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    <title>NOPR Collection:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/31859</link>
    <description />
    <pubDate>Sat, 10 Oct 2026 22:35:08 GMT</pubDate>
    <dc:date>2026-10-10T22:35:08Z</dc:date>
    <item>
      <title>Dielectric properties of black soil with chemical fertilizers at X-band</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/31865</link>
      <description>Title: Dielectric properties of black soil with chemical fertilizers at X-band
Authors: Navarkhele, V V; Kapre, A K; Shaikh, A A
Abstract: &lt;span style="font-size:11.0pt;font-family:&#xD;
" times="" new="" roman";mso-fareast-font-family:"times="" roman";mso-bidi-font-family:="" mangal;mso-ansi-language:en-gb;mso-fareast-language:en-us;mso-bidi-language:="" hi"="" lang="EN-GB"&gt;Dielectric properties of black soil with the addition of chemicals were&#xD;
measured at microwave frequency. The dielectric measurements have been achieved&#xD;
by using X-band set up. The dielectric properties, that is dielectric constant&#xD;
(&lt;img src='http://www.niscair.res.in/jinfo/belongs.gif' border=0&gt;') and dielectric loss (&lt;img src='http://www.niscair.res.in/jinfo/belongs.gif' border=0&gt;") have been measured for two&#xD;
frequencies (8 and 10 GHz) at room temperature. From the experimental data, it&#xD;
is confirmed that the dielectric constant and dielectric loss increase with&#xD;
increasing percentage volume of chemical fertilizers and decrease with increase&#xD;
in frequency of oscillation. The results also show that the dielectric constant&#xD;
and dielectric loss are higher for the urea than that of potassium carbonate.&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 102-105</description>
      <pubDate>Mon, 01 Jun 2015 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/31865</guid>
      <dc:date>2015-06-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Study of pre-monsoon thunderstorms over Kalyani from radio frequency spectra</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/31864</link>
      <description>Title: Study of pre-monsoon thunderstorms over Kalyani from radio frequency spectra
Authors: Bhattacharya, A B; Raha, B; Pandit, J; Sarkar, Shalini; Sarkar, Sumit; Mondal, Somasree
Abstract: &lt;span style="font-size:11.0pt;mso-bidi-font-size:10.0pt;&#xD;
font-family:" times="" new="" roman";mso-fareast-font-family:calibri;mso-bidi-font-family:="" "times="" roman";mso-ansi-language:en-in;mso-fareast-language:en-us;="" mso-bidi-language:ar-sa"=""&gt;Lightning in the form of electromagnetic radiation, in&#xD;
very low frequency (VLF) and low frequency (LF) bands, is received on 1 April&#xD;
and 7 April 2015 from 10 kHz to 300 kHz over Kalyani &lt;span style="font-size:11.0pt;mso-bidi-font-size:10.0pt;font-family:" times="" new="" roman";="" mso-fareast-font-family:calibri;mso-bidi-font-family:"times="" mso-ansi-language:en-us;mso-fareast-language:en-us;mso-bidi-language:ar-sa"="" lang="EN-US"&gt;during&#xD;
pre-monsoon thunderstorms.&lt;span style="font-size:11.0pt;&#xD;
mso-bidi-font-size:10.0pt;font-family:" times="" new="" roman";mso-fareast-font-family:="" calibri;mso-bidi-font-family:"times="" roman";mso-ansi-language:en-in;="" mso-fareast-language:en-us;mso-bidi-language:ar-sa"="" lang="EN-US"&gt; &lt;span style="font-size:11.0pt;mso-bidi-font-size:10.0pt;font-family:" times="" new="" roman";="" mso-fareast-font-family:calibri;mso-bidi-font-family:"times="" mso-ansi-language:en-in;mso-fareast-language:en-us;mso-bidi-language:ar-sa"=""&gt;Their&#xD;
characteristics, viz. the spectral pattern and other relevant properties, are&#xD;
examined with the help of radio frequency (RF) spectra. &lt;span style="font-size:11.0pt;mso-bidi-font-size:10.0pt;font-family:" times="" new="" roman";="" mso-fareast-font-family:"times="" roman";mso-bidi-font-family:"times="" mso-ansi-language:en-in;mso-fareast-language:en-us;mso-bidi-language:ar-sa"=""&gt;Another&#xD;
severe thunderstorm experienced, over a wide area covering different parts of South Bengal including Kalyani, on 11 April 2013 has also&#xD;
been recorded in the form of integrated field intensity of atmospherics at 27&#xD;
kHz receiver. After analysing, some interesting results are reported related to&#xD;
radio signal reception originating from lightning as electromagnetic radiation.&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;&lt;/span&gt;
Page(s): 96-101</description>
      <pubDate>Mon, 01 Jun 2015 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/31864</guid>
      <dc:date>2015-06-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Variability of ion density due to solar flares as measured by SROSS–C2 satellite</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/31863</link>
      <description>Title: Variability of ion density due to solar flares as measured by SROSS–C2 satellite
Authors: Bardhan, Ananna; Sharma, D K; Kumar, Sarvesh
Abstract: In the present paper the effect of solar&#xD;
flares on ion density has been studied. The ion densities have been measured for&#xD;
the period 1995-1998 using RPA payload of SROSS-C2 satellite. Solar flare data&#xD;
has been obtained from National Geophysical Data Center (NGDC) Boulder,&#xD;
Colorado (USA). The study indicates considerable decrease (1.2 to 2.8 times) in&#xD;
total ion density during flare time as compared to normal time. Out of four ion&#xD;
species, i.e. O&lt;sup&gt;+&lt;/sup&gt;, O&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt;, H&lt;sup&gt;+&lt;/sup&gt; and He&lt;sup&gt;+&lt;/sup&gt;,&#xD;
the O&lt;sup&gt;+&lt;/sup&gt; ion density is most affected by the effects of the flare as&#xD;
measured by SROSS–C2. There is considerable decrease in O&lt;sup&gt;+&lt;/sup&gt; ion&#xD;
density while O&lt;sub&gt;2&lt;/sub&gt;&lt;sup&gt;+&lt;/sup&gt;, H&lt;sup&gt;+&lt;/sup&gt; and He&lt;sup&gt;+&lt;/sup&gt;&#xD;
density show negligible change during flare time as compared to normal time.&#xD;
Furthermore, relation between change in ion density (∆N) as a response to&#xD;
change in ion temperature (∆T) during flare time and normal days has been&#xD;
estimated. A comparison of ion density obtained from SROSS-C2 with IRI–2012&#xD;
during the flare time indicates an overestimation by IRI-2012.
Page(s): 88-95</description>
      <pubDate>Mon, 01 Jun 2015 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/31863</guid>
      <dc:date>2015-06-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Correlation of foF2 and M(3000)F2 over low latitude stations during  low solar activity period</title>
      <link>http://nopr.niscpr.res.in/handle/123456789/31862</link>
      <description>Title: Correlation of foF2 and M(3000)F2 over low latitude stations during  low solar activity period
Authors: Nagar, Anju; Mishra, S D; Vijay, S K
Abstract: This paper aims&#xD;
to investigate the relationship between propagation parameter M(3000)F2 and&#xD;
F2-layer critical frequency (foF2) during 2006-2010. Data from three low&#xD;
latitude stations, namely Jicamarca (12ºS, 283ºE), Kwajalein (09ºN, 167ºE) and&#xD;
Madimbo (22ºS, 031ºE) for the months of January (winter) and July (summer)&#xD;
during 2006-2010 are used for the study. It is found that the daily values of&#xD;
M(3000)F2 cannot be estimated from foF2 using a simple linear equation. It is&#xD;
concluded that that two procedures (day-to-day and hour-to-hour) do not give&#xD;
different results and the correlation coefficients between the daily values of&#xD;
M(3000)F2 and foF2 are generally lower than 0.6 and could be positive or&#xD;
negative.
Page(s): 78-87</description>
      <pubDate>Mon, 01 Jun 2015 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://nopr.niscpr.res.in/handle/123456789/31862</guid>
      <dc:date>2015-06-01T00:00:00Z</dc:date>
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