1 / 15

Piggyback seal Micromegas

Piggyback seal Micromegas. D. Attié, A. Chaus, D. Durand, D. Deforges, E. Ferrer Ribas , J. Galán, I.Giomataris, A. Gongadze, F.J. Iguaz, F. Jeanneau, R. De Oliveira, T. Papaevangelou, A. Peyaud, A. Teixeira CERN and IRFU (CEA-Saclay). Concept.

haroun
Download Presentation

Piggyback seal Micromegas

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Piggyback seal Micromegas • D. Attié, A. Chaus, D. Durand, D. Deforges, E. Ferrer Ribas, J. Galán, I.Giomataris, A. Gongadze, F.J. Iguaz, F. Jeanneau, R. De Oliveira, T. Papaevangelou, A. Peyaud, A. Teixeira • CERN and IRFU (CEA-Saclay)

  2. Concept • Separation of the amplification structure and the readout plane Resistive layer (RuO2)~10 µm Resistive thin layer (1 MΩ /□ to 100 GΩ /□) Standard bulk structure • Signal is transmitted by capacitive coupling to the readout plane • Optimisation of the induced signal : tinsulator << tgasεinsulator/εgas • εinsulator should be as high as possible (first prototype alumina with ε~10 ) Insulator (Ceramic substrate~100-500 µm) Readout plane

  3. First set-up -HVdrift -HVamp -HVresist Ground 3 detectors with active area: 3×3 cm2 1 cm drift, 128 µm amplification gap, 20 µm of RuO2 with 100 MΩ/□, ceramic layer 300 µm Argon + 5%Iso and Ne + 5% Ethane and a standard buk in Argon + 5%Iso I. Giomataris

  4. First experimentalresults Checking possibles looses by the ceramic layer: signal entirely transmitted Test with a 252Cf (fission fragments signals) reading simultaneously mesh and anode Amplitude within 5% Same rise time for both polarities

  5. I. Giomataris

  6. I. Giomataris

  7. Rate capability With X-rays from a gun (8keV) I. Giomataris

  8. Comparison with Monte Carlo I. Giomataris

  9. 10 M/sq 100 M/sq 1 G/sq 10 G/sq I. Giomataris

  10. CMOS chip readout Medipix2/Timepix CMOS chip 256×256 square pixels of 55 µm side each To be used with MPGD the MPGD needs to be covered by a layer of high resistivity material (amorphous silicon or silicon-rich nitride) Set-up with Piggyback 30×20 mm2 bulk Amplification gap 128 µm Drift gap 10 mm Signal observed on Medipix chip with Ar + 5% Iso No damage of the chip during operation at high gain 105

  11. 55Fe events (G ~ 50 000) Spot diameter about 500 mm With a ceramic plate of 100 mm We expect to get it down to 150 mm

  12. Second set-up: towards a sealed detector Ar+5% Iso Gain

  13. Second set-up: towards a sealed detector Detector chamber glued One night oven at 60°C + pumping Flushed with gas for only 4 hours Stability over 14 days

  14. Latestresult for a sealed detector Piggyback resistive Micromegas , D. Attié et ale-Print: arXiv:1310.1242 [physics.ins-det] Stability over 30 days Small fluctuations due to day night effects Big amplitude fluctuation due to the removal of the source

  15. Conclusions and outlook • Floating mesh, Bulk Micromegas, Microbulk, Ingrid and now Piggyback • Piggyback resistive Micromegas provides spark protection • Detector dissociated from readout plane • Can optimise dead space • High rate vs resistivity has been studied • Test higher values of resistivity, different thickness of ceramic • Seal detector is under development

More Related