Preparation of TIF Hall for Production

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Preparation of TIF Hall for Production Andrey Marinov On behalf of GEMs for CMS Collaboration

description

Preparation of TIF Hall for Production. Andrey Marinov On behalf of GEMs for CMS Collaboration. TIF – bldg. 186. Plan of the working space. Part of the Working area. Possible Scenarios. Scenario 1 – Gluing procedure, assembly and QC at the TIF hall. - PowerPoint PPT Presentation

Transcript of Preparation of TIF Hall for Production

Page 1: Preparation of TIF Hall for Production

Preparation of TIF Hall for Production Andrey MarinovOn behalf of GEMs for CMS Collaboration

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TIF – bldg. 186

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Plan of the working space

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Part of the Working area

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Possible ScenariosScenario 1 – Gluing procedure,

assembly and QC at the TIF hall.Scenario II – Using the self

stretching method and assembly at CERN’s workshop. The TIF will be used only for QC of the final detectors.

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Scenario I – Using the Gluing procedure and thermo stretching method.

TIF hall will be used for assembly and QC.

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Production Flow High Eta CMS MPGDs in TIF by Using the Thermo Stretching and Gluing Method

HV test of the GEM

Foil

Heating the GEM foil in

the oven up to 37C

Gluing the foil with the

frame

Storage Foils

HV test of the GEM Frame

Storage Frames

Assembly and Gluing

Assembly the electronics and

servicesQC tests certification

cleaning

Gas tight test

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Scenario IIUsing self stretching method

◦The detectors will be fully assembled at CERN workshop. The TIF will be used only as QC facility

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Gas Setup

Ar

CO2

CF4

OutsideGas Zone at bldg.186

InsideBldg 186 – GEM Lab

premixed

Open/Close Valves

Exhaust LinePatch Panel

Safety ValvePressure reducer

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Outside Gas Zone

Very Big Gas zone – enough for the production project

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TIF Hall – Gas Infrastructure

GASMixer

8m

6m

13.2m

2.3m

7.2m

GAS access points

Mainpanel

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QC StandsCosmic Telescope

◦Possibility to test up to 10 detectors together

X-ray stand for uniformity scan and gain calibrations.

Long Term HV test stand

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Cosmic Telescope

Testing the GE 1/1 detectors with cosmic rays

•Time distribution• Strip Profile• Efficiency• Cluster Size

• Reconstruction of the tracks

GEM detectors

Scintilator Counters

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X-ray Stand

Gain Calibration of the Detector

Precise Uniformity Scan

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Long Term HV stand

GAS Supply

HV SupplyEvery detector is on independent HV channel

GAS Return

Fully monitored environmentT, H and Atmospheric pressure need to be continuously recorded

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Plan of ActivitiesPreparing the internal gas

infrastructure◦Placing cable trays for the pipes and

cables – Ongoing, should be finished next week. 28.06.2011

◦Planning the main gas mixer based on the production and test processes requirements

Preparing the external gas setup.

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Thank You