Control of undulator radiation using a ...
Document type :
Communication dans un congrès avec actes
Title :
Control of undulator radiation using a Laser Plasma Acceleration Source
Author(s) :
Ghaith, Amin [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Oumbarek-Espinos, Driss [Auteur]
Synchrotron SOLEIL [SSOLEIL]
André, Thomas [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Roussel, Eléonore [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Loulergue, Alexandre [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Labat, Marie [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Corde, S.Ébastian [Auteur]
Kononenko, Olena [Auteur]
Valléau, Mathieu [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Marcouillé, Olivier [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Bielawski, Serge [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Malka, Victor [Auteur]
Couprie, Marie-Emmanuelle [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Synchrotron SOLEIL [SSOLEIL]
Oumbarek-Espinos, Driss [Auteur]
Synchrotron SOLEIL [SSOLEIL]
André, Thomas [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Roussel, Eléonore [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Loulergue, Alexandre [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Labat, Marie [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Corde, S.Ébastian [Auteur]
Kononenko, Olena [Auteur]
Valléau, Mathieu [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Marcouillé, Olivier [Auteur]
Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Bielawski, Serge [Auteur]

Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 [PhLAM]
Malka, Victor [Auteur]
Couprie, Marie-Emmanuelle [Auteur]
Synchrotron SOLEIL [SSOLEIL]
Conference title :
4th European Advanced Accelerator Concepts Workshop
City :
La Biodola
Country :
Italie
Start date of the conference :
2019-09-15
Book title :
J.Phys.Conf.Ser.
Publication date :
2020
HAL domain(s) :
Physique [physics]/Physique [physics]/Physique des accélérateurs [physics.acc-ph]
English abstract : [en]
Spontaneous undulator radiation emission, after the COXINEL line using a Laser Plasma acceleration (LPA) source, has been observed. The line enables to manipulate the electron beam phase space such as emittance, dispersion ...
Show more >Spontaneous undulator radiation emission, after the COXINEL line using a Laser Plasma acceleration (LPA) source, has been observed. The line enables to manipulate the electron beam phase space such as emittance, dispersion and energy spread along a 10 m long transport. The large divergence is handled at a very early stage to mitigate the chromatic emittance, using high gradient permanent magnet based quadrupoles mounted on translation tables. The operating energy is between 161-180 MeV focused in a 2-m long cryo-ready undulator with a period of 18 mm emitting light in the Ultra-Violet range. The spectral flux is characterized using a spectrometer. The wavelength is tuned by either changing the electron beam energy or by adjusting the undulator gap. The radiation pattern signature is illustrated alongside its dependence on the energy spread that is modified by introducing a slit in a magnetic chicane where a small relative bandwidth of 5% has been achieved.Show less >
Show more >Spontaneous undulator radiation emission, after the COXINEL line using a Laser Plasma acceleration (LPA) source, has been observed. The line enables to manipulate the electron beam phase space such as emittance, dispersion and energy spread along a 10 m long transport. The large divergence is handled at a very early stage to mitigate the chromatic emittance, using high gradient permanent magnet based quadrupoles mounted on translation tables. The operating energy is between 161-180 MeV focused in a 2-m long cryo-ready undulator with a period of 18 mm emitting light in the Ultra-Violet range. The spectral flux is characterized using a spectrometer. The wavelength is tuned by either changing the electron beam energy or by adjusting the undulator gap. The radiation pattern signature is illustrated alongside its dependence on the energy spread that is modified by introducing a slit in a magnetic chicane where a small relative bandwidth of 5% has been achieved.Show less >
Language :
Anglais
Peer reviewed article :
Non
Audience :
Internationale
Popular science :
Non
Source :
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