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The Applicability of a 5–18 μm Array Camera to Solar Imaging

Published online by Cambridge University Press:  03 August 2017

Daniel Y. Gezari
Daniel Y. Gezari*
Affiliation:
NASA/Goddard Space Flight Center, Infrared Astrophysics Branch, Code 685, Greenbelt, MD 20771, U.S.A.

Abstract

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The anticipated requirements and operating conditions are considered for using a mid-infrared array camera in broad- and narrow-band solar imaging observations. The array camera system was designed for high-background 5–18 μm general astronomical imaging observations. The electronic and optical design of the camera, its photometric characteristics, examples of observational results, and the requirements for imaging in both high- and low-background solar applications are discussed.

Keywords

infrared: generalinstrumentation: detectorsSun: general
Type
Part 7: Infrared Technology and the Future
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 595 - 601
Copyright
Copyright © Kluwer 1994 

References

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