z-logo
open-access-imgOpen Access
The Rainwater Memorial Calibration Facility for X-Ray Optics
Author(s) -
Nicolai F. Brejnholt,
Finn E. Christensen,
Charles J. Hailey,
Nicolas M. Barrière,
William W. Craig,
Brian W. Grefenstette,
Jason E. Koglin,
Kristin K. Madsen,
Julia K. Vogel,
Hongjun An,
Kenneth L. Blaedel,
J.S. Brown,
Todd A. Decker,
Zeshan Haider,
Anders C. Jakobsen,
Carsten P. Cooper-Jensen,
Kaya Mori,
Melania Nynka,
M. J. Pivovaroff,
Clio Sleator,
Dennis Stefanik,
Marcela Stern,
Gordon Tajiri,
Douglas Thornhill,
J. S. Cushman
Publication year - 2011
Publication title -
x-ray optics and instrumentation
Language(s) - English
Resource type - Journals
eISSN - 1687-7640
pISSN - 1687-7632
DOI - 10.1155/2011/285079
Subject(s) - calibration , telescope , physics , optics , x ray telescope , x ray optics , beamline , range (aeronautics) , wafer , beam (structure) , aerospace engineering , x ray , optoelectronics , engineering , quantum mechanics
The Nuclear Spectroscopic Telescope ARray (NuSTAR) is a NASA Small Explorer mission that will carry the first focusing hard X-ray (5–80 keV) telescope to orbit. The ground calibration of the optics posed a challenge as the need to suppress finite source distance effects over the full optic and the energy range of interest were unique requirements not met by any existing facility. In this paper we present the requirements for the NuSTAR optics ground calibration, and how the Rainwater Memorial Calibration Facility, RaMCaF, is designed to meet the calibration requirements. The nearly 175 m long beamline sports a 48 cm diameter 5–100 keV X-ray beam and is capable of carrying out detailed studies of large diameter optic elements, such as the NuSTAR optics, as well as flat multilayer-coated Silicon wafers.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom