ARGOS receiver 1GHz … 2GHz → 0.1MHz…1GHz Components panel Front panel Back panel and connectors.

Slides:



Advertisements
Similar presentations
HARP-B Local Oscillator
Advertisements

1 Chelmsford Amateur Radio Society Advanced Licence Course Anthony Martin M1FDE Slide Set 12: v1.4, 2-Dec-2012 (4) Receiver Demodulation Chelmsford Amateur.
Preliminary Design Review EVLA 1 st and 2 nd Local Oscillators.
Analog Devices FMCOMMS1-EBZ WINLAB – Rutgers University Date : April 22, 2013 Authors : Prasanthi Maddala,
AAVS receiver Federico Perini AAVP December, ASTRON, Dwingeloo.
RADIO FREQUENCY MODULE. Introduction  An RF module is a small electronic circuit used to transmit and receive radio signals.  As the name suggests,
Spectrum analyser basics Spectrum analyser basics 1.
Tracing The Signal Ron Maddalena July Typical Components Amplifiers Mixers Attenuators Power Detectors Synthesizers Splitters Couplers Filters.
Ideal Response Simulated Response Measured Response Nathan Roth Advisors Dr. Brian Huggins Dr. Prasad Shastry Mr. James Jensen, Northrop Grumman Corporation.
. ARGOS Double - Heterodyne - FFT - Radio - Spectrometer RAPP ETH Zürich Minikolloquium June 11th 2002 Michael Arnold / Christian Monstein Astronomical.
Sensor for cellular activity Supervised by : Yossi Hipsh Preformed by : Assaf Haim Ohad Fremder.
2.4-GHZ RF TRANSCEIVER FOR IEEE B WIRELESS LAN UF# UF#
HIAPER Cloud Radar Transceiver Exciter Receiver Oscillators High-Powered Amplifier Calibration Exciter Receiver Oscillators High-Powered Amplifier Calibration.
Notebook Telescope 1m BPF AR 5000 BPF FFT LO 21cm (1.42 GHz) IF 1 ≈152 MHz 10.7 MHz H2-Converter PSU COM RS-232 L-Band (Neutral Hydrogen, 21 cm / 1421.
Spectrum Analyzer Basics Copyright 2000 Agenda Overview: What is spectrum analysis? What measurements do we make? Theory of Operation: Spectrum analyzer.
Spectrum Analyzer Basics Copyright 2000 Agenda Overview: What is spectrum analysis? What measurements do we make? Theory of Operation: Spectrum analyzer.
Bilal Saqib. Courtesy: Northrop Grumman Corporation.
Doc.: IEEE /211r2 Submission September, 2000 Jeyhan Karaoguz, Broadcom CorporationSlide 1 Project: IEEE P Working Group for Wireless Personal.
Student: Vikas Agarwal Guide: Prof H S Jamadagni
1 Chelmsford Amateur Radio Society Intermediate Licence Course Anthony Martin M1FDE Slide Set 7 (4) Receivers Chelmsford Amateur Radio Society Intermediate.
ZVx - The Network Analyzer Family
Tracing The Signal Ron Maddalena July Typical Components Amplifiers Mixers Attenuators Power Detectors Synthesizers Splitters Couplers Filters.
ADS Design Guide.
Summary Thus far we have: ECE 4710: Lecture #39
Vector Modulator AMC board Marcin Smelkowski Warsaw University od Technology PERG – ISE Presentation is based on „Draft.
Scanning Digital Radar Receiver Ryan Hamor Advisor: Dr. Huggins Bradley University ECE Department 5/02/2006.
A 1.5-V 6-10-GHz Low LO-Power Broadband CMOS Folded-Mirror Mixer for UWB Radio H.-W. Chung, H.-C. Kuo, and H.-R. Chuang Institute of Computer and Communication.
Software Defined Radio How I learned to love DSP Tom McDermott, N5EG October 2, 2008.
Back End Downconverter Wes Grammer NRAO March 15-17, 2012EOVSA Preliminary Design Review1.

Simplified Transceiver Architecture. Role of a Transmitter 0 90 A D A D HPMX-2007 The lkhefw wlkhq wilehr wejklh wajkhrqwilu wae. esjlkh qwh wlh lihewrw.
Integrated receivers for mid-band SKA Suzy Jackson Engineer, Australia Telescope National Facility SKADS FP6 Meeting – Chateau de Limelette – 4-6 November,
IP-BPM status Siwon Jang KNU. Contents The electronics repair status –Repair work status –Electronics RF test (by using Oscilloscope) –Electronics shipment.
The Progress Report for KVN Construction Seog-Tae Han and KVN staffs Korea Astronomy and Space Science Institute March18 th 2009.
SPECTRUM ANALYZER 9 kHz GHz
˜ SuperHeterodyne Rx ECE 4710: Lecture #18 fc + fLO fc – fLO -fc + fLO
XFEL The European X-Ray Laser Project X-Ray Free-Electron Laser 1 Frank Ludwig, DESY XFEL-LLRF-ATCA Meeting, 3-4 December 2007 Downconverter Cavity Field.
Technical notes about Anti aliasing differential filter- november 2014 R. Assiro - P.Creti.
Student: Vikas Agarwal Guide: Prof H S Jamadagni
EMBRACE receiver 8th SKADS Board Meeting Château de Limelette, Belgium, 3 November 2009 DS5 EMBRACE IRA&ASTRON DS5 Eng. Group Presentation by Jader Monari.
Paul Harden VLA Veteran EVLA LO-IF PDR 22 January EVLA IF/LO EVLA “LOW BAND” CONVERTERS For 4/P/L/S/C and Ku Bands.
Travis Newton LO-IF Engineer EVLA LO/IF PDR January IF Downconverter Travis Newton LO/IF Engineer.
Tests of STO IF Components S. Weinreb April 15, 2009 Two 1-2 GHz IF amplifier plates and one 5 GHz converter plate for the Texas test flight have been.
Tracing The Signal Ron Maddalena July Typical Components Amplifiers Mixers Attenuators Power Detectors Synthesizers Splitters Couplers Filters.
Chuck KutzEVLA Front-End CDR – LO/IF System April 24, EVLA Front-End CDR EVLA Front-Ends and the EVLA LO/IF System.
Bob Hayward Receiver Engineer Feed & Front End PDR Feb Feed & Front End PDR Hot Off the Press Q, Ka, K-Band Cost Savings.
Brent WilloughbyEVLA Front-End CDR – WVR Option 24 April EVLA Front-End CDR Water Vapor Radiometer Option.
Chapter4 Transmitter and Receiver Applications AM and FM Radios
April 12 | Comparison of Sophisticated Synthesizer Concepts and Modern Step Attenuator Implementations | 2 Comparison of Sophisticated Synthesizer Concepts.
Design Approaches for the X band LLRF Systems Uros Mavric, XB-10, 2 nd of December 2010, Cockcroft Institute, UK
By. Jadhav Avinash J Roll no - 2K13E11. Reference: Hewlett Packard Agilent Technology Wikipedia GwINSTEK.
RF Spectrum Analyzer Dong-Yo Jheng 2012/07/12. RF (Radio Frequency) Frequency: 3 kHz ~ 300 GHz 2.
SUPERHETERODYNE SPECTRUM ANALYZER. TOPICS Superheterodyne spectrum analyzer – Basic architecture – Frequency resolution – Sweep time – Video section.
1 Transmitters A transmitter must generate a signal with the right type of modulation, with sufficient power, at the right carrier frequency, and with.
Beam Secondary Shower Acquisition System: RF design techniques for 40MHz ADC Student Meeting Jose Luis Sirvent PhD. Student 30/09/2013.
CI Lecture Series Summer 2010 An Overview of IQ Modulation and Demodulation Techniques for Cavity LLRF Control.
Communication 40 GHz Anurag Nigam.
Medichats 14 October 2008 ADC bit number and input power needed, in new radio-astronomical applications View of the Medicina Radiotelescopes - Italy Eng.
12.4: SRF HOM Diagnostics: Experimental Results and Future Plans
MTCA.4 Based Local Oscillator and Clock Generation Module for the European XFEL. Uroš Mavrič on Behalf of the MSK Group / DESY and ISE / Technical University.
The Hardware of Software Defined Radios
Principles & Applications
RF Front End Radio Design- Simulations and Specifications
High Performance IF and Transverter Design
A New OEO Design Using Optical Phase Modulation and Modulation Suppression G. John Dick and Nan Yu Jet Propulsion Laboratory, California Institute of Technology.
Tracing The Signal Ron Maddalena July 9, 2007.
Tracing The Signal Ron Maddalena July 9, 2007.
AM-7026 Down Converter-Receiver
SN-553 Frequency Synthesizer
Performance of the Band 3 ( GHz) receiver for ALMA
Presentation transcript:

ARGOS receiver 1GHz … 2GHz → 0.1MHz…1GHz Components panel Front panel Back panel and connectors

Localoscillator #1 10,000GHz 13dBm min Aircable from antenna-tower to receiver 1,415GHz RF-amplifier / equalizer att -3dB 1. mixer IF-isolator -0,7dB 1. IF-filter 8,500GHz B3dB=+-500MHz=1GHz -1dB BPF 2. mixer LO-isolator 2. IF amplifier 0.1MHz...1GHz Overview Digital FFT Radio-Spektrograf File: RX1GHz.pptRevision: 1.5 Updated by: Chr. Monstein, Created by : Chr. Monstein, Astronomical Institute ETHZ Synthesizer- isolator 26dB min NF<5dB IFRF LO RFIF LO 41dB -6dB 15dB att -3dB 1. IF-amplfier 8-12,4GHz ADC 8bit 2Gs/sec PC & FFT Lowpassfilter F3dB=1GHz a=-1dB Localoscillator #2 9,000GHz 13dBm min Frf Fsy IF1 IF2 IF2=IF1-Flo IF1=Fsy-Frf Frf=Fsy-IF2-Flo IF2=Fsy-Flo-Frf Flo IF-isolator -0,7dB Level: 104dB SMA- bridge SMA- bridge N/SMA Power Divider -6dB +6dBm+-3dBm 10MHz Ref. Input Power Divider -6dB Log. Detector Video out N/SMA +15V RX3 N/SMA DSP +5.0V

Frequency diagram F1h=9,00GHz F1z=8,50GHz F1l=8,00GHz Fh=2,0 GHz Fl=1,0 GHz Power Frequency 1. mixer stage F2h = 1000 MHz F2l = 0.1 MHz 2. Localoscillator LO2 = 9,000 GHz Power Frequency 2. mixer stage Selection with lowpassfilter F1 = LO1 ± Frf = 8,500 GHz ± 500 MHz F2 = F1 - LO2 = 500 MHz ± 500 MHz Upper sideband USB will not be used Selection of lower sideband LSB by bandpassfilter Frf =1,5 GHz 1. Localoscillator LO1 = 10,000 GHz

ARGOS receiver as a frontend to CALLISTO radio-spectrometer ARGOS baseband 0.1MHz…1GHz received by CALLISTO which accepts 45MHz…870MHz Input freqeuncy