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The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mu mbai, December 15-17, 2003 1 Development of RPCs for INO B.Satyanarayana TIFR, Mumbai, INDIA [email protected]

Development of RPCs for INO

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Development of RPCs for INO. B.Satyanarayana TIFR, Mumbai, INDIA [email protected]. Principle of operation. RPC test setup. Telescope. Cosmic muon trigger and timing. NIM and CAMAC electronics. Telescope rate monitoring. Gas mixing unit. Typical efficiency plot. Studies with gas mixtures. - PowerPoint PPT Presentation

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Page 1: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 1

Development of RPCs for INO

B.Satyanarayana

TIFR, Mumbai, [email protected]

Page 2: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 2

A passing charged particle induces an avalanche, which develops into a spark. The discharge is quenched when all of the locally ( ) available charge is consumed.

2cm 1.0r

The discharged area recharges slowly through the high-resistivity glass plates.

Before spark After spark

Signal pickup(X)

Signal pickup(Y)

GlassPlates

Graphite

Graphite

Spacer

++++++++++++++++++++

-------------------------++++++ ++++++

---------- -------

Principle of operation

Page 3: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 3

RPC test setup

Telescope

Page 4: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 4

P1P2

P3

P4P5

P6

RPC under test

Muon Trigger =654321 PPPPPP

Cosmic muon trigger and timing

Page 5: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 5

NIM and CAMAC electronics

Page 6: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 6

Telescope rate monitoring

215000

225000235000

245000

255000265000

275000

1 4 7 10 13 16 19 22 25 28 31 34 37 40

Time, Hours

Padd

le ra

tes

120000

125000

130000

135000

140000

145000

150000

1 3 5 7 9 11 13 15 17 19 21 23 25 27 29 31 33 35 37 39

Time, Hours

Padd

le ra

tes

32000

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34000

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36000

37000

1 3 5 7 9 11 13 15 17 19 21 23 25 27 29 31 33 35 37 39

Time, Hours

Pad

dle

rate

s

150

200

250

300

350

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1 4 7 10 13 16 19 22 25 28 31 34 37 40

Time, Hours

Trig

ger r

ates

Page 7: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 7

Gas mixing unit

Page 8: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 8

Typical efficiency plot

Page 9: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 9

Studies with gas mixtures

Page 10: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 10

Typical timing distribution plot

Page 11: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 11

Typical time response plot

Page 12: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 12

Typical time resolution plot

Page 13: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 13

Typical charge distribution plots

Page 14: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 14

Typical mean charge plot

Page 15: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 15

Typical noise rate plot

Page 16: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 16

Typical cross-talk plots

Page 17: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 17

Summary of cross-talk measurements

Gas Mixture Slit Size(mm) Cross talk(%)

62:8:30 10 6.8

62:8:30 15 6.7

62:8:30 20 6.2

57:8:35 20 6.5

52:8:40 20 5.9

46:8:46 20 6.3

Page 18: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 18

Effects of wet gases

Page 19: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 19

Recovering a damaged RPC

• Purging with pure Argon at high flow rate.• Bubbling pure Argon through pure ethyl

alcohol.• Bubbling pure Argon through 25% Ammonia

solution for 24 hours without electric field.• Recovers efficiency and brings down noise rate.• Detailed studies underway.

Page 20: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 20

RPC recovery plots

No of hours of gas flow

Page 21: Development of RPCs for INO

The 6th ACFA Workshop on Physics and Detector at Linear Collider, TIFR, Mumbai, December 15-17, 2003 21

Future plans

• Study of effect of wet gases on RPC performance, aging etc.

• Study of pickup strip materials, geometries & pulse characteristics

• Long term studies with small chambers.• Improvements in the gas mixing unit, Cosmic test

setup, etc.• Procurement of dry gases.• Production of 120cm X 90cm RPCs for prototype

detector