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Head tail instability observation and studies at the proton synchrotron booster

Since many years the Proton Synchrotron Booster (PSB) high intensity beams have shown head tail instabilities in all of the four rings at around 100 ms after the injection. In this paper we present the latest observations together with the evaluation of the instability rise time and its dependence o...

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Detalles Bibliográficos
Autores principales: Quatraro, D, Findlay, A, Mikulec, B, Rumolo, G
Lenguaje:eng
Publicado: 2010
Materias:
Acceso en línea:http://cds.cern.ch/record/1269902
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author Quatraro, D
Findlay, A
Mikulec, B
Rumolo, G
author_facet Quatraro, D
Findlay, A
Mikulec, B
Rumolo, G
author_sort Quatraro, D
collection CERN
description Since many years the Proton Synchrotron Booster (PSB) high intensity beams have shown head tail instabilities in all of the four rings at around 100 ms after the injection. In this paper we present the latest observations together with the evaluation of the instability rise time and its dependence on the bunch intensity. The acquired head tail modes and the growth rates are compared with HEADTAIL numerical simulations, which together with the Sacherer theory points at the resistive wall impedance as a possible source of the instability.
id cern-1269902
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2010
record_format invenio
spelling cern-12699022022-08-17T13:24:33Zhttp://cds.cern.ch/record/1269902engQuatraro, DFindlay, AMikulec, BRumolo, GHead tail instability observation and studies at the proton synchrotron boosterAccelerators and Storage RingsSince many years the Proton Synchrotron Booster (PSB) high intensity beams have shown head tail instabilities in all of the four rings at around 100 ms after the injection. In this paper we present the latest observations together with the evaluation of the instability rise time and its dependence on the bunch intensity. The acquired head tail modes and the growth rates are compared with HEADTAIL numerical simulations, which together with the Sacherer theory points at the resistive wall impedance as a possible source of the instability.CERN-ATS-2010-071oai:cds.cern.ch:12699022010-06-04
spellingShingle Accelerators and Storage Rings
Quatraro, D
Findlay, A
Mikulec, B
Rumolo, G
Head tail instability observation and studies at the proton synchrotron booster
title Head tail instability observation and studies at the proton synchrotron booster
title_full Head tail instability observation and studies at the proton synchrotron booster
title_fullStr Head tail instability observation and studies at the proton synchrotron booster
title_full_unstemmed Head tail instability observation and studies at the proton synchrotron booster
title_short Head tail instability observation and studies at the proton synchrotron booster
title_sort head tail instability observation and studies at the proton synchrotron booster
topic Accelerators and Storage Rings
url http://cds.cern.ch/record/1269902
work_keys_str_mv AT quatrarod headtailinstabilityobservationandstudiesattheprotonsynchrotronbooster
AT findlaya headtailinstabilityobservationandstudiesattheprotonsynchrotronbooster
AT mikulecb headtailinstabilityobservationandstudiesattheprotonsynchrotronbooster
AT rumolog headtailinstabilityobservationandstudiesattheprotonsynchrotronbooster