High-accuracy x-ray foil optic assembly

Physics – Optics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Achieving arcsecond angular resolution in a grazing-incidence foil optic X-ray telescope, such as the segmented mirror approach being considered for the Constellation-X Spectroscopy X-Ray Telescope (SXT), requires accurate placement of individual foils. We have developed a method for mounting large numbers of nested, segmented foil optics with sub- micrometer accuracy using lithographically defined and etched silicon alignment micro-structures. A system of assembly tooling, incorporating the silicon micro-structures, is used to position the foils which are then bonded to a flight structure. The advantage of this procedure is that the flight structure has relaxed tolerance requirements while the high accuracy assembly tooling can be reused. A companion paper by Bergner et al. discusses how our process could be used for the SXT. We have built an assembly truss with a simplified rectilinear geometry designed to experimentally test this alignment and mounting technique. We report results of tests with this system that demonstrate its ability to provide sub- micrometer alignment of rigid test optics.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

High-accuracy x-ray foil optic assembly does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High-accuracy x-ray foil optic assembly, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-accuracy x-ray foil optic assembly will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1116367

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.