RTT TECHNOLOGY TOPIC January 2015 Defence Spectrum – the New Battleground?
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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. -
Wireless Backhaul Evolution Delivering Next-Generation Connectivity
Wireless Backhaul Evolution Delivering next-generation connectivity February 2021 Copyright © 2021 GSMA The GSMA represents the interests of mobile operators ABI Research provides strategic guidance to visionaries, worldwide, uniting more than 750 operators and nearly delivering actionable intelligence on the transformative 400 companies in the broader mobile ecosystem, including technologies that are dramatically reshaping industries, handset and device makers, software companies, equipment economies, and workforces across the world. ABI Research’s providers and internet companies, as well as organisations global team of analysts publish groundbreaking studies often in adjacent industry sectors. The GSMA also produces the years ahead of other technology advisory firms, empowering our industry-leading MWC events held annually in Barcelona, Los clients to stay ahead of their markets and their competitors. Angeles and Shanghai, as well as the Mobile 360 Series of For more information about ABI Research’s services, regional conferences. contact us at +1.516.624.2500 in the Americas, For more information, please visit the GSMA corporate +44.203.326.0140 in Europe, +65.6592.0290 in Asia-Pacific or website at www.gsma.com. visit www.abiresearch.com. Follow the GSMA on Twitter: @GSMA. Published February 2021 WIRELESS BACKHAUL EVOLUTION TABLE OF CONTENTS 1. EXECUTIVE SUMMARY ................................................................................................................................................................................5 -
ATHENA NGSO SATELLITE EXHIBIT 1 Technical Information To
REDACTED FOR PUBLIC INSPECTION ATHENA NGSO SATELLITE EXHIBIT 1 Technical Information to Supplement Form 442 and Application Narrative A.1 Scope and Purpose This exhibit supplements FCC Form 442 and contains the technical information referenced in the application narrative that is required by Parts 5 and 25 of the Commission’s rules. A.2 Radio Frequency Plan (§25.114(c)(4)) The Athena satellite will have two E-band uplinks and two E-band downlinks. The downlink emissions are nominally centered at 72 GHz and 75 GHz and the uplink emissions are nominally centered at 82 GHz and 85 GHz1. The bandwidth for both the uplinks and downlinks is 2.1852 GHz. The TT&C uplink will be conducted at 2082 MHz with an occupied bandwidth of 1.5 MHz. The TT&C downlink will be conducted at 8496.25 MHz with an occupied bandwidth of 2.3 MHz. Table A.2-1 shows the frequency ranges to be used by the Athena satellite. 1 There is the possibility that mild tuning may be performed from the planned 72, 75, 82 and 85 GHz centered carriers (e.g., 74.8 and 82.2 GHz may be used for example to mitigate any potential, mild “inter-channel interference” due to spectral regrowth issues and limited transmit- to-receive isolation). In addition, a limited number of tests, estimated at one to two dozen, may be performed with continuous wave (CW), unmodulated carriers as far out as the band edges (i.e., 71-76 GHz and 81-82 GHz) to measure the atmospheric attenuation characteristics. -
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 .............................................................................. -
Monopatch Antenna
MONOPATCH ANTENNA High efficiency, hemispherical antenna L3Harris Monopatch Antennas are designed with a unique, patent- BENEFITS pending architecture that provides greater geographical coverage The increased geographical coverage than is possible with common communications antennas. of the L3Harris Monopatch Antennas provides today’s warfighters with CLEAR LINE-OF-SIGHT SUCCESSFUL TRACK RECORD greater capabilities on the battlefield. COMMUNICATION The Monopatch Antenna has been success- > Extended range The unique design of the antenna creates fully deployed on light aircraft, helicopters > Passive operation a three-dimensional hemispherical pattern and ground vehicles with two of the most > Single radio frequency with full 360-degree azimuthal and commonly utilized commercially available (RF) interconnect 180-degree elevation coverage. MANET radios. > Lightweight The Monopatch Antenna is well suited for a Future developments for the antenna variety of missions and applications, espe- include additional L and S band versions, cially for use with relay or terminal nodes in MIMO and TSMx compatibility. mobile ad hoc network (MANET) systems. The Monopatch Antenna is currently avail- With full azimuthal and elevation coverage, able in two frequency ranges for use with the warfighter can maintain clear line-of- commercially available MANET radios: 1) sight communication in challenging terrain a dual frequency version in the L/S bands environments. In addition, loitering aircraft (NATO D/E) and 2) a wider S band version or unmanned aerial vehicles can operate at (NATO E band). greater standoff distances when deployed The antenna uses a common aluminum as air relay assets. housing and dome cover with two options for location of the TNC(F) connector. -
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 . -
Terahertz Band: the Last Piece of RF Spectrum Puzzle for Communication Systems Hadeel Elayan, Osama Amin, Basem Shihada, Raed M
1 Terahertz Band: The Last Piece of RF Spectrum Puzzle for Communication Systems Hadeel Elayan, Osama Amin, Basem Shihada, Raed M. Shubair, and Mohamed-Slim Alouini Abstract—Ultra-high bandwidth, negligible latency and seamless communication for devices and applications are envisioned as major milestones that will revolutionize the way by which societies create, distribute and consume information. The remarkable expansion of wireless data traffic that we are witnessing recently has advocated the investigation of suitable regimes in the radio spectrum to satisfy users’ escalating requirements and allow the development and exploitation of both massive capacity and massive connectivity of heterogeneous infrastructures. To this end, the Terahertz (THz) frequency band (0.1-10 THz) has received noticeable attention in the research community as an ideal choice for scenarios involving high-speed transmission. Particularly, with the evolution of technologies and devices, advancements in THz communication is bridging the gap between the millimeter wave (mmW) and optical frequency ranges. Moreover, the IEEE 802.15 suite of standards has been issued to shape regulatory frameworks that will enable innovation and provide a complete solution that crosses between wired and wireless boundaries at 100 Gbps. Nonetheless, despite the expediting progress witnessed in THz Fig. 1. Wireless Roadmap Outlook up to the year 2035. wireless research, the THz band is still considered one of the least probed frequency bands. As such, in this work, we present an up-to-date review paper to analyze the fundamental elements I. INTRODUCTION and mechanisms associated with the THz system architecture. THz generation methods are first addressed by highlighting The race towards improving human life via developing the recent progress in the electronics, photonics as well as different technologies is witnessing a rapid pace in diverse plasmonics technology. -
Qatar National Frequency Allocation Plan and Specific
Communications Regulatory Authority 2 Table of Contents Qatar National Frequency Allocation Plan and Specific Assignments Table of Contents Part 01. GENERAL INFORMATION .............................................................................................................. 1. Introduction ...................................................................................................................................................5 2. Principals of Spectrum Management .................................................................................................5 3. Definition of terms used ..........................................................................................................................7 4. How to read the frequency allocation table .................................................................................. 11 5. Radio Wave Spectrum ............................................................................................................................ 12 Part 02. FREQUENCY ALLOCATION PLAN ............................................................................................... Qatar Frequency Allocation Plan ............................................................................................................ 15 Part 03. QATAR’S FOOTNOTES ................................................................................................................... Footnotes Relevant to Qatar................................................................................................................. -
The Need for E-Band
Sky Light Research Mobile World Congress 2013 Mobile Data Backhaul: The Need For E‐Band by Emmy Johnson We’ve been hearing about the bandwidth bottleneck for years, and as LTE and more broadband intensive applications are rolled out, rapidly increasing mobile data traffic will continue to threaten the stability of the network. This is especially a critical issue in urban centers where subscribers and mobile data traffic are the most concentrated. Thanks to the increasing popularity of smart phones from the likes of Apple and Samsung, mobile data is expected to continue to grow unabated the foreseeable future. Cisco’s most recent mobile data forecast predicted that mobile data will grow 13x over the next five years, from 0.9 Exabytes per month in 2012 to 11.2 Exabytes in 2017. Thus the question becomes, how do operators keep up with this level of exponential growth while keeping mobile services on par with customers’ expectations? There are several ways that operators are combatting this growth, through innovation in both the RAN and backhaul segments of the networks. The concept of small cells through heterogeneous networks is undoubtedly the most touted modernization, and although this is new, and very promising, there are still regulatory and cost details that need to be worked out to create cost-effective ROIs, especially in the outdoor model. In the interim, another, but not as sexy, solution exists in the backhaul - replacing legacy SDH microwave links with faster, packet based millimeterwave radio links. While it’s true that fiber is the preferred mode of backhauling traffic, it is not always available and cost effective. -
UV-Vis) Absorption Vs
授課教師: Professor 吳逸謨 教授 Warning: Copyrighted by textbook publisher. Do not use outside class. Principles of Instrumental Analysis Section III – Molecular Spectroscopy Chapter 13 Introduction to Ultraviolet-Visible Absorption Spectrometry + Chapter 14 Applications of Ultraviolet-Visible Absorption Spectrometry Reference: p. 423, Visible and UV spectra, in “Organic Chemistry” textbook – Solomons, 3rd Ed] 1 Molecular Spectroscopy Ultraviolet–visible (UV-Vis) absorption vs. fluorescence Spectroscopy Ultraviolet–visible spectroscopy or ultraviolet-visible spectrophotometry (UV-Vis or UV/Vis) refers to absorption spectroscopy or reflectance spectroscopy in the ultraviolet-visible spectral region. This means it uses light in the visible and adjacent (near-UV and near- infrared [NIR]) ranges. The absorption or reflectance in the visible range directly affects the perceived color of the chemicals involved. In this region of the electromagnetic spectrum, molecules undergo electronic transitions. Fluorescence spectroscopy is based on molecular emission: The “UV-Vis” technique is complementary to fluorescence spectroscopy, in that fluorescence deals with transitions from the excited state to the ground state, while UV-Vis absorption measures transitions from the ground state to the excited state.[1] 2 (2007/3) UV-Vis Spec 儀器 -實驗課 3 FIGURE 6-3 Regions of the electromagnetic spectrum. (For UV-Vis, λ = 100~500 nm, 500~1000 nm) 4 Ch6 An Introduction to Spectrometric Methods P.135 Apendix: Chap. 7E - Radiation Transducers p. 191 Read the texts in Chap. 7 7E-2 Photon Transducers for optical spectroscopy – Barrier-Layer Photovoltaic Cells – Vacuum Phototubes – Photomultiplier tubes (PMT), picture on p. 195 – Silicon Photodiodes (Fig. 7-32) [semiconductor type] [A silicon photodiode transducer consists of a reverse- biased p-n junction.] (The latter two types of transducers are more commonly used in UV-Vis.) – We will discuss more details later. -
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.