patterns are&#xD;
used, as many practical difficulties have been encountered during&#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;measurements. Aperture&#xD;
integration in conjunction with geometric theory of diffraction has been used&#xD;
for simulation of secondary pattern of offset parabolic reflector. The&#xD;
simulated and measured results are presented and fairly good agreement has been&#xD;
observed between them.&lt;/span&gt;
Page(s): 43-52</description>
      <pubDate>Mon, 01 Feb 1999 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/17325</guid>
      <dc:date>1999-02-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Field aligned current and parallel electric field between magnetosphere and ionosphere of Mars</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/17324</link>
      <description>Title: Field aligned current and parallel electric field between magnetosphere and ionosphere of Mars
Authors: Haider, S A; Seth, S P; Raina, K S
Abstract: A steady state kinetic&#xD;
model is used to estimate the electron current density at different potential&#xD;
differences between the magnetosphere&#xD;
and ionosphere of Mars. For this calculation it is assumed that&#xD;
Mars has a weak dipole magnetosphere whose plasma sheet is connected to the&#xD;
ionosphere along the magnetic field lines. The total electron flux of 5.79×10&lt;sup&gt;8&lt;/sup&gt; cm&lt;sup&gt;-2&lt;/sup&gt;&#xD;
s&lt;sup&gt;-1&lt;/sup&gt; is calculated&#xD;
in the Martian magnetosphere corresponding to the downward current density of&#xD;
1.0×10&lt;sup&gt;-6&lt;/sup&gt;  A/m&lt;sup&gt;2&lt;/sup&gt;&lt;i&gt; &lt;/i&gt;at&#xD;
zero potential difference. The maximum flux of thermal electrons escaping&#xD;
towards the plasma sheet of Mars&lt;i&gt; &lt;/i&gt;at zero current&#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;density is calculated to be&#xD;
3.0×10&lt;sup&gt;8&lt;/sup&gt; cm&lt;sup&gt;-2&lt;/sup&gt; s&lt;sup&gt;-1&lt;/sup&gt;. At zero current density the&#xD;
precipitating flux of plasma sheet electrons is approximately equal to maximum&#xD;
escape flux of thermal electrons. The calculated results are found to be in&#xD;
reasonable agreement with the experimental data obtained from Hyperbolic Ret&#xD;
arding Potential Analyzer (HARP) experiment onboard Phobos-2 .&lt;/span&gt;
Page(s): 36-42</description>
      <pubDate>Mon, 01 Feb 1999 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/17324</guid>
      <dc:date>1999-02-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Performance analysis of an HF radio link between India and Antarctica</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/17323</link>
      <description>Title: Performance analysis of an HF radio link between India and Antarctica
Authors: Pasricha, P K; Vijayakumar, P N; Aggarwal, S; Lakshmi, D R; Reddy, B 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;This paper presents an analysis of the performance of the HF radio link,&#xD;
via the ionosphere, between a place near Delhi&#xD;
and the indian Antarctic station Maitri. The observations pertain to the rising&#xD;
part of solar activity in 1988-89. An analysis of optimum traffic frequency&#xD;
(FOT) and circuit  reliability has been&#xD;
made separately at the two stations. The operational frequencies are found to&#xD;
be compatible with some of the available predictions of FOT. The theoretically&#xD;
computed periods of HF propagation are seen to match with the observed&#xD;
operation periods and demonstrate the utility of HF for communications with Antarctica.&lt;/span&gt;
Page(s): 26-35</description>
      <pubDate>Mon, 01 Feb 1999 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/17323</guid>
      <dc:date>1999-02-01T00:00:00Z</dc:date>
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