COLD FRONT END STATUS. OUTLINE RF Cryo System Mounting Apparatus 27-m cryo upgrades.

Slides:



Advertisements
Similar presentations
Receiver Systems Alex Dunning.
Advertisements

HARP-B Local Oscillator
Antennas for MeerKAT March TDP AWG, 13-14/3/08, San Francisco MeerKAT Semantics K.A.T. = Karoo Array Telescope –KAT is Afrikaans for cat –MeerKAT:
BEPCII RF POWER SYSTEM RF group, IHEP Sep ~ April 1.The 1 st transmitter had finished installing,commissioning and SAT (Site Acceptance Test).
Present status of the laser system for KAGRA Univ. of Tokyo Mio Lab. Photon Science Center SUZUKI, Ken-ichiro.
AAVS receiver Federico Perini AAVP December, ASTRON, Dwingeloo.
Spectrum analyser basics Spectrum analyser basics 1.
08/16/01.
Mid-Semester Design Review High Frequency Radio with BPSK Modulation.
STARLight PDR 3 Oct ‘01 L. van Nieuwstadt Receiver - Page 1 STARLight Objective To design, build and test RF front end receiver as small as possible, meeting.
MICE RFCC Module Update Allan DeMello Lawrence Berkeley National Lab MICE CM26 at Riverside California March 26, 2010.
ATA Antennas Feeds and Systems NSF Review 8/05/08 Jack Welch.
Radio Telescopes. Jansky’s Telescope Karl Jansky built a radio antenna in –Polarized array –Study lightning noise Detected noise that shifted 4.
Modulation is the process of conveying a message signal, for example a digital bit stream or an analog audio signal, inside another signal that can be.
Receiver Systems Suzy Jackson – based on previous talks by Alex Dunning & Graeme Carrad.
ESTeem Training Class Antenna Fundamentals. Decibels (dB) Used for all mathematical calculations in the radio world. – dB is a logarithmic number dB =10.
WP06_AntennaIF. WP06_AntennaIF 3 principal modules switch amplifier (= ATA ‘PAM’) –includes attenuators (0-60 dB), power detector, and bias tee for the.
Performance of the DZero Layer 0 Detector Marvin Johnson For the DZero Silicon Group.
System Elements HighPoint Broadband Delivery System Sector 1 Sector 3
18/7/2002Ivan Hruska EP/ATE1 LV brick for TILECAL  How to power the electronics of TILECAL ? Power supply as close as possible to electronics ?  Positives.
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.
COLD FRONT END Stephen Muchovej Caltech. CONSIDERATIONS RF System Itself Physical Considerations Packaging Mounting.
Oct. 16, 2006 Midterm Next Class Assignment #4 is Marked
KFPA LO Modifications (from single pixel results) Critical Design Review January 30, 2009 G. Anderson.
Integrated receivers for mid-band SKA Suzy Jackson Engineer, Australia Telescope National Facility SKADS FP6 Meeting – Chateau de Limelette – 4-6 November,
Codan 5700 Series C-Band Transceiver Technical Overview.
Dan MertelyEVLA Front-End CDR – C-Band Receiver April 24, EVLA Front-End CDR C-Band (4-8 GHz) EVLA Receiver.
Bob Hayward Receiver Engineer Feed & Front End PDR Feb Feed & Front End PDR Q, Ka, K, Ku & X-Band Receivers Backup Slides.
˜ SuperHeterodyne Rx ECE 4710: Lecture #18 fc + fLO fc – fLO -fc + fLO
Thoughts on the Design of a WVR for Alan Roy (MPIfR) the Twin Telescope at Wettzell.
Amplifiers Amplifier Parameters Gain = Po/Pi in dB = 10 log (Po/Pi)
A Modular K-Band Focal Plane Array for the Green Bank Telescope Matt Morgan National Radio Astronomy Observatory 9/28/2007.
Ding Sun and David Wildman Fermilab Accelerator Advisory Committee
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.
Author EVLA Feed & FE PDR 12/13 Feb, EVLA Receivers PDR (4m, P,) L, S, C BAND RECEIVERS Daniel (Mert) Mertely.
Q, Ka, K, Ku & X-Band Receivers
CRYOGENICS Stephen Muchovej Caltech.
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.
K-Band Focal Plane Array Project Engineering Overview Matt Morgan National Radio Astronomy Observatory 2/27/2008.
MICE Prototype Coupling Coil Fabrication Update Allan DeMello Lawrence Berkeley National Laboratory MICE CM38 - Napa California February 25, 2014 February.
Brent WilloughbyEVLA Front-End CDR – WVR Option 24 April EVLA Front-End CDR Water Vapor Radiometer Option.
MICE RFCC Module Update Allan DeMello Lawrence Berkeley National Laboratory Oxford, UK July 7, 2011 July 7, 2011.
SPHENIX MECHANICAL D. Lynch August 21, /15/2014sPHENIX Mechanical Design.
Copyright © 2005 Heathkit Company, Inc. All Rights Reserved Automating and Integrating Residential Systems Presentation 4 – Control of Entertainment Equipment.
RF Phase Reference Distribution for the European XFEL Krzysztof Czuba Warsaw University of Technology, ISE For the RF Synchronization Team P. Jatczak,
High power fibered optical components for gravitational waves detector Matthieu Gosselin, PhD Student at EGO ELiTES : 3 rd general meeting February 10.
A discussion on the Readout Schedule leading to PDR Ganesan Rajagopalan Cornell University.
Status of Vertical Test Stand at RRCAT P Shrivastava, P Mohania,D.Baxy, Vikas Rajput S C Joshi, S Raghavendra,S K Suhane RRCAT, Indore November 26, 2012.
DESIGN OF A 9MHZ 15KW CW AMPLIFIER FOR RHIC Shane Dillon CTO.
FUNCTION GENERATOR.
Single Cryocooler 1.2 to 116 GHz Receiver for ngVLA S. Weinreb, A. Soliman, and H. Mani July 30, Rationale 2.Synergistic Reflector Design 3.Dewar.
Cosmic Microwave Technology, Inc.
Plans for this week MWPC: wire stretching today
(4) Filters.
ANTENNA MEASUREMENTS Measurement of Radiation Pattern Gain
WP02 PRR: Master Oscillator and RF Reference Distribution
RF cables calibration Matteo Volpi Thomas Geoffry Lucas
iSHELL Design Review Cryostat & Optics Bench
System Considerations for Submillimeter Receiver
Chapter Five: Transmitters
LO/IF Switches Doug Scott
Terry Cotter LO/IF Group Leader
ECE 3336 Introduction to Circuits & Electronics
CH-6 CABLE TV.
AM-7026 Down Converter-Receiver
ECE 5233 Satellite Communications
ECE 5233 Satellite Communications
System Specifications Lab Tests
Presentation transcript:

COLD FRONT END STATUS

OUTLINE RF Cryo System Mounting Apparatus 27-m cryo upgrades

RF System Need as much amplification as needed to satisfy power requirements of RF-fiber converter (which is 7dBm, requiring about 86dB of gain). Most likely 2 amps in addition to the LNAs. Noise temps of < 50K from 1-18GHz 1% Amp Stability, 1 degree phase stability Polar accuracy: 15 dB isolation

Horns Single horn not available for cover full band. Dual-Pol horns with low spillover available from Sandy Weinreb’s lab that operate over factors of 6 in frequency. RF System

Horns Split into 1-6GHz and 3-18GHz. Physical size of 1-6GHz horn, means we can only easily cool the higher-frequency horn. RF System

Horns Ahmed Agkiray currently refining design (best design so far has aperture efficiencies of ~50% at highest frequency. Once design is complete, they will be machined at OVRO by Tomi Hovatta/Stan Hudson. RF System Cost of tools for machining < $1K. Cost for metal is < few $K (getting estimate) Can make one large horn in 2 weeks.

Couplers Since there are before the LNAs, must have lowest insertion loss possible. They must also work at cryo temps. Available vendors are Krytar and Atlantec Cryo testing last week showed both perform at cryo temperatures, and IL reduces by 0.1dB at low frequencies and up to 0.4dB at higher frequencies. RF System

Couplers for 1-6GHz system The large size of Krytar requires a cable with right- angle connectors which increases the IL by 0.1dB. Resulting change in receiver temperature is K. Using Atlantec 1-4GHz gives rx temps 3K lower, but sacrifices 4-6GHz. RF System CompanyModel Number Operating Frequency Insertion Loss (dB) Cost/ unit Physical Dimensions (LxWxH in) KRYTAR GHz< x0.72x0.53 KRYTAR GHz< x0.73x0.53 ATLANTECA GHz< x0.60x0.38 ATLANTECA GHz< x0.70x0.38

Couplers for 3-18GHz system In this case, Krytar seems like the better option. NOTE: ATLANTEC components are manufactured in the UK. RF System CompanyModel Number Operating Frequency Insertion Loss (dB) Cost/ unit Physical Dimensions (LxWxH in) KRYTAR GHz< x0.69x0.53 KRYTAR GHz< x0.73x0.53 ATLANTECA GHz< x0.70x0.50 ATLANTECA GHz< x0.70x0.38

Low-noise Amplifiers Components with longest lead-time. These have already been ordered (~4K each) CIT1-12GHz amps have typical gain of 32dB and noise below 5K. Measurements from first 3-18GHz amps already built show a gain of ~35dB and noise below 10K across whole band. Should be delivered in December. RF System

Isolators Isolators are analogous to RF diodes: they let power go through over a given band but reject most of what comes back. These are necessary if the interaction of amps with subsequent components have poor matches  leads to high reflection. This can cause standing waves which can induce oscillations. There are NO isolators available which work over the frequency we need, so one way to deal with reflections is by using attenuators. Depending on how much attenuation we need to use, this might require additional amplification to get to desired power levels. RF System

Secondary Amps We will need at least one stage of secondary amplification (and most likely two) Placing the secondary amp on the 77K radiation shield could lower the receiver temperature of the warm system by up to 5K**, so we would ideally want an amplifier that can be cooled to cryogenic temperatures. To save cost (buy in bulk), these should operate over full band. RF System ProductFrequencyTypical GainTypical NoiseUnit CostCryo-ready Atlantec AOX1-20 GHz27 dB dB869YES CIAO GHz26 dB<2.0 dB (300K)900YES CIAO GHz28 dB3.0 dB (300K)975YES MINI ZVA GHz26 dB3.0 dB845NO RF-LAMBDA1-18 GHz29 dB3.5 dB1040NO

Filters (notch) Due to Sprint signal, we need a notch filter for GHz. Rejection needed is >40dB (so it can go after 2 nd stage amp) Only 3 vendors said they could make a notch filter that would still preserve the 1-6GHz passband. RF System VendorNotch Depth Lower passband Lower ILUpper Passband Upper ILUnit Cost AMTI40dB0-1.8GHz2.0dB GHz2.0dB492 Atlantec50dB GHz<1.5dB GHz <1.5dB375 Q45dB <1.0dB GHz <1.0dB510

Filters (bandpass) The main advantage to having a bandpass filter is to reject RFI outside our band, which can be pretty severe. 4 vendors quoted us on bandpass filters. Info for low-frequency bandpass (1-6GHz) RF System VendorLow-nu rejectionHigh-nu rejectionIn-band ILcost AtlantecDC-0.8GHz – 30dB>7.0GHz – 30dB<2.0dB300 AMTIDC-0.8GHz – 40dB7.2GHz – 20dB >8.0GHz – 35dB 2.0 dB486 QDC-0.8GHz – 30dB>7.5GHz – 30dB<1.5dB420 ReactelDC-0.85GHz – 40dB>6.9GHz – 40dB<1.0dB952

Filters (bandpass) The main advantage to having a bandpass filter is to reject RFI outside our band, which can be pretty severe. 4 vendors quoted us on bandpass filters. Info for HIGH-frequency bandpass (3-18GHz) RF System VendorLow-nu rejectionHigh-nu rejectionIn-band ILcost AtlantecDC-2.2GHz – 30dB>19GHz – 30dB<2.0dB450 AMTIDC-2.4GHz – 40dB>21GHz – 30dB<2.5dB486 QDC-2.3GHz – 30dB>25.0GHz – 30dB<1.5dB420 ReactelDC-2.5GHz – 40dB>20.7GHz – 40dB<1.0dB1077

RF Switch Over our wide bandwidth, we need a mechanical switch to change between the output between the two systems. James Lamb has tested many different companies and says many are unreliable. He suggests we use Dow-Key. Quote has been requested. Will need one for each polarization. RF System

Cryostat Design Cryostat must be able to house the full 3-18GHz system, and the components for the 1-6GHz system. Will use a CTI 350 Fridge-head for cooling Must allow for range of horn sizes. Should be as compact as possible 3-18GHz horn + fridge-head are main elements in determining its size. RF System

Cryostat – Physical Dimensions Pretty big, but not unwieldy (QUIET cryostat weighed 800 pounds and was a cylinder of diameter ~4 feet)!!! Ours is an L-shape rectangular box. 24”x18” with a 15”x7” rectangle chopped out of it. 9” total thickness. ~15” translation between horns, 1” focus diff. RF System

Cryostat – Walk Through RF System

Cryostat – Walk Through RF System

Cryostat – Walk Through RF System

Cryostat – Walk Through RF System

Cryostat – Status RF System All pieces insides the cryostat (cold plate, radiation shield, filter bank, G-10 supports, bracketry for components, thermal connectors) will be machined at OVRO. Cryo case too big for our machine shop. Quote for cryo case was sent out last week -- should be in later this week. Cryostat currently under review by James Lamb and Sandy Weinreb.

Still to finalize RF System Whether location of horns is ok (from Sandy) Horn design Cost of machining. Components to use. Full Cost (including connectors and coax). I plan on making the cables myself. (BeCu vs. SS). Feed-throughs/connectors should be less than $1K. Should have a lot more info next week.

Prime Focus Apparatus Install a new self-contained system that bolts onto the ring platform. Uses tracks for linear (and vertical -- focus) translations with actuators in z, gears otherwise. Uses a gear motor for rotation. Adjust y once on installation. Mounting Apparatus

Apparatus Walk-through Mounting Apparatus

Apparatus Walk-through Mounting Apparatus

Apparatus Walk-through Mounting Apparatus

Apparatus Walk-through Mounting Apparatus

Minimal info on dish distortion/focus change – makes it hard to define translation/rotation tolerances. So… Translation in x-axis: +-7” Translation in y: +-3” (fix) Translation in z: -4”->+7” Hard stops in x, z-range limited by actuators (up to 3000 pounds). Total weight (including screws) = 350lbs + receiver. Cost: ~$35K total (Tomi’s document) Still need Final PDR Getting quotes on parts we can’t machine at OVRO Mounting Apparatus Apparatus Details

27-m Cryo Upgrades Cryo Upgrade Russ finishing up design of how to get cryo lines up to prime focus. Compressor in pedestal. He lines in the equatorial mount need a 4-port rotary union ($~5K) 2-port rotary union at exit Most straightforward part of whole upgrade!

Cryo Upgrade Inventory Receiver Focus apparatus Compressor/Cryo lines Temp Controlled (TECA) box with: Bias for amps Temp Stable noise diode source Temp monitoring RF switch Pre-amp module RF-optical converter Ethernet Switch Ethernet controllable power supply Small computer to control Noise Diode, Bias, and Alignment jig (rotation, x, and z) Programming said computer/interface with CS.

Timeline September/October: Finalize Cryo design. Select (and order) RF components. Select rest of hardware inside TECA box. Purchase hardware needed for cryo upgrade. Start machining apparatus and cryostat. November: Control subsystem development, testing of individual RF components (as they arrive), machining of rest of apparatus and cryostat. Begin machining horns. December: Cryostat machining complete. Begin cryo testing in lab. January: Apparatus machining complete. Begin testing of apparatus with control system. He line installation complete. February/March: Extensive testing of Cryostat/Apparatus April: Installation? Could be done earlier depending on results from Feb/March. May: Science! ;-)