Paper
10 November 1998 Design and performance of the Global Ultraviolet Imager (GUVI)
David C. Humm, Larry J. Paxton, Andrew B. Christensen, Bernard S. Ogorzalek, C. Thompson Pardoe, Ching-I. Meng, Daniel Morrison, Douglas J. Strickland, J. Scott Evans, Michele B. Weiss, W. Crain, Patricia H. Lew, Dan J. Mabry, John O. Goldsten, Stephen A. Gary, Keith Peacock, David F. Persons, Mark J. Harold, E. Brian Alvarez, Carl J. Ercol
Author Affiliations +
Abstract
The Global UV imager (GUVI) is an imaging spectrometer on the NASA TIMED spacecraft. GUVI produces simultaneous monochromatic images at five 'colors' as its field of view is scanned from horizon to horizon. The instrument consists of a scan mirror feeding a parabolic telescope and Rowland circle spectrometer, with a wedge-and-strip detector at the focal plane. We describe the design, and give an overview of the environmental parameters that will be measured. GUVI is a modified version of the Special Sensor UV Spectrographic Imager (SSUSI), which will fly on the DMSP Block 5D3 satellites S-16 through S-20, We present some results from the optical calibration of the five SSUSI units.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David C. Humm, Larry J. Paxton, Andrew B. Christensen, Bernard S. Ogorzalek, C. Thompson Pardoe, Ching-I. Meng, Daniel Morrison, Douglas J. Strickland, J. Scott Evans, Michele B. Weiss, W. Crain, Patricia H. Lew, Dan J. Mabry, John O. Goldsten, Stephen A. Gary, Keith Peacock, David F. Persons, Mark J. Harold, E. Brian Alvarez, and Carl J. Ercol "Design and performance of the Global Ultraviolet Imager (GUVI)", Proc. SPIE 3445, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX, (10 November 1998); https://doi.org/10.1117/12.330325
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Cited by 23 scholarly publications.
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KEYWORDS
Sensors

Mirrors

Spectrographs

Imaging systems

Ultraviolet radiation

Electronics

Spatial resolution

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