Report on Measurements in the Lab with R11, R12, R13 Alexandra - - PowerPoint PPT Presentation

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Report on Measurements in the Lab with R11, R12, R13 Alexandra - - PowerPoint PPT Presentation

Report on Measurements in the Lab with R11, R12, R13 Alexandra Moskaleva What is a resistive chamber? Non-resistive Micromegas Resistive Micromegas (R11, R12, R13) Resistive Characteristics CHAMBER R11 R12 R13 Resistance to 15 45 20


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SLIDE 1

Report on Measurements in the Lab with R11, R12, R13

Alexandra Moskaleva

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SLIDE 2

What is a resistive chamber?

Non-resistive Micromegas Resistive Micromegas (R11, R12, R13)

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SLIDE 3

Resistive Characteristics

CHAMBER

R11 R12 R13

Resistance to Ground (MΩ) 15 45 20 Resistance along strip (MΩ/cm) 2 5 0.5

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SLIDE 4

Types of Measurements

 Properties

 Gain  Transparency  Response to cosmics  Charge-up  High rate behavior

 Tools

 5 keV 55Fe source  8 keV X-ray gun at various rates  120 GeV pion test beam

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SLIDE 5

Gain & Transparency Measurement – Set up

HV Drift HV Mesh Gas in Gas out

55Fe tablet

Read out connectors Protective cover with holes

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SLIDE 6

 Each read-out connector connected to 72 strips

 Covers a cross-section of 18 mm

 Strips that are not read out are grounded

18 mm

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SLIDE 7
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SLIDE 8

Example Spectrum

55Fe (5.9 keV) Peak

Ar escape peak (3 keV lower)

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SLIDE 9

 Peak of 55Fe taken in arbitrary units from spectrum

 Rate, counts, live time, start time also displayed

 Converted to gain via calibration signal

 Calibration pulse = 104 gain

 Gain measurements taken for:

 R11, 93% Ar 7% CO2  R12, 93% Ar 7% CO2  R12, 85% Ar 15% CO2  R13, 93% Ar 7% CO2  R13, 85% Ar 15% CO2

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SLIDE 10

Gain Measurements - Results

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SLIDE 11
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SLIDE 12
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SLIDE 13

Transparency Measurements

 Transparency =

(# of e– that make it to the amplification field) (Total # of e– produced)

 Transparency measurements taken for:

 R12, 93% Ar 7% CO2  R12, 85% Ar 15% CO2  R13, 93% Ar 7% CO2  R13, 85% Ar 15% CO2

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SLIDE 14

Transparency Measurements – Set up

 Measured gain as a function of Eamplification/Edrift

 Kept Vmesh constant  Varied Vdrift  E=V/d, where V is the voltage difference and d is the

distance  Edrift = (Vmesh-Vdrift)/d ≈ 300V/5mm ≈ 600 V/cm  Eamplification = (Vmesh-Vground)/d ≈ 500V/.128mm ≈ 40 kV/cm

 Normalized highest gain = 1

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SLIDE 15
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SLIDE 16
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SLIDE 17

Cosmic Measurements – Set up

 Stacked R11, R12, R13 with 15mm spacers  Used R11 and R13 to trigger, R12 to acquire

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SLIDE 18

HV Drift R11 R12 R13

Top

HV Mesh top

Bottom

HV Mesh bottom HV Mesh middle

MCA

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SLIDE 19

Top Threshold NIM  TTL Gate for MCA Bottom Threshold

Cosmics – Logic

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SLIDE 20

Cosmics - Results

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SLIDE 21

55Fe (5.9 keV) Peak

Cosmic most probable value

55Fe produces 225 e– in drift region, with a peak ≈ 420

Cosmics produce a peak ≈ 100 (a factor of ¼)

Therefore, cosmics produce ≈ 50 e– in 5mm drift region

Agrees with 90 e–/cm for Ar and for CO2

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SLIDE 22

Charge Up – Theory

 Charge is deposited on the detector in <2mm radius for

every photon  Due to dispersion in electron avalanche

 Some charge deposits on resistive strips

 Runs to ground due to relatively low resistance

 Some charge deposits on insulative area

 Cannot drain away as quickly  builds up an excess of

negative charge

 No longer at ground

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SLIDE 23

 Charge is deposited on resistive and insulative strips  Footprint of roughly 2mm in diameter

≈2mm

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SLIDE 24

 Charge leaks away through the resistive strips  Takes much longer to leak away charge from insulative

portion

 If the rate of deposition >> rate of discharge, then there

is a buildup of charge

 Eamplification decreases

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SLIDE 25

 Charge deposited per second:  Rate = 200 Hz

 (200 Hz) × (225 e– per photon) × (104 gain) × (1.6 × 10-19)

≈ .06 nA

 Rate = 20k Hz

 (20000 Hz) × (225 e– per photon) × (104 gain) × (1.6 × 10-19)

≈ 6 nA

 Δ Voltage (very rough estimations of what to expect)

 In resistor

 Low rate: V = IR = .06 nA × 108 Ω = .006 V  High rate: V = IR = 6 nA × 108 Ω = .6 V

 In insulator

 Low rate: V = IR = .06 nA × 1010 Ω = .6 V  High rate: V = IR = 6 nA × 1010 Ω = 60 V

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SLIDE 26

 Gain decreases due to decrease in Emesh

Δgain≈1600

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SLIDE 27

Δgain≈2000 Δgain≈1000

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SLIDE 28

Δgain≈5000 Δvoltage≈15V

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SLIDE 29

Conclusions

 Gain

 All chambers reach gain of ≈30k  With 93:7 Ar:CO2, the chambers can be operated at a HV 40V lower than

for 85:15 Ar:CO2

 R12 has highest gain, R11 has lowest

 Transparency

 For good transparency, Eamp/Edrift > 80  85:15 Ar:CO2 rises faster, but shows similar behavior to 93:7 Ar:CO2 in

steady state

 Cosmics

 Cosmic measurements show good results (Landau curve) with most

probable value showing creation of 50 e– in 5mm drift region, as expected

 Charge up

 Charge up is observed

 As function of rate (reducing gain by 10% at 200 Hz, 20% at 20 kHz)

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SLIDE 30

This has been an amazing summer! Thank you to everyone who has guided me in this experience!!!