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The concept of the Pinhole/Occulter FacilityThe Pinhole/Occulter Facility is based on a simple idea for obtaining high angular resolution in astronomical X-ray observations, for example for solar flares at energies 10 keV. The scheme uses a coded aperture device (multiple pinhole camera) with a large separation between the aperture encoder and the detector. Such an imaging device can have an angular resolution much better than 1 arc s if desired. A large structure would also make it possible to have a large external occulter, which would have powerful applications, notably for high-sensitivity observations of the corona in EUV and white light. This capability leads to the definition of the Pinhole/Occulter Facility, which combines both X-ray and coronal observations. The present concept is based on a 35-m deployable boom, erected in the cargo bay of the Space Shuttle and pointed in the solar direction by the Instrument Pointing System of Spacelab.
Document ID
19860015144
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hudson, H. S.
(California Univ. La Jolla, CA, United States)
Date Acquired
August 12, 2013
Publication Date
April 1, 1986
Publication Information
Publication: NASA. Marshall Space Flight Center Solar Flares and Coronal Physics Using P(OF as a Research Tool
Subject Category
Ground Support Systems And Facilities (Space)
Accession Number
86N24615
Funding Number(s)
CONTRACT_GRANT: NSG-7161
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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