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Scientific goals of the instrument Status before the CR

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Presentation on theme: "Scientific goals of the instrument Status before the CR"— Presentation transcript:

1 AMO Instrumentation Lehman Review Presentation, July 2007 John Bozek, LCLS
Scientific goals of the instrument Status before the CR Effects of the CR & other descoping Current designs Looking forward AMO Team Leaders: Louis DiMauro (OSU) Nora Berrah (WMU)

2 Scientific Goals of the AMO instrumentation
Investigate multiphoton and high-field x-ray processes in atoms, molecules and clusters Multi-photon ionization/excitation in atoms/molecules/clusters are well known in optical and recently EUV regime – little known about multi-photon inner-shell processes Accessible intensity on verge of high-field regime where field of light interacts with electrons in the sample Study time-resolved phenomena in atoms, molecules and clusters using ultrafast x-rays Inner-shell side band experiments using LCLS and laser photons Photoionization of aligned molecules Temporal evolution of state-prepared systems

3 Scientific Goals – Multiphoton Ionization

4 Scientific Goals – Multiphoton Ionization

5 Scientific Goals – Field Ionization
Multiphoton ionization Tunneling ionization Above-threshold-ionization (ATI) And subsequent high harmonic generation (HHG) Keldysh parameter:

6 Scientific Goals - Sidebands
Two photons of different energy in interaction region at same time can result in multiphoton ionization (i.e. FLASH FEL & laser) Phenomenon provides a means to measure temporal overlap of two pulses – i.e. providing measure of temporal overlap between LCLS & laser Measured relative jitter between two beams of 250fs using Xe 5p photoionization P. Radcliffe et al, APL, 90, , 2007.

7 Scientific Goals – Temporal Evolution
Femtosecond time scale of LCLS pulse allows us to follow evolution of chemical reactions, but not fast enough for electron dynamics (requires <1fs).

8 Scientific Goals – Imaging Small System
Motivated by strong desire to image free clusters Recent results from T. Moeller’s group at FLASH Large RG clusters Sometimes see twins sometimes two in beam

9 Proposed AMO High Field Instrument Concept

10 Review of Concept…Dec 08, 2006 Reviewers: Phil Heimann (ALS, LBNL), Gunther Haller (SLAC), Donghui Lu (SSRL, SLAC) Review Findings: “The committee found the science & technical requirements well-undestood…recommend that the experimental team move forward to preparing a baseline design…” 20 individual comments addressing different areas of the instrumentation which will be addressed in the PDR

11 Instrument Concept as presented:
Along with particle imaging, laser and controls

12 Conceptual Instrument designs
Gas jet (from below) Five electron TOF spectro’s 1of 3 ion spectrometers X-ray emission spectrometers

13 Layout of instrument into hutch 2

14 Changes since SCR & previous Lehman review
Continuing resolution – reduction of funds available in FY07 & FY08 with bifurcation of project completion into 4a and 4b Delayed focusing optics, x-ray emission spectrometers, ion imaging spectrometers Descoped Particle Imaging end-station and high-power amplifier for laser system to cover cost of timing fibre Advanced design towards a Preliminary Design Review

15 Schematic of Instrument at 4a
4A instrument has capability of measuring ions and electrons from gaseous targets together with diagnostics

16 Schematic of Instrument at 4b
Add remaining capabilities for 4b

17 CR impacts on AMO Scientific Capabilities
Retained most of core capabilities in 4a instrument Gas jet source for low density atomic – cluster targets Electron & ion spectrometers to monitor photoionization processes 2-3mJ laser to provide pulsed ionization capabilities for off-line testing/debugging etc Diagnostics to monitor pulse wavelength, bandwidth, temporal overlap with laser, size and position Primary limitation – lack of focusing optics will preclude high-field studies initially

18 AMO Instrument Design - Overview
Mechanical Design Team – Nadine Kurita (LUSI Lead Engineer), Jean Charles Castagna, Michael Kosovsky, Jim Defever

19 AMO Instrument Design – beam rate shutter
LCLS rate 120Hz Some detectors/exp. Schemes may want lower rate or even single shot

20 AMO Instrument Design – focusing optics
Peak intensity depends on size of beam focus – accessible physics depends on intensity Focus W/cm2 1mm 7×1012 100μm 7×1014 10 μm 7×1016 1 μm 7×1018 100nm 7×1020

21 AMO Instrument Design – electron spec’s
Based on a successful time-of-flight (TOF) design from D. Lindle’s (UNLV) group Five spectrometers arrayed around interaction region to measure dipole & non-dipole angular distributions

22 AMO Instrument Design – diff. pumping
Isolate chamber from optics & diagnostics Use of rare gases requires turbo pumps Conflicting requirements of pumping & access

23 AMO Instrument Design – gas jet
120Hz LCLS rate suggests pulsed valve Good experience with Proch & Tickl piezo actuated valve 3 axes motion, pulse duration & sync control

24 AMO Instrument Design – ion spectrometers
One of three spectrometers – simple ion TOF, velocity map imaging & ColTRIMS momentum imaging Ion TOF will measure charge state & probe multiple ionization Velocity map imaging maps ion velocity onto concentric rings on detector – provides quick look at ion momenta ColTRIMS is the ultimate AMO detection (especially when combined with coincident electron detection Suffers many limitations due to detector

25 AMO Instrument Design – magnetic shielding
Detection of charged particles requires nulling of magnetic field Two schemes – high permeability shielding (mu-metal) – OR – Helmholtz coils Shielding is passive but careful design required to ensure adequate attenuation, particularly junctions Helmholtz coils are dynamically tunable but possible to set them wrong Pursuing shielding option since high KE electron from inner-shell photoionization not very sensitive

26 AMO Diagnostics – magnetic bottle spectrometer
Primary diagnostic – provides wavelength, bandwidth, temporal overlap with laser High collection efficiency – up to 2π angle P. Kruit & F.H. Read, J. Phys. E (1983).

27 AMO Diagnostics – differential pumping
Transparent AMO sample allows diagnostics AFTER experiment Want to decouple high-field end-station from diagnostics – may want to use each independently Differential pumping optically aligned to axis of diagnostics chamber, then whole chamber aligned to beam axis

28 AMO Diagnostics – beam screens
Simple diagnostic of beam position/size Two YAG screens positioned ~1m apart monitored simultaneously Requires 500nm YAG coating on 200nm SiN membrane for ~50% transmission

29 AMO Diagnostics – total energy monitor
Pulse power will vary dramatically shot-to-shot XTOD is providing gas detector in FEE to measure pulse energy Simultaneous measurement in diagnostics will highlight any significant losses in transport of pulse through 5 optics and multiple differential pumping stages

30 AMO Diagnostics - interconnectivity
High-field physics chamber and diagnostics chamber connected by bellows – make sure not to overextend Significant difference in position depending on optics in/out – 30mrad deflection

31 AMO Instrument – looking forward
Complete Preliminary Design Review – Aug 07 Finish detailing high field physics chamber, diagnostics Advance design of Particle Imaging Make decisions on emission spectrometers Carry design to completion – Nov 07 Build/buy and assemble – Jul 08 Testing with laser – Nov 08 Ready for first light – Jan 09


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