Wideband Beam Steering Concept for Terahertz Time-Domain Spectroscopy: Theoretical Considerations
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
RTT TECHNOLOGY TOPIC January 2015 Defence Spectrum – the New Battleground?
RTT TECHNOLOGY TOPIC January 2015 Defence Spectrum – the new battleground? In this month’s technology topic we look at contemporary military radio developments, the integration of LTE user devices into defence communication systems, the relevance of military research to 5 G deployment efficiency and related spectral utilisation and regulatory issues. Defence communication systems are deployed across the whole radio spectrum from long wave to light. This includes mobile communication systems at VHF and UHF and L Band and S band, LEO, MEO and GSO satellite systems (VHF to E band) and mobile and fixed radar (VHF to E band). Legacy defence systems are being upgraded to provide additional functionality. This requires more rather than less spectrum. Increased radar resolution requires wider channel bandwidths; longer range requires more power and improved sensitivity. Improved sensitivity increases the risk of inter system interference. Emerging application requirements including unmanned aerial vehicles require a mix of additional terrestrial, satellite and radar bandwidth. These requirements are geographically and spectrally diverse rather than battlefield and spectrally specific. The assumption in many markets is that the defence industry will be willing and able to surrender spectrum for mobile broadband consumer and civilian use. The AWS 3 auction in the US is a contemporary example with a $5 billion transition budget to cover legacy military system decommissioning in the DOD coordination zone between 1755 and 1780 MHz This transition strategy assumes an increased use of LTE network hardware and user hardware in battlefield systems. While this might imply an opportunity for closer coordination and cooperation between the mobile broadband and defence community it seems likely that an increase in the amount of defence bandwidth needed to support a broadening range of RF dependent systems could be a problematic component in the global spectral allocation and auction process. -
Ncar S-Pol Second Frequency (K -Band) Radar
P12R.6 NCAR S-POL SECOND FREQUENCY (KA-BAND) RADAR Gordon Farquharson,∗ Frank Pratte, Milan Pipersky, Don Ferraro, Alan Phinney, Eric Loew, Robert Rilling, Scott Ellis, and Jothiram Vivekanandan National Center for Atmospheric Research, Boulder, Colorado 1. INTRODUCTION The National Center for Atmospheric Research (NCAR) has recently extended the observational capability of the S-band dual-polarimetric weather radar system (S-Pol, Keeler et al. (2000)) by adding a Ka-band (35 GHz) po- larimetric Doppler radar (Vivekanandan et al., 2004). The Transmitter Ka-band radar employs a dual channel receiver and can be configured for either HH and HV, or HH and VV polari- metric measurements. The Ka-band and S-band antenna beams are matched and aligned, and timing signals for both systems are generated from the Global Position Sys- tem (GPS) ensuring that a common resolution volume is sampled by both systems. This dual-wavelength capabil- ity provides the potential for retrieving water vapor profiles Radar Processor (Ellis et al., 2005) and liquid water content in Rayleigh scattering conditions (Vivekanandan et al., 1999), im- proving remote sensing of various precipitation types, and studies on cloud microphysics. 2. RADAR DESCRIPTION Receiver The K -band radar is housed in three enclosures which a Figure 1: K -band radar attached to the S-band dish. The are mounted to the S-Pol S-band dish and pedestal struc- a transmitter, receiver, and processor enclosures are vis- ture (Figure 1); these include the transmitter enclosure, ible. The K -band antenna is mounted to the receiver the receiver enclosure, and the radar processor enclo- a enclosure and is facing away from the viewer in the pho- sure. -
Spectrum and the Technological Transformation of the Satellite Industry Prepared by Strand Consulting on Behalf of the Satellite Industry Association1
Spectrum & the Technological Transformation of the Satellite Industry Spectrum and the Technological Transformation of the Satellite Industry Prepared by Strand Consulting on behalf of the Satellite Industry Association1 1 AT&T, a member of SIA, does not necessarily endorse all conclusions of this study. Page 1 of 75 Spectrum & the Technological Transformation of the Satellite Industry 1. Table of Contents 1. Table of Contents ................................................................................................ 1 2. Executive Summary ............................................................................................. 4 2.1. What the satellite industry does for the U.S. today ............................................... 4 2.2. What the satellite industry offers going forward ................................................... 4 2.3. Innovation in the satellite industry ........................................................................ 5 3. Introduction ......................................................................................................... 7 3.1. Overview .................................................................................................................. 7 3.2. Spectrum Basics ...................................................................................................... 8 3.3. Satellite Industry Segments .................................................................................... 9 3.3.1. Satellite Communications .............................................................................. -
X-Band Tt&C and K-Band Downlink Antennas For
X-BAND TT&C AND K-BAND DOWNLINK ANTENNAS FOR FUTURE LEO MISSIONS Martin Wenåker [email protected] RUAG Space AB Jan Zackrisson [email protected] Hans Ekström [email protected] Gothenburg, Sweden Johan Petersson [email protected] Patrik Dimming [email protected] P-1342182-RSE Presentation Outline . Introduction . Design Background and Heritage . X-Band TT&C Antenna . K-/Ka-Band Beacon/DDL Antenna . Conclusion 2/17 | X-BAND TT&C AND K-BAND DOWNLINK ANTENNAS FOR FUTURE LEO MISSIONS | RUAG Space | January 22, 2020 Introduction . X-Band TT&C antenna . K-/Ka-Band Beacon/DDL Antenna − Designed and manufactured as an EM − Pre-development running in parallel activity in an add-on to the original with the X-Band continuing study study − Novel dual band design 3/17 | X-BAND TT&C AND K-BAND DOWNLINK ANTENNAS FOR FUTURE LEO MISSIONS | RUAG Space | January 22, 2020 Design Background and Heritage – Ruag Space . Ruag space antenna activities started in the mid 70’s within wide coverage antennas > 300 helix antennas delivered . Other types of antennas are also designed and developed − Reflector antennas (JWST, SIRAL/Cryosat) − Array antennas (Array elements for telecom) − Slot antennas (ERS1/ERS2 , MetOp SG Scatterometer) 4/17 | X-BAND TT&C AND K-BAND DOWNLINK ANTENNAS FOR FUTURE LEO MISSIONS | RUAG Space | January 22, 2020 Design Background and Heritage – Ruag Space . Several variants are used for our helix antennas . Three main variants − Wires - shaped to a helix radiator − Etched metallic strips on substrates - shaped to a helix radiator − Machined in one piece of metal - shaped to a helix radiator 5/17 | X-BAND TT&C AND K-BAND DOWNLINK ANTENNAS FOR FUTURE LEO MISSIONS | RUAG Space | January 22, 2020 X-Band TT&C Antenna . -
Agile 3-D Beam-Steering for 60 Ghz Wireless Networks Anfu Zhou∗, Leilei Wu∗, Shaoqing Xu∗, Huadong Ma∗, Teng Wei†, Xinyu Zhang‡ ∗ Beijing Key Lab of Intell
Following the Shadow: Agile 3-D Beam-Steering for 60 GHz Wireless Networks Anfu Zhou∗, Leilei Wu∗, Shaoqing Xu∗, Huadong Ma∗, Teng Weiy, Xinyu Zhangz ∗ Beijing Key Lab of Intell. Telecomm. Software and Multimedia, Beijing University of Posts and Telecomm. y Department of Electrical and Computer Engineering, University of Wisconsin-Madison z Department of Electrical and Computer Engineering, University of California San Diego Email: fzhouanfu,layla,donggua,[email protected], [email protected], [email protected] Abstract—60 GHz networks, with multi-Gbps bitrate, are Much effort has been devoted to design agile beam-steering, considered as the enabling technology for emerging applications from the hierarchical beam scanning defined in standards [1], such as wireless Virtual Reality (VR) and 4K/8K real-time [9], to heuristic-based shortcuts [10], [11] or sensing-inspired Miracast. However, user motion, and even orientation change, can cause mis-alignment between 60 GHz transceivers’ directional solutions [12], [13]. However, these methods mainly focus on beams, thus causing severe link outage. Within the practical 3D two dimensional (2D) beam-steering, e.g., assuming a phased- spaces, the combination of location and orientation dynamics array that can steer the main beam among different angles leads to exponential growth of beam searching complexity, which within a 2D plane. In practice, the users and radios move in 3D substantially exacerbates the outage and hinders fast recovery. space; and a 60 GHz array can comprise a planar “matrix” of In this paper, we first conduct an extensive measurement to analyze the impact of 3D motion on 60 GHz link performance, antenna elements, steering the beams towards different angles in the context of VR and Miracast applications. -
Integrated Optical Phased Arrays for Beam Forming and Steering
applied sciences Review Integrated Optical Phased Arrays for Beam Forming and Steering Yongjun Guo 1,2, Yuhao Guo 1,2, Chunshu Li 1,2, Hao Zhang 1,2, Xiaoyan Zhou 1,2 and Lin Zhang 1,2,* 1 Key Laboratory of Opto-Electronics Information Technology of Ministry of Education, School of Precision Instruments and Opto-Electronics Engineering, Tianjin University, Tianjin 300072, China; [email protected] (Y.G.); [email protected] (Y.G.); [email protected] (C.L.); [email protected] (H.Z.); [email protected] (X.Z.) 2 Key Laboratory of Integrated Opto-Electronic Technologies and Devices in Tianjin, School of Precision Instruments and Opto-Electronics Engineering, Tianjin University, Tianjin 300072, China * Correspondence: [email protected] Abstract: Integrated optical phased arrays can be used for beam shaping and steering with a small footprint, lightweight, high mechanical stability, low price, and high-yield, benefiting from the mature CMOS-compatible fabrication. This paper reviews the development of integrated optical phased arrays in recent years. The principles, building blocks, and configurations of integrated optical phased arrays for beam forming and steering are presented. Various material platforms can be used to build integrated optical phased arrays, e.g., silicon photonics platforms, III/V platforms, and III–V/silicon hybrid platforms. Integrated optical phased arrays can be implemented in the visible, near-infrared, and mid-infrared spectral ranges. The main performance parameters, such as field of view, beamwidth, sidelobe suppression, modulation speed, power consumption, scalability, and so on, are discussed in detail. Some of the typical applications of integrated optical phased arrays, such as free-space communication, light detection and ranging, imaging, and biological sensing, are shown, with future perspectives provided at the end. -
Planar Pattern Reconfigurable Antenna Integrated with a Wifi System for Multipath Mitigation and Sustained High Definition Video
Planar Pattern Reconfigurable Antenna Integrated With a WiFi System for Multipath Mitigation and Sustained High Definition Video Networking in a Complex EM Environment Amit Mehta1, Shivam Gautam1, Hasanga Goonesinghe1, Arpan Pal1, Rob Lewis2 and Nathan Clow3 1College of Engineering, Swansea University, Swansea, U.K. [email protected] 2BAE Systems, Chelmsford, UK 3DSTL, Fort Halstead, UK Abstract—A planer pattern reconfigurable square loop antenna integrated in a complete wireless system is presented. II. ANTENNA CONFIGURATION The antenna is designed to operate at 5 GHz WiFi band of Fig. 1 shows the top and side view of the SLA designed IEEE 802.11 ac. The antenna under electronic switching for 5 GHz WiFi band. The Antenna structure is inspired generates four tilted beams in the four space quadrants. These four beams are moved intelligently and automatically in space from [4]. The SLA has four conducting arms, each of length using a C# program for achieving and sustaining maximum 32 mm and a track width of 1.5 mm. The square loop is possible throughput. This auto beam steering is advantageous etched on top of a Rogers 4350B (ɛr=3.66, tanδ=0.009) for scenarios where a mobile user suffers from multipath substrate having a thickness of 9.6 mm and an area of 60 fading in a complex electromagnetic environment. mm × 60 mm. The entire structure is backed by a metal ground plane. The SLA is excited at the center point of each I. INTRODUCTION arm (A, B, C and D) by four vertical probes of diameter 1.3 Indoor wireless communication in 5 the GHz WiFi band of mm which are connected to the four SMA ports (A0, B0, C0 IEEE 802.11 ac is becoming popular today due to the and D0) at the bottom of the antenna. -
Error Analysis of Programmable Metasurfaces for Beam Steering Hamidreza Taghvaee, Albert Cabellos-Aparicio, Julius Georgiou, and Sergi Abadal
1 Error Analysis of Programmable Metasurfaces for Beam Steering Hamidreza Taghvaee, Albert Cabellos-Aparicio, Julius Georgiou, and Sergi Abadal Abstract—Recent years have seen the emergence of pro- global or local reconfigurability [16]. Further, recent years grammable metasurfaces, where the user can modify the EM re- have seen the emergence of programmable metasurfaces, this sponse of the device via software. Adding reconfigurability to the is, metasurfaces that incorporate local tunability and digital already powerful EM capabilities of metasurfaces opens the door to novel cyber-physical systems with exciting applications in do- logic to easily reconfigure the EM behavior from the outside. mains such as holography, cloaking, or wireless communications. Two main approaches have been proposed for the im- This paradigm shift, however, comes with a non-trivial increase of plementation of programmable metasurfaces, namely, (i) by the complexity of the metasurfaces that will pose new reliability interfacing the tunable elements through an external Field- challenges stemming from the need to integrate tuning, control, Programmable Gate Array (FPGA) [17], [18], or (ii) by and communication resources to implement the programmability. While metasurfaces will become prone to failures, little is known integrating sensors, control units, and actuators within the about their tolerance to errors. To bridge this gap, this paper metasurface structure [19]–[22]. examines the reliability problem in programmable metamaterials Programmable metasurfaces have opened the door to dis- by proposing an error model and a general methodology for error ruptive paradigms such as Software-Defined Metamaterials analysis. To derive the error model, the causes and potential (SDMs) and Reconfigurable Intelligent Surfaces (RISs), lead- impact of faults are identified and discussed qualitatively. -
Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping: Monte Carlo Simulations
DRAFT VERSION MARCH 2, 2021 Typeset using LATEX default style in AASTeX62 Geometric Distances of Quasars Measured by Spectroastrometry and Reverberation Mapping: Monte Carlo Simulations YU-YANG SONGSHENG,1, 2 YAN-RONG LI,1 PU DU,1 AND JIAN-MIN WANG1, 2, 3 1Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 2University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, China 3National Astronomical Observatories of China, Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, China (Received ***; Revised ***; Accepted ***) ABSTRACT Recently, GRAVITY onboard the Very Large Telescope Interferometer (VLTI) first spatially resolved the structure of the quasar 3C 273 with an unprecedented resolution of 10µas. A new method of measuring ∼ parallax distances has been successfully applied to the quasar through joint analysis of spectroastrometry (SA) and reverberation mapping (RM) observation of its broad line region (BLR). The uncertainty of this SA and RM (SARM) measurement is about 16% from real data, showing its great potential as a powerful tool for precision cosmology. In this paper, we carry out detailed analyses of mock data to study impacts of data qualities of SA observations on distance measurements and establish a quantitative relationship between statistical uncertainties of distances and relative errors of differential phases. We employ a circular disk model of BLR for the SARM analysis. We show that SARM analyses of observations generally generate reliable quasar distances, even for relatively poor SA measurements with error bars of 40% at peaks of phases. Inclinations and opening angles of ◦ BLRs are the major parameters governing distance uncertainties. -
A Revision of the X-Ray Properties of MWC 297
A&A 447, 1041–1048 (2006) Astronomy DOI: 10.1051/0004-6361:20053630 & c ESO 2006 Astrophysics Chandra X-ray observations of the stellar group near the Herbig Be star MWC 297 A revision of the X-ray properties of MWC 297 F. Damiani, G. Micela, and S. Sciortino INAF - Osservatorio Astronomico di Palermo G.S.Vaiana, Piazza del Parlamento 1, 90134 Palermo, Italy e-mail: [email protected] Received 14 June 2005 / Accepted 11 October 2005 ABSTRACT We present a Chandra ACIS-I X-ray observation of the region near the Herbig early-Be star MWC 297, where we detect a tight group of point X-ray sources. These are probably physically associated to MWC 297, because of their obvious clustering with respect to the more scattered field-source population. These data are compared to earlier ASCA data with much poorer spatial resolution, from which the detection of strong quiescent and flaring emission from MWC 297 itself was claimed. We argue that this star, contributing only 5% to the total X-ray emission of the group, was probably not the dominant contributor to the observed ASCA emission, while the X-ray brightest star in the group is a much better candidate. This is also supported by the spectral analysis of the Chandra data, with reference to the ASCA spectra. We conclude that none of the X-ray data available for MWC 297 justify the earlier claim of strong magnetic activity in this star. The X-ray emission of MWC 297 during the Chandra observation is even weaker than that found in other Herbig stars with the same spectral type, even accounting for its large line-of-sight absorption. -
Uva-DARE (Digital Academic Repository)
UvA-DARE (Digital Academic Repository) Terahertz-assisted excitation of the 1.5mm photoluminescence of Er in crystalline Si Moskalenko, A.S.; Yassievich, I.N.; Forcales Fernandez, M.; Klik, M.A.J.; Gregorkiewicz, T. Publication date 2004 Document Version Final published version Published in Physical Review B Link to publication Citation for published version (APA): Moskalenko, A. S., Yassievich, I. N., Forcales Fernandez, M., Klik, M. A. J., & Gregorkiewicz, T. (2004). Terahertz-assisted excitation of the 1.5mm photoluminescence of Er in crystalline Si. Physical Review B, 70, 155201. General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:29 Sep 2021 PHYSICAL REVIEW B 70, 155201 (2004) Terahertz-assisted excitation of the 1.5-m photoluminescence of Er in crystalline Si A. -
A Design Approach of Optical Phased Array with Low Side Lobe Level and Wide Angle Steering Range
hv photonics Article A Design Approach of Optical Phased Array with Low Side Lobe Level and Wide Angle Steering Range Xinyu He, Tao Dong *, Jingwen He and Yue Xu State Key Laboratory of Space-Ground Integrated Information Technology, Beijing Institute of Satellite Information Engineering, Beijing 100095, China; [email protected] (X.H.); [email protected] (J.H.); [email protected] (Y.X.) * Correspondence: [email protected] Abstract: In this paper, a new design approach of optical phased array (OPA) with low side lobe level (SLL) and wide angle steering range is proposed. This approach consists of two steps. Firstly, a nonuniform antenna array is designed by optimizing the antenna spacing distribution with particle swarm optimization (PSO). Secondly, on the basis of the optimized antenna spacing distribution, PSO is further used to optimize the phase distribution of the optical antennas when the beam steers for realizing lower SLL. Based on the approach we mentioned, we design a nonuniform OPA which has 1024 optical antennas to achieve the steering range of ±60◦. When the beam steering angle is 0◦, 20◦, 30◦, 45◦ and 60◦, the SLL obtained by optimizing phase distribution is −21.35, −18.79, −17.91, −18.46 and −18.51 dB, respectively. This kind of OPA with low SLL and wide angle steering range has broad application prospects in laser communication and lidar system. Keywords: optical phased array; antenna array; low side lobe; wide angle steering range 1. Introduction Citation: He, X.; Dong, T.; He, J.; Xu, Optical phased array (OPA) is an array operating at optical frequency that achieves Y.