Ka Band Satellite Communications Design Analysis and Optimisation
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Complex Radio Spectral Energy Distributions in Luminous and Ultraluminous Infrared Galaxies
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Caltech Authors - Main The Astrophysical Journal Letters, 739:L25 (6pp), 2011 September 20 doi:10.1088/2041-8205/739/1/L25 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A. COMPLEX RADIO SPECTRAL ENERGY DISTRIBUTIONS IN LUMINOUS AND ULTRALUMINOUS INFRARED GALAXIES Adam K. Leroy1,8, Aaron S. Evans1,2, Emmanuel Momjian3, Eric Murphy4,Jurgen¨ Ott3, Lee Armus5, James Condon1, Sebastian Haan5, Joseph M. Mazzarella5, David S. Meier3,6, George C. Privon2, Eva Schinnerer7, Jason Surace5, and Fabian Walter7 1 National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA 2 Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904, USA 3 National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801, USA 4 Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA 5 Spitzer Science Center, California Institute of Technology, MC 314-6, Pasadena, CA 91125, USA 6 New Mexico Institute of Mining and Technology, 801 Leroy Place, Socorro, NM 87801, USA 7 Max Planck Institut fur¨ Astronomie, Konigstuhl¨ 17, Heidelberg D-69117, Germany Received 2011 April 15; accepted 2011 June 21; published 2011 August 29 ABSTRACT We use the Expanded Very Large Array to image radio continuum emission from local luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in 1 GHz windows centered at 4.7, 7.2, 29, and 36 GHz. This allows us to probe the integrated radio spectral energy distribution (SED) of the most energetic galaxies in the local universe. -
Overview of Sensors for Applications
OVERVIEW OF SENSORS FOR APPLICATIONS Deepak Putrevu Head, MTDD/AMHTDG EM SPECTRUM Visible 0.4-0.7μm Near infrared (NIR) 0.7-1.5μm Optical Infrared Shortwave infrared (SWIR) 1.5-3.0μm Mid-wave infrared (MWIR) 3.0-8.0μm (OIR) Region Longwave IR(LWIR)/Thermal IR(TIR) 8.0-15μm Far infrared (FIR) Beyond15μm Gamma Rays X Rays UV Visible NIR SWIR Thermal IR Microwave P-band: ~0.25 – 1 GHz Microwave Region L-band: 1 -2 GHz S-band: 2-4 GHz •Sensors are 24x365 C-band: 4-8 GHz •Signal data characteristics X-band: 8-12 GHz unique to the microwave region of the EM spectrum Ku-band: 12-18 GHz K-band: 18-26 GHz •Response is primarily governed by geometric Ka-band: 26-40 GHz structures and hence V-band: 40 - 75 GHz complementary to optical W-band: 75-110 GHz imaging mm-wave: 110 – 300GHz Basic Interactions between Electromagnetic Energy and the Earth’s Surface Incident Power reflected, ρP Reflectivity: The fractional part of the radiation, P incident radiation that is reflected by the surface. Power absorbed, αP Absorptivity: the fractional part of the = Power emitted, εP incident radiation that is absorbed by the surface. Power transmitted, τP Emissivity: The ratio of the observed flux emitted by a body or surface to that of a P= Pr + Pt + Pa blackbody under the same condition. 푃 푃 푃 푟 + 푡 + 푎 = 1 푃 푃 푃 Transmissivity: The fractional part of the ρ + τ + α =1 radiation transmitted through the medium. At thermal equilibrium, absorption and emission are the same. -
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 .............................................................................. -
A Layman's Interpretation Guide L-Band and C-Band Synthetic
A Layman’s Interpretation Guide to L-band and C-band Synthetic Aperture Radar data Version 2.0 15 November, 2018 Table of Contents 1 About this guide .................................................................................................................................... 2 2 Briefly about Synthetic Aperture Radar ......................................................................................... 2 2.1 The radar wavelength .................................................................................................................... 2 2.2 Polarisation ....................................................................................................................................... 3 2.3 Radar backscatter ........................................................................................................................... 3 2.3.1 Sigma-nought .................................................................................................................................................. 3 2.3.2 Gamma-nought ............................................................................................................................................... 3 2.4 Backscatter mechanisms .............................................................................................................. 4 2.4.1 Direct backscatter ......................................................................................................................................... 4 2.4.2 Forward scattering ...................................................................................................................................... -
Federal Communications Commission FCC 20-158
Federal Communications Commission FCC 20-158 Before the Federal Communications Commission Washington, D.C. 20554 In the Matter of ) ) Amendment of Parts 2 and 25 of the Commission’s ) IB Docket No. 20-330 Rules to Enable GSO Fixed-Satellite Service ) (Space-to-Earth) Operations in the 17.3-17.8 GHz ) RM-11839 (terminated) Band, to Modernize Certain Rules Applicable to ) 17/24 GHz BSS Space Stations, and to Establish ) Off-Axis Uplink Power Limits for Extended Ka- ) Band FSS Operations. ) NOTICE OF PROPOSED RULEMAKING Adopted: November 18, 2020 Released: November 19, 2020 Comment Date: 30 days after date of publication in the Federal Register Reply Comment Date: 45 days after date of publication in the Federal Register By the Commission: Chairman Pai issuing a statement. TABLE OF CONTENTS Heading Paragraph # I. INTRODUCTION .................................................................................................................................. 1 II. BACKGROUND .................................................................................................................................... 4 A. Current Allocations and Use of the 17.3-17.8 GHz Band ................................................................ 4 B. SES Americom Petition for Rulemaking ......................................................................................... 7 III. DISCUSSION ...................................................................................................................................... 12 A. Proposed GSO FSS Allocation in -
Spectrum-Secure Communications for Autonomous Uas/Uav Platforms
SPECTRUM‐SECURE COMMUNICATIONS FOR AUTONOMOUS UAS/UAV PLATFORMS Andrew L. Drozd ANDRO Computational Solutions, LLC Advanced Applied Technology Division Rome, NY 26 October 2015 Secure UAS Communications Panel 1 Unclassified // Distribution A: Unlimited Distribution Topics • ANDRO Technology Summary • Background of key technical issues related to UAS/UAV spectrum, safety, security and airspace integration . Potential spectrum contention and management issues Frequencies Used for Remote Control A Typical UAV Link UAS Integration to NAS . Spectrum, Security and RTCA‐228 Relevant Issues • Conclusion 2 ANDRO Technology / Application Spaces C2 (Cross‐layer RF Cyber‐Spectrum RF Resource Exploitation Management & Communications / Cyber Security) (Wireless Anti‐ EMI Avoidance Dynamic Spectrum Hacking) (Coexistence) Access/Sharing Spectrum Pre‐test M&S Detect & Avoid (Spectral Contention) Cyber‐Spectrum Exploitation / Secure Wireless Comms / Cognitive Radio Networking / 3 Trusted Routing Technologies for Autonomous Systems (RF sensor‐edge processing) BACKGROUND • ANDRO has access to AFRL’s Stockbridge Controllable Contested Environment Facility and Griffiss FAA UAS Test Site Rome, NY for communications up/down‐link experiments with large or small UAS/UAV platforms. • Member of Northeast UAS Airspace Integration Research Alliance (NUAIR). • Our overall focus is on assessing, pre‐certifying or assuring the following for C2/CDL, payload data link (VDL) and other future RF comms technologies: – RF spectrum collision/contention – Coexistence – Cyber -
Position Paper on Interference with Satellite Communications
Position Paper on Interference in C-band by Terrestrial Wireless Applications to Satellite Applications Adopted by International Associations of the Satellite Communications Industry Position Statement: National administrations should recognize the potential for massive disruptions to C band satellite communications, radar systems and domestic microwave links, if spectrum is inappropriately allocated to, and frequencies inappropriately assigned for, terrestrial wireless applications in the C- band (specifically 3.4 – 4.2 GHz). Executive summary: Satellite communications technology in the C band is used for broadcasting television signals, Internet delivery, data communication, voice telephony and aviation systems. The satellite systems that operate in the 3.4-4.2 GHz band (C band) are suffering substantial interference, to the point of system failure, in places where national administrations are allowing Broadband Wireless Access systems like wi-fi and wi-max to share the same spectrum bands already being used to provide satellite services. The same will happen if 3G and the planned 4G mobile systems (also referred to as IMT systems) are allowed to use the frequencies used in the C band for satellite downlink services as is being contemplated by some administrations in the context of WRC-07 agenda item 1.4. To eliminate this harmful interference, operators of satellite earth stations and users of satellite communications services have united to communicate their positions and technical requirements to national and international telecommunications regulators. Regulators and radio frequency managers need to allocate spectrum in ways that recognize the reality of harmful interference and validate the right of incumbent operators to operate, and their customers to enjoy their services, without disruption by new users. -
The Space Mission at Kwajalein
THE SPACE MISSION AT KWAJALEIN The Space Mission at Kwajalein Timothy D. Hall, Gary F. Duff, and Linda J. Maciel The United States has leveraged the Reagan The Reagan Test Site (RTS), located on Kwajalein Atoll in the central western Test Site’s suite of instrumentation radars and » Pacific, has been a missile testing facility its unique location on the Kwajalein Atoll to for the United States government since the enhance space surveillance and to conduct early 1960s. Lincoln Laboratory has provided technical space launches. Lincoln Laboratory’s technical leadership for RTS from the very beginning, with Labo- ratory staff serving assignments there continuously since leadership at the site and its connection to May 1962 [1]. Over the past few decades, the RTS suite the greater Department of Defense space of instrumentation radars has contributed significantly to community have been instrumental in the U.S. space surveillance and space launch activities. The space-object identification (SOI) enterprise success of programs to detect space launches, was motivated by early data collected with the Advanced to catalog deep-space objects, and to provide Research Projects Agency (ARPA)-Lincoln C-band exquisite radar imagery of satellites. Observables Radar (ALCOR), the first high-power, wide- band radar. Today, RTS sensors continue to provide radar imagery of satellites to the intelligence community. Since the early 1980s, RTS radars have provided critical data on the early phases of space launches out of Asia. RTS also supports the Space Surveillance Network’s (SSN) catalog-maintenance mission with radar data on high-priority near-Earth satellites and deep-space satellites, including geosynchronous satellites that are not visible from the other two deep-space radar sites, the Millstone Hill radar in Westford, Massachusetts, and Globus II in Norway. -
Ultra-Wideband WDM Optical Network Optimization
hv photonics Article Ultra-Wideband WDM Optical Network Optimization Stanisław Kozdrowski 1,* , Mateusz Zotkiewicz˙ 1 and Sławomir Sujecki 2,3 1 Department of Computer Science, Faculty of Electronics, Warsaw University of Technology, Nowowiejska 15/19, 00-665 Warsaw, Poland; [email protected] 2 George Green Institute, the University of Nottingham, Nottingham NG7 2RD, UK; [email protected] 3 Telecommunications and Teleinformatics Department, Wroclaw University of Science and Technology, 50-370 Wroclaw, Poland * Correspondence: [email protected] Received: 6 December 2019; Accepted: 13 January 2020; Published: 21 January 2020 Abstract: Ultra-wideband wavelength division multiplexed networks enable operators to use more effectively the bandwidth offered by a single fiber pair and thus make significant savings, both in operational and capital expenditures. The main objective of this study is to minimize optical node resources, such as transponders, multiplexers and wavelength selective switches, needed to provide and maintain high quality of network services, in ultra-wideband wavelength division multiplexed networks, at low cost. A model based on integer programming is proposed, which includes a detailed description of optical network nodal resources. The developed optimization tools are used to study the ultra-wideband wavelength division multiplexed network performance when compared with the traditional C-band wavelength division multiplexed networks. The analysis is carried out for realistic networks of different dimensions and traffic demand sets. Keywords: ultra-Wideband WDM system design; optical network optimization; CDC-F technology; optical node model; network congestion; Linear Programming (LP); Integer Programming (IP) 1. Introduction Optical networks based on Wavelength Division Multiplexing (WDM) technology that operate within the C-band are near the limit of their capacity. -
Low-Cost Ka-Band Cloud Radar System for Distributed Measurements Within the Atmospheric Boundary Layer
remote sensing Letter Low-Cost Ka-Band Cloud Radar System for Distributed Measurements within the Atmospheric Boundary Layer Roberto Aguirre 1 , Felipe Toledo 2 , Rafael Rodríguez 3,4, Roberto Rondanelli 5,6,7 , Nicolas Reyes 1,8 and Marcos Díaz 1,6,* 1 Electrical Engineering Department, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago 8370451, Chile; [email protected] (R.A.); [email protected] (N.R.) 2 Laboratoire de Météorologie Dynamique, École Polytechnique, Institut Polytechnique de Paris, 91128 Palaiseau, France; [email protected] 3 Institute of Electricity and Electronics, Facultad de Ciencias de la Ingeniería, Universidad Austral, General Lagos 2086, Valdivia 5110701, Chile; [email protected] 4 CePIA, Astronomy Department, Universidad de Concepción, Casilla 160-C, Concepción 4030000, Chile 5 Department of Geophysics, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago 8370449, Chile; [email protected] 6 Space and Planetary Exploration Laboratory, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago 8370451, Chile 7 Center for Climate and Resilience Research, Faculty of Physical and Mathematical Sciences, University of Chile, Santiago 8370449, Chile 8 Max Planck Institute for Radioastronomy, Auf dem Hugel 69, 53121 Bonn, Germany * Correspondence: [email protected]; Tel.: +56-2-2978-4204 Received: 18 June 2020; Accepted: 31 August 2020; Published: 3 December 2020 Abstract: Radars are used to retrieve physical parameters related to clouds and fog. With these measurements, models can be developed for several application fields such as climate, agriculture, aviation, energy, and astronomy. In Chile, coastal fog and low marine stratus intersect the coastal topography, forming a thick fog essential to sustain coastal ecosystems. -
ITU Regulations for Ka-Band Satellite Networks
ITU Regulations for Ka-band Satellite Networks Jorn Christensen, Ph.D. AsiaSat Almaty, September 5-7, 2012 Ka-band Allocations Ka-band not defined in the Radio Regulations Will take as Ka-band range 17.3 to 31 GHz. Both GSO and NGSO satellites in Ka-band Many different services share Ka-band Many allocated services do not share well For example, terrestrial and satellite services using ubiquitous terminals do not share well The administration decides which services to favor on its territory High Throughput Satellites Not only in Ka-band Characterized by: - many small beams (up to about 200) with high gain - high gain of the small spot beams allows for closing the link to relatively small user terminals - allows for multiple frequency re-use Due to the high frequency re-use factor (up to 20) the resulting throughput of the satellite is in the range of 100s of Gigabits per second (Gbps). Spot beams of Anik F2 and WildBlue (WB-1) Ka-band Frequencies for HTS Most HTS typically file for 3.5 GHz bandwidth in the following Ka- bands: 27.5 – 31 GHz uplink 17.7 – 21.2 GHz downlink This range of frequencies is subject to various regulatory procedures. One way to divide these bands is as follows: a) Bands identified for High-Density FSS b) Bands used by many administrations for FS including LMDS c) Bands where GSO and non-GSO satellites have equal rights d) Bands where equivalent pfd (epfd) applies e) Military bands Simplified summary of Ka-band satellite allocations Annex 1 Simplified summary of Ka-band satellite frequency allocations for communication satellite networks UPLINK DOWNLINK 27.0 GHz----------------------------------------------------- ----17.3 GHz FSS uplink in In Regions 1 and 3 band 17.3-18.1 GHz Region 2 and 3 only limited to feeder links for BSS. -
A Comparison and Analysis of KA-Band Radar Vs. X-Band Radar
FHWA-NJ-2007-022 A Comparison and Analysis of KA-Band Radar vs. X-Band Radar FINAL REPORT December 2007 Submitted by Dr. Allen Katz Prof. Electrical/Computer Engineering The College of New Jersey NJDOT Research Project Manager Edward S. Kondrath In cooperation with New Jersey Department of Transportation Bureau of Research And U.S. Department of Transportation Federal Highway Administration DISCLAIMER STATEMENT “The contents of this report reflect the views of the author(s) who is (are) responsible for the facts and the accuracy of the data presented herein. The contents do not necessarily reflect the official views or polices of the New Jersey Department of Transportation or the Federal Highway Administration. This report does not constitute a standard, specification, or regulation.” 2 F TECHNICAL REPORT STANDARD TITLE PAGE 1. Report No. 2.Government Accession No. 3. Recipient’s Catalog No. FHWA-NJ-2007-022 4. Title and Subtitle 5. Report Date A Comparison and Analysis of December 2007 KA-Band Radar vs. X-Band Radar 6. Performing Organization Code 7. Author(s) 8. Performing Organization Report No. Dr. Allen Katz 9. Performing Organization Name and Address 10. Work Unit No. The College of New Jersey PO Box 7718 11. Contract or Grant No. Ewing, NJ 08628-0718 12. Sponsoring Agency Name and Address 13. Type of Report and Period Covered New Jersey Department of Transportation PO 600 14. Sponsoring Agency Code Trenton, NJ 08625 15. Supplementary Notes 16. Abstract This project focuses on the New Jersey State Police commitment to highway safety by enforcing posted speed limits. Effective enforcement of speeding statutes requires measured speed to be accurate and state of the art.