TY - JOUR
T1 - Control of undulator radiation using a Laser Plasma Acceleration Source
AU - Ghaith, Amin
AU - Oumbarek-Espinos, Driss
AU - André, Thomas
AU - Roussel, Eléonore
AU - Loulergue, Alexandre
AU - Labat, Marie
AU - Corde, Sébastian
AU - Kononenko, Olena
AU - Valleáu, Mathieu
AU - Marcouillé, Olivier
AU - Bielawski, Serge
AU - Malka, Victor
AU - Couprie, Marie Emmanuelle
N1 - Publisher Copyright:
© Published under licence by IOP Publishing Ltd.
PY - 2020/9/18
Y1 - 2020/9/18
N2 - 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.
AB - 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.
U2 - 10.1088/1742-6596/1596/1/012045
DO - 10.1088/1742-6596/1596/1/012045
M3 - Conference article
AN - SCOPUS:85092529441
SN - 1742-6588
VL - 1596
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012045
T2 - 4th European Advanced Accelerator Concepts Workshop, EAAC 2019
Y2 - 15 September 2019 through 20 September 2019
ER -