1. AWAKE Electron Spectrometer Design Simon Jolly 4 th September 2012

2. Spectrometer Specifications Wakefield accelerated electrons ejected colinear with proton beam: need to separate the 2 and measure energy of electron beam only. Must be able to resolve energy spread as well as energy: spectrometer must accept a range of energies, probably 0-5 GeV. Simple conceptual layout: –Dipole mounted at plasma exit separates proton and electron beams. –Scintillator screen 4 m downstream of dipole intercepts electron beam ONLY. –Dispersion gives energy-dependent position spread on screen. –Scintillator imaged by intensified CCD camera viewing upstream face of scintillator screen. 04/09/12Simon Jolly, University College London2

3. Spectrometer Layout 04/09/12Simon Jolly, University College London3 Dipole separates protons from electrons AND puts energy-dependent spread in beam. Electrons intercepted by scintillator screen, imaged by high speed iCCD camera. Screen nominally 4 m from dipole. Dipole Proton beam Electron beam Screen iCCD Image Low energy High energy iCCD Camera

4. Browne-Beuchner Spectrometer (Alexey) 04/09/12Simon Jolly, University College London4 C. P. Browne and W. W. Buechner, Rev. Sci. Instrum. 27, 899 (1956). Removes angular convolution from energy measurement, but needs ~3 m magnet for 5 GeV at 1.5 T… Focusing in broad energy range is achieved via pole face curvature.

5. Spectrometer Beam Trajectories (Alexey) 04/09/12Simon Jolly, University College London5

6. With Quadrupole Doublet (Alexey) 04/09/12Simon Jolly, University College London6

7. With Fringe Fields (Alexey) 04/09/12Simon Jolly, University College London7

8. Proton Microbunches After Plasma (Alexey) 04/09/12Simon Jolly, University College London8 0 m after plasma 2 m after plasma 6 m after plasma Transverse Distributions -60 mm < s < - 40 mm

9. CERN 1 m Dipole (Edda, Alexey) 04/09/12Simon Jolly, University College London9

10. AWAKE Spectrometer Layout Edge of scintillator screen is aligned with dipole coils (position will depend on resolution). Screen mounted at 45 degrees to beam axis. Camera is 4m from centre of screen, mounted at 90 degrees to beam axis. Camera shown in horizontal bending plane. Camera can also be mounted vertically, directly above screen, with screen tilted at 45 degrees to vertical as well as 45 degrees to beam axis. Dipole to screen distance remains unchanged (independent of screen- camera orientation). 04/09/12Simon Jolly, University College London10 4 m 1.6 m 1 m Camera Dipole Screen

11. AWAKE Spectrometer Layout 2 Simon Jolly, University College London 2 m 1.6 m 1 m Camera Dipole Screen 04/09/1211

12. Layout Questions Do we need 2 dipoles? –Difficult to get good low/high field from single dipole. –Weak dipole (Browne-Buechner?) upstream of strong dipole analyses 1- 20 MeV electrons. –Reduces available longitudinal space, increases complexity: need 2 nd screen & camera + larger vacuum vessel. Can we include quadrupole doublet? –Alexey’s simulations show improvement in energy range on screen with doublet. –Is there enough longitudinal space? How close should screen be to dipole? –Closer gives better range, less effect of emittance, higher light output. –Greater distance improves resolution, requires smaller dipole. –Probably needs to be closer due to low beam intensity, large energy spread. Optimum camera location? –Camera not radiation hard (waiting on specs from manufacturer), so needs to be well shielded ie. far from beamline. –Intensifier enhances low light output from screen (single photon detection) but more light into camera gives better signal-to-noise ie. close to beamline. –Mount camera above beamline? Increases distance from beamline while reducing distance to screen. 04/09/12Simon Jolly, University College London12

13. Spectrometer Camera 04/09/12Simon Jolly, University College London13 Camera already purchased. Andor iStar 340T iCCD camera: –2048 x 512 total pixels (1850 x 512 active with 25 mm intensifier). –13.5 um pixels. –Gen-2 W-AGT P43 intensifier, gated at 7 ns. –Nikon F-mount lens mount. –16-bit readout, 150 ke - pixel full well. –http://www.andor.com/scientific_c ameras/istar_iccd_camera/340- intensified-sensor/http://www.andor.com/scientific_c ameras/istar_iccd_camera/340- intensified-sensor/ Camera setup: –DAQ and control software. –Data analysis software to give online measurement of witness beam energy spectrum. –Mechanical design of camera support system for tests and installation in SPS tunnel (comes later).

14. Scintillator Choices Scintillator requirements: –High light output (very low intensity electron beam). –Radiation hard (survive proton beam?). –Vacuum safe (screen inside vacuum vessel). Scintillator choices from 3 different fields: –Accelerators (survive higher current): Al 2 O 3 (“ruby” powder, used in LHC BTV). YAG:Ce (high light output). Quartz (very rad hard, low light output). –Detectors (high light output): CdWO 4 /PbWO 4 /ZnWO 4 (CMS ECal). CsI(Tl) (very high light output, not rad hard). BGO/LYSO (more rad hard for lower light). Plastics (less rad hard, cheap). –Plasma Wakefield (large area): Lanex (large screens, vacuum safe?) P43/P46/P47 phosphors (x-ray phosphors). Need highest number of photons per solid angle to give maximum screen-to- camera distance. Manual lens probably means no zoom (prime lens), so resolution fixed by mechanical layout. 04/09/12Simon Jolly, University College London14

15. Conclusions Baseline design is evolving rapidly: this is good! Looks like optimum will be 45 degree screen close to dipole: –Alexey’s simulations show energies already well separated at dipole exit. –Get as close to dipole exit as possible while still imaging whole screen (camera view not obscured by dipole yoke). –Light path needs to be absolutely light tight (light from plasma exit?) but not necessarily vacuum tight. Need input on scintillators to know what possibilities are: –Why is Lanex never used in HEP? –Need specs on light output to set maximum camera-to- screen distance. Spectrometer design will probably evolve from all constraints ie. beamline space, radiation, vacuum vessel, then optimised within those constraints. 04/09/12Simon Jolly, University College London15