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The ISOLDE Solenoidal Spectrometer project
Robert Page
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Spectrometer Systems for TSR@ISOLDE
The original plan: Move TSR to ISOLDE UK STFC funded project ~£5M investment Internal spectrometer External spectrometer Start January 2015 Completion March 2019
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Physics Motivation
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Solenoidal spectrometer concept
z θcm θlab vlab v0 Vcm CM Energy: CM Angle:
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Spectrometer Systems for TSR@ISOLDE
Challenges: TSR not in CERN MTP
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Internal Spectrometer
Plan to exploit Si detector system on
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Spectrometer Systems for TSR@ISOLDE
Challenges: TSR not in CERN MTP ISS on XT02 beam line No TSR – beam quality (beam manipulation) No funding for magnet
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Magnet procurement Magnet available from Brisbane (UQ)
OR66 4T ex-MRI magnet “Active shield” reduces stray field Installed February 2003 Discharged then warmed ~2013 Funding request (STFC/UoL) June 2015
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Magnet in Wesley Hospital, Brisbane, September 2015
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Magnet procurement Magnet available from Brisbane (UQ)
OR66 4T ex-MRI magnet “Active shield” reduces stray field Installed February 2003 Discharged then warmed ~2013 Funding request (STFC/UoL) June 2015 Magnet ordered November 2015
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Magnet leaving Brisbane hospital February 2016
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sailing across the globe…
Calicanto Bridge
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sailing across the globe…
Sarah
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& arriving at CERN, April 2016
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Preparation & cleaning
magnet bore ~90 cm diameter
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Vacuum test
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Cooling down, January 2017 Thanks to CERN cryogenics team, Patrick Retz, ...
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Energising, February 2017 ramped up to 2.75 T, held for 1 hour then ramped down
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In the ISOLDE Hall ~18 tons – too heavy for ISOLDE hall crane!
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on its stand, aligned & connected
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Stray field
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Magnetic shielding design
Jérémie Bauche, Kevin Buffet & Yacine Kadi (CERN)
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ISS inside the magnet beam
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ISS Mechanical Design Target & detector drive systems
Hexagonal Si tube ~50 cm long 4 DSSDs per face ASIC readout Cooled
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ISS Si detector module 6 R3B ASICs 0 – 50 MeV 128 channels
100 MHz time stamp daisy-chained
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Si detectors DSSDs: 1 mm thick x: 128 × 0.95 mm y: 11 × 2 mm
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132Sn(d,p) with TSR beam quality
simulations by Marc Labiche
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PCBs
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PCB trial assembly
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Si tube cross section
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Reconstructing the z position
CM Energy: Algorithm devised by P. Butler Implemented in GEANT4 by M. Labiche
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Exploitation plans early exploitation before LS2
stable & long-lived isotope running during LS2 + commissioning of the ISS Si array + commissioning of gas recoil detector… followed by ISS running after LS2
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Conclusions Design work well advanced First Si DSSDs delivered
Prototype tests under way Magnet recommissioned ISOLDE integration continuing
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