Plenary Round Table Interoperable Space and Enabling Technologies and Capabilities The State of Key Technologies that Ease Interoperability Between Government.

Slides:



Advertisements
Similar presentations
Operational Amplifiers
Advertisements

Satellite Communication
Reverse IMD Performance Presented by: Chris Brinton Advisors: Dr. Allen Katz Dave McGee The College of New Jersey (Ewing, NJ) Linearizer Technology, Inc.
Slide 1 Weidong Gao(Potevio) Project: IEEE P Working Group for Wireless Personal Area Networks (WPANs) Submission Title: Injection Locked Receiver.
Pseudo-Random Noise Radar n Prototype Design –Small inexpensive “correlation-type” receiver –Digitally produced Pseudo-Random Noise (PRN) for transmitter.
Faisal Abedin Advisor: Dr. Mohammod Ali
To produce the highest quality, cost effective microwave products to meet our customers’ needs with either Dorado standard catalog devices or custom products.
RF Wakeup Sensor – On-Demand Wakeup for Zero Idle Listening and Zero Sleep Delay.
Satellite Communication
RF MEMS devices Prof. Dr. Wajiha Shah. OUTLINE  Use of RF MEMS devices in wireless and satellite communication system. 1. MEMS variable capacitor (tuning.
ECE1352F University of Toronto 1 60 GHz Radio Circuit Blocks 60 GHz Radio Circuit Blocks Analog Integrated Circuit Design ECE1352F Theodoros Chalvatzis.
 Defining the RF jamming system and showing the importance and need of using it in many places.  Giving a complete RF jamming system design based on.
NASA Perspective on Optical Link Study Group Findings John Rush Director, Technology & Standards Division NASA Space Communication and Navigation Office.
VSOP-2 Ground Link Station - Tracking Station Requirements - National Astronomical Observatory of Japan Y. Kono.
An Enhanced/Permanent Amateur Radio Station Proposal L. McFadin, W5DID K. Banke N6IZW
Microwave semiconductor devices
High Electron Mobility Transistors (HEMT)
Microwave Engineering, 3rd Edition by David M. Pozar
New MMIC-based Millimeter-wave Power Source Chau-Ching Chiong, Ping-Chen Huang, Yuh-Jing Huang, Ming-Tang Chen (ASIAA), Shou-Hsien Weng, Ho-Yeh Chang (NCUEE),
Microwave Traveling Wave Amplifiers and Distributed Oscillators ICs in Industry Standard Silicon CMOS Kalyan Bhattacharyya Supervisors: Drs. J. Mukherjee.
Presenter: Chun-Han Hou ( 侯 鈞 瀚)
1 學生 : 李國彰 指導教授:林志明 A Fully Matched High Linearity 2- w PHEMT MMIC Power Amplifier for 3.5 GHz Application ( IEEE MICROWAVE AND WIRELESS COMPONENTS LETTERS,
Final Project in RFCS in the MINT Program of the UPC by Sven Günther
18/10/20151 Calibration of Input-Matching and its Center Frequency for an Inductively Degenerated Low Noise Amplifier Laboratory of Electronics and Information.
Codan 5700 Series C-Band Transceiver Technical Overview.
An Ultra-low Voltage UWB CMOS Low Noise Amplifier Presenter: Chun-Han Hou ( 侯 鈞 瀚 ) 1 Yueh-Hua Yu, Yi-Jan Emery Chen, and Deukhyoun Heo* Department of.
MMIC design activities at ASIAA Chau-Ching Chiong, Ping-Chen Huang, Yuh-Jing Huang, Ming-Tang Chen (ASIAA), Ho-Yeh Chang (NCUEE), Ping-Cheng Huang, Che-Chung.
Travelling Wave Tube For Broadband amplifier helix TWTs (proposed by Pierce and others in 1946 ) are widely used For High average power purposes the.
Sanae Boulay, Limelette, Nov 05 th 20091/20 S. Boulay, B. Boudjelida, A. Sharzad, N. Ahmad, M. Missous Novel Ultra Low Noise Amplifiers based on InGaAs/InAlAs.
Amplifiers Amplifier Parameters Gain = Po/Pi in dB = 10 log (Po/Pi)
1. Physical Transmission Transmission Media Wire (guided) Coaxial cable Twisted Pair UTP STP Fiber Optic Wireless (unguided) Radio waves Microwave Infrared.
Communication, Navigation, and Networking reConfigurable Testbed (CoNNeCT): An International Space Station National Lab Ann P. Over Project Manager NASA.
ECE 4710: Lecture #37 1 Link Budget Analysis  BER baseband performance determined by signal to noise ratio ( S / N ) at input to detector (product, envelope,
Device Development for NASA Space Communications Novel Power Combiner for Solid State Power Amplifiers Andrew Abraham Edwin Wintucky Communications, Instrumentation,
Basic Satellite Communication (3) Components of Communications Satellite Dr. Joseph N. Pelton.
Ka and W Band TE 01 Gyro-Devices Stutend : Yo-Yen Shin Advisor : Yi Sheng Yeh Department of Electrical Engineering, Southern Taiwan University of Technology,
3-Stage Low Noise Amplifier Design at 12Ghz
BY….. SU BMITTED TO… MANVENDRA SINGH Mr. R.A. AGARWALA B.TECH (3 rd YEAR) Mrs. SHILPI PATIL ELECTRONICS & COMM. B.B.D.I.T GHAZIABAD.
PRESENTED BY : P:MARREDDY07681A0453 WIRELESS SYSTEM WIRELESS SYSTEM.
Introduction: Basic Concept of RF and Microwave circuits
Table 1. The Comparison of Li-Fi & Wi-Fi & WiMAX and Bluetooth
Power Amplifiers Anurag Nigam Non-Constant Envelope Signal Peak Power
RF components Design for the Internet Over TV Band Adaptor
Adam Schlesinger NASA – JSC November 3, 2011
EARTH SEGMENT & SPACE LINK
Communication 40 GHz Anurag Nigam.
SatCOM Products Wavelab Inc’s Introduction.
A High-Dynamic-Range W-band
Visit for more Learning Resources
Internet Over TV Bandwidth
Development of X-band 50MW klystron in BVERI
Contacts:- For enquiries, please contact the following members:
Introducing: LTC5553 A 3GHz to 20GHz Microwave Mixer with Integrated LO Buffer ©2017 Analog Devices, Inc. All rights reserved.
Power Amplifiers Anurag Nigam Non-Constant Envelope Signal Peak Power
NASA Perspective on Optical Link Study Group Findings
Presentation On “Overview of Satellite Communication System”
Overview High-Powered Amplifier Exciter Receiver Oscillators
Variable Gain CMOS LNA MOREIRA E SILVA, Paulo Marcio, DE SOUSA, Fernando Rangel Introduction Simulation.
Jessore University of Science and Technology,
A 3.1–10.6 GHz Ultra-Wideband CMOS Low Noise Amplifier With Current-Reused Technique Microwave and Wireless Components Letters, IEEE Volume 17,  Issue.
Adam Schlesinger NASA – JSC November 3, 2011
A Novel 1. 5V CMFB CMOS Down-Conversion Mixer Design for IEEE 802
Wireless Networking Radio frequency constraints Current standards
Physical Transmission
5.8GHz CMOS 射頻前端接收電路 晶片設計實作 5.8GHz CMOS Front-End Circuit Design
Communication Systems.
Tri-Band RF Jamming System
University of California
January 2005 Project: IEEE P Working Group for Wireless Personal Area Networks (WPANs) Submission Title: [Band plan and PRF considerations] Date.
S21 (at center frequency) 19 dB
Presentation transcript:

Plenary Round Table Interoperable Space and Enabling Technologies and Capabilities The State of Key Technologies that Ease Interoperability Between Government and Commercial Networks Rainee N. Simons, Ph.D. Program Officer, Planetary Science Division Science Mission Directorate, NASA HQ, Washington, DC 20024 (On Detail from NASA Glenn Research Center) Mobile: (216) 789-0237; Email: Rainee.N.Simons@nasa.gov 25th Ka and Broadband Communications Conference Sorrento, Italy, September 30, 2019

Outline Gaps Being Addressed Power Amplifiers LNAs Wideband Front-Ends CP Power Amplifiers LNAs SDR Waveforms Wideband Front-Ends Gaps Being Addressed

Power and Frequency Flexible Ka-band Traveling-Wave Tube Amplifiers Up to 250-W for Space Communications L3 Model 999HA TWT - WR-28 waveguide ports in a conduction cooled package Saturated performance over 5-GHz bandwidth Saturated performance over 9-GHz bandwidth Saturated performance over 31.8 to 32.3 GHz Wide Bandwidth Enables: (a) Cognitive Communications & Interoperability Between Networks, & (b) LEO User Spacecraft to communicate with TDRSS (25.25-27.5 GHz) and with GEO Commercial Communications Satellites (27.5-31.0 GHz)

Power and Frequency Flexible Traveling-Wave Tube Amplifiers with WR-34 & WR-22 Waveguide Ports for Space Communications L3 EDD Model 999HA K-Band TWTA with WR-34 Waveguide Ports 18.0 to 26.5 GHz L3 EDD Model 2000HDA-A16 Q-Band TWTA with WR-22 Waveguide Ports 33.0 to 50.0 GHz RF Power Amplification Flexible Across the 18.0 to 40 GHz Range Enables LEO User Spacecraft to be Interoperable and Downlink Data Either to NASA NEN Stations (25.5-26.5 GHz) or to Commercial Ground Stations (18-21.2 GHz) Q-band Enables Downlinking Data to Commercial Ground Stations

Ultra-Broadband Low Noise Amplifiers for Flexible Wideband Receiver Front End Circuit* is fabricated using 0.15 micron GaAs E-mode pseudomorphic high-electron-mobility transistor (pHEMT) process Frequency range: 1 to 40 GHz (DC to Ka-Band) Average gain: 26.5 dB Input/output return loss: better than 9 dB Noise figure: 2.8 to 3.9 dB Peak OP1 dB: 4.9 to 12.7 dB Supply voltage: 4.5 V Chip area: 1.06 mm2 *J. Hu and K. Ma, “A 1-40 GHz LNA MMIC Using Multiple Bandwidth Extension Techniques,” IEEE Microwave & Wireless Components Lett., vol. 29, no. 5, pp. 336-338, May 2019.

Front End Design/Development & SDR Waveforms for Interoperability NASA & Harris Wideband Front-End Development Cooperative Agreement Historically, NASA & Harris developed the 1st SDR – flew 7 years on ISS & supported the SCaN Testbed Harris now offers a new product line of SDRs for satcom Wideband Front-End Design Goals: Cover frequencies from 18.3-34.7 GHz Bandwidth > 500 MHz Interoperability between Government and commercial satellite networks with the selection of appropriate waveform and modulation Capability to port a wide variety of waveforms Compatibility of Up & Down Converter with AppSTAR Micro SDR in 3U form factor Leverages components developed through IR&D Plan to deliver a prototype by early CY2020 Harris SDR transceiver to fly on STPSat-6 & support the NASA LCRD experiment