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F-line Optics Upgrade for Improved High-heat-load and MAD Capabilities

F-cave layout
 

  • With the continued increase in CESR currents, the front-end x-ray optics at A- and F- wiggler lines at CHESS require considerable redesign and improvements. The F-line front-end has now been com-pletely rebuilt and will have a new water-cooled white-beam mirror as the first optical element. 
  • The white-beam mirror serves two crucial functions. First, it operates as a power filter so that the heat loads at F1 and F2 monochromator crystals are cut down by two-thirds. Second, the mirror can be vertically bent to make the x-ray beam more parallel, increasing the energy resolution for MAD experiments by about a factor of two at the F2 station without significant loss of x-ray flux. 
  • The redesigned new F-line also employs separate vacuum-compatible boxes for monochromators and mirrors to reduce the heat-load interference among crucial optical components. The double-bounce energy-tunable monochromator for F2 has been completely redesigned and will be more suitable for rapid energy changes used by MAD crystallographers. Also in the plan are longer focusing mirrors for F1 and F2 with state-of-the-art optical flatness that is at least a factor of two better than the current ones. 
  • In other improvement areas, new shielding walls of the F-cave area will increase the attenuation of neutron radiation by an order of magnitude, which is necessary in anticipation of the CESR current increases in the near future. A new capability is being added to the F3 bend-magnet station so that focusing multilayer monochro-mators can be installed and operated with ease. 
New Monochromator Design for F2 MAD Experiments

F2 monochromator
 

  • The optics for the F2 station have been re-designed to be optimized for work in the fast growing field of MAD crystallography. A new monochromator, along with a new collimating white beam mirror located upstream on F-line, will provide many advantages for MAD experiments at F2. 
  • The upstream mirror will reduce heat load by two-thirds and increase the energy resolution at the MAD experiment to its source-size limit. Even though Si (111) will remain the work-horse monochromator, a set of Si (220) crystals is being planned which, when used with the upstream collimating mirror, will provide an energy resolution at the core-hole life-time limit for the K-edges of selenium and other elements. 
  • The new single-rotation-stage monochromator is able to change wavelengths quickly and reliably. Two separate angle-segment stages, one for each crystal, are used to fine tune the second-crystal translation tilt so that a fixed-exit beam can be maintained throughout the useable energy range of 6-18 keV. 
  • The reduction of high-energyphotons by the upstream mirror and the new separated vacuum chambers for each optical element in the F-cave area will greatly reduce energy drifts due to secondary heating sources and thermal cross-talks between the optical components
High-Heat-Load Management for Wiggler Beamlines & Optics

Wiggler spectrum

  • White-beam mirrors: Given the recent successful operation of a water-cooled white-beam glid-cop mirror at A2 wiggler station, we are planning to install similar Rh-coated glid-cop mirrors for all F, G, and A wiggler beamlines. These 1m-long mirrors (or a possible multilayer for A1) located upstream of the monochromators will substantially reduce the heat loads on the monochromator crystals, by a factor of about three. Together with the new lower-critical-energy G/A-line wiggler, these power-filters will allow more manageable designs of high-heat-load monochromators using conventional water-cooling.
  • Beam stops: Both A- and F-wiggler beam stops have been completely redesigned and rebuilt so that these crucial devices can be safely operated at high CESR currents of 500 mA. A water-cooled 5-deg horizontal V-shape copper block serves as the main heat absorber for each beam stop. Similar cooling designs have been implemented in other critical beam-line components such as beam position monitors and apertures. 
  • Beryllium windows: A graphite-filter/beryllium-window design has been implemented in the A-line and the F-line vacuum window sections. This design employs a 0.25-0.5 mm thick highly-oriented pyrolitic graphite (HOPG) as a prefilter to reduce the heat load on the first vacuum beryllium window. Unlike most graphite filter designs in other synchrotron sources that rely entirely on radiative cooling, the HOPG filter in this design is brazed onto a water-cooled copper flange which substantially lowers its maximum temperature and prolongs its operational lifetime. 
  • Monochromators: Significant improvements to the high-heat-load monochromators have been made at the high-resolution wiggler stations such as F2. Due to the large beam-footprint and the high total power of the wigglers, our effort has been focused on internally-water-cooled silicon monochromators with optimized coolant channels. One of such designs, involving a set of mini-cooling-channels, a high-flow-rate water supply-return manifold, and an innovative high-temperature metal-diffusion bond by Karl Smolenski, has been successfully operated at F2 station for the past three years. The metal-diffusion bond proves to be the crucial step in the design, since it needs to provide a water-tight radiation-resistant seal that does not strain the silicon crystal. The test result shows an almost linear response in x-ray throughput versus CESR current and the total flux delivered to the station is an order-of-magnitude higher than the old externally-cooled designs.
Recent Publications 
on High-Heat-Load Engineering & Optics Development

Book

  • Qun Shen, C. Henderson, M. Keeffe, M. Marston, K.D. Finkelstein, and B.W. Batterman, "Design of beam line components for high power wiggler beam line at CHESS", Nucl. Instrum. Meth. A 347, 609 (1994). 
  • P. Doing, J. White, and Qun Shen, "A high power and high flux x-ray wiggler station at CHESS", Nucl. Instrum. Meth. A 347, 73 (1994). 
  • K.W. Smolenski, C. Conolly, P. Doing, B. Kiang, and Qun Shen, "Bonding techniques for the fabrication of internally cooled x-ray monochromators", SPIE Proceedings 2856, 246 (1996). 
  • K.W. Smolenski, Qun Shen, and Park Doing, "Improved internally water-cooled monochromators for a high-power wiggler beam line at CHESS", SPIE Proceedings, 3151, 181-187 (1997). 
  • Qun Shen, K.W. Smolenski, and E. Fontes, "Design of graphite power-filters and beryllium windows at wiggler beam lines at CHESS", SPIE Proceedings, 3151, 116-122 (1997). 
  • K.W. Smolenski, Qun Shen, and P. Doing, "Silver bonded, internally water-cooled monochromators for CHESS wiggler beamlines", AIP Conference Proceedings 417, 66-70 (1997). 
  • Qun Shen, "New monochromator upgrades at CHESS", Synch. Rad. News, vol.10, no.3, pp.38-39 (1997). 
  • K.W. Smolenski, R.L. Headrick, A.M. Khounsary, C. Liu, A.T. Macrander, and Q. Shen, "Water-cooled multilayer optics for a wiggler beam line", SPIE Proceedings 3448, 27 (1998). 
  • P. Doing, S. Kycia, and Q. Shen, "Mosaic monochromator applications at CHESS", SPIE Proceedings 3448, 32 (1998).
  • Stefan Kycia, Karl W. Smolenski, R. Headrick, and Qun Shen, "Multilayer design for wiggler beam line at CHESS", AIP Conference Proceedings, in press (1999).
Engineering and Design Team at CHESS

CHESS logo

  • These are the people who really make things happen:
  • Karl SmolenskiAlan PaulingDana RichterTom Krawczyk

    ... and many others.


This page is written by Qun Shen (qs11@cornell.edu). Last updated 1/3/00.