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    <title>NOPR Community:</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/37372</link>
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        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/37640" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/37639" />
        <rdf:li rdf:resource="http://nopr.niscpr.res.in/handle/123456789/37637" />
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    <dc:date>2026-10-09T16:33:53Z</dc:date>
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  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/37640">
    <title>Secondary Maxima in Total Electron Content over Hawaii</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/37640</link>
    <description>Title: Secondary Maxima in Total Electron Content over Hawaii
Authors: Prakash, Sant
Abstract: An observation of the secondary maxima occurrences over Hawaii both at daytime and nighttime has been made using electron content versus time data. These data were obtained over Hawaii by measuring Faraday rotation of the polarization of vhf telemetry carrier transmissions from the geostationary satellite. The occurrence of secondary maxima is more pronounced during winter than in any other season and also during nighttime than daytime.
Page(s): 336-337</description>
    <dc:date>1976-12-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/37639">
    <title>Microwave Absorption in the Martian Atmosphere</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/37639</link>
    <description>Title: Microwave Absorption in the Martian Atmosphere
Authors: Johri, Rakesh K; Joshi, Jagdish C
Abstract: Microwave absorption in the Martian atmosphere (in the frequency range 21-117 GHz) from 0 to 185 km, has been computed. The total absorption coefficient ϒ, absorption coefficient at peak resonance frequency ϒ&lt;sub&gt;0&lt;/sub&gt;, and half-width of the absorption line Δ&lt;i&gt;v&lt;/i&gt; are calculated for all the important constituents of the Martian atmosphere. A comparison of the ϒ&lt;sub&gt;0&lt;/sub&gt;and Δ&lt;i&gt;v&lt;/i&gt; values for the Martian and terrestrial atmospheres indicater that the ϒ&lt;sub&gt;0&lt;/sub&gt; values are greater for Martian atmosphere, while reverse is true for Δ&lt;i&gt;v&lt;/i&gt; values.
Page(s): 332-336</description>
    <dc:date>1976-12-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/37637">
    <title>Forbush Decrease &amp; Geomagnetic Storms in relation to Varying Interplanetary Parameters</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/37637</link>
    <description>Title: Forbush Decrease &amp; Geomagnetic Storms in relation to Varying Interplanetary Parameters
Authors: Agrawal, S P; Singh, R L
Abstract: Using the hourly neutron monitor data for the present solar cycle, the characteristics of all the Forbush decreases (FDs) have been studied. Statistically, the rigidity spectral exponent is found to be &lt;img src='/image/spc_char/wave.gif' border=0&gt; 0·8 ± 0·2. It is seen that most of the FDs occur in coincidence with sudden storm commencements and the largest FDs are produced by solar flares occurring near the central meridian. These results are discussed in terms of earlier observations.
Page(s): 330-332</description>
    <dc:date>1976-12-01T00:00:00Z</dc:date>
  </item>
  <item rdf:about="http://nopr.niscpr.res.in/handle/123456789/37635">
    <title>Anomalous Variations in F-Region Phase Path Records</title>
    <link>http://nopr.niscpr.res.in/handle/123456789/37635</link>
    <description>Title: Anomalous Variations in F-Region Phase Path Records
Authors: Murthy, B Suryanarayana; Rao, B Ramachandra
Abstract: Some peculiar complexities observed in F-region phase path records, taken on a frequency of 5'6 MHz, during daytime at Waltair, are presented. These complexities are discussed in terms of reflections coming from curved surfaces produced by travelling ionospheric disturbances in the ionosphere.
Page(s): 328-329</description>
    <dc:date>1976-12-01T00:00:00Z</dc:date>
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