Optimizing X-ray mirror thermal performance using matched profile cooling

被引:27
|
作者
Zhang, Lin [1 ,2 ]
Cocco, Daniele [1 ]
Kelez, Nicholas [1 ]
Morton, Daniel S. [1 ]
Srinivasan, Venkat [1 ]
Stefan, Peter M. [1 ]
机构
[1] SLAC Natl Accelerator Lab, LCLS, Menlo Pk, CA 94025 USA
[2] European Synchrotron Radiat Facil, ISDD, F-38043 Grenoble, France
关键词
KB mirror; FEL beam; thermal deformation; variable cooling length; adjustable electric heater; finite-element modelling; water cooling; COOLED SILICON MONOCHROMATORS; HEAT LOAD; OPTICAL-ELEMENTS; LIMITS;
D O I
10.1107/S1600577515013090
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
To cover a large photon energy range, the length of an X-ray mirror is often longer than the beam footprint length for much of the applicable energy range. To limit thermal deformation of such a water-cooled X-ray mirror, a technique using side cooling with a cooled length shorter than the beam footprint length is proposed. This cooling length can be optimized by using finite-element analysis. For the Kirkpatrick-Baez (KB) mirrors at LCLS-II, the thermal deformation can be reduced by a factor of up to 30, compared with full-length cooling. Furthermore, a second, alternative technique, based on a similar principle is presented: using a long, single-length cooling block on each side of the mirror and adding electric heaters between the cooling blocks and the mirror substrate. The electric heaters consist of a number of cells, located along the mirror length. The total effective length of the electric heater can then be adjusted by choosing which cells to energize, using electric power supplies. The residual height error can be minimized to 0.02 nm RMS by using optimal heater parameters (length and power density). Compared with a case without heaters, this residual height error is reduced by a factor of up to 45. The residual height error in the LCLS-II KB mirrors, due to free-electron laser beam heat load, can be reduced by a factor of similar to 11 below the requirement. The proposed techniques are also effective in reducing thermal slope errors and are, therefore, applicable to white beam mirrors in synchrotron radiation beamlines.
引用
收藏
页码:1170 / 1181
页数:12
相关论文
共 50 条
  • [41] X-ray Holographic Microscopy using Total -Reflection Mirror Interferometer
    Suzuki, Yoshio
    Takeuchi, Akihisa
    JAPANESE JOURNAL OF APPLIED PHYSICS, 2008, 47 (11) : 8595 - 8599
  • [42] X-RAY HALOES AND COOLING FLOWS
    FABIAN, AC
    IAU SYMPOSIA, 1991, (144): : 237 - 244
  • [43] X-ray imaging of cooling flows
    Bohringer, H
    GALACTIC AND CLUSTER COOLING FLOWS, 1997, 115 : 11 - 20
  • [44] Ignition and cooling of X-ray bursts
    Wiescher, M
    Schatz, H
    REVISTA MEXICANA DE FISICA, 2000, 46 : 128 - 132
  • [45] Ignition and cooling of X-ray bursts
    Wiescher, M
    Schatz, H
    PROGRESS OF THEORETICAL PHYSICS SUPPLEMENT, 2000, (140): : 11 - 32
  • [46] Structural analysis of a Mo/Si multilayered x-ray mirror by x-ray diffraction
    Kim, DE
    Cha, DH
    JOURNAL OF THE KOREAN PHYSICAL SOCIETY, 1996, 29 (01) : 74 - 78
  • [47] X-ray spectroscopy of cooling clusters
    Peterson, JR
    Fabian, AC
    PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2006, 427 (01): : 1 - 39
  • [48] X-ray cavities and cooling flows
    Nulsen, Paul E. J.
    McNamara, Brian R.
    David, Laurence P.
    Wise, Michael W.
    HIGHLIGHTS OF ASTRONOMY, VOL 13, 2005, 13 : 307 - 311
  • [49] PREDICTED AND PRELIMINARY EVALUATION OF THE X-RAY PERFORMANCE OF THE AXAF TECHNOLOGY MIRROR ASSEMBLY
    VANSPEYBROECK, L
    REID, P
    SCHWARTZ, D
    BILBRO, J
    X-RAY/EUV OPTICS FOR ASTRONOMY AND MICROSCOPY, 1989, 1160 : 94 - 107
  • [50] Performance and time stability of Ir/SiC X-ray mirror coatings for ATHENA
    Svendsen, S.
    Massahi, S.
    Ferreira, D. D. M.
    Christensen, F. E.
    Jafari, A.
    Henriksen, P. L.
    Collon, M.
    Landgraf, B.
    Girou, D.
    Krumrey, M.
    Cibik, L.
    Schubert, A.
    Handick, E.
    Shortt, B.
    OPTICS FOR EUV, X-RAY, AND GAMMA-RAY ASTRONOMY IX, 2019, 11119