Engineering Design Review

Slides:



Advertisements
Similar presentations
GEM Chambers at BNL The detector from CERN, can be configured with up to 4 GEMs The detector for pad readout and drift studies, 2 GEM maximum.
Advertisements

08 September 2009 A.Kashchuk INFN-Ferrara and PNPI-St.Petersburg 1 A.Kashchuk
Drift velocity Adding polyatomic molecules (e.g. CH4 or CO2) to noble gases reduces electron instantaneous velocity; this cools electrons to a region where.
D. Peterson, “Measurements of GEM electron and ion transmission…”, Valencia LC Workshop, Measurements of GEM electron and ion transmission.
Bulk Micromegas Our Micromegas detectors are fabricated using the Bulk technology The fabrication consists in the lamination of a steel woven mesh and.
1 Sep. 19, 2006Changguo Lu, Princeton University Induced signal in RPC, Configuration of the double gap RPC and Grouping of the strips Changguo Lu Princeton.
1 VCI, Werner Riegler RPCs and Wire Chambers for the LHCb Muon System  Overview  Principles  Performance Comparison: Timing, Efficiency,
Werner Riegler CERN, November 2003 CARIOCA Werner Riegler, CERN November 24 th, 2003, LHCb week Discussion of the final Prototype results Plans for CARIOCA.
PNPI in LHCb A.Vorobyov HEPD Scientific Board meeting, December 26,2003 Status report for 2003.
D. Peterson, “The Cornell/Purdue TPC”, LCWS05, Stanford, 21-March The Cornell/Purdue TPC Information available at the web site:
Prototype TPC Tests C. Lu 12/9/98 V = 0. Gas gain test for the low pressure chamber The chamber is constructed with the following parameters: D anode.
D. Peterson, “ILC Detector Work”, Cornell Group Meeting, 4-October ILC Detector Work This project is supported by the US National Science Foundation.
Ionization. Measuring Ions A beam of charged particles will ionize gas. –Particle energy E –Chamber area A An applied field will cause ions and electrons.
D. Peterson, “The Cornell/Purdue TPC”, ALCPG, Snowmass, 23-August The Cornell/Purdue TPC Information available at the web site:
Detectors. Measuring Ions  A beam of charged particles will ionize gas. Particle energy E Chamber area A  An applied field will cause ions and electrons.
PRODUCTION and CERTIFICATION of Multi Wires Proportional Chambers for the LHCb Muon System at CERN K.Mair for the LHCb Muon Group CERN* Poster anlässlich.
Mauro Raggi Status report on the new charged hodoscope for P326 Mauro Raggi for the HODO working group Perugia – Firenze 07/09/2005.
A.Kashchuk Muon meeting, CERN Presented by A.Kashchuk.
Chamber parameters that we can modify and that affect the rising time Number of ionisation clusters produced in the drift gap: Poisson Distribution Probability.
1 Small GEM Detectors at STAR Yi Zhou University of Science & Technology of China.
6 Feb (update) A.P.Kashchuk (LNF/INFN, on leave from PNPI) 1 Triple GEM is the best candidate for station M1 regions R1/R2 Triple GEM has better.
PHENIX Drift Chamber operation principles Modified by Victor Riabov Focus meeting 01/06/04 Original by Sergey Butsyk Focus meeting 01/14/03.
Chevron / Zigzag Pad Designs for Gas Trackers
David Emschermann CBM Collaboration Meeting - GSI – 12/04/2010 TRD geometry in CBMroot and conclusions for detector module design David Emschermann Institut.
VCI 2004Gaia Lanfranchi-LNF/INFN1 Time resolution performances and aging properties of the MWPC and RPC for the LHCb muon system Gaia Lanfranchi – INFN/LNF.
EPS-HEP 2015, Vienna. 1 Test of MPGD modules with a large prototype Time Projection Chamber Deb Sankar Bhattacharya On behalf of.
LHCb VErtex LOcator & Displaced Vertex Trigger
Elba, 27 May 2003Werner Riegler, CERN 1 The Physics of Resistive Plate Chambers Werner Riegler, Christian Lippmann CERN.
Using delay lines on a test station for the Muon Chambers Design considerations (A. F. Barbosa, Jul/2003)
A TPC for ILC CEA/Irfu, Apero, D S Bhattacharya, 19th June Deb Sankar Bhattacharya D.Attie, P.Colas, S. Ganjour,
Main Drift Chamber Yuanbo Chen Ihep Motivation (MDC IV) The BGO crystal used in L3 will be used for BES III ’ s Calorimeter. The space for MDC.
3D Event reconstruction in ArgoNeuT Maddalena Antonello and Ornella Palamara 11 gennaio 20161M.Antonello - INFN, LNGS.
Tests of RPCs (Resistive Plate Chambers) for the ARGO experiment at YBJ G. Aielli¹, P.Camarri¹, R. Cardarelli¹, M. Civardi², L. Di Stante¹, B. Liberti¹,
CBM workshop on Muon ID B.Schmidt Muon Identification in LHCb Workshop on Muon Detection in the CBM Experiment Outline: Introduction –Physics.
2002 LHC days in Split Sandra Horvat 08 – 12 October, Ruđer Bošković Institute, Zagreb Max-Planck-Institute for Physics, Munich Potential is here...
Abstract Beam Test of a Large-area GEM Detector Prototype for the Upgrade of the CMS Muon Endcap System V. Bhopatkar, M. Hohlmann, M. Phipps, J. Twigger,
Beam Test of a Large-Area GEM Detector Prototype for the Upgrade of the CMS Muon Endcap System Vallary Bhopatkar M. Hohlmann, M. Phipps, J. Twigger, A.
15/6/2006Gaia Lanfranchi - LNF-INFN1 Why do we have to measure efficiencies in the Muon Detector? Muon Software Meeting, June 15th G. Lanfranchi LNF-INFN.
1 9 December 2002A.P.Kashchuk (LNF/INFN), Frascati) New approach to CPC design.
Development of a Single Ion Detector for Radiation Track Structure Studies F. Vasi, M. Casiraghi, R. Schulte, V. Bashkirov.
Eight fully instrumented PC1 mounted on top of the Drift Chamber. Qualities * Efficiency close to 100% and good spatial resolution. Noise free operation.
Werner Riegler, CERN1 Electric fields, weighting fields, signals and charge diffusion in detectors including resistive materials W. Riegler, RD51 meeting,
Engineering: MWPC design configuration schemas. Wire Pad Chamber (WPC), one gap Avalanche Cdet in parallel to current source (not shown) will reduce current.
Performances of a GEM-based TPC prototype for the AMADEUS experiment Outline: GEM-TPC in AMADEUS experiment; Prototype design & construction; GEM: principle.
FWD Meeting, Torino, June 16th, News from Cracow on the forward tracking J. Smyrski Institute of Physics UJ Tests of CARIOCA and LUMICAL preamplifiers.
Werner Riegler, Christian Lippmann CERN Introduction
1 straw tube signal simulation A. Rotondi PANDA meeting, Stockolm 15 June 2010.
Space Charge Effects and Induced Signals in Resistive Plate Chambers
The ALICE-TOF system 1. Quick overview of the TOF system that we are building 2. The Multigap Resistive Plate Chamber -what is it? 3. Difference in.
GEM TPC Resolution from Charge Dispersion*
An extension of Ramo's theorem to include resistive elements
Comments on 2mm MWPC pitch
Activities on straw tube simulation
ATLAS-MUON Trigger hardware developments
CMS muon detectors and muon system performance
Integration and alignment of ATLAS SCT
Numerical simulations on single mask conical GEMs
News on second coordinate readout
Numerical simulations on single mask conical GEMs
TPC Paul Colas Technical meeting, Lyon.
A Fast Binary Front - End using a Novel Current-Mode Technique
High Precision Wire Chambers
Ionization detectors ∆
Performance of a Multigap RPC prototype for the LHCb Muon System
Status of the CARIOCA project
High Rate Photon Irradiation Test with an 8-Plane TRT Sector Prototype
Pre-installation Tests of the LHCb Muon Chambers
Resistive Plate Chambers performance with Cosmic Rays
Werner Riegler, Christian Lippmann CERN Introduction
A DLC μRWELL with 2-D Readout
Presentation transcript:

Engineering Design Review MWPC requirements Engineering Design Review April 16th 2003 Werner Riegler CERN Delia is a technical student (engineer), Nicolas is a project associate (engineer) Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 LHCb Muon System 5 muon stations, one in front (M1), 4 behind (M2-M5) the calorimeter A muon trigger requires the coincidence of hits in all 5 stations within the bunchcrossing time of 25ns in a certain spatial window that selects the muon momentum. Granularity 1x2 cm to 10x20cm. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 PNPI proposal: 1.5/2mm pitch, 5mm full gap, 30m wire, Ar/CO2/CF4 gas mixture, double gap, wire pads, cathode pads Wire pad chamber for LHCb muon system, B. Botchine, A.Kashchuk, V. Lazarev, N. Sagidova, A. Vorobiev, A. Vorobyov, LHCb-2000-003 Detector physics and performance simulations of the MWPCs for the LHCb muon system, W. Riegler, LHCb-2000-060 Crosstalk, cathode structure and electrical parameters and of the MWPCsfor the LHCb muon system, W. Riegler, LHCb-2000-061 Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Detector 2 chamber layers are connected into one frontend. 4 layers of MWPCs are combined into one station. Werner Riegler CERN, April 16th, 2003

Difference to ATLAS, CMS The ATLAS Cathode Strip Chambers are intended for position resolution. Amplifier peaking time 80ns, bipolar shaping, ‘crosstalk intended’ on cathode strips for center of gravity. The CMS Cathode Strip Chambers are intended for position resolution (cathodes strips) and timing (wires). Cathode amplifier peaking time 100ns, wire amplifier peaking time 30ns. The LHCb MWPCs are intended for highly efficient timing within a certain spatial granularity at the LVL0 trigger. Amplifier peaking time of 10ns, pulse width<50ns, unipolar shaping, low crosstalk. Since crosstalk is  RinCpp and since  (20 MHz) is high we have to minimize the pad-pad capacitance Cpp and amplifier input impedance Rin. Because we want unipolar shaping we need a baseline restorer in the front end. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Geometry and Fields Volt /cm Pitch 2 mm Gap 5 mm Wire 30 m HV 2750 V Cathode field 6.2 kV/cm Wire field 262 kV/cm cm Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Gas Properties For 10 GeV muons we expect about  42/45 clusters/cm    0.24/0.22 mm  2.35/2.38 e-/cluster,  99/107 e-/cm Drift velocity of 90-100m/ns is ‘saturated’ meaning that a small change in electric field does not affect the time resolution. Werner Riegler CERN, April 16th, 2003

Electron Drift Isochrones (ns) 2mm pitch 1.5mm pitch 5 5 10 10 15 15 20 20 25 30 25 30 Average arrival of electrons is  30ns. It seems that time resolution can always be improved by reducing the wire pitch, BUT Werner Riegler CERN, April 16th, 2003

Ionization Statistics Because the primary ionization statistics I.e. Poisson distributed cluster number =exponentially distributed distance between clusters around average of 0.23mm the Time resolution doesn’t improve for pitch <1.5mm. This is a fundamental limit of time resolution for an MWPC at 1bar. Werner Riegler CERN, April 16th, 2003

Choice of Parameters and Specifications Wire Pitch Gas Gap Wire Diameter Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 ra: anode wire radius Va: anode wire voltage : ion mobility q: charge per hit R: hits/cm2 1) rc=(s/2) Exp(h/s) Equivalent cathode radius 2) Ea=Va/(ra ln(rc/ra)) Anode wire surface field 3) Ec= Va/(s ln(rc/ra)) Cathode surface field 4) t0= ra2 ln(rc/ra)/(2Va) Signal tail 5) I(t)= q/2ln(rc/ra) 1/(t+t0) Induced Signal 6) Q(t)=q/(2ln(rc/ra))*ln(1+t/t0) Induced charge (ions) after time t 7) V=Rsh2q ln(rc/ra)/(4Va0) Voltage drop due to space charge effect 8) Ec/Ea= ra/s Ratio of wire to surface field (3)/(4) 9) Va= Eara (h/s+ ln(s/2  ra)) Voltage for a given surface field (1),(2) 10) G = [V/(ra ln(rc/ra)Emin)]^[Vln2/ (ln(rc/ra)dV)] Gas Gain, Emin, dV Diethorn param. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Choice of Wire Pitch At fixed gap 5mm, gas gain 0.75*105 and wire diameter 30m: Increasing the pitch 1.5 2 2.5 mm is HV 3.15 2.75 2.53 kV/cm  good Cathode surface field 8.24 6.2 4.95 kV/cm  good Wire surface field 262 262 262 kV/cm  ------ Sensitivity to imperfections  good Signal tail t0 1.5 1.5 1.5  ------ Signal integrated after 10ns 12.7 14.6 15.8 %  bad Pulse width, last electron: 30 30 30 ns  ------ Time Resolution  bad dV @ 1MHz (300e-/cm) 20 27 34 V  bad Cathode charge distribution  ------ Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Choice of Gas Gap At fixed pitch 2mm, gas gain 0.75*105 and wire diameter 30m: Increasing the Gap 4 5 6 mm is HV 2.44 2.75 3.06 kV/cm  bad Cathode surface field 6.2 6.2 6.2 kV/cm  ------ Wire surface field 262 262 262 kV/cm  ------ Sensitivity to imperfections  good Signal tail t0 1.5 1.5 1.5  ------ Signal integrated after 10ns 16.4 14.6 13.1 %  bad Pulse width, last electron: 24 30 36 ns  bad dV @ 1MHz (300e-/cm) 14 27 47 V  bad Cathode charge distribution  bad Werner Riegler CERN, April 16th, 2003

Choice of Wire Diameter At fixed pitch 2mm, gas gain 0.75*105 and gap 5mm Increasing Wire Diameter 10 30 50 m is HV 2.23 2.75 3.11 kV  bad Cathode Surface Field 4.33 6.2 7.5 kV/cm  bad Wire Surface Field 552 263 192 kV/cm  good Sensitivity to imperfections  ----- Signal tail t0 0.24 1.5 3.4 ns  bad Signal integrated after 10ns 23 15 10 %  bad Pulse width, last electron: 30 30 30 ns  ----- dV @ 1MHz (300e-/cm) 39 27 22 V  good Wire Stability  good Cathode charge distribution  ----- Werner Riegler CERN, April 16th, 2003

Sensitivity of the performance on chamber imperfections The drift velocity is saturated I.e. it has a very weak dependence on the electric field. Therefore we mainly worry about gas gain variations that can move the working point within the plateau. If G0 is the nominal gas gain, we want the gas gain in 95% of the area of a single gap to be within G0/1.25 and G0*1.25 I. e. between 0.8G0 and 1.25G0. The remaining 5% of the area should have a gain within a factor 1.5 I.e. between 0.67G0 and 1.5G0 A gain change of a factor 1.25(1.50) corresponds to Voltage change of 34(62)V on top of the 2750V corresponding to 1.25(2.25)%. The gas gain changes by a factor 1.25(1.5) if the wire surface field changes by 1.25(2.25)%.  What chamber imperfections are allowed in order to keep the wire surface field within 1.25(2.25)% ? Werner Riegler CERN, April 16th, 2003

Measured Efficiencies 40V 40V 60V 60V Wires Cathodes Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 The entire wire plane has to be within 370(490)m in y direction. The cathode - cathode has to be within 113(202)m. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003  y  x A single wire has to be within 350(450)m in y direction. A single wire has to be within 163(293)m in x direction. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Specifications Keeping everything else in perfect position, for a single gap chamber with 5mm gap, 30m wire and 2mm pitch, the allowed offset in order to find a wire surface field difference of 1.25(2.25)% is gap: 113 (202) m single wire X: 163 (293) m single wire Y: 350 (450) m wire plane Y: 370 (490) m Which we translate into specifications of gap: 95% in 90m 1% 5% in 180m 2% pitch: 95% in 50m 0.35% 5% in 100m 0.7% wire y-offset: 95% in 100m 0.1% 5% in 200m 0.4% wire plane y-offset: 95% in 100m 0.1% 5% in 200m 0.42% Added in squares: 1.07% 2.2% Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Specifications Moving everything in the worst direction: gap: -90m 1.00% wire plane: +100m 1.12% single wire Y: +100m 1.14% 1.38% 1.14% single wire X: -50m/0/+50m 1.18% 2.10% 1.18% Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Guard Wire Without a guard wire the wire surface fields and gas gains on the edge wires would be 301 269 263 262 … kV/cm 11 1.2 0.8 0.7 … x 105 Using a 200m diameter guard wire at the same pitch of 2mm gives 70.4 251 260 262 … kV/cm 0.0012 0.4 0.6 0.7 … x 105 Werner Riegler CERN, April 16th, 2003

Wire Tension, Instability We use a 30m wire with 60g tension (half of the elastic limit). The maximum allowed wire length for a gas gain of 106 would be 65cm. We use a maximum wire length of 30cm i.e. we are safe. Wire sag is not an issue since the wires are vertical. We specify that no wire should have a tension of less than 50g. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Many ‘different’ chamber types with different capacitance, grounding, signal flow … Werner Riegler CERN, April 16th, 2003

Crosstalk Specification Double gap chamber 95% efficiency if the threshold is set to 30% of the average signal. 99% efficiency if the threshold is set to 20% of the average signal. In order to have a double gap chamber well within the plateau we want to be able to use a threshold of 15% of the average signal. Werner Riegler CERN, April 16th, 2003

Specification of Capacitive Crosstalk Crosstalk due to ‘direct induction’ is ‘irreducible’ and given by our choice of 2.5mm cathode-wire distance. In case of a hit on a given pad, the probability that a neighboring pad fires should be < 5%. We want to be able to operate the chamber at a threshold of 15% of the average muon signal. This specifies the ‘crosstalk ratio’ I.e. the fraction of signal allowed signal on a neighbor pad: Assuming 95% of the signals within 3x average the crosstalk ratio has to be < 15%/3 = 5%. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Pads, Readout Traces 0.5mm guard trace between pads 0.4mm gap between pad and guard trace 1.6mm boards in case of traces 0.8mm board otherwise 0.25mm readout traces 0.25mm guard traces at 0.25mm pitch We carefully studied readout and guard trace geometries to minimize crosstalk. Calculations were done with MAXWELL. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Crosstalk Simulation We modeled each chamber including all pads, mutual capacitances, amplifiers … Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Crosstalk Simulation 35-95 pF Cathode Pad Capacitance 15-209 pF Wire Pad Capacitance maximum pad-pad capacitance 3.95 pF maximum crosstalk 2.27 % maximum opposite sign crosstalk - 7.31 % Werner Riegler CERN, April 16th, 2003

Crosstalk Measurement Crosstalk on M2M3R1 prototype at very high gas gain (1.8 x 105) is still <5%. Werner Riegler CERN, April 16th, 2003

Werner Riegler CERN, April 16th, 2003 Crosstalk, Stability We have a very good clue and understanding of the ‘smooth RC’ behavior of the chambers. Since we have large capacitances (up to 220pF), even very small voltage drops due to parasitic inductances and ‘bad’ grounding can cause problems. E.g. a 20V signal on the ground together with a 200pF capacitance fires the 5fC threshold. Although we had every chamber type in stable conditions in a testbeam the frontend-board to chamber connection has still to be properly engineered. Werner Riegler CERN, April 16th, 2003