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Studies of the micro-bunching instability in multi-bunch operation at the ANKA storage ring

Brosi, Miriam; Blomley, Edmund ORCID iD icon; Bründermann, Erik ORCID iD icon; Caselle, Michele; Kehrer, Benjamin; Kopmann, Andreas ORCID iD icon; Rämisch, Florian; Rota, Lorenzo; Schedler, Manuel; Schönfeldt, Patrik; Schuh, Marcel; Schwarz, Markus; Steinmann, Johannes L. ORCID iD icon; Weber, Marc; Müller, Anke-Susanne ORCID iD icon

Abstract (englisch):

The test facility and synchrotron light source ANKA at the Karlsruhe Institute of Technology (KIT) operates in the energy range from 0.5 to 2.5 GeV and can generate brilliant coherent synchrotron radiation in the THz range employing a dedicated bunch length-reducing optic at 1.3 GeV beam energy. The high degree of spatial compression leads to complex longitudinal dynamics and to time evolving sub-structures in the longitudinal phase space of the electron bunches. The results of the micro-bunching instability are time-dependent fluctuations and strong bursts in the radiated THz power. To study these fluctuations in the emitted THz radiation simultaneously for each individual bunch in a multi-bunch environment, fast THz detectors are combined with KAPTURE, the dedicated Karlsruhe Pulstaking and Ultrafast Readout Electronics system, developed at KIT. In this contribution we present measurements conducted to study possible multi-bunch effects on the characteristic bursting behavior of the micro-bunch instability. Supported by BMBF (05K13VKA, 05K16VKA), the HGF (VH-NG-320) and the HIRST.

Zugehörige Institution(en) am KIT Institut für Beschleunigerphysik und Technologie (IBPT)
Institut für Prozessdatenverarbeitung und Elektronik (IPE)
Laboratorium für Applikationen der Synchrotronstrahlung (LAS)
Publikationstyp Vortrag
Publikationsjahr 2017
Sprache Deutsch
Identifikator KITopen-ID: 1000078387
HGF-Programm 54.01.01 (POF III, LK 01) ps- und fs-Strahlen
Veranstaltung DPG-Frühjahrstagung der Sektion Kondensierte Materie (SKM), Arbeitskreis Beschleunigerphysik, Dresden, 19.-24.März 2017
Bemerkung zur Veröffentlichung Verhandlungen der Deutschen Physikalischen Gesellschaft, R.6, B.52(2017) AKBP 7.8
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