Cryogenics, Cryostat, Optics Technology Development

Slides:

Advertisements

Similar presentations

Piero Rapagnani I.N.F.N. Sezione di Roma

Advertisements

ET-meeting, 22 th Oct N. KIMURA/KEK The Latest Status of the KAGRA Cryogenics N. KIMURA A, D. CHEN B, T. KUME A, S. KOIKE A, Y. SAKAKIBARA B, T.

9 th /July/2013 Amaldi 10 C3 15:24~15:42 N.KIMURA/KEK Progress on the Cryogenic System for the Interferometric Cryogenic Gravitational Wave Telescope,

Current status of AMoRE-10 cryostat

Liquid Hydrogen Absorber

Área de Instrumentación NAHUAL Mechanical Concept Current Status F. Javier Fuentes Instituto de Astrofísica de Canarias September

KAGRA subgroup report Cryogenics T. Suzuki, Y. Sakakibara KEK/ICRR

Vibration Analysis of a Cryocooler for CDMS Lauren Coutant SULI, summer 2007.

April 27th, 2006 Paola Puppo – INFN Roma ILIAS Cryogenic payloads and cooling systems (towards a third generation interferometer) part II: the Vibration.

B-pol optical configurations Telescopes and Focal plane options B. Maffei for the B-pol collaboration G. Pisano A. Murphy T. Peacocke.

Trip Report on the visit to ICST of HIT, Harbin, China Derun Li Mike Green Steve Virostek Mike Zisman Lawrence Berkeley National Laboratory (from December.

23 October 2005MICE Meeting at RAL1 MICE Tracker Magnets, 4 K Coolers, and Magnet Coupling during a Quench Michael A. Green Lawrence Berkeley Laboratory.

Cryogenics for B-Pol S. Masi, reporting from F.X. Desert L. Piccirillo …. Use SAMPAN as a baseline, and look for improvements/variations.

BICEP: B ackground I maging of C osmic E xtragalactic P olarization “The Muscle Behind Curls” Jamie Bock Hien Nguyen Caltech/JPL Andrew Lange Brian Keating.

Electric cooling from room temperature down to 200 mK M.Tarasov, L.Kuzmin, and I.Agulo, Chalmers University of Technology, S41296, Göteborg, Sweden V.Mikheev,

ATA Antennas Feeds and Systems NSF Review 8/05/08 Jack Welch.

12 March 2006NFMCC Meeting, IIT, Chicago1 Progress on the MICE Cooling Channel and Tracker Magnets Michael A. Green Lawrence Berkeley Laboratory.

Einstein Polarization Interferometer for Cosmology (EPIC) Peter Timbie University of Wisconsin - Madison Beyond Einstein SLAC May

1 CMB Polarimetry with BICEP: Probing Inflationary Gravitational Waves IAS - Polarization 2005 Denis Barkats.

Thoughts on Ground-based lensing measurements Chao-Lin Kuo Stanford/SLAC KIPAC.

SLAC, May 12th, 2004J.L. Puget PLANCK J.L. Puget Institut d'Astrophysique Spatiale Orsay.

Summer Fun with Optics Stephen Muchovej UC Berkeley CARA - REU Program.

MICE Collaboration Meeting CM-151 Is the the pulse tube cooler a must or is it simply better for the MICE AFC module? Michael A. Green Lawrence Berkeley.

The Atacama B-mode Search: A TES-Based CMB Polarization Instrument CMBpol Workshop, Chicago July 2, 2009 Joe Fowler Princeton University.

Cardiff University Astronomy Instrumentation Group IRAM Camera meeting October 13-14, Cardiff University Astronomical Instrumentation Peter Ade.

1 Engineering the James Webb Space Telescope Paul Geithner JWST Deputy Project Manager - Technical March 26, 2011.

Progress on the MuCool and MICE Coupling Coils * L. Wang a, X. K Liu a, F. Y. Xu a, A. B. Chen a, H. Pan a, H. Wu a, X. L. Guo a, S. X Zheng a, D. Summers.

Avi Friedman Master’s Student Mechanical Engineering Room: 1337 ERB Hometown: Owings Mills, MD Thesis: Design and Development.

Status and Integration of the Spectrometer Solenoid Magnets Steve Virostek Lawrence Berkeley National Lab MICE RAL June 15, 2007.

Advanced Research Systems, Inc.

Utilities 14 October 2008 Martin Nordby, Gordon Bowden.

1 Approved for public release, distribution unlimited Workshop on X Ray Mission Architectural C oncepts December 14-15, 2011 Approved for public release,

LCGT Cryogenics Status Report KEK T.Suzuki.

Materials and Cooling Techniques G. Frossati, A.de Waard, L.Gottardi and O.Usenko Kamerlingh Onnes Laboratory Leiden, The Netherlands.

FIRST/Planck 12 December 2000PT The FIRST Mission Implementation Status and Schedule T. Passvogel The Promise of FIRST.

Cryo AIP Muon Campus AIP Review Arkadiy Klebaner January 23, 2012.

3.1 Optomechanical systems (1) Scientific and engineering resources are available to carry out the optomechanical work on DECam. The highly distributed.

B-pol optical configurations B. Maffei (JBCA – University of Manchester) C. O’Sullivan (NUI Maynooth)

Spectrometer Solenoid: Plans to Fix Magnet 2 Steve Virostek Lawrence Berkeley National Lab Spectrometer Solenoid Review November 18, 2009.

Status of the HINS Linac Front End Focusing Lens Development Can we use these lenses in the SSR1 crymodule of PXIE ? 9/27/20111 I.Terechkine for PXIE Cryomodule.

MICE Status & Plans MICE-UK paul drumm 15 th September 2004.

„Cryogen-free“ Dilution Refrigerators

B-Pol L. Piccirillo Jodrell Bank Centre for Astrophysics (University of Manchester) A European mission to get a CMB polarization measurement limited only.

Summery of the power coupler session at the LCWS13 workshop E. Kako W.-D. Möller H. Hayano A. Yamamoto All members of SCRF WG November 14, 2013.

EDM Engineering Issues General Mechanical Considerations EDM Cryostat Plan D ANSYS EMAG Calculations ANSYS MECH Calculations 3 June ‘03 J. Boissevain.

Extended Detector Cutoff Considerations WFIRST Project Office May

LCGT f2f meeting/ICRR, 04/Aug./2011 N. KIMURA Status of the Cryogenics Design N. KIMURA A, S. KOIKE B, T. KUME B, T. OHMORI D, Y. SAITO C, Y. SAKAKIBARA.

Cryostat & LHC Tunnel Slava Yakovlev on behalf of the FNAL team: Nikolay Solyak, Tom Peterson, Ivan Gonin, and Timergali Khabibouline The 6 th LHC-CC webex.

Dilution Refrigerators with Superconducting Magnets

GWADW2011 Elba/Italy, 23/May/2011 N. KIMURA and Y. SAKAKIBARA Present Design of LCGT Cryogenic Payload - Status of Cryogenic Design - N. KIMURA*, Y. SAKAKIBARA**,

Power couplers Timergali Khabiboulline (FNAL) FNAL-LBNL meeting on NGLS April 13, 2012.

Report on Payload and Calibration splinter meeting B. Maffei M. Bersanelli 1CERN May 2016.

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.

Cryostat sub-system for QUBIC

Michael Niemack, Cornell University for the CCAT-prime Collaboration

1 K thermal model for QUBIC

CMBPol Instrument Technology Study and Workshop

Beam Measurement Characterization and Optics Tolerance Analysis of a 900 GHz HEB receiver for the ASTE telescope Alvaro Gonzalez, K. Kaneko, Y. Uzawa.

Design Fabrication and Processing Group H. Padamsee

Large bolometer arrays on radio telescopes.

TEMPERATURE SENSOR LOCATIONS

Supporting Observations TPX – dust Polarized Sources

Optical Response of TES Bolometer Arrays for SAFARI

System Considerations for Submillimeter Receiver

X-Y Planar Precision Scanner

Daresbury ESS In-Kind Contributions

Optics Alan Title, HMI-LMSAL Lead,

Agenda, Day 1, Tuesday, June 19

Budker Institute of Nuclear Physics,

Optical fiber based sensors for low temperature and superconductors

Presentation transcript:

Cryogenics, Cryostat, Optics Technology Development Maria Salatino & Abby Vieregg Argonne-2018: Cosmology with CMB-S4 March 5 2018

PEOPLE WHO CONTRIBUTED TO THE CMB-S4 CCO WORKING GROUP D. Barkats, B. Benson, S. Bryan, C. Coppi, M. Hasselfield, C. Hill, H. Hui, A. Kusaka, F.T. Matsuda, J. McMahon, L. Moncelsi, J. Nagy, G. Pisano, J. Ruhl, A. Schillaci, A. Suzuki, K. L. Thompson, Z. Xu

THE STARTING POINT: THE CDT REPORT The portion of the CDT strawperson concept related to Cryogenics+Optics 100mK operating temperature w/ dilution refrigerator Frequency coverage up to 270 GHz band Two telescope designs: 14x 0.5m aperture, (30-270)GHz cameras entirely cryogenic 3x 6m aperture, (20-270)GHz cameras cold reimaging optics Polarization modulators required? Informed from Stage-III results

STARTING POINT WE USED TO PROCEED WITH TECHNOLOGY DEVELOPMENT PRIORITIZATION Large Aperture: Three telescopes ~20 optical tubes per telescope Small Aperture: 14 telescopes 1 optical tube per telescope => ~75 optical tubes for all of CMB-S4 x 2~4 lenses per tube [150 to 300 lenses!] x 2~?? metal mesh filters per tube [150 or more filters!] x 0 ~ 1 HWP per tube (Chile, at least) [10’s of HWPs!] x 1 - 2 cryocoolers per receiver [~20 PULSE-TUBES, ~250kW] => LOTS of optical elements!!

TECHNOLOGY DEVELOPMENT (TD) TOPICS WE INVESTIGATED Category Sub-category TD topic 4K cooling systems Sub-K cooling systems Cryogenics Design Fabrication Testing Performance Modeling Cryostat Filters Windows Lenses HWP HWP rotators Baffles Optical modeling Optics

TOP CCO TECHNOLOGY DEVELOPMENT ITEMS Sidelobe-related systematics and measurements Characterization of optical properties of materials at operating temperature AR production methods and rates Metal-mesh filter production rate and maximum size Lens production rate for both lens options (silicon/alumina) HWP continuous rotation at cryo temp (on going S3 development) AR coating on lens and HWP performance/ systematics Magnetic shielding Window manufacturing Cryostat delivery and assembly complexity Cryogenics mK: dilution fridge (S3 dev), Kelvin: PT Coolers Color code: Critical benefits from TD Potentially significant benefits from TD Fairly mature technology (may still benefit from TD)

WHERE TO GO FROM HERE We still need input on a few topics: baffles, sidelobes, HWP in particular So far, we have identified schedule, sensitivity, and systematics impacts on most topics Next step: identifying cost impacts Tomorrow’s Parallel Session: move toward a reference design of CMB-S4 for the Decadal CDR Wednesday morning: organization of the CCO work after the Argonne meeting.