<?xml version="1.0" encoding="UTF-8"?>
<rss xmlns:dc="http://purl.org/dc/elements/1.1/" version="2.0">
  <channel>
    <title>NOPR Community:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/36646</link>
    <description />
    <pubDate>Sat, 10 Oct 2026 03:35:44 GMT</pubDate>
    <dc:date>2026-10-10T03:35:44Z</dc:date>
    <item>
      <title>Relative Contribution of Various Secondary X-ray Components below  100keV at Balloon Altitudes</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/36829</link>
      <description>Title: Relative Contribution of Various Secondary X-ray Components below  100keV at Balloon Altitudes
Authors: Manchanda, R K
Abstract: A large fraction of total X-ray flux below 100keV at balloon altitudes consists of secondary components. Experimentally   derived data for these different components for designing new detector systems for X-ray studies are presented. It is shown   that, in case of a crystal scintillator, intrinsic production overtakes the other contribution if the aperture is made too narrow.
Page(s): 255-256</description>
      <pubDate>Wed, 01 Dec 1982 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/36829</guid>
      <dc:date>1982-12-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Dependence of Ionospheric Drift Speed on Geomagnetic Activity</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/36828</link>
      <description>Title: Dependence of Ionospheric Drift Speed on Geomagnetic Activity
Authors: Sardesai, D V; Badala, P; Rai, R K
Abstract: Effect of geomagnetic activity on ionospheric drift speed is studied for Udaipur (geomag.lat., 14.55°N).To reduce the effect of solar activity, the study is made with the data obtained during Mar. 1974-Oct. 1975, a low activity period, and only those days for which 10.7 cm solar flux was below 90 have been considered. A negative correlation is found between noontime E-region apparent drift speed and geomagnetic &lt;i&gt;K&lt;sub&gt;p&lt;/sub&gt;&lt;/i&gt; index. An identical relationship is obtained for nighttime apparent drift speed with &lt;i&gt;K&lt;sub&gt;p&lt;/sub&gt;&lt;/i&gt; in case of F-region. The correlation coefficients deduced in the two cases are -0.81 and -0.86, respectively.
Page(s): 252-254</description>
      <pubDate>Wed, 01 Dec 1982 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/36828</guid>
      <dc:date>1982-12-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Radiation from an Alford Loop Antenna in Two component Warm Plasma</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/36827</link>
      <description>Title: Radiation from an Alford Loop Antenna in Two component Warm Plasma
Authors: Kumar, Anil; Gupta, R K
Abstract: Expressions for the electromagnetic and the electroacoustic field components of a loop antenna radiating in a two component warm plasma are obtained. Assuming a plausible current distribution, variation of the radiation resistancy of an Alford loop antenna in two-component warm plasma with plasma frequency is compared with the experimentally measured values of the radiation resistance of a loop antenna on the Ariel-3 satellite. It is observed that the theoretically computed values of the radiation resistance are now closer than the values calculated by using earlier theory.
Page(s): 247-251</description>
      <pubDate>Wed, 01 Dec 1982 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/36827</guid>
      <dc:date>1982-12-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Equatorial Radio Scintillations of ATS-6 Radio Beacons: Phase II-Ootacamund 1975-76</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/36826</link>
      <description>Title: Equatorial Radio Scintillations of ATS-6 Radio Beacons: Phase II-Ootacamund 1975-76
Authors: Rastogi, R G; Chandra, H; Deshpande, M R
Abstract: Temporal variations of the amplitude fluctuations of the radio beacon signals on 40, 140 and 360 M Hz transmitted from the ATS-6 satellite (at 34°E longitude) received at Ootacamund (11.4 N, 76.7 E, magnetic dip 6° N) during the second phase ofthe ATS-6 programme (1975-76) are described. For 360 MHz beacon, the mean scintillations index had two minima of about1% (about 0.1 dB) during the sunrise and sunset periods; a flat maximum of about 4% (0.4 dB) around midday and another maximum of about 13% (1.2 dB) around 2100-2200 hrs LT. The mean scintillation index on 140 MHz was minimum (0.6 dB) around sunrise and sunset hours and maxima of about 2 dB were at midday and nighttime. The magnitude of scintillations of 40 MHz was about 3 dB around sunrise and sunset periods and about 5 dB during midday and midnight hours. The nighttime scintillations were strongest in October 1975 (thus during equinoxes) while daytime scintillations did not indicate any definite seasonal variation.
Page(s): 240-246</description>
      <pubDate>Wed, 01 Dec 1982 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/36826</guid>
      <dc:date>1982-12-01T00:00:00Z</dc:date>
    </item>
  </channel>
</rss>

