Article (Scientific journals)
The Far Ultra-Violet Imager on the Icon Mission
Mende, Stephen; Frey, Harald; Rider, Kodi et al.
2017In Space Science Reviews
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Keywords :
Space-borne far ultraviolet spectral imager; Imaging the Earth’s atmosphere/ionosphere; Instrument for observing the upper atmosphere
Abstract :
[en] ICON Far UltraViolet (FUV) imager contributes to the ICON science objectives by providing remote sensing measurements of the daytime and nighttime atmosphere/ ionosphere. During sunlit atmospheric conditions, ICON FUV images the limb altitude profile in the shortwave (SW) band at 135.6 nm and the longwave (LW) band at 157 nm perpendicular to the satellite motion to retrieve the atmospheric O/N2 ratio. In conditions of atmospheric darkness, ICON FUV measures the 135.6 nm recombination emission of O+ ions used to compute the nighttime ionospheric altitude distribution. ICON Far Ultra- Violet (FUV) imager is a Czerny–Turner design Spectrographic Imager with two exit slits and corresponding back imager cameras that produce two independent images in separate wavelength bands on two detectors. All observations will be processed as limb altitude profiles. In addition, the ionospheric 135.6 nm data will be processed as longitude and latitude spatial maps to obtain images of ion distributions around regions of equatorial spread F. The ICON FUV optic axis is pointed 20 degrees below local horizontal and has a steering mirror that allows the field of view to be steered up to 30 degrees forward and aft, to keep the local magnetic meridian in the field of view. The detectors are micro channel plate (MCP) intensified FUV tubes with the phosphor fiber-optically coupled to Charge Coupled Devices (CCDs). The dual stack MCP-s amplify the photoelectron signals to overcome the CCD noise and the rapidly scanned frames are co-added to digitally create 12-second integrated images. Digital on-board signal processing is used to compensate for geometric distortion and satellite motion and to achieve data compression. The instrument was originally aligned in visible light by using a special grating and visible cameras. Final alignment, functional and environmental testing and calibration were performed in a large vacuum chamber with a UV source. The test and calibration program showed that ICON FUV meets its design requirements and is ready to be launched on the ICON spacecraft.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Mende, Stephen;  Berkeley University of California - UC Berkeley > Space Science Laboratory
Frey, Harald;  Berkeley University of California - UC Berkeley > Space science Laboratory
Rider, Kodi;  Berkeley University of California - UC Berkeley > Space Science Laboratory
Chou, Cathy;  Berkeley University of California - UC Berkeley > Space Science Laboratory
Harris, Stue;  Berkeley University of California - UC Berkeley > Space Science Laboratory
Siegmund, Oswald;  Berkeley University of California - UC Berkeley
England, Scott;  Berkeley University of California - UC Berkeley > Space Science Laboratory
Craig, William;  Berkeley University of California - UC Berkeley > Space science Laboratory
Immel, Thomas;  Berkeley University of California - UC Berkeley > Space Science Laboratory
Turin, Paul;  Berkeley University of California - UC Berkeley > Space Scien Laboratory
Darling, N.;  Berkeley University of California - UC Berkeley > Space science laboratory
Loicq, Jerôme ;  Université de Liège > CSL (Centre Spatial de Liège)
Blain, Pascal ;  Université de Liège > CSL (Centre Spatial de Liège)
Syrstad, E.;  Utah State University > Space Dynamics Lab
Thompson, B.;  Utah State University > Space Dynamics Lab.
Burt, R.;  Utah State University > Space Dynamics Lab
Champagne, J.;  Utah State University > Space Dynamics Lab.
Sevilla, P.;  Utah State University > Space Dynamics Lab
Ellis, Scott;  Photon Engineering -Tuscon USA
More authors (9 more) Less
Language :
English
Title :
The Far Ultra-Violet Imager on the Icon Mission
Publication date :
01 August 2017
Journal title :
Space Science Reviews
ISSN :
0038-6308
eISSN :
1572-9672
Publisher :
Springer Science & Business Media B.V., Dordrecht, Netherlands
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 16 August 2017

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