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        <identifier>oai:www.ideals.illinois.edu:2142/69288</identifier>
        <datestamp>2023-07-11</datestamp>
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        <thesis xmlns="http://www.ndltd.org/standards/metadata/etdms/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.ndltd.org/standards/metadata/etdms/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdms11.xsd http://purl.org/dc/elements/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdmsdc.xsd">
          <dc:creator>Franke, Steven John</dc:creator>
          <dc:date>2014-12-15T19:04:48Z</dc:date>
          <dc:date>2014-12-15T19:04:48Z</dc:date>
          <dc:date>10000-01-01</dc:date>
          <dc:date>1984</dc:date>
          <dc:date>1984</dc:date>
          <dc:description>Experimental measurements of signal level fluctuations (scintillation) on VHF and microwave signals from two geostationary communications satellites are studied in detail. The signals were recorded at an equatorial location which is almost directly beneath the satellites. The scintillation is caused by refraction and diffraction of the signals by variations of the refractive index in the F layer of the ionosphere. This study is directed toward using the observed multifrequency scintillation to remotely sense the characteristics of the ionospheric irregularities. This is done by considering both statistical and deterministic models for the scintillation producing irregularities. The models are combined with existing propagation theory using analytical and numerical simulation techniques in order to predict the spatial and temporal characteristics of the multifrequency scintillation. Comparison with the observations is used to verify the models. Extensive use is made of numerical simulation. This makes it possible to study both &amp;quot;weak&amp;quot; and &amp;quot;strong&amp;quot; scintillations which occur simultaneously on the microwave and VHF frequencies, respectively. In all cases, the models are chosen to be consistent with results from other remote sensing techniques and in situ measurements. Geophysical implications of the results are discussed in light of what is known about equatorial irregularities from previous experimental and theoretical studies.</dc:description>
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  Previous issue date: 1984</dc:description>
          <dc:description>Embargo set by: Seth Robbins for item 69454
Lift date: Forever
Reason: Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs</dc:description>
          <dc:description>Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs</dc:description>
          <dc:description>U of I Only</dc:description>
          <dc:description>275 p.</dc:description>
          <dc:description>Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 1984.</dc:description>
          <dc:identifier>http://hdl.handle.net/2142/69288</dc:identifier>
          <dc:identifier>(UMI)AAI8502144</dc:identifier>
          <dc:subject>Engineering, Electronics and Electrical</dc:subject>
          <dc:subject>Remote Sensing</dc:subject>
          <dc:title>Remote Sensing of Irregularities in the Equatorial Ionosphere Using the Radio Scintillation Technique</dc:title>
          <dc:type>text</dc:type>
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            <level>Dissertation</level>
            <name>Ph.D.</name>
            <department>Electrical Engineering</department>
            <discipline>Electrical Engineering</discipline>
            <grantor>University of Illinois at Urbana-Champaign</grantor>
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