Paper
15 September 2004 GOES solar EUV detector calibration at the NSLS
Author Affiliations +
Abstract
A solar ultraviolet detector prototype for the GOES spacecraft has been calibrated using the X24C beamline at the Brookhaven NSLS. Similar in design to the 3-channel SOHO CELIAS SEM, the GOES EUV uses a combination of transmission gratings and silicon photodiodes with thin-film metal overcoats to provide the required bandpasses. Four of the channels position the photodiodes at the first to fourth orders of 2500 and 5000 L/mm transmission gratings to provide spectral information over four wavelength bands from approximately 5-80 nm. The fifth channel positions the photodiode at first order of a 1667 L/mm transmission grating in combination with a bandpass filter centered at approximately 120 nm to provide coverage in the Lyman alpha region of teh solar spectrum. The GOES EUV will provid continuous monitoring of solar EUV in bandpasses that are known to have a large variability in the amount of energy deposition in the earth's ionosphere over a solar cycle. Prototype detector design and calibration procedure are discussed. Absolute responses of the design model and synchrotron beamline properties relevant to calibration are presented.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
John E Wise, Geoffrey Gaines, Arthur Gaudet, Mark A Gummin, Fred A. Hanser, Allen Harris, Stephen Hersey, and Benjawan Kjornrattanawanich "GOES solar EUV detector calibration at the NSLS", Proc. SPIE 5549, Weather and Environmental Satellites, (15 September 2004); https://doi.org/10.1117/12.559986
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Cited by 2 scholarly publications.
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KEYWORDS
Extreme ultraviolet

Photodiodes

Calibration

Sensors

Data modeling

Prototyping

Solar energy

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