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LHCb MUON. Plans on GIF++ (16.65 TBq). What has been done for study of aging in MUON MWPCs and GEMs before RUN1: Six months on GIF ( 137 Cs, 675GBq of 662keV g ) in 2001 – four gap MWPC (prototype) accumulated ~0.255 C/cm of wire and 0.83 C/cm 2 of cathodes - PowerPoint PPT Presentation
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20.02.14 1
LHCb MUON. Plans on GIF++ (16.65 TBq)
Oleg Maev
What has been done for study of aging in MUON MWPCs and GEMs before RUN1:
- Six months on GIF (137Cs, 675GBq of 662keV) in 2001 – four gap MWPC (prototype) accumulated ~0.255 C/cm of wire and 0.83 C/cm2 of cathodes
- One month on Casaccia Calliope Facility with ~1,25MeV(60Co, ~1015Bq) – four MWPCs and one GEM tested. MWPCs accumulated ~0.44C/cm of wire.
In both tests no gain loss or other significant effect was detected.
20.02.14 2
New requirements on upgraded MUON
Oleg Maev
2008: “LHCb Detector at the LHC” J.Instrum.3 (2008) S08005
At a luminosity of 2x1032 cm2 s-1 the highest rates expected in the inner regions of M1 and M2 are respectively 80 kHz=cm2 and 13 kHz=cm2 per detector plane. In the detector design studies, a safety factor of 2 was applied to the M1 hit multiplicity and the low energy background in stations M2-M5 has been conservatively multiplied by a factor of 5 to account for uncertainties in the simulation.
2013:”LHCb PID Upgrade Technical Design Report”Instantaneous luminosity of 2x1033 cm2 s-1 and for an integrated luminosity of 50 fb-1
Average deposited charge (C/cm of wire) after 50 fb-1 in the most irradiated chamberof each station and region of the muon system.
R1 R2 R3 R4
M2 0.67 0.42 0.1 0.02
M3 0.17 0.08 0.02 0.01
M4 0.22 0.06 0.01 0.004
M5 0.15 0.03 0.01 0.003
At L~2x1032 cm2s-1 ~1C/cm ofwire expected at max. in 10 years- M1 in the detector
At L~2x1033 cm2s-1 ~3C/cm ofwire expected at max. in 10 years (50fb-1)- M1 removed
20.02.14 3
Plans (very preliminary)
Oleg Maev
In order of priority:1. Aging study with set of chambers from inner regions and probably with couple of
chambers from outer regions in shadow – approximately 3-4 months on GIF++ in 2015.2. Some aging study would be desirable with prototypes of high granularity detectors (new
MWPCs and new GEMs) which are under design now for LS2-LS3. It depends on readiness of prototypes. Apparently, it could happened not early than in second half of 2015.
3. As a byproduct study it would be very interest to investigate on GIF++ a method for curing MUON chambers suffered with Malter currents by adding a small amount of oxygen (~0.2-2%) in the nominal Ar(40%)/CO2(55%)/CF4(5%) gas mixture with reverse polarity (negative) and at nominal HV.
See first results in https://indico.cern.ch/getFile.py/access?contribId=3&resId=1&materialId=slides&confId=289760
It could be organized in shadow of 1.
- optimizing the percentage of oxygen in gas mixture- test the method on number chambers suffered with Malter-currents to prove it even
statistically.
20.02.14 4
Infrastructure
Oleg Maev
Aging:1. Gas: MWPCs – nominal mixture:Ar(40%)/CO2(55%)/CF4(5%) 2- 10 l/h GEM – nominal mixture: Ar(45%)/CO2(15%)/CF4(40%) 10-15 l/h - for GEM the mixture potentially could be changed a bit with reducing of CF4
2. HV: MWPCs – CAEN SY2527 GEM – INFN’s PS3. Environment, monitoring atm P,T, H
Malter-currents study:
In general, infrastructure same as for aging, just a couple of additional options:1. Option for admixing a few percent (0,2 -5%) of oxygen2. Very likely a picoampermeter and precise flow mass controller would be
needed
20.02.14 5
News from GIF++ meeting
Oleg Maev
Schedule
612/02/2014A. Fabich, EN-MEF-LE
EDMS 1328252 V0.3
Functional specs:
-Juli 2013
Functional specs:
-Juli 2013 Design-Dec. 2013
Design-Dec. 2013
CE startJan. 2014CE start
Jan. 2014
Infrastructure installation
March-July 2014
Infrastructure installation
March-July 2014Irradiator delivery
Aug. 2014
Irradiator delivery
Aug. 2014
Commissioning Sept.-Oct. 2014Commissioning Sept.-Oct. 2014
Mid May: ready for PH equipment in gas zone
Beginning June: ready for lower muon tracker
Beginning July: ready for PH/users’ equipment in bunker
Decommissioning in the West Area
March: removal of blocks upstream of GIF (no impact on operation)
August/September: secure irradiator
Autumn 2014: removal of infrastructure and concrete castle (SBA)
GIF++ layout (1)
712/02/2014A. Fabich, EN-MEF-LE
dump
secondary beam
PPE (entrance)
MAD
PPG
PPX (only emergency)
dump
service zone
Preparation zone
cable trays to control room
Irradiation area
Service zone: gas (mixing) zone
8
Supply lines for 15 gases simultaneously
40 m2 net area
8 distribution panels with each 6 return lines
17 racks for gas equipment
6 km of piping (304L / 316L)
12/02/2014A. Fabich, EN-MEF-LE
Irradiator
9
hosting a 137 Caesium source: 14 TBq
Irradiator will be equipped with a identical filter system on both sides (up- and down-stream)
30/1/2014
A. Fabich, EN-MEF-LE
DCS ReminderUse PVSS/WinCC OA (as in LHC experiments)
Many components, devices, HW and SW already available (CAEN System, CAN PSU, ELMB, ENV Sensors, VME crates etc.)
CAEN Easy Power System
1 mainframe, 1 Power Generator, 1-2 crates + with HV and LV boards(*) and 1 ADC A-3801 board for monitoring (128 channels), this includes also ENV and gas monitoring
(*) Some Low Voltage possibly external (non CAEN) with remote control via PVSS
Mainframe and PCs possibly placed proximity of the control room (non radiation area) along with DAQ PCs and equipment.
EASY crates and other equipment, more close to detector area.
10A. Polini
10
Mainframe
OP
C
BranchControllers HV/LV Boards
Crate1 Crate2
…
AC/DC converter
48V 48V
…
Hostile Area
Counting Room
A. Polini
Gif++ CERN February 12th 2014 A. Polini
20.02.14 Oleg Maev
20.02.14 12
Preliminary conclusions
Oleg Maev
1. In overall, infrastructure provided by GIF++ facility looks quite good for an
aging test of muon chambers.2. Looks reasonable to use own cables and HV PSs.3. Number of gas mixers and distributors allows to plan most of work and
even studies for MUON, but oxygen for Malter-study4. Proposed strategy: to be ready for an aging test of existing chambers and
prototypes of high granularity detectors before second half of 20155. Some program for Malter-current study in shadow of aging test would be
desirable.6. During preparation of this test, it would be good to continue Malter study in
the PIT this year.7. For the control of aging test on GIF++ a WINCC OA – project would be
useful.8. Involving additional manpower for 2015 is needed.9. Problem – visit’s money for this year at least.
20.02.14 13
Backup
Oleg Maev
20.02.14 Oleg Maev
Malter effect SOURCES:
Avalanche producing polymers deposits
Some oxides are highly resistive.
Constructions material and gas pollutants.
Insulating deposits left from sparks.
Corona on sharp point on the cathode.
Fingerprints
Etc. Ignition mechanisms:
a) Highly ionizing heavy ions.
b) X-rays.
c) Sparks.
d) Sharp points on electrodes causing corona.
Necessary condition for electron emission:a) Localized primary ionization deposit.b) An insulator on the cathode.c) A rate of the charge build up is higher than its removal rate.d) Excessive field cathode gradients help to trigger it.e) To start the effect, it needs an ignition.
14
20.02.14 Oleg Maev
“Good” additive – OxygenOxygen ionization reactions in avalanche:
e-+ O2→ O2+ +2e-
e-+ O2→ 2O* + e-
e-+ O2→ O2-
e-+ O2→ e- + O+ + O-
It well known in the Plasma Chemistry that the oxygen radicals and ions excellent reacts with organic compounds and the end product of this reaction are volatile molecules such as CO, CO2, H2O, H2 etc. which are most stable,
and can be removed by gas flow
Practical examples:
The rate of removal of organic polymeric material can be often increased in an oxygen plasma (H. Boeing, Plasma Sci.&Tech., page 281) 1987.
Cleaning of mirrors of the contaminating films by a glow discharge in oxygen plasma. (R. Gillette et al., Vac. Sci. Tech., 7 (1070) 534)
Recovery from the Malter effect deposits by Oxygen (A. Boyarski – BaBar R&D study) 2001.
15
Inverted HV
20.02.14 Oleg Maev
Scanning the CMB with radioactive sources
Scanning with Sr90 - J~70 nA/cm2 ignited the Malter current in two places in GAP A
Scanning with source Am241
(J~0.3 nA/cm2) - no visible effect
16
Beam in 2012:
J~0.1 nA/cm2