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	<title>Spectrum Detector</title>
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		<title>Relay Architectures for 3GPP LTE-Advanced</title>
		<link>http://www.spectrumdetector.com/relay-architectures-for-3gpp-lte-advanced/</link>
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		<pubDate>Fri, 13 Jan 2012 10:09:35 +0000</pubDate>
		<dc:creator>Spectrum</dc:creator>
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		<description><![CDATA[EURASIP Journal on Wireless Communications and Networking Volume 2009 (2009), Article ID 618787, 14 pages doi:10.1155/2009/618787 Research ArticleRelay Architectures for 3GPP LTE-Advanced Steven W. Peters, Ali Y. Panah, Kien T. Truong, and Robert W. HeathDepartment of Electrical and Computer Engineering, The University of Texas at Austin, 1 University Station C0803, Austin, TX 78712-0240, USA Received [...]]]></description>
			<content:encoded><![CDATA[<p><span style="color: #000000;">EURASIP Journal on Wireless Communications and Networking</span><br />
<span style="color: #000000;"> Volume 2009 (2009), Article ID 618787, 14 pages</span><br />
<span style="color: #000000;"> doi:10.1155/2009/618787</span></p>
<p><span style="color: #000000;">Research ArticleRelay Architectures for 3GPP LTE-Advanced</span></p>
<p><span style="color: #000000;">Steven W. Peters, Ali Y. Panah, Kien T. Truong, and Robert W. HeathDepartment of Electrical and Computer Engineering, The University of Texas at Austin, 1 University Station C0803, Austin, TX 78712-0240, USA</span></p>
<p><span style="color: #000000;">Received 17 February 2009; Accepted 31 May 2009</span></p>
<p><span style="color: #000000;">Academic Editor: Angel LozanoCopyright © 2009 Steven W. Peters et al.</span></p>
<p><span style="color: #000000;">This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.</span></p>
<p><span style="color: #000000;">AbstractThe Third Generation Partnership Project&#8217;s Long Term Evolution-Advanced is considering relaying for cost-effective throughput enhancement and coverage extension. While analog repeaters have been used to enhance coverage in commercial cellular networks, the use of more sophisticated fixed relays is relatively new. The main challenge faced by relay deployments in cellular systems is overcoming the extra interference added by the presence of relays. Most prior work on relaying does not consider interference, however. This paper analyzes the performance of several emerging half-duplex relay strategies in interference-limited cellular systems: one-way, two-way, and shared relays. The performance of each strategy as a function of location, sectoring, and frequency reuse are compared with localized base station coordination. One-way relaying is shown to provide modest gains over single-hop cellular networks in some regimes. Shared relaying is shown to approach the gains of local base station coordination at reduced complexity, while two-way relaying further reduces complexity but only works well when the relay is close to the handset. Frequency reuse of one, where each sector uses the same spectrum, is shown to have the highest network throughput. Simulations with realistic channel models provide performance comparisons that reveal the importance of interference mitigation in multihop cellular networks.1. Introduction  The Third  Generation Partnership Program&#8217;s Long-Term Evolution Advanced (3GPP-LTE-Advanced) group is developing  a new standard for mobile broadband access that will meet the throughput and coverage requirements of a fourth generation cellular technology [1]. One of the main challenges faced by the developing standard is providing high throughput at the cell edge. Technologies like multiple input multiple output (MIMO), orthogonal frequency division multiplexing  (OFDM), and advanced error control codes enhance per-link throughput but do not inherently mitigate the effects of interference. Cell edge performance is becoming more important as cellular systems employ higher bandwidths with the same amount of transmit power and use higher carrier frequencies with infrastructure designed for lower carrier frequencies [2]. One solution to improve coverage is the use of fixed relays, pieces of infrastructure without a wired backhaul connection, that relay messages between the base station (BS) and mobile stations (MSs) through multihop communication [3–11].</span> <a href="http://www.hindawi.com/journals/wcn/2009/618787/">more</a></p>
<p><span style="color: #000000;">This article demonstrates the advantages of cellular repeater, or <a title="cell phone booster" href="http://cellularphoneboosters.net/"><span style="color: #000000;">cell phone booster</span></a> usage in areas where signal strength may be inadequate.</span></p>
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		<title>A New LFM-Signal Detector Based on Fractional Fourier Transform</title>
		<link>http://www.spectrumdetector.com/a-new-lfm-signal-detector-based-on-fractional-fourier-transform/</link>
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		<pubDate>Thu, 12 Jan 2012 20:36:19 +0000</pubDate>
		<dc:creator>Spectrum</dc:creator>
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		<description><![CDATA[A New LFM-Signal Detector Based on Fractional Fourier Transform Zhiping Yin and Weidong Chen* * Corresponding author: Weidong Chen wdchen@ustc.edu.cn EURASIP Journal on Advances in Signal Processing 2010, 2010:876282 doi:10.1155/2010/876282 Published: 12 July 2010 Abstract New LFM-signal detectors formulated by the integration of the 4th-power modulus of the fractional Fourier transform are proposed. They have similar [...]]]></description>
			<content:encoded><![CDATA[<h1>A New LFM-Signal Detector Based on Fractional Fourier Transform</h1>
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<p><strong>Zhiping Yin</strong> and <strong>Weidong Chen</strong><sup>*</sup></p>
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<li>* Corresponding author: Weidong Chen <a href="mailto:wdchen@ustc.edu.cn">wdchen@ustc.edu.cn</a></li>
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</div>
<p><em>EURASIP Journal on Advances in Signal Processing</em> 2010, <strong>2010</strong>:876282 doi:10.1155/2010/876282</p>
<p>Published: 12 July 2010 <a name="abstract"></a></p>
<h3>Abstract</h3>
<p><span style="color: #000000;">New LFM-<span style="color: #000000;">signal detectors</span> formulated by the integration of the 4th-power modulus of the fractional Fourier transform are proposed. They have similar performance to the modulus square detector of Radon-ambiguity transform because of the equivalence relationship between them. But the new detector has much lower computational complexity in the case that the number of the searching angles is far less than the length of the signal. Moreover, it is proved that the new <a title="signal detector" href="http://007spygear.com/products/Wireless-Signal-Detector.html"><span style="color: #000000;">signal detector</span></a> can be generalized to the integration of the <em>n</em>th-power (<img src="http://asp.eurasipjournals.com/content/inline/1687-6180-2010-876282-i1.gif" alt="" />) modulus of the fractional Fourier transform via mathematical derivation. Computer simulation results have confirmed the effectiveness of the proposed detector in LFM-signal detection.</span></p>
<p style="text-align: center;"><a href="http://asp.eurasipjournals.com/content/2010/1/876282/abstract">-more-</a></p>
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		<title>Uncooled detectors of continuum terahertz radiation</title>
		<link>http://www.spectrumdetector.com/uncooled-detectors-of-continuum-terahertz-radiation/</link>
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		<pubDate>Fri, 06 Jan 2012 20:20:21 +0000</pubDate>
		<dc:creator>Spectrum</dc:creator>
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		<description><![CDATA[This excerpt was taken from Journal of Microwaves, Optoelectronics and Electromagnetic Applications On-line version ISSN    2179-1074 P. KaufmannI;    R. MarconII; A.S. KudakaIII; M. M. CassianoIII;    L.O.T. FernandesIII; A. MarunIV; P. PereyraIV;    R. GodoyIV; E. BortolucciV; M. Beny ZakiaV;    J.A. DinizV; A.M. Pereira Alves da SilvaV; A.V. TimofeevskyVI;    V.A. NikolaevVI IUniversidade     Presbiteriana Mackenzie, CRAAM &#8211; Escola [...]]]></description>
			<content:encoded><![CDATA[<p>This excerpt was taken from</p>
<h2><a href="http://www.scielo.br/scielo.php?script=sci_serial&amp;pid=2179-1074&amp;lng=en&amp;nrm=iso">Journal of Microwaves, Optoelectronics and Electromagnetic Applications</a></h2>
<h2 id="printISSN"><span style="color: #0000a0;"><em>On-line version</em> ISSN    </span>2179-1074</h2>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;"><strong>P. Kaufmann<sup>I</sup>;    R. Marcon<sup>II</sup>; A.S. Kudaka<sup>III</sup>; M. M. Cassiano<sup>III</sup>;    L.O.T. Fernandes<sup>III</sup>; A. Marun<sup>IV</sup>; P. Pereyra<sup>IV</sup>;    R. Godoy<sup>IV</sup>; E. Bortolucci<sup>V</sup>; M. Beny Zakia<sup>V</sup>;    J.A. Diniz<sup>V</sup>; A.M. Pereira Alves da Silva<sup>V</sup>; A.V. Timofeevsky<sup>VI</sup>;    V.A. Nikolaev<sup>VI</sup></strong></span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;"><sup>I</sup>Universidade     Presbiteriana Mackenzie, CRAAM &#8211; Escola de Engenharia, São Paulo, SP,    Brazil, and Universidade Estadual de Campinas, CCS &#8211; Centro de Componentes Semicondutores,    Campinas, SP, Brazil, <a href="mailto:pierrekau@gmail.com">pierrekau@gmail.com</a>       <sup>II</sup>Universidade Estadual de Campinas, IFGW, Campinas, SP, Brazil and    Observatório Solar &#8220;Bernard Lyot&#8221;, Campinas, SP, Brazil, <a href="mailto:rmarcon@mpcnet.com.br">rmarcon@mpcnet.com.br</a>       <sup>III</sup>Universidade Presbiteriana Mackenzie, CRAAM &#8211; Escola de Engenharia,    São Paulo, SP, Brazil, <a href="mailto:kudaka@mackenzie.br">kudaka@mackenzie.br</a>       <sup>IV</sup>Complejo Astronomico El Leoncito, CONICET San Juan, Argentina,    <a href="mailto:amarun@casleo.gov">amarun@casleo.gov</a>       <sup>V</sup>Universidade Estadual de Campinas, CCS &#8211; Centro de Componentes Semicondutores,    Campinas, SP, Brazil, <a href="mailto:emilio@ccs.unicamp.br">emilio@ccs.unicamp.br</a>       <sup>VI</sup>Tydex J.S. Co, St. Petersburg, Russia, <a href="mailto:alexandertymofeevsky@tydex.ru">alexandertymofeevsky@tydex.ru</a></span></p>
<p>&nbsp;</p>
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<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;"><strong>ABSTRACT</strong></span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">THz continuum spectral    photometry has new and unique applications in different civil and military areas    presenting a number of distinctive advantages on the well known microwaves or    mid- to near-infrared technologies. THz sensing is essential to investigate    the emission mechanisms by high energy particle acceleration processes. Technical    challenges appear to diagnose radiation produced by solar flare burst emissions    measured from space as well as radiation produced by high energy electrons in    laboratory accelerators. THz filters and detectors have been investigated for    the construction of solar flare high cadence radiometers to operate outside    the terrestrial atmosphere. Experimental setups have been assembled for testing    THz continuum radiation response from distinct detectors: adapted commercial     microbolometer array, pyroelectric module, and opto-acoustic (Golay cell). The    results permitted the final design of a THz double radiometer using Golay cells    to be flown in stratosphere balloon missions.</span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;"><strong>Index Terms<em>-</em></strong>    Far IR continuum spectral photometry,THz radiometers, THz sensors, Solar THz    radiation</span></p>
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<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: small;"><strong>I.</strong> </span>    <span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: small;"><strong>INTRODUCTION</strong></span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">Technologies for    photometry and imaging in the THz range (arbitrarily 0.1 &#8211; 30 THz) are in full    expansion for a variety of new and unique applications in different civil and    military areas presenting a number of distinctive advantages on the well known    microwaves or mid- to near-infrared technologies. THz radiation propagates well    through cloth, dust and fog [1,2,3]. Sensing in this range is proving    to be particularly useful to determine internal characteristics of materials,    in the search for drugs, mines, and explosive materials. New biological and    medical THz imaging applications are far reaching. Aerospace THz remote sensing    applications include new approaches to determine atmospheric inhomogeneities    and cloud characteristics [4,5,6].</span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">Photometry and    imaging at THz frequencies have important application in the diagnostics of    radiation produced by high energy electrons, observed in laboratory accelerators    [7] as well as by thermal and non-thermal space plasmas [8,9].    Solar flare accelerates electrons to high energies. Their radiation by synchrotron    mechanism predicts intense fluxes in the far IR or THz range of frequencies    [10]. The radiometry of temperature enhancements above a pre-existent    bright level &#8211; as it is the case of flare radiation excess over the solar disk    intense emission &#8211; requires the effective suppression of the incoming visible   and near-infrared (NIR) radiation. This has been accomplished with the use of    a number of THz low-pass filters [11], consisting in a combination of    rough surface mirrors [12,13,14] and commercially available membranes    [15,16]. We present the performance of distinct uncooled sensors in    response to black body THz radiation for different sensors: microbolometer array,    pyroelectric module, and Golay cell.</span></p>
<p>&nbsp;</p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: small;"><strong>II. TEST OF    UNCOOLED THZ DETECTORS</strong></span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;"><em>A. Adapted microbolometer    array</em></span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">A custom-made detector    consisted in a room-temperature vanadium oxide micro-bolometer focal plane array    (FPA) camera IRM 160A with HRFZ-Si THz window provided by INO Company, Quebec,    Canada [17]. The camera total-power response for black body temperatures    ranging 300-1000 K was measured at El Leoncito laboratory. A nichrome resistor,    assumed as close to an ideal black body radiator, was placed at the focus of    150 mm concave reflector to produce an image occupying nearly 70 % of the FPA.    We selected the Region Of Interest (ROI) over the area in the frame filled by    the heated resistor image. All pixels readings on the ROI were added and averaged    for every frame reading, quoted in camera reading units. Several sets of measurements    were taken, for temperatures ranging from ambient (about 290 K) to about 900    K, without any low-pass filter, and using the two membrane low-pass filters     described elsewhere [11,15,16]. One set of measurements is summarized    in Fig. 1 (a). Figure    1(b) shows another expanded set of data showing the camera response using   the Zitex G110 [15] and the TydexBlack [16] low-pass membranes.</span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">The fluctuation    of data points can be attributed to measurement uncertainties (of about ±    1 reading unit), since they were taken with high cadence (30 frames/s). It can    be noted that the camera readings with Zitex G110 low pass filter interposed    is about 20-40 reading units above the TydexBlack readings, for the whole range    of temperatures. This effect was repeatedly observed for all series of measurements.    It might correspond to the fraction of power in the visible-NIR transmitted    by Zitex G110 [11].</span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">The substantial    reduction in the camera response to black body temperature changes when interposing    the low-pass membranes proves their effectiveness in the readings increase suppressing    the visible and NIR radiation. Indeed the predicted ratio of power increase    for a black body heated about 100 K, at the 700 K level, for the whole main    spectrum (</span><span style="font-size: x-small;">λ</span><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">    &gt; 0.5 </span><span style="font-size: x-small;">μ</span><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">m)    in comparison to the THz part of the spectrum (</span><span style="font-size: x-small;">λ</span><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">    &gt; 15 </span><span style="font-size: x-small;">μ</span><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">m     ) is close to 60. This might be compared to ratio of about 40 between the camera    ROI readings increase in that range compared to with the membrane low-pass filters.</span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">The camera scale    of about 25 K per reading unit (± 1 reading unit) was too large to allow    any measurable differences when adding one resonant metal mesh band-pass filter    [18].</span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;"><em>B. Pyroelectric    detector module</em></span></p>
<p><span style="font-family: Verdana, Arial, Helvetica, sans-serif; font-size: x-small;">The pyroelectric    modular detector made by Spectrum Detector Inc. [19], model SPH65-THz,    was tested at the laboratory of the Center for Semiconductor Components (CCS),    State University of Campinas. The setup utilised a standard laboratory Newport    model 67030 black body source with a build-in wheel chopper, set at 20 Hz. The    detector response to black body temperatures is shown in Fig.    2 for open conditions (responding to the visible &#8211; THz range) and for low-pass    membranes interposed.</span></p>
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