<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Spectrum Sensing | Dr. Jorge Querol</title><link>https://jorge.querol.org/tags/spectrum-sensing/</link><atom:link href="https://jorge.querol.org/tags/spectrum-sensing/index.xml" rel="self" type="application/rss+xml"/><description>Spectrum Sensing</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-US</language><lastBuildDate>Sat, 01 Jan 2022 00:00:00 +0000</lastBuildDate><image><url>https://jorge.querol.org/media/sharing.png</url><title>Spectrum Sensing</title><link>https://jorge.querol.org/tags/spectrum-sensing/</link></image><item><title>ESA NGSO-SENSE – Prototype for Measuring NGSO Satellite Network Interference</title><link>https://jorge.querol.org/project/ngso-sense/</link><pubDate>Sat, 01 Jan 2022 00:00:00 +0000</pubDate><guid>https://jorge.querol.org/project/ngso-sense/</guid><description>&lt;div class="mb-4"&gt;
&lt;span class="badge-agency badge-esa"&gt;European Space Agency&lt;/span&gt;
&lt;/div&gt;
&lt;p&gt;&lt;strong&gt;Role:&lt;/strong&gt; Vice-Principal Investigator&lt;br&gt;
&lt;strong&gt;Funding:&lt;/strong&gt; European Space Agency (&lt;strong&gt;ESA ARTES IC&lt;/strong&gt;, Contract No. &lt;code&gt;4000138641/22/UK/AL&lt;/code&gt;, in collaboration with &lt;strong&gt;SES&lt;/strong&gt;) · €650,000 (2022–2025)&lt;br&gt;
&lt;strong&gt;Official Page:&lt;/strong&gt; &lt;a href="https://www.uni.lu/snt-en/research-projects/esa-ngso-sense/" target="_blank" rel="noopener"&gt;uni.lu/snt-en/research-projects/esa-ngso-sense/&lt;/a&gt;&lt;/p&gt;
&lt;h3 id="executive-summary"&gt;Executive Summary&lt;/h3&gt;
&lt;p&gt;&lt;strong&gt;ESA NGSO-SENSE&lt;/strong&gt; (&lt;em&gt;Prototype for Measuring NGSO Satellite Network Interference and Radiofrequency Characteristics&lt;/em&gt;) designs, integrates, and validates an automated ground-station hardware/software prototype to detect, quantify, and attribute inline and aggregate radio-frequency interference (RFI) between Non-Geostationary Orbit (NGSO) mega-constellations (e.g., Starlink, OneWeb) and Geostationary (GEO) satellite networks (e.g., SES ASTRA) across Ku-band and Ka-band.&lt;/p&gt;
&lt;h3 id="verified-ground-station--rf-chain-architecture"&gt;Verified Ground Station &amp;amp; RF Chain Architecture&lt;/h3&gt;
&lt;ul&gt;
&lt;li&gt;&lt;strong&gt;Motorized &lt;code&gt;1.2 m&lt;/code&gt; Dual-Band Ka/Ku Parabolic Antenna (&lt;code&gt;65%&lt;/code&gt; efficiency, orthogonal OMTs)&lt;/strong&gt;:
&lt;ul&gt;
&lt;li&gt;&lt;strong&gt;Ka-Band Chain (&lt;code&gt;17.30 – 22.30 GHz&lt;/code&gt;)&lt;/strong&gt;: Antenna gain $G_a = 41.5\text{ dBi}$, $T_a = 50\text{ K}$ (clear sky at zenith), dual circular polarization (&lt;strong&gt;RHCP&lt;/strong&gt; &amp;amp; &lt;strong&gt;LHCP&lt;/strong&gt;), wideband LNA ($\text{NF} = 1.8\text{ dB}$, $G_{\text{LNA}} = 60 \pm 2\text{ dB}$, $T_{\text{noise}} = 149\text{ K}$), and &lt;strong&gt;Quad 4-BDC system per polarization&lt;/strong&gt; (&lt;code&gt;B1: 17.30–18.55 GHz&lt;/code&gt;, &lt;code&gt;B2: 18.55–19.80 GHz&lt;/code&gt;, &lt;code&gt;B3: 19.80–21.05 GHz&lt;/code&gt;, &lt;code&gt;B4: 21.05–22.30 GHz&lt;/code&gt; $\rightarrow$ &lt;code&gt;950–2150 MHz&lt;/code&gt; L-band IF).&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;Ku-Band Chain (&lt;code&gt;10.70 – 12.75 GHz&lt;/code&gt;)&lt;/strong&gt;: Antenna gain $G_a = 45.8\text{ dBi}$, $T_a = 70\text{ K}$, dual linear polarization (&lt;strong&gt;H&lt;/strong&gt; &amp;amp; &lt;strong&gt;V&lt;/strong&gt;), wideband LNA ($\text{NF} = 2.0\text{ dB}$, $G_{\text{LNA}} = 60 \pm 3\text{ dB}$, $T_{\text{noise}} = 75\text{ K}$), and &lt;strong&gt;Dual PLL 2-BDC system&lt;/strong&gt; (&lt;code&gt;Low: 10.70–11.70 GHz&lt;/code&gt; with $\text{LO } 9.75\text{ GHz}$; &lt;code&gt;High: 11.70–12.75 GHz&lt;/code&gt; with $\text{LO } 10.60\text{ GHz}$ $\rightarrow$ &lt;code&gt;950–2150 MHz&lt;/code&gt; L-band IF).&lt;/li&gt;
&lt;/ul&gt;
&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;Hybrid Coarse/Fine Satellite Tracking Loop&lt;/strong&gt;: Antenna Control Unit (ACU) and Az/El rotors executing periodic CelesTrak TLE coarse orbit propagation in parallel with a closed-loop fine-tracking controller driven by beacon power measurements from a &lt;strong&gt;PTR50 Beacon Receiver (&lt;code&gt;925–2150 MHz&lt;/code&gt;, &lt;code&gt;2 kHz&lt;/code&gt; PLL BW)&lt;/strong&gt; tracking Starlink (&lt;code&gt;11.325 GHz&lt;/code&gt;) and ASTRA (&lt;code&gt;11.7115 / 12.491 / 18.8015 GHz&lt;/code&gt;) beacons.&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;L-Band Switching Matrix &amp;amp; Receivers&lt;/strong&gt;: &lt;strong&gt;DEV Systemtechnik DEV 1985 (&lt;code&gt;16×16 / 16×8&lt;/code&gt;, &lt;code&gt;850–2450 MHz&lt;/code&gt;)&lt;/strong&gt; distributing matrix dynamically routing the 12 L-band feeds to a &lt;strong&gt;Rohde &amp;amp; Schwarz FPC1000&lt;/strong&gt; spectrum analyzer, &lt;strong&gt;USRP SDR&lt;/strong&gt; I/Q recorder, and automated &lt;strong&gt;Energy Detector + ML Autoencoder&lt;/strong&gt; anomaly identification pipeline.&lt;/li&gt;
&lt;/ul&gt;
&lt;h3 id="project-details"&gt;Project Details&lt;/h3&gt;
&lt;ul&gt;
&lt;li&gt;&lt;strong&gt;Funding Agency&lt;/strong&gt;: European Space Agency (&lt;strong&gt;ESA ARTES IC&lt;/strong&gt;, Contract &lt;code&gt;4000138641/22/UK/AL&lt;/code&gt;)&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;Industrial Partner&lt;/strong&gt;: &lt;strong&gt;SES&lt;/strong&gt;&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;Budget&lt;/strong&gt;: €650,000&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;Duration&lt;/strong&gt;: 2022 – 2025&lt;/li&gt;
&lt;li&gt;&lt;strong&gt;Role&lt;/strong&gt;: Vice-Principal Investigator&lt;/li&gt;
&lt;/ul&gt;
&lt;hr&gt;
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