Paper
28 July 2000 Holographic telescope design for narrowband imaging in the far ultraviolet
Erik Wilkinson, Remy Indebetouw
Author Affiliations +
Abstract
We report on the status of a novel imaging spectrometer design based on aberration-corrected holographic gratings. The goal of the work is to develop optical designs with high spatial resolution and high sensitivity over a narrow wavelength bandpass, thus effectively creating a narrow-band imaging capability. Ideally the narrow-band capability can be used to observe astrophysical phenomena at key diagnostic lines short-ward the short-wavelength transmission cut-off of lithium fluoride (1050 angstroms) while simultaneously controlling the intense geocoronal Lyman alpha emission at 1216 angstroms. For example OVI 1032, 1038 angstroms emission from a fast shock can be observed with arc-second resolution over a 5 arc-minute field of view.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Erik Wilkinson and Remy Indebetouw "Holographic telescope design for narrowband imaging in the far ultraviolet", Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); https://doi.org/10.1117/12.394025
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KEYWORDS
Holography

Telescopes

Space telescopes

Optical design

Monochromatic aberrations

Far ultraviolet

Spectrographs

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