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CERN Accelerating science

Article
Report number arXiv:1110.2641
Title New developments in Micromegas Microbulk detectors
Author(s) Iguaz, F.J. (IRFU, Saclay) ; Andriamonje, S. (CERN) ; Belloni, F. (IRFU, Saclay) ; Berthoumieux, E. (IRFU, Saclay) ; Calviani, M. (CERN) ; Dafni, T. (Zaragoza U.) ; De Oliveira, R. (CERN) ; Ferrer-Ribas, E. (IRFU, Saclay) ; Galan, J. (IRFU, Saclay) ; Garcia, J.A. (Zaragoza U.) ; Giomataris, I. (IRFU, Saclay) ; Guerrero, C. (CERN) ; Gunsing, F. (IRFU, Saclay) ; Herrera, D.C. (Zaragoza U.) ; Irastorza, I.G. (Zaragoza U.) ; Papaevangelou, T. (IRFU, Saclay) ; Rodriguez, A. (Zaragoza U.) ; Tomas, A. (Zaragoza U.)
Publication 2012
Imprint 13 Oct 2011
Number of pages 9
Note Comments: To be published in the Proceedings of the TIPP2011 conference (Physics Procedia)
To be published in the Proceedings of the TIPP2011 conference (Physics Procedia)
In: Phys. Procedia 37 (2012) pp.448-455
In: 2nd International Conference on Technology and Instrumentation in Particle Physics, Chicago, IL, USA, 9 - 14 Jun 2011, pp.448-455
DOI 10.1016/j.phpro.2012.02.392
Subject category Detectors and Experimental Techniques
Abstract A new Micromegas manufacturing technique, based on kapton etching technology, has been recently developed, improving the uniformity and stability of this kind of readouts. Excellent energy resolutions have been obtained, reaching 11% FWHM for the 5.9 keV photon peak of 55Fe source and 1.8% FWHM for the 5.5 MeV alpha peak of the 241Am source. The new detector has other advantages like its flexible structure, low material and high radio-purity. The two actual approaches of this technique will be described and the features of these readouts in argon-isobutane mixtures will be presented. Moreover, the low material present in the amplification gap makes these detectors approximate the Rose and Korff model for the avalanche amplification, which will be discussed for the same type of mixtures. Finally, we will present several applications of the microbulk technique.
Copyright/License publication: © 2012-2024 Elsevier (License: CC-BY-NC-ND-3.0)

Corresponding record in: Inspire


 Record created 2011-10-14, last modified 2023-03-14


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Physics Procedia - 448 - Download fulltextPDF
10.1016_j.phpro.2012.02.392 - Download fulltextPDF
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