Ground Station for Satellite Operation (CySat) May 10-07 Client: Matthew Nelson Advisor: John Basart Team: Karl Deakyne, SungHo Yoon, Luke Olson Cyclone.

Slides:



Advertisements
Similar presentations
Stratagem EH4 Field Evaluation of Data Quality.
Advertisements

Noise Lecture 6.
Localization with RSSI Method at Wireless Sensor Networks Osman Ceylan Electronics Engineering PhD Student, Istanbul Technical University, Turkiye
Analog Basics Workshop RFI/EMI Rejection
RF Circuit Design Chris Fuller /7/2012.
Software Defined Radio Testbed Team may11-18 Members: Alex Dolan, Mohammad Khan, Ahmet Unsal Adviser: Dr. Aditya Ramamoorthy.
By: Deepika Thakur. Conceptual design of the Communication Subsystem.
08/16/01. Link Budgets for Cellular Networks Presented by Eric Johnson.
PRIME Antenna Inc. Antenna Test Team Adam Straubinger Alan Condino Thanh Hong Ronnie Berg Sam Gregorio.
08/16/01.
ECE 5233 Satellite Communications
COMMUNICATION SYSTEM EECB353 Chapter 2 Part IV AMPLITUDE MODULATION Dept of Electrical Engineering Universiti Tenaga Nasional.
Checking Antenna Systems
 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.
Satellite Digital Audio Radio Service Receiver Front-End (SDARS)
General Licensing Class Your Receiver Your organization and dates here.
Automatic Directional Antenna Azimuth Controller Cezanne Camacho, Andrew Curtis, and Tyler Bowen Department of Electrical Engineering, University of Washington,
RF Equipment AFFORDABLE, SIMPLE, RELIABLE.. Compact and Reliable All of our equipment is packaged in sturdy powder- coated aluminum cases just a few inches.
Meteor Receiver Olajide Durosinmi Hugh Kinsel Kenny Mills Austin Pierce Nick Stelmashenko October 21, 2009.
Bi-Directional RF Data Communication A Robot Control Device Team BDRFC.
Agenda Introduction Overview of RF Design Process Case Study: RF Front-End  Low-Noise Amplifier (LNA)  Duplexer  Power Amplifier Measurement for Design.
Namaste Project 3.4 GHz Interference Study Preliminary document - Work in Progress updated The intent of this study is to collect data which may.
Ongo 2-C Radio Telescope
2.4 GHz CubeSat Communications System Robert Bui Communications Subsystem Lead.
Power Control System for a Concrete Durability Test Cabinet – Phase 2 Jacob Jameson Madhav Kothapalli Thomas Persinger Andrew Versluys.
Summary Thus far we have: ECE 4710: Lecture #39
DEC RADIO TELESCOPE Dane Coffey, Charles Wakefield, Stephanie Kaufman, Seung Hyun Song.
1 Capstone Design Project Silent Alarm System Students: Su Huang & Fenghua Chen Advisor: Professor James Hedrick March 03, 2007.
Lab Group L2Bx EECE 380 – Electrical Engineering Design Studio (Spring 2014) 1 Spectrum Analyzer Michael Halpenny-Mason, Presenter 2, Presenter 3, Presenter.
BI day 2011 T Bogey CERN BE/BI. Overview to the TTpos system Proposed technical solution Performance of the system Lab test Beam test Planning for 2012.
Senior Project – Electrical Engineering Amateur Radio Repeater Daniel Harkenrider Advisor – Professor James Hedrick Abstract There are a number.
SSOL: Radio Telescope IRP Presentation Team Ongo-02c April 26, 2006 Client: Iowa Space Grant Consortium Advisor: Dr. Basart.
Abstract The purpose of this project is to create a fully functional 8.5 meter radio telescope which can receive signals at a frequency of 1.42 GHz. The.
Codan 5700 Series C-Band Transceiver Technical Overview.
For Electric Vehicle Team Members Pramit Tamrakar - EE Jimmy Skadal - EE Hao Wang - EE Matthew Schulte - EE William Zimmerman - EE Advisor Ayman Fayed.
University of Kansas 2004 ITTC Summer Lecture Series Network Analyzer Operation John Paden.
Channels of Communication HL – Option F.4 Mr. Jean.
Abstract The goal of our project is the continued restoration of the 8.5 meter dish at the Fick observatory in Boone, IA. Before restoration began, the.
Meteor Receiver Andrew Thoni Charlie Hunter Greg Watkins Nick Nicholson Will Marshall.
System noise temperature and G/T ratio
Harmonic Mixers for Spectrum Analyzers
PC Based Spectrum Analyzer April 29, 2003 May03-10 Faculty Advisor: Dr. DJ Chen Michael Cain Paul Heil Eric Rasmussen Aung Thuya Client: Teradyne Inc.
Abstract The purpose of this project is to design a high-performance FPGA-controlled amplifier for Teradyne Corporation. This will constitute Phase IV.
RF low level control & synchronization A. Gallo, M. Bellaveglia, L. Cacciotti SPARC review committee – ENEA Frascati – 16/11/2005.
EMC issues for cabling and racks layout design. (Belle II – Grounding) F.Arteche.
RF Presentation.
Evaluating Active Components Presenter: Blaine Davidge Westell Technologies 4/8/161Copyright © 2016 | CIBET | All rights reserved.
Spectrum Policy Technological Solutions for Policy Problems Allen Petrin ©2003 all rights reserved 1 System Architecture for a Dynamic-Spectrum.
ECEN5533 Modern Communications Theory Lecture #91 February 2016 Dr. George Scheets n Read 5.6 n Problems 5.14 – 5.16 n Exam #1, 10 February.
Telecommunication Laboratories Jia-Lun Wang, Shinn-Yan Lin, Yi-Jiun Huang, Huang-Tien Lin and Chia-Shu Liao APMP 2012 November 26, 2012 MSL Wellington,
Developing a Sonar Sub-System for a Submarine to Obtain Time Delays between Received Signals Gary Eades Dy Eang Diana Fuertes 12/04/2007 ECE4884 L03 Dr.
Get the Best from your Masthead Preamp Ian White GM3SEK Click to view the slides.
Cosmic Microwave Technology, Inc.
Beam Secondary Shower Acquisition System: Front-End RF Design
RFI Protection Activities in IAA RAS
RF components Design for the Internet Over TV Band Adaptor
(4) Filters.
RFI Protection Activities in IAA RAS
Lets Design an LNA! Anurag Nigam.
CT-474: Satellite Communications
Understanding Receiver Specifications
Overview Calibration Exciter Receiver Oscillators
Lesson 11: Transducer Electrical Interfaces
Tri-Band RF Jamming System
Image Acquisition and Processing of Remotely Sensed Data
CH-6 CABLE TV.
AM-7026 Down Converter-Receiver
FPGA Controlled Amplifier Module May 06-14
Near Field Probe Configuration
Presentation transcript:

Ground Station for Satellite Operation (CySat) May Client: Matthew Nelson Advisor: John Basart Team: Karl Deakyne, SungHo Yoon, Luke Olson Cyclone Satellite (CYSAT)

Project Plan  Overall goal: Ground Station for CySat Team Fick Observatory, Dish Antenna High sensitivity receiving Automatic Tracking  Previous Team: Dish control from computer Build 440 MHz Sub reflector Rotary Encoders for tracking dish position  Our team: Ensure strength and signal to noise ratio of received signal is adequate Tracking

3 Requirements  Functional The system shall be able to receive a signal that is sent from an orbiting satellite with a sent power of 1W (or 3 dBm) and the signal should be easily recognizable by a standard radio located in the observatory The system shall be able to automatically track an orbiting satellite  Non-Functional The system shall fit inside the dish The system shall be weatherproof

Project Plan  Work Breakdown Luke ○ Develop Tracking Software SungHo, Karl ○ Design and Build Front-End

Schedule

Design – Front End  Calculations – Without modification  Analysis: Signal-to-Noise Ratio = dBm – ( dBm) = 8.68 dB (Input power) - (Sensitivity) = 6.99 dBm These numbers do not yet meet the specifications!  Solution: Front-End Box for amplification Received power at the satellite dish (worst case) dBm (by link budget) Coax Cable (Belden 9913 (RG-8), 200ft)-5.8dB/200ft(Insertion Loss) Radio Input Power dBm Power of Radio Sensitivity (Standard Radio)-121.9dBm

7 Design Front-End Progression 3 First Full Parts Design

Design Front-End Progression Design Before Purchasing Parts

9 Band Pass Filter  Problems with BPFs Commercial filters not perfect for our range Custom filter not immediately available  Solutions Considered putting LPF and HPF in series Advised advised to continue without BPFs, but to leave room for eventual installation  Effects Radio filters around center frequency Pre-filtering desirable, but not necessary Slight decrease in SNR, but this is negligible

10 Design Front End Progression 5 Final Design Apr 2010

Design – Tracking Software  Requirement: Automatically track an orbiting satellite Solution: ○ Pull azimuth and elevation from Ham Radio Deluxe ○ Track the position of the dish with existing rotary encoders ○ Move dish through an Ethernet connection with the motor control microcontroller

Design – Tracking Software

Implementation –Tracking Software  Java Based Application GUI ○ Allows user to manually control dish, track a satellite, and set calibration settings Data Monitoring ○ Two Threads DDEThread: Continuously pulls azimuth and elevation from Ham Radio Deluxe, using Dynamic Data Exchange DishPositionThread: Monitors the rotary encoders to track the azimuth and elevation of the dish Calibration ○ Automatic Calibration to ensure accurate tracking

Implementation – Tracking Software

15 Implementation – Front End 6

16 Required Specifications  Filter Design Frequency, 440 MHz Filters out harmonics Low power  Switch Must work at 440 MHz, minimal losses High Power Rating (~10W) Electrically controlled  Radio High Sensitivity Low Cost  Amplifier 440 MHz Low Noise Amplifier Low noise figure (<3) Moderate gain (~20dB)

17 Device Specifications  ZX60-33LN+ (LNA) L ow noise Amplifier Low noise figure = 1.1 Gain = MHz  881-CCR-33S6O (Switch) Loss at 440 MHz <.4 dB Power Rating at 440 MHz = 100W CW Electrically controlled  Filter Too costly to get device within specification  Radio Too costly for budget, the CySat team will have to provide the radio Our Recommendation: Icom 208H Sensitivity =.18 uV, -37dBm Cost = $310

18 Final Parts List 7

Calculations – With Front-End  Analysis: Signal-to-Noise Ratio (at Satellite Dish) = dBm – ( dBm) = dB Power into the Radio > Radio Sensitivity : Radio is able to decode the input signal. (Input power) - (Sensitivity) = 23.0 dBm Power in process (440MHz) Received power at the satellite dish (worst case) dBm (by link budget) System noise power dBm (by Noise Temperature) Coax Cable (Carol® C1166(RG-8), 30ft)-2.76dB/30ft(Insertion Loss) LNA (ZX60-33LN+)21dB(Gain) RF Switch (ZX80-DR230+), 3units-2.1dB(Insertion Loss) SMA to SMA adapter (SM-SM50+), 4units-0.12dB(Insertion Loss) Coax Cable (Belden 9913 (RG-8), 200ft)-5.8dB/200ft(Insertion Loss) Radio Input Power-98.9dBm Power of Radio Sensitivity-121.9dBm

Test Plan  Individual Part Testing  Front-End Testing  Tracking Software prototyping  Overall System Evaluation and Testing

Test  Place: SSCL Lab at Howe Hall  Devices: Signal Generator (Model: ) Spectral Analyzer (Model: ) DC Voltage Generator (Model: )  Methods: RF Switches ○ Apply 440MHz signal to the input of switch, using a signal generator. ○ Change 0 DCV to 12 DCV supplied to switches. ○ Observe if signal path is changed from “Normally Closed” to “Normally Open”. Low Noise Amplifier (LNA) ○ Apply 440MHz signal to LNA. ○ Connect into spectral analyzer ○ Observe if the incoming signal is amplified as we expected. Whole Front-End System ○ Combine two methods above.  Checkpoints: if switches are working properly depending on voltage change. if the amplifier(LNA) is working properly as we expected. RF Switch LNA

Test Results Switch 1 Normally Open (N.O.)Normally Closed (N.C.) FrequencyPowerFrequencyPower 0V AppliedNoise-67dBm440MHz10.06dBm 12V Applied440MHz10.05dBmNoise-66dBm Switch 2 Normally Open (N.O.)Normally Closed (N.C.) FrequencyPowerFrequencyPower 0V AppliedNoise-68dBm440MHz10.04dBm 12V Applied440MHz10.06dBmNoise-67dBm Switch 3 Normally Open (N.O.)Normally Closed (N.C.) FrequencyPowerFrequencyPower 0V AppliedNoise-67dBm440MHz10.06dBm 12V Applied440MHz10.05dBmNoise-66dBm Signal(440MHz): dBm Noise power: -50 ~ -80 dBm  Switch Test (Model: Mouser CCR-33SC-N) Normally OpenNormally Closed Conclusion: Verified its switching operation

Test Results InputOutput Center frequency: 440MHz Magnitude of Signal: -58.6dBm Center frequency: 440MHz Magnitude of signal: -38.1dBm Experimental Gain: 20.5 dB Expected Gain:21.1 dB Conclusion: Similar gain as expected  Low Noise Amplifier (Mini-circuits ZX60-33LN+)

Test Results  Whole Front-End System Testing Frequency: 439.9MHz Signal In: -39.9dBm Signal Out: dBm  Experimental Gain from the system: dB  Expected Gain:16.01 dB  Analysis Better Gain than expected Gain Error reasoning: Gain and loss in parts’ manual are less accurate for 440MHz.  Conclusion: The whole system is working as expected.

Prototyping/Testing – Tracking Software  Ham Radio Deluxe Test

Prototyping/Testing – Tracking Software  Motor Control Test Tested with microcontroller

Evaluation of Overall System  Ideally Install sub reflector Install front-end box Install software Test entire system with orbiting satellites Train CySat on how to use the system But… 27

Evaluation of Overall System  Issues During winter the dish was frozen ○ Unable to do anything until March In March we discovered that the dish does not move up/down Numerous trips to the Fick Observatory to attempt to fix issue failed Rotary Encoders are only partially installed, can’t install them until the dish moves down Can’t install sub reflector or front-end box until dish can be moved down 28

Conclusions  Implemented systems that we designed  Unable to successfully implement final product, due to unforeseen issues at the Fick Observatory  Future work: Fix issues at Fick Observatory ○ Motor Control ○ Rotary Encoders Install Sub-reflector, front-end box

Questions