<?xml version="1.0" encoding="UTF-8"?>
<feed xmlns="http://www.w3.org/2005/Atom" xmlns:dc="http://purl.org/dc/elements/1.1/">
  <title>NOPR Collection:</title>
  <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25571" />
  <subtitle />
  <id>http://nopr.niscpr.res.in/handle/123456789/25571</id>
  <updated>2026-10-10T05:21:11Z</updated>
  <dc:date>2026-10-10T05:21:11Z</dc:date>
  <entry>
    <title>Estimation of scattering coefficient of dry and wet soil with different moisture content at microwave frequencies</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25872" />
    <author>
      <name>Calla, O P N</name>
    </author>
    <author>
      <name>Hannan, I</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25872</id>
    <updated>2016-07-20T04:38:07Z</updated>
    <published>2001-04-01T00:00:00Z</published>
    <summary type="text">Title: Estimation of scattering coefficient of dry and wet soil with different moisture content at microwave frequencies
Authors: Calla, O P N; Hannan, I
Abstract: Microwave&#xD;
backscattering of the soil depends on its dielectric constant, which varies&#xD;
with change in the moisture content of the soil. The knowledge of the&#xD;
variability of the soil moisture is important for agriculture. With the&#xD;
database of the dielectric constant of a typical soil of Rajasthan, the&#xD;
computation of the scattering coefficients has been carried out using the&#xD;
&#xD;
perturbation&#xD;
model. The database of the estimated scattering coefficient at microwave&#xD;
frequencies (2-20 GHz) for dry and wet soil with different moisture contents&#xD;
has been generated. This will be useful for microwave remote sensing of soil, which&#xD;
will provide additional input for agriculture.
Page(s): 106-111</summary>
    <dc:date>2001-04-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>An interlaced phased array antenna for atmospheric radars</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25871" />
    <author>
      <name>Janardhanan, K V</name>
    </author>
    <author>
      <name>Mukundan, K K</name>
    </author>
    <author>
      <name>Shenoy, K S V</name>
    </author>
    <author>
      <name>Reddy, C A</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25871</id>
    <updated>2016-07-20T04:37:25Z</updated>
    <published>2001-04-01T00:00:00Z</published>
    <summary type="text">Title: An interlaced phased array antenna for atmospheric radars
Authors: Janardhanan, K V; Mukundan, K K; Shenoy, K S V; Reddy, C A
Abstract: The paper&#xD;
describes the design, construction details and test results of a 4×15 phased&#xD;
array Yagi antenna capable of producing three switchable beam orientations in a&#xD;
single plane. The antenna operates at a fixed frequency of 54.95 MHz and is&#xD;
useful for atmospheric studies. The array makes use of the 'interlaced phased&#xD;
array (IPA)’ concept to reduce the number&#xD;
&#xD;
of feed points&#xD;
and phase shifters, resulting in considerable reduction in cost and complexity&#xD;
of the array antenna. The 4×15 array was constructed using four-element&#xD;
Yagi-Uda antennas and was fed using a combination of co-axial and open-wire transmission&#xD;
lines. The performance of the antenna was qualitatively checked using the&#xD;
electrojet as a target. Moreover, the beam orientations and beamwidths of the&#xD;
antenna were verified using the sun as a radio source when it transitted over&#xD;
the beams. The performance parameters of the antenna were found to be very&#xD;
close to those computed theoretically.
Page(s): 98-105</summary>
    <dc:date>2001-04-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Vertical velocity, horizontal divergence and turbulence associated with tropical mesoscale convective system</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25870" />
    <author>
      <name>Rao, D Narayana</name>
    </author>
    <author>
      <name>Singh, H Randhir</name>
    </author>
    <author>
      <name>Rao, S Vijaya Bhaskara</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25870</id>
    <updated>2016-07-20T04:36:32Z</updated>
    <published>2001-04-01T00:00:00Z</published>
    <summary type="text">Title: Vertical velocity, horizontal divergence and turbulence associated with tropical mesoscale convective system
Authors: Rao, D Narayana; Singh, H Randhir; Rao, S Vijaya Bhaskara
Abstract: The MST radars&#xD;
have been used to measure directly the vertical motions above the radar site.&#xD;
Vertical velocity profiles and horizontal divergence/convergence derived from&#xD;
the vertical velocity using the mass continuity equation as well as eddy dissipation&#xD;
rate estimated under strong-to-moderate convection period are presented in the&#xD;
paper. Data obtained from the&#xD;
&#xD;
Indian MST radar&#xD;
located at Gadanki(13.5&lt;sup&gt;o&lt;/sup&gt;N, 79.8°E) have been used. The height range&#xD;
of the study is from 4 km&#xD;
to&#xD;
20 km. The aim of the&#xD;
present study is to calculate the horizontal divergence from the vertical&#xD;
velocity and then to find the extent of the enhancement in the vertical velocity&#xD;
and horizontal divergence as well as turbulence distribution during the well&#xD;
&#xD;
developed&#xD;
tropical mesoscale disturbances. Strong enhancement is observed in the vertical&#xD;
velocity and the horizontal divergence/convergence. Maximum turbulence has been&#xD;
observed near the top of the cloud and above. Eddy dissipation rate of the&#xD;
order of 0.007m&lt;sup&gt;2&lt;/sup&gt;s&lt;sup&gt;-3&lt;/sup&gt; has also been observed.
Page(s): 91-97</summary>
    <dc:date>2001-04-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>HF backscatter radar at the magnetic equator : System details and preliminary results</title>
    <link rel="alternate" href="http://nopr.niscpr.res.in/handle/123456789/25869" />
    <author>
      <name>Janardhanan, K V</name>
    </author>
    <author>
      <name>Rao, D Ramakrishna</name>
    </author>
    <author>
      <name>Viswanathan, K S</name>
    </author>
    <author>
      <name>Murthy, B V Krishna</name>
    </author>
    <author>
      <name>Shenoy, K S V</name>
    </author>
    <author>
      <name>Mohankumar, S V</name>
    </author>
    <author>
      <name>Kamath, K P</name>
    </author>
    <author>
      <name>Mukundan, K K</name>
    </author>
    <author>
      <name>Sajitha, G</name>
    </author>
    <author>
      <name>Shajahan, M</name>
    </author>
    <author>
      <name>Ayyappan, C</name>
    </author>
    <id>http://nopr.niscpr.res.in/handle/123456789/25869</id>
    <updated>2016-07-20T04:35:54Z</updated>
    <published>2001-04-01T00:00:00Z</published>
    <summary type="text">Title: HF backscatter radar at the magnetic equator : System details and preliminary results
Authors: Janardhanan, K V; Rao, D Ramakrishna; Viswanathan, K S; Murthy, B V Krishna; Shenoy, K S V; Mohankumar, S V; Kamath, K P; Mukundan, K K; Sajitha, G; Shajahan, M; Ayyappan, C
Abstract: A phase&#xD;
coherent, pulsed, monostatic and moderately high power HF Doppler radar,&#xD;
operating at 18 and 9 MHz has been installed at the magnetic equatorial&#xD;
station, Trivandrum (8.5°N, 77°E; dip 0.5°N), India. It is a powerful tool to&#xD;
study the plasma instability processes responsible for the generation of&#xD;
equatorial electrojet (EEJ) and equatorial spread-F (ESF) irregularities. A&#xD;
novelty in the radar system is the usage of the same phased array antenna at&#xD;
the two harmonically related frequencies of 18 and 9 MHz. The radar employs&#xD;
Doppler beam swinging (DBS) technique with beam orientations of vertical and&#xD;
±30° off zenith in the E-W plane, providing the unique capability of obtaining&#xD;
both zonal and vertical drifts of the ionospheric irregularities. The radar is&#xD;
also capable of providing zonal wind information in the region of 80-95 km. The&#xD;
new radar has opened up the possibilities of investigating different aspects of&#xD;
EEJ, like the E-W spectral asymmetry, diurnal pattern of the electric field and&#xD;
the effect of small scale plasma turbulence on the large scale EEJ altitude&#xD;
structure. In this paper the detailed system description, data processing&#xD;
scheme and some preliminary results obtained using the radar at 18 MHz are&#xD;
presented.
Page(s): 77-90</summary>
    <dc:date>2001-04-01T00:00:00Z</dc:date>
  </entry>
</feed>

