Published June 23, 2010
| Version v1
Journal article
Mirror profile optimization for nano-focusing KB mirror
- 1. European Synchrotron Radiation Facility, BP 220, F-38043 Grenoble Cedex (France)
Description
A KB focusing mirror width profile has been optimized to achieve nano-focusing for the nano-imaging end-station ID22NI at the ESRF. The complete mirror and flexure bender assembly has been modeled in 3D with finite element analysis using ANSYS. Bender stiffness, anticlastic effects and geometrical non-linear effects have been considered. Various points have been studied: anisotropy and crystal orientation, stress in the mirror and bender, actuator resolution and the mirror-bender adhesive bonding... Extremely high performance of the mirror is expected with residual slope error smaller than 0.6 μrad, peak-to-valley, compared to the bent slope of 3000 μrad.
Additional details
Identifiers
- DOI
- 10.1063/1.3463335;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1234
- Journal Issue
- 1
- Journal Page Range
- p. 801-804
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 10. international conference on radiation instrumentation
- Acronym
- SRI 2009
- Dates
- 27 Sep - 2 Oct 2009
- Place
- Melbourne (Australia)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42008115
- Subject category
- S77: NANOSCIENCE AND NANOTECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACTUATORS; ADHESIVES; ANISOTROPY; BONDING; CRYSTALS; EUROPEAN SYNCHROTRON RADIATION FACILITY; FINITE ELEMENT METHOD; FLEXIBILITY; FOCUSING; MIRRORS; NONLINEAR PROBLEMS; OPTICS; OPTIMIZATION; ORIENTATION; RESOLUTION; X RADIATION
- Descriptors DEC
- CALCULATION METHODS; ELECTROMAGNETIC RADIATION; FABRICATION; IONIZING RADIATIONS; JOINING; MATHEMATICAL SOLUTIONS; MECHANICAL PROPERTIES; NUMERICAL SOLUTION; RADIATION SOURCES; RADIATIONS; SYNCHROTRON RADIATION SOURCES; TENSILE PROPERTIES
Optional Information
- Notes
- (c) 2010 American Institute of Physics