Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Preliminary characteristics of a grating crystal monochromator for use with synchrotron radiation

Not Accessible

Your library or personal account may give you access

Abstract

The grating/crystal monochromator (GCM) consists of an initial 2° grazing angle paraboloidal mirror which collimates the synchrotron radiation from the electron beam source; a final identical paraboloidal mirror which focuses collimated monochromatic radiation to the fixed exit slit in a 1:1 image of the source; and a pair of plane diffracting elements or a mirror/diffracting element pair which monochromatize the radiation in the region of collimated light between the paraboloidal mirrors. The diffracting elements can be either crystals or gratings giving an unprecedented spectral range in one instrument from the UV to 2 keV. The two-crystallike scanning motion is ideal for an always on-blaze condition with diffraction gratings. We will report on performance tests with a plane mirror/grating pair (600 g/mm) installed in the scanning system. We present measurements of the exit slit image, the quality of which is fundamental to the resolving power of the instrument. The image quality is influenced by the source size and stability, mirror alignment, and possible mirror figuring errors. Preliminary results on spectral flux, higher-order flux, and absorption edge resolution to 100 eV are presented. Calibration and stability of the mechanical system of the GCM and the critical laser angle interferometer that encodes the orientation of the mirror/grating pair are discussed. Wavelength calibration via absorption edge spectral location is outlined.

© 1985 Optical Society of America

PDF Article
More Like This
Ultrahigh vacuum reflectometer for use with synchrotron radiation

W. R. Hunter and J. C. Rife
WL7 OSA Annual Meeting (FIO) 1985

X-ray microscopy with synchrotron radiation

Harvey Rarback, Christopher Jacobsen, John Kenney, Janos Kirz, and Roy Rosser
WL1 OSA Annual Meeting (FIO) 1985

Okazaki synchrotron radiation source

K. Kimura
TUC1 OSA Annual Meeting (FIO) 1985

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.