SM18 INFRASTRUCTURE Crab Cavity CryoModule – Conceptual Design Meeting

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Presentation transcript:

SM18 INFRASTRUCTURE Crab Cavity CryoModule – Conceptual Design Meeting A. Benoit, O. Brunner, J. Chambrillon, E. Jensen, K. Liao , P. Maesen, K. Schirm, M. Therasse, W. Venturini BE/RF at CERN 01/08/2013 Mathieu Therasse CERN BE/RF

Mathieu Therasse CERN BE/RF OUTLINE CAVITY PREPARATION AND ASSEMBLY AT CERN - EXISTING ASSEMBLY AREA AND CLEAN ROOMS - CLEANROOM LAYOUT (Existing facility in SM18) - CLEANROOM LAYOUT (Updated) - HIGH PRESSURE RINSING (HPR) AND ULTRA PURE WATER PRODUCTION RF TEST FACILITES - NEW RF CRYO INFRASTRUCTURE AT SM18 - RF POWER ZONE - AVAILABILITY FOR CRAB CAVITY - RF CONTROL ROOM DIAGNOSTIC SYSTEMS - OSCILLATING SUPERLEAK TRANSDUCER AND TEMPERATURE MAPING - OPTICAL INSPECTION CONCLUSIONS 01/08/2013 Mathieu Therasse CERN BE/RF

CAVITY PREPARATION AND ASSEMBLY AT CERN 01/08/2013 Mathieu Therasse CERN BE/RF

CLEANROOM LAYOUT (Existing facility in SM18) Cleanroom facility RF facilities Magnet Cryogenic SM18, plan 01/08/2013 Mathieu Therasse CERN BE/RF

EXISTING ASSEMBLY AREA AND CLEAN ROOMS IN SM18 Assembly area ≈ 120 m2 “Baldaquin”: ISO 5 clean room (for tall items such as HIE ISOLDE cavities, main couplers) Two 13 meters long clean rooms (ISO 7, ISO 4) used for the LHC cryo module assembly 01/08/2013 Mathieu Therasse CERN BE/RF

CLEANROOM LAYOUT (Actual) ISO 7 ISO 4 Air Box ISO 14644-1 FS 209 4 10 5 100 7 10 000 Built in 1991. Goals : Increase cleanliness. Create a rinsing room. Get ride of the Air Box to gain space. 01/08/2013 Mathieu Therasse CERN BE/RF

CLEANROOM LAYOUT (Updated facility in SM18) Arragement of the area will start in September 2013 01/08/2013 Mathieu Therasse CERN BE/RF

CLEANROOM LAYOUT (Updated) ISO 5 ISO 4 ISO 5 ISO 4 Optical Inspection Daldrop will start the refurbishment by end of 2013 Extension of the rinsing room Creation of a preparing room outside of the facility 01/08/2013 Mathieu Therasse CERN BE/RF

CLEANROOM LAYOUT (Updated) Refurbishment of the filtering system with Fan Filter Unit (FFU). Rinsing room extended to 4.5m height to support the HPR. Preparing room based on softwall design. 01/08/2013 Mathieu Therasse CERN BE/RF

HIGH PRESSURE RINSING (HPR) We will receive the HPR in September 2013 HPR from SPEC (US) HP pump (140 bar, 1.1 m3/h) @ 3 stages to prevent vibration Rinsing cabinet with top wand design (needed in SM18) Cabinet should shall have a pass trough design => load/unload from different class cleanrooms Drying of the cavity by blowing hot N2 We will receive the HPR in September 2013 01/08/2013 Mathieu Therasse CERN BE/RF

ULTRA PURE WATER PRODUCTION From Veolia France Production capacity of 1 m3/h Installation will start mid of September 2013 01/08/2013 Mathieu Therasse CERN BE/RF

Mathieu Therasse CERN BE/RF RF TEST FACILITES 01/08/2013 Mathieu Therasse CERN BE/RF

NEW RF CRYO INFRASTRUCTURE AT SM18 The new cryo line is available since April 2013 Restart of each test stand is ongoing Vertical test stands 2 new cryostats for measurement at 2K - 1 Long (h= 4m) for Crab (400 MHz) and SPL (704 MHz) cavities 1 short cryostat (2.5m) - Welded connection - Integrated pumping - Active screening - Earth magnetic field compensation 2 cryostats for measurement at 4.5K - 1 long (4m) for spare LHC cavities - 1 short (2.4m) for HIE-ISOLDE 01/08/2013 Mathieu Therasse CERN BE/RF

NEW RF CRYO INFRASTRUCTURE AT SM18 Horizontal test stands Bunker A: - Linac 4 RF structure tests Makes use of the existing 352 MHz power system & rad. safe bunker - SPL: 2013 704 MHz RF power system will replace the 352 MHz system 4.5K and 2K measurement Hard cryogenic connection Bunker B: - LHC Spare cryo modules tests, development of LLRF electronics & control tool - HIE-ISOLDE cryo modules Flexible or Hard cryogenic connection CCDTL Dismantling old lines 01/08/2013 Mathieu Therasse CERN BE/RF

Mathieu Therasse CERN BE/RF RF POWER ZONE Equipped with: Demineralized cooling water 100 kV, 40 A power converter 400 MHz, 300 kW CW LHC power system 352 MHz, 1.2 MW pulsed power system (1.6ms/2Hz) - Later a 704 MHz pulsed power system will be installed (1.6 ms / 50 Hz) Very crowded area: Cannot be significantly extended (unfortunately) Installation of additional power source + associated power distribution system to be studied in details…but look rather complicated! 01/08/2013 Mathieu Therasse CERN BE/RF

AVAILABILITY FOR CRAB CAVITY Cavity tests: -1st test was done in November 2012 (cavity was leaky) -The cavity is installed in the cryostat with a new support -The test will be done in August with the test of the new cryo cooldown process Cryo-module tests: Power source is ok (400 MHz, 300 KW) Bunker A: need to install a new power distribution Complicated (no space), we have to study this in detail, and manage with the other projects Bunker B: need of adaption for the cryo connection for 2K (flexible or hard) 01/08/2013 Mathieu Therasse CERN BE/RF

Mathieu Therasse CERN BE/RF RF CONTROL ROOM Common control room for: Each vertical cryostats Each RF bunkers - Complete LLRF system 01/08/2013 Mathieu Therasse CERN BE/RF

RF CONTROL RACK FOR VERTICAL TEST STAND 01/08/2013 Mathieu Therasse CERN BE/RF

TEST CONTROL PANEL PROGRAM Labview Program by A. Benoit BE/RF 01/08/2013 Mathieu Therasse CERN BE/RF 19

Mathieu Therasse CERN BE/RF DIAGNOSTIC SYSTEMS 01/08/2013 Mathieu Therasse CERN BE/RF

OSCILLATING SUPERLEAK TRANSDUCER AND TEMPERATURE MAPING OSTs installed around the 4 rods Temperature mapping for elliptical cavity : Using Allen-Bradley resistors temperature sensor (K.Liao) can be adapted for crab cavity Localized hot spot (default) with 2nd sound propagation in He superfluid method 01/08/2013 Mathieu Therasse CERN BE/RF Ref: K. Liao BE/RF

Mathieu Therasse CERN BE/RF OPTICAL INSPECTION Camera: 3488 x 2616 pix @ 2.5 ips Cavity can: Slide Rotate Camera can: Rotate over 180° We have to study how can we adapt it for the crab cavity inspection (support, diameter 70 mm) 01/08/2013 Mathieu Therasse CERN BE/RF Ref: J.Chambrillon BE/RF

Mathieu Therasse CERN BE/RF CONCLUSIONS Preparation and assembly: - Clean room upgrade for high performance cavity at SM18 - New HPR Diagnostic systems: - OST - Temperature mapping - Optical inspection Low power tests: - Four vertical cryostats (2 K & 4.5 K) - New RF cryo line High power tests: - Two bunkers - Bunker A (4.5K): LHC, HIE ISOLDE - Bunker B (2 K): Linac4, SPL - High power area: - 352 & 400 MHz high power sources available Difficult @ 400 MHz or/and 2 K need adaptation for the cryo connections or need to install a new power distribution line over cost 01/08/2013 Mathieu Therasse CERN BE/RF