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Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory

The design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory is presented. The bleeder is purely resistive. The base comprises two outputs: one from the anode and another one from the last dynode followed by an amplifier. The charge ratio between the anode and th...

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Detalles Bibliográficos
Autores principales: Genolini, B, Nguyen-Trung, T, Pouthas, J, Lhenry-Yvon, I, Parizot, E, Suomijärvi, T
Lenguaje:eng
Publicado: 2001
Materias:
Acceso en línea:http://cds.cern.ch/record/507111
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author Genolini, B
Nguyen-Trung, T
Pouthas, J
Lhenry-Yvon, I
Parizot, E
Suomijärvi, T
author_facet Genolini, B
Nguyen-Trung, T
Pouthas, J
Lhenry-Yvon, I
Parizot, E
Suomijärvi, T
author_sort Genolini, B
collection CERN
description The design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory is presented. The bleeder is purely resistive. The base comprises two outputs: one from the anode and another one from the last dynode followed by an amplifier. The charge ratio between the anode and the amplified dynode is around 30. The design ensures a low consumption (less than 100 mu A at 2 kV), a stability of the gain and of the base line during the whole period of measurement (20 mu s per event) and for the whole dynamic range (max. 1 to 3x10^4 in amplitude). First measurement with a prototype base on the Hamamatsu R5912 photomultiplier tube are presented.
id cern-507111
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2001
record_format invenio
spelling cern-5071112019-09-30T06:29:59Zhttp://cds.cern.ch/record/507111engGenolini, BNguyen-Trung, TPouthas, JLhenry-Yvon, IParizot, ESuomijärvi, TDesign of the photomultiplier bases for the surface detectors of the Pierre Auger ObservatoryDetectors and Experimental TechniquesThe design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory is presented. The bleeder is purely resistive. The base comprises two outputs: one from the anode and another one from the last dynode followed by an amplifier. The charge ratio between the anode and the amplified dynode is around 30. The design ensures a low consumption (less than 100 mu A at 2 kV), a stability of the gain and of the base line during the whole period of measurement (20 mu s per event) and for the whole dynamic range (max. 1 to 3x10^4 in amplitude). First measurement with a prototype base on the Hamamatsu R5912 photomultiplier tube are presented.EXT-2001-040IPNO-DR-2001-010oai:cds.cern.ch:5071112001-07-03
spellingShingle Detectors and Experimental Techniques
Genolini, B
Nguyen-Trung, T
Pouthas, J
Lhenry-Yvon, I
Parizot, E
Suomijärvi, T
Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory
title Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory
title_full Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory
title_fullStr Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory
title_full_unstemmed Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory
title_short Design of the photomultiplier bases for the surface detectors of the Pierre Auger Observatory
title_sort design of the photomultiplier bases for the surface detectors of the pierre auger observatory
topic Detectors and Experimental Techniques
url http://cds.cern.ch/record/507111
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