Paper
15 December 2000 PtSi IRFPA camera and its application in infrared solar spectrum observation
Author Affiliations +
Abstract
Although the interest in PtSi infrared focal plane array (IRFPA) has waned due to its low quantum efficiency compared with InSb and HgCdTe arrays, it is very potential in observing brighter celestial objects. We explored the possibility of applying it to the observation of infrared solar spectrum. In the paper, the methods of the simulation and calibration in our observation are introduced and discussed in detail. Using this kind of camera, a new observational band (FeI 1.56 micrometers ) is added to the Two- Dimensional Multi-Band Solar Spectrograph at Yunnan Observatory. The dispersion for FeI 1.56 micrometers of the new infrared solar spectrograph is 0.0722 angstrom per pixel, and each vertical pixel represents 0.51 inch of solar disk. It is specially suitable for 2D spectroscopic observation of the deepest solar photosphere. Some primary observation results are also presented.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Wenda Cao, Binxun Ye, and J. He "PtSi IRFPA camera and its application in infrared solar spectrum observation", Proc. SPIE 4130, Infrared Technology and Applications XXVI, (15 December 2000); https://doi.org/10.1117/12.409833
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Infrared radiation

Mirrors

Spectrographs

Cameras

Observatories

Quantum efficiency

Sensors

RELATED CONTENT

C RED One the infrared camera using the...
Proceedings of SPIE (August 08 2016)
IRCAL the infrared camera for adaptive optics at Lick...
Proceedings of SPIE (August 16 2000)
Infrared camera and spectrograph for the Subaru Telescope
Proceedings of SPIE (August 21 1998)
Instrumentation for the Keck Observatory
Proceedings of SPIE (August 16 2000)

Back to Top