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The ALMA Front End John C. Webber National Radio Astronomy Observatory, Charlottesville VA 22903, USA ALMA Front End Organization • Work is done by: – The National Radio Astronomy Observatory (NRAO, USA) – The European Southern Observatory (ESO, Germany) – The National Astronomical Observatory of Japan (NAOJ, Japan) – – – – – – – The Herzberg Institute for Astrophysics (HIA, Canada) The Institut de Radioastronomie Millimétrique (IRAM, France and Spain) The Netherlands Research School For Astronomy (NOVA, The Netherlands) Onsala Space Observatory (OSO, Sweden) Rutherford Appleton Laboratory (RAL, UK) The Centro Astronomico de Yebes (CAY, Spain) The University of Cambridge / Astrophysics (CA, UK) – The Academia Sinica (Taiwan) URSI Boulder 2008 2 Front End Key Design Goals • Noise performance as good as the best mm and sub-mm receivers • Single sideband systems when possible, to minimize noise from the image sideband (all except Bands 9 & 10) • Beam pointing controlled by mechanical tolerances (except Bands 3 & 4, which have mirrors on top of the cryostat) • No moving parts except for cryogenics and amplitude calibration loads • Short-term phase stability good enough for >90% coherence at 950 GHz • Long-term phase stability good enough to go 30 minutes without instrumental calibration • Ambient and heated RF loads for amplitude calibration • WVR for atmospheric phase calibration by radiometry • Rapid switching between bands for atmospheric phase calibration by position switching on a 10-second time scale URSI Boulder 2008 3 Front End Key Programmatic Challenges • Build 70 complete FE assemblies (66 on antennas plus 4 spares) and 3 more sets of spare subassemblies on time and on budget • Distribute the work to multiple groups around the world and have everything play together when integrated URSI Boulder 2008 4 Typical results for Bands 3, 6, 7, and 9. Bands 4, 8, and 10 are in development (dashed lines). The horizontal lines are the specification which applies over 80% of the band. Above 600 GHz, mixers are DSB. URSI Boulder 2008 5 Front End Wiring Diagram POWER M&C OFFSET LO REF IF OUT URSI Boulder 2008 OPTICAL LO REF 6 3D Model of Front End Assembly URSI Boulder 2008 7 Front End Assembly Bottom View URSI Boulder 2008 8 Cryostats Cryostat and prototype chassis mounted on tilt table • Cryostat is 1 meter in diameter, mass ~450 kg • Sumitomo 3-stage refrigerator cools below 4K • Internal clamp rings provide thermal contact to cold stages URSI Boulder 2008 9 Optics 1. Optics design concept completed: • • • All ALMA Bands 1-10 and WVR pick off mirror have been designed and incorporated into cartridge designs Detailed designs of all windows and IR filters Widget space containing: • amplitude calibration device • ¼ wave plate holder for Band 7 • Solar filter 2. Design verification: • • • • Complete physical optics calculations made for bands 3-10 Prototypes tested warm except for bands 5 & 10 Cold tests: done during testing of assembly Tests on the sky at 5000m elevation to begin before the end of 2008 URSI Boulder 2008 10 Cartridge 7 Block Diagram Warm Cartridge Cold Cartridge URSI Boulder 2008 11 Cold Cartridges Bands 3 (84-116 GHz), 6 (211-275 GHz), 7 (275-373 GHz), and 9 (602-720 GHz) SIS mixer receivers URSI Boulder 2008 12 Cold Cartridges Band 4, 125-169 GHz Band 8, 385-500 GHz (qualification model) (4K stage in test dewar) URSI Boulder 2008 13 Front End Local Oscillators • Warm Cartridge Assemblies (WCA) – Contain YIG-Tuned Oscillator, Phase Lock Loop, Active Multiplier Chain, and output Power Amplifiers – Locked to output of photomixer driven by photonic signal from Back End – Phase and amplitude noise meet ALMA specifications – Band 3 WCA drives SIS mixer directly – For other bands, WCAs drive cold frequency multipliers mounted in cold cartridge • Frequency Multipliers – Wideband varistor designs from Virginia Diodes, Inc. – Designs final for Bands 4, 6, 7, and 9 – Band 8 and 10 prototypes being tested URSI Boulder 2008 14 183 GHz Water Vapor Radiometer • Development status – Two prototype WVRs (Cambridge and Onsala) were completed and fully tested – Extensive testing was carried out at the SMA – Final design is a single channel, Dickeswitched radiometer – First production unit is under test and will be delivered in mid-2008 Dicke switched WVR RF Front End URSI Boulder 2008 15 Ambient/Hot Load Amplitude Calibration Device URSI Boulder 2008 16 Integration of Front End Warm Optics Warm Cartridge Assembly Band 3 (1st LO, Bias, M&C) Band 3 Cartridge Warm Cartridge Assembly Band 6 (1st LO, Bias, M&C) Band 6 Cartridge Warm Cartridge Assembly Band 7 (1st LO, Bias, M&C) Band 7 Cartridge Warm Cartridge Assembly Band 9 (1st LO, Bias, M&C) Band 9 Cartridge Cryostat FE Assembly FE M&C unit Front end IF Front end chassis URSI Boulder 2008 17 Assembly and Test The first FE assembly rear view with side panels removed (minus the LO Photonic Receiver) URSI Boulder 2008 18 Principal Test Requirements • • • • • • • • • • • Noise temperature Image rejection Beam patterns Amplitude stability Phase stability IF output power Gain flatness Gain compression Polarization alignment Vacuum compatibility Electromagnetic compatibility URSI Boulder 2008 19 Schedule • FE#01 – Assembled and tested at the North American integration center (Charlottesville, Virginia) – Delivered as an “engineering model” without phase stability measurements (waiting for photonic reference test module) – Installed on a Mitsubishi antenna in November 2008 • FE#02 – Assembled and tested at the East Asian integration center (Academica Sinica, Taiwan) – Delivered as an “engineering model” without phase stability measurements (waiting for photonic reference test module) • FE#03 – Assembled and under test at the European integration center (Rutherford Appleton Laboratory, England) – Will be delivered in February 2009 as an “engineering model” without phase stability measurements (waiting for photonic reference test module) URSI Boulder 2008 20 Schedule • FE#04-06 – One each to be assembled and tested at the three integration centers – Qualification and verification of integration center equipment and procedures – Delivery as fully qualified units June-August 2009 • FE #07-70 – To be delivered over the period October 2009-October 2012 – Output rate of each integration center: one every 51 days! URSI Boulder 2008 21