Paper
6 October 2011 LEMUR (Large European Module for solar Ultraviolet Research): a VUV imaging spectrograph for the JAXA Solar-C Mission
Clarence M. Korendyke, Luca Teriaca, George A. Doschek, Louise K. Harra, Udo H. Schühle, Toshifumi Shimizu
Author Affiliations +
Abstract
LEMUR is a VUV imaging spectrograph with 0.28" resolution. Incident solar radiation is imaged onto the spectrograph slit by a single mirror telescope consisting of a 30-cm steerable f/12 off-axis paraboloid mirror. The spectrograph slit is imaged and dispersed by a highly corrected grating that focuses the solar spectrum over the detectors. The mirror is coated with a suitable multilayer with B4C top-coating providing a reflectance peak around 18.5 nm besides the usual B4C range above 500Å. The grating is formed by two halves, one optimized for performances around 185Å and the other above 500Å. Three intensified CCD cameras will record spectra above 50 nm while a large format CCD array with an aluminum filter will be used around 185Å.
© (2011) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Clarence M. Korendyke, Luca Teriaca, George A. Doschek, Louise K. Harra, Udo H. Schühle, and Toshifumi Shimizu "LEMUR (Large European Module for solar Ultraviolet Research): a VUV imaging spectrograph for the JAXA Solar-C Mission", Proc. SPIE 8148, Solar Physics and Space Weather Instrumentation IV, 81480I (6 October 2011); https://doi.org/10.1117/12.893622
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Space telescopes

Spectrographs

Mirrors

Solar processes

Sensors

Coronagraphy

Back to Top