17 March 2005Edda Gschwendtner1 MICE Cooling Channel: Can we predict cooling to 10 -3 ? Edda Gschwendtner Challenge Systematics Cooling Channel Beam Line.

Slides:



Advertisements
Similar presentations
1 MICE Beamline: Plans for initial commissioning. Kevin Tilley, 16 th November. - 75days until commissioning Target, detectors, particle production Upstream.
Advertisements

Progress in the construction of the MICE cooling channel and first measurements Adam Dobbs, EPS-HEP, 23 rd July 2011.
MICE CM Berkeley 9-12 Feb February 2005 Edda Gschwendtner 1 Parameter List Edda Gschwendtner Introduction Parameter list for sub-systems of MICE.
9 March 2005Edda Gschwendtner1 DAQ Terminology ISIS Terminology MICE Terminology Parameter Definitions.
MICE Superconducting Solenoids: Status and Update RAL: T W Bradshaw M Courthold J Rochford M Hills D Baynham Oxford: J Cobb W Lau S Yang MICE.
MICE the Muon Ionization Cooling Experiment Emilio Radicioni, INFN EPS-HEP Aachen 2003.
Magnet quench during a training run Magnet electrical circuit schematic PROGRESS ON THE MODELING AND MODIFICATION OF THE MICE SUPERCONDUCTING SPECTROMETER.
Target & Capture for PRISM Koji Yoshimura On behalf of PRISM Target Group Institute of Particle and Nuclear Science High Energy Accelerator Research Organization.
Progress on the MICE Cooling Channel Solenoid Magnet System
Changing the absorbers: how does it fit in the MICE experimental programme? Besides the requirement that the amount of multiple scattering material be.
CHIPP Sept 2005Jean-Sébastien GraulichSlide 1 What is MICE  Muon Ionisation Cooling Experiment  What is Ionisation Cooling ? Cooling = Reduction of Beam.
Paul drumm daq&c-ws august/september Cooling Channel.
Alain Blondel MICE: Constraints on the solenoids 2.Field Homogeneity: or ? this will be dictated by the detector requirements. TPG will be.
9 June 2006MICE CM-15 Fermilab1 Progress on the MICE Cooling Channel and Tracker Magnets since CM-14 Michael A. Green Lawrence Berkeley Laboratory.
2/7/2002 RolMUCOOL/MICE1 20b. Gaseous Energy Absorber, 21a. High Pressure RF Cavities New Money for New Approaches DOE Small Business Innovation Research.
Slow controls and instrumentation of MICE 1.Physics and systematics 2.How the state of the cooling channel gets defined 3.Engineering for the signal readout.
Safety Review: RF Issues Derun Li Absorber Safety Review December 9-10, 2003 Lawrence Berkeley National Laboratory Berkeley, CA
MOM Report Paul Soler MICE Operations Manager University of Glasgow MICO April 12, 2010.
LH2 Absorber Heat Load and Homeostasis. What has happened before… 1.Huge LH2 volumes, low heat deposition: Bubble chambers 2.Small LH2 volumes, low heat.
Control, Monitoring and DAQ Makoto Yoshida Osaka Univ. MICE Frascati June 28, 2005.
Controls Review  Want to record a full configuration of the experiment at every possible “event”, including controls data.  Event trigger = accelerator.
1 Superconducting Magnets for the MICE Channel Michael A. Green Oxford University Physics Department Oxford OX1-3RH, UK.
MICE analysis meeting Alain Blondel 5 August MICE -- what running strategy? disclaimer: of course we will evolve the running strategy as problems.
Goal of MICE:   out /  in of   Assuming a standard (or agreed to) definition of 6-D cooling.  We can also assume that the tracker can give.
12 March 2006NFMCC Meeting, IIT, Chicago1 Progress on the MICE Cooling Channel and Tracker Magnets Michael A. Green Lawrence Berkeley Laboratory.
1 Progress on the MICE Cooling Channel Magnets Michael A. Green Lawrence Berkeley National Laboratory 28 June 2005.
MICO 15 th February 2010 Terry Hart (MOM) - Decay Solenoid and Target - MICE Machine Physics runs - User Run Plans.
1 Effect of staging on module connection and support arrangement Yury Ivanyushenkov RAL.
CMPB Alain Blondel 14 April STATUS OF MICE.
MuCool RF Status MICE Collaboration Meeting June 7-10, 2006, Fermilab A. Moretti June 9, 2006.
Test plan for the MICE SS cryostat and magnet Tapio Niinikoski LBNL Spectrometer Solenoid Workshop May 10, 2011.
MICE magnetic measurements Sequence of events and MICE hall movements Alain Blondel – 10-April 2012 revision from 13 December 2012.
MICE Video meeting Alain Blondel 7 December MICE -- what running strategy? reflections on steps I and II.
MICE - UK Project Progress Roy Preece 30 th April 2013.
MICE CM February 08Jean-Sébastien GraulichSlide 1 Detector DAQ Hardware Status o Introduction o Preliminary list o Plan for action o Summary Jean-Sebastien.
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices iteratively to determine trace.
R&D Status and Plan on The Cryostat N. Ohuchi, K. Tsuchiya, A. Terashima, H. Hisamatsu, M. Masuzawa, T. Okamura, H. Hayano 1.STF-Cryostat Design 2.Construction.
Emittance measurement: ID muons with time-of-flight Measure x,y and t at TOF0, TOF1 Use momentum-dependent transfer matrices to map  path Assume straight.
Status of the Muon Ionization Cooling Experiment (MICE) Yagmur Torun Illinois Institute of Technology April 1, 2013.
MICE: The International Muon Ionization Cooling Experiment Ulisse Bravar University of Oxford ICHEP ‘04 1 MICE: The International Muon Ionization Cooling.
MICE CM at OSAKA Alain Blondel, August MICE collaboration meeting at OSAKA (thanks to Mike Zisman, Makoto Yoshida, and Koji Yoshimura)Mike ZismanMakoto.
The status of the construction of MICE Step IV K. Long, on behalf of the MICE collaboration.
Results from Step I of MICE D Adey 2013 International Workshop on Neutrino Factories, Super-beams and Beta- beams Working Group 3 – Accelerator Topics.
MICE magnetic measurements: AFC considerations Alain Blondel see a previous discussion for reference in CM35 (Feb 2013 slides by V. Blackmore, A. Blondel.
J. Pozimski UKNF WP1 meeting 10 March 2010 UKNF WP1 milestone table status.
UKNF OsC RAL – 31 st January 2011 UKNF - Status, high lights, plans J. Pozimski.
805 MHz Status IIT NFMCC Meeting March 12-15, 2006 A. Moretti March 12, 2006.
MCTF 8/17/06 A. Bross MTA Activities and Plans MCTF August 17, 2006 A. Bross.
MICE at STFC-RAL The International Muon Ionization Cooling Experiment -- Design, engineer and build a section of cooling channel capable of giving the.
MICE Status & Plans MICE-UK paul drumm 15 th September 2004.
MICE RF Workshop Alain Blondel MICE = critical R&D for neutrino factory and muon collider 1 neutrino factory: accelerate muons and store to produce.
Controls for Particle ID/tracking in MICE 1.Physics and systematics 2.Controls types 3.Controls list 4.Needed for particle ID/tracking M. A. Cummings May.
1 HIGH ENERGY ACCELERATOR RESEARCH ORGANIZATION KEKB Review Committee/ NAKAI Hirotaka KEK Crab Cavity - Cryogenics - KEKB Crab Cavity Group - presented.
MICE: The International Muon Ionisation Cooling Experiment MOPLT106 Abstract The provision of intense stored muon beams would allow the properties of neutrinos.
M. Ellis - MICE Collaboration Meeting - Thursday 28th October Sci-Fi Tracker Performance Software Status –RF background simulation –Beam simulation.
MICE Coupling Coil Testing at Fermilab All Experimenters Meeting Ruben Carcagno March 19, R. Carcagno - MICE CC Testing at Fermilab3/19/2012.
Progress in the construction of the MICE cooling channel and first measurements Adam Dobbs, EPS-HEP, 23 rd July 2011.
Summary of Nufact-03 Alain Blondel NuFact 03 5th International Workshop on Neutrino Factories & Superbeams Columbia University, New York 5-11 June 2003.
Controls and monitoring in MICE 1.Physics and systematics 2.Controls types 3.Controls list 4.Data record M. A. Cummings April 2004 CERN.
ch/~bdl/lepc/lepc.ppt 1 MICE Status and Plans Rikard Sandström Université de Geneve International Scoping Study CERN,
(one of the) Request from MPB
MICE S TEP IV P HYSICS ‘D ELIVERABLES ’ V. Blackmore MAP 2014 Spring Meeting 30 th May, /15 AKA “What will we learn from Step IV?”
August 8, 2007 AAC'07 K. Yonehara 1 Cooling simulations for Muon Collider and 6DMANX Katsuya Yonehara Fermilab APC MCTF.
Muons, Inc. Feb Yonehara-AAC AAC Meeting Design of the MANX experiment Katsuya Yonehara Fermilab APC February 4, 2009.
Spokesman's update.
MuCool Test Area Dedicated facility built at the end of the Linac to address MuCool needs RF power 805MHz, 201MHz)
Why do we need to know the fields / map the magnets?
M. Migliorati, C. Vaccarezza INFN - LNF
Design of the MANX experiment
Controls & Monitoring in MICE
Presentation transcript:

17 March 2005Edda Gschwendtner1 MICE Cooling Channel: Can we predict cooling to ? Edda Gschwendtner Challenge Systematics Cooling Channel Beam Line Summary

17 March 2005Edda Gschwendtner2 Challenges of MICE Operate RF cavities of relatively low frequency (200MHz) at high gradient (up to16MV/m) in highly inhomogeneous magnetic fields (1-3T) Dark currents (can heat up LH 2 )  breakdowns Emittance measurement to relative precision of in environment of RF background requires  low mass and precise tracker  Low multiple scattering  Redundancy to fight dark current induced background  Excellent immunity to RF noise Hydrogen safety  substantial amounts of LH 2 in vicinity of RF cavities and SC magnets

17 March 2005Edda Gschwendtner3 Goal of MICE Science fiction example: MICE measures ( ε out / ε in ) exp = ± err stat and compares with ( ε out / ε in ) sim =  Try to understand the difference.  10% cooling of 200MeV/c muons  With measurement precision: Δ (ε out / ε in ) = Theory uncertainties:  Model and simulation choices Experimental uncertainties:  Design of detectors/cooling elements

17 March 2005Edda Gschwendtner4 Sources of Experimental Systematic Uncertainties Particle tracker  Assume: tracker can give precision of particle position and momentum that won’t contribute significantly to the error. Particle ID  Assume: Particle ID < 1% error Cooling channel / detector solenoid  Main source of systematic errors!  Should be under control to a level such that up to 10 independent sources of systematics will be < (  each of them < 3 ·10 -4 ) (Beam line) This talk!

17 March 2005Edda Gschwendtner5 Cooling Channel  three Absorber and Focus Coil modules (+ three LH 2 handling systems)  two RF Cavity and Coupling Coil modules (+ RF power systems)  power supplies, field monitoring, and quench protection for magnets  infrastructure items  vacuum systems (pumps, valves, monitoring equipment)

17 March 2005Edda Gschwendtner6 How to Handle Systematics Design considerations Define tolerances Monitoring Calibration measurements with the muon beam

17 March 2005Edda Gschwendtner7 QuantityTolerancesMonitoring Calibration with muon beam RF CAVITIESRF field 3·10 -3 measure E to  E/E= Measure phase measure energy of muons vs RF phase before and after cooling channel. ABSORBER Amount of absorber (in g/cm 2 ) 3·10 -3 = 1mm/35cm Cryogenics… Density through T & P measure energy loss of muons for 0 absorber, 1 absorber, 2 absorbers with RF off. MAGNETS Positions of coils some mmalignment transfer matrix: e.g.: (p t, p L, phi, x 0, y 0 ) in (p t, p L, phi, x 0, y 0 ) out measure with no RF and empty absorbers each time one changes the magnetic set-up. Currents some amp-meter Magnetic field some magn. probes Cooling Channel NB thickness of H2 absorbers cannot be easily measured in situ (safety windows are in the way)

17 March 2005Edda Gschwendtner8 RF dark currents were measured at Fermilab on 805MHz cavities in magnetic field  Extrapolation to 201 MHz  Simulation of RF backgrounds  Will resume tests on 201 MHz prototype in spring 2005 RF Cavities I (Calibration & Design)

17 March 2005Edda Gschwendtner9 RF Cavities II (Monitoring) Monitoring of:  Voltage, phase and temperature in each cavity  temperature of Be windows  Cavity position and alignment w.r.t. solenoid  cavity and cryostat vacuum, incl. couplers  cryopump performance (P, compressor control, valve status)  roughing system (pump status, pump vacuum, pump valves)  tuner hydraulic reservoir pressure and dynamic control

17 March 2005Edda Gschwendtner10 ΔE = (E out -E in )(GeV) of muons  measures E RF (t) RF Cavities III (Calibration with Beam) (Simulation by P. Janot in 2001 at 88 MHz) ΔE 1  -E loss + E RF ΔE 2  -E loss - E RF ΔE1ΔE1 ΔE2ΔE2

17 March 2005Edda Gschwendtner11 Absorber Monitoring of:  H2 gas system and He gas system Pressure gauge  LH 2 reservoir at 1 st stage of Cryocooler Thermometers Level sensor 2 Heater  Hydrogen absorber Thermometer Level sensor  Absorber windows Thermometer Heater  Safety windows Thermometer  Absorber vacuum and Safety vacuum Pressure gauge Pirani & cold cathode gauge Mass spectrometer → Windows will be measured before and after a run (by photogrammetry or laser) to verify that they did not suffer inelastic deformations

17 March 2005Edda Gschwendtner12  - STEP I: spring 2007 STEP II: summer 2007 STEP III: winter 2008 STEP IV: spring 2008 STEP V: fall 2008 STEP VI: 2009

17 March 2005Edda Gschwendtner13 Magnets I Variety of currents and even polarities Field maps: not simply the linear superposition of those measured on each single magnet  Forces are likely to squeeze the supports and move the coils in the cryostat  Measure magnetic field with field probes

17 March 2005Edda Gschwendtner14 Magnets II Monitoring of :  current in each individual supply (incl. trim supplies, if any)  magnetic field at external probes (Bx, By, Bz);  proposal is 4 probes per coil  quench protection system  cryocooler, coil temperatures  He level sensors  correlations between current, field, and temperature need to be obtainable as a diagnostic tool  cryostat vacuum

17 March 2005Edda Gschwendtner15 dipole quads solenoid quads Diffuser bar-code reader? v v v v v v VV Target ISIS: -BLM -Cycle information Solenoid Cryogenics & control system MICE Diagnostics DAQ  Control System Hybrid Beam Line I

17 March 2005Edda Gschwendtner16 Beam Line II Beam Line:  All magnets Qs (9), Ds(2), decay solenoid  Currents Alarms on temperature, cryogenics, vacuum etc Target:  Synchronisation inputs ISIS Machine Start (once per injection) ISIS clock (200 kHz)  Control Settings insertion depth insertion time  Operational monitors Up to 8 temperature measurements per cycle (inner coil, outer coil, cooling water inlet, water outlet,...) Target position

17 March 2005Edda Gschwendtner17 Summary Systematics must be understood to level. Main sources are Cooling Channel  Detailed monitoring is in most cases possible and being designed.  Muons will provide very powerful cross-checks for themselves (energy loss, energy gain, transfer matrix…)  Dedicated ’monitoring runs’ will be possible and necessary. Strategy being discussed. 10% cooling of 200MeV/c muons with measurement precision: Δ (ε out / ε in ) = 10 -3