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  <title>NOPR Collection:</title>
  <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25572" />
  <subtitle />
  <id>http://nopr.niscpr.res.in/handle/123456789/25572</id>
  <updated>2026-10-10T23:54:35Z</updated>
  <dc:date>2026-10-10T23:54:35Z</dc:date>
  <entry>
    <title>Noise considerations in Gunn integrated rectangular microstrip antenna</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25879" />
    <author>
      <name>Nayak, Anjali</name>
    </author>
    <author>
      <name>Vishvakarma, Babau R</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25879</id>
    <updated>2014-01-23T16:35:36Z</updated>
    <published>2001-06-01T00:00:00Z</published>
    <summary type="text">Title: Noise considerations in Gunn integrated rectangular microstrip antenna
Authors: Nayak, Anjali; Vishvakarma, Babau R
Abstract: In the present paper,&#xD;
noise behaviour of the active patch antenna (GaAs Gunn integrated patch and InP&#xD;
Gunn integrated patch) has been theoretically investigated and consequently the&#xD;
noise figure, noise temperature and noise power are calculated as a function of&#xD;
bias voltage. The noise performance of InP Gunn integrated patch is found to be&#xD;
much better than&#xD;
&#xD;
that of the GaAs&#xD;
Gunn integrated patch.
Page(s): 148-154</summary>
    <dc:date>2001-06-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Microstrip array antenna with and without airgap in plasma environment</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25878" />
    <author>
      <name>Gupta, Anubha</name>
    </author>
    <author>
      <name>Pourush, P K S</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25878</id>
    <updated>2014-01-29T16:36:44Z</updated>
    <published>2001-06-01T00:00:00Z</published>
    <summary type="text">Title: Microstrip array antenna with and without airgap in plasma environment
Authors: Gupta, Anubha; Pourush, P K S
Abstract: The present paper&#xD;
explores the important characteristics of an array of 4×4-element planar array&#xD;
of circular patch microstrip antenna (CPMA) designed on RT-duroid substrate(ɛ&lt;sub&gt;r&lt;/sub&gt;=&#xD;
2.32) at 1.155 GHz (L-band) for on-board applications in mobile communication through&#xD;
satellite. An airgap is introduced in between the dielectric and the ground plane&#xD;
which improves the bandwidth and maintain the gain of the antenna geometry. This&#xD;
antenna geometry is studied in presence of plasma environment and the effect of&#xD;
generation of electroacoustic waves on the radiation characteristics of the&#xD;
given geometry is determined. For this, a well established linearized hydrodynamic&#xD;
theory and vector wave function technique is used to derive the expression for&#xD;
the field pattern and radiated power by the antenna. The important antenna&#xD;
parameters like radiation conductance, efficiency, directive gain and bandwidth&#xD;
along with radiation patterns are computed and plotted for both plasma as well as&#xD;
for the free space.
Page(s): 143-147</summary>
    <dc:date>2001-06-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Markov chain models for pre-monsoon thunderstorm in Calcutta, India</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25877" />
    <author>
      <name>Dasgupta, S</name>
    </author>
    <author>
      <name>De, U K</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25877</id>
    <updated>2014-01-21T16:36:17Z</updated>
    <published>2001-06-01T00:00:00Z</published>
    <summary type="text">Title: Markov chain models for pre-monsoon thunderstorm in Calcutta, India
Authors: Dasgupta, S; De, U K
Abstract: Markov chain models&#xD;
of first, second and third order have been used to provide a probabilistic&#xD;
description of the occurrence of the thunderstorm phenomenon in the pre-monsoon&#xD;
season (March-May) in Calcutta (India). The analysis is based on the relevant&#xD;
data for the 10-year period 1985-94. Use of Akaike’s information criterion (AIC)&#xD;
reveals that the Markov chain of the third order is perhaps the model that&#xD;
describes best the phenomenon. This finding is also supported by actual verification&#xD;
of the fact that the Markov chain of third order simulates the observed data&#xD;
best. Besides, the time independent behaviour of the chain has also been&#xD;
studied with the help of the steady state probabilities. The theoretical values&#xD;
of the mean recurrence time for thunderstorm and fair weather days hence&#xD;
obtained are in close agreement with the observed data.
Page(s): 138-142</summary>
    <dc:date>2001-06-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Ionospheric E-region irregularities during equatorial counter electrojet</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25876" />
    <author>
      <name>Rastogi, R G</name>
    </author>
    <author>
      <name>Subbarao, K S V</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25876</id>
    <updated>2014-01-20T16:36:42Z</updated>
    <published>2001-06-01T00:00:00Z</published>
    <summary type="text">Title: Ionospheric E-region irregularities during equatorial counter electrojet
Authors: Rastogi, R G; Subbarao, K S V
Abstract: The paper describes&#xD;
a coordinated study of the geomagnetic fields at Trivandrum and Alibag, digital&#xD;
vertical incidence ionograms and oblique VH F backscatter radar echoes at Thumba&#xD;
on a day with a large counter electrojet (CEJ) event in the afternoon hours. It&#xD;
is shown that the cusp type of sporadic-E (&lt;i&gt;E&lt;/i&gt;&lt;sub&gt;sc&lt;/sub&gt;), above the normal&#xD;
E-layer continues to descend with time after the start of CEJ up to about 110 km,&#xD;
indicating downward Hall electric field. When the &lt;i&gt;E&lt;/i&gt;&lt;sub&gt;sc&lt;/sub&gt; layer descends&#xD;
to around 110 km, the downward Hall polarization field due to CEJ, acting on the&#xD;
downward gradient of plasma density in the top side of the layer, generates irregularities&#xD;
by the cross-field instability mechanism. These irregularities give the signature&#xD;
of the &lt;i&gt;q-&lt;/i&gt;type of sporadic-E (&lt;i&gt;E&lt;/i&gt;&lt;sub&gt;sc&lt;/sub&gt;) on the ionograms and&#xD;
type-2 VHF Doppler spectra of scatter echoes. With continued descent, &lt;i&gt;E&lt;/i&gt;&lt;sub&gt;sc&lt;/sub&gt;&#xD;
disappears and no VHF echoes are recorded. With intensification of CEJ, the eastward&#xD;
streaming velocity of the electrons exceed the ion acoustic velocity and strong&#xD;
type -l echoes are observed on VHF backscatter radar. With the decrease of CEJ even&#xD;
type-2 echoes disappear and no scatter echoes are observed by HF ionosonde or on&#xD;
VHF radar.
Page(s): 130-137</summary>
    <dc:date>2001-06-01T00:00:00Z</dc:date>
  </entry>
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