Title of article :
Results from the Daresbury Compton backscattering X-ray source
Author/Authors :
Laundy، نويسنده , , D. and Priebe، نويسنده , , G. and Jamison، نويسنده , , Moshan S.P and Graham، نويسنده , , D.M. and Phillips، نويسنده , , PJ and Smith، نويسنده , , S.L. and Saveliev، نويسنده , , Y. and Vassilev، نويسنده , , S. V. Seddon، نويسنده , , E.A.، نويسنده ,
Pages :
7
From page :
108
To page :
114
Abstract :
The Daresbury Compton Backscattering X-ray Source uses a high power Ti Sapphire laser interacting in head on geometry with electron bunches in the ALICE energy recovery linear accelerator. X-ray photons with peak energy of 21 keV were generated with the accelerator operating at an energy of 29.6 MeV. The spatial profile of the X-rays emitted near the electron beam axis was measured. The characteristics of the X-ray yield measured as a function of relative timing between the laser pulse and the interacting electron bunch was found to be consistent with the modelled intensity behaviour using measured electron and laser beam parameters.
Keywords :
Ti sapphire laser , Compton backscattering , Inverse Compton scattering , Pulsed X-rays , Relativistic electron beams
Journal title :
Astroparticle Physics
Record number :
2019680
Link To Document :
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