Fast beam monitor diamond-based devices for VUV and X-ray synchrotron radiation applications.

CVD diamond beam monitor detectors instrumentation synchrotron

Journal

Journal of synchrotron radiation
ISSN: 1600-5775
Titre abrégé: J Synchrotron Radiat
Pays: United States
ID NLM: 9888878

Informations de publication

Date de publication:
01 Mar 2019
Historique:
received: 16 10 2018
accepted: 16 01 2019
entrez: 12 3 2019
pubmed: 12 3 2019
medline: 12 3 2019
Statut: ppublish

Résumé

The improved performance of third-generation light sources and the advent of next-generation synchrotron radiation facilities require the use of extremely precise monitoring of the main photon-beam parameters, such as position, absolute and relative intensity, and temporal structure. These parameters, and associated real-time feedbacks, are fundamental at the beamline control level and at the machine control level, to improve the stability of the photon beams and to provide bunch-to-bunch quantitative information. Fast response time, high radiation hardness and visible-blind response are main features of photon-beam monitors for VUV and X-ray synchrotron radiation beamlines; hence diamond-based detectors are outstanding candidates. Here, results are presented of an extensive measurement campaign aiming at optimizing the capabilities of diamond detectors to discern time structures below the 100 ps timescale. A custom-built device has been fabricated and tested at the Italian Synchrotron Radiation Laboratory Elettra in Trieste. The results obtained show that diamond is an excellent material for ultra-fast photon pulses with picosecond time resolution; finally the possibilities for application at free-electron laser sources are discussed.

Identifiants

pubmed: 30855247
pii: S1600577519000791
doi: 10.1107/S1600577519000791
doi:

Types de publication

Journal Article

Langues

eng

Pagination

386-392

Auteurs

Michele Di Fraia (M)

Elettra - Sincrotrone Trieste S.C.p.A., Basovizza, Trieste, Italy.

Antonio De Sio (A)

Dipartimento di Fisica e Astronomia, Universitá di Firenze, Firenze, Italy.

Matias Antonelli (M)

Elettra - Sincrotrone Trieste S.C.p.A., Basovizza, Trieste, Italy.

Renzo Nesti (R)

Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Firenze, Italy.

Dario Panella (D)

Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Firenze, Italy.

Ralf H Menk (RH)

Elettra - Sincrotrone Trieste S.C.p.A., Basovizza, Trieste, Italy.

Giuseppe Cautero (G)

Elettra - Sincrotrone Trieste S.C.p.A., Basovizza, Trieste, Italy.

Marcello Coreno (M)

Elettra - Sincrotrone Trieste S.C.p.A., Basovizza, Trieste, Italy.

Daniele Catone (D)

CNR-ISM, Area della Ricerca di Roma Tor Vergata, Roma, Italy.

Nicola Zema (N)

CNR-ISM, Area della Ricerca di Roma Tor Vergata, Roma, Italy.

Carlo Callegari (C)

Elettra - Sincrotrone Trieste S.C.p.A., Basovizza, Trieste, Italy.

Emanuele Pace (E)

Dipartimento di Fisica e Astronomia, Universitá di Firenze, Firenze, Italy.

Classifications MeSH