1 / 18

XTOD Mirrors: Physics-based specifications, fabrication approach and expected performance

XTOD Mirrors: Physics-based specifications, fabrication approach and expected performance. Lehman Review 11 July 2007 Michael Pivovaroff Contributors: R Soufli, P Stefan, J Krzywinski.

kirar
Download Presentation

XTOD Mirrors: Physics-based specifications, fabrication approach and expected performance

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. XTOD Mirrors: Physics-based specifications, fabrication approach and expected performance Lehman Review 11 July 2007 Michael Pivovaroff Contributors: R Soufli, P Stefan, J Krzywinski This work was performed under the auspices of the U.S. Department of Energy by University of California, Lawrence Livermore National Laboratory under Contract W-7405-Eng-48.

  2. Outline • Overview of mirror system layout • Mirror fabrication • Two-step approach • Physics drivers for specifications: • Substrate quality (figure and finish) and size • Reflective coatings • Performance modeling

  3. Layout of mirror systems SOMS: 0.8 < E < 2 keV • Total of four mirrors (3 reflections) • Choose between 3rd and 4th mirrors HOMS: 2 < E < 24.8 keV • Two mirrors/two reflections • Withdraw 1st SOMS mirror to access beamline

  4. SOMS-1 HOMS: Hard X-ray offset mirror system • Periscope design, 30 mm horizontal offset • Withdraw first SOMS mirror to send hard beam to Fall Experimental Hall (FEH) HOMS-2 1.324 mrad incident angle 30 mm HOMS-1 11.333 m

  5. SOMS: Soft X-ray offset mirror system • Three reflection design to maximize horizontal deflections • Creates two lines in Near Experimental Hall (NEH) • Translate last pair of mirrors to select line SOMS-3/4 13.9 mrad incident angle 570 mm SOMS-2 SOMS-1 11.5660 m

  6. Overview of mirror fabrication • Must use FEL-proof materials (e.g., Be, B4C or SiC) for reflective surface • Impossible or infeasible to procure as monolithic mirrors • Instead, deposit thin films on Si substrates using LLNL expertise and facilities

  7. LLNL magnetron sputtering • Developed for EUVL program; most recently, delivered optics for NASA solar observatory • System can fit multiple large-area substrates in a single deposition Underneath view of LLNL chamber lid with 5 sputtering targets

  8. Risk mitigation for coatings • SOMS will use B4C; HOMS will likely use SiC • No way to tests coatings under exact X-ray FEL conditions; • Test thin films at FLASH • Damage occurs well-above LCLS operational conditions; • Agrees well with theoretical expectations (Hau-Riege et al., Ap Phys L, 90, 173128, 2007) • Lifetime testing of ~1 year shows no changes in B4C film properties • Identified deposition parameters to minimize film stress

  9. Specifications: underlying philosophy • Captured in Physics Requirement Document (SOMS complete; HOMS will be signed this week) • Principal is to minimize impact of mirrors • Maximize throughput (high reflectivity, sufficiently long mirrors) • Limit increase in beam size • Minimize wave-front distortions • Balance against state of the art vendor capabilities • Start with metrology data from recent mirrors delivered to SSRL

  10. Specifications: detailed • Details presented at October 2006 Lehman review • Power spectral density well-described by power law • Use formalism developed by Church & Takacs (and others) • Look at errors in three spatial frequency regimes; same for both SOMS and HOMS • High-spatial (finish): 0.5 μm-1 – 50 μm-1 σ 4Å rms • Mid-spatial: 10-3μm-1– 0.5 μm-1 σ 2.5Å rms • Low-spatial (figure): [clear aperture]-1– 10-3μm-1 0.25 μrad rms (slope errors)*  20 Å rms (height errors)* * vendor limited

  11. Optical profilometry (Zygo) AFM Full-aperture interferometry Validation of approach (1) • Request coupons from potential vendors • Four vendors provided samples • Perform metrology at LLNL

  12. Validation of approach (2) • Vendor 1 slightly better in mid- and high- spatial frequency ranges • Two vendors can meet our specs

  13. SOMS details • SOMS mirrors ordered from InSync at the end of June • SOMS characteristics: • 250 mm long; 175 mm long clear aperture • Ensures at least 95% of beam captured (increases with energy) • Operates at 13.9 mrad incidence angle • 500 Å thick B4C coating • Good 3rd order harmonic rejection

  14. SOMS reflectivity Primary pass-band 3rd harmonic pass-band

  15. HOMS details • HOMS system concept review (SCR) scheduled for late July • HOMS characteristics: • 450 mm long—limited by coating facility • 50% of beam captured at 2 keV; 100% of beam captured at 8.3 keV • Operates at 1.324 mrad incidence angle • 500 Å thick SiC coating [candidate: TBR] • >94% throughput at all energies • Other options can increase throughput to 98%

  16. HOMS reflectivity

  17. Modeling update • Combination of ray-tracing, analytic codes and first-principle calculations used to assemble performance • Will integrate all components into comprehensive end-to-end simulation • Options: (1) insert relevant physics into existing LCLS Monte Carlo package developed by XTOD or (2) fold in models of spontaneous + FEL emission into ray-tracing codes

  18. Six-month outlook • SOMS substrates at LLNL; coating possibly underway • HOMS substrates ordered; SiC deposition process and parameters optimized • Progress on an end-to-end performance model

More Related