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Proceedings Paper

PtSi IRFPA camera and its application in infrared solar spectrum observation
Author(s): Wenda Cao; Binxun Ye; Qian Song; J. He; X. D. Zhou; Kaifan Ji
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Paper Abstract

Although the interest in PtSi IR focal pane array 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 IR 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 is added to the 2D Multi-band Solar Spectrograph at Yunnan Observatory. The dispersion for FeI 1.56 micrometers of the new IR 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.

Paper Details

Date Published: 16 August 2000
PDF: 8 pages
Proc. SPIE 4008, Optical and IR Telescope Instrumentation and Detectors, (16 August 2000); doi: 10.1117/12.395539
Show Author Affiliations
Wenda Cao, Yunnan Observatory and National Astronomical Observatories (China)
Binxun Ye, Beijing Astronomical Observatory and National Astronomical Observatories (China)
Qian Song, Yunnan Observatory and National Astronomical Observatories (China)
J. He, National Information Industry Ministry (China)
X. D. Zhou, National Information Industry Ministry (China)
Kaifan Ji, UCO/Lick Observatory (United States)

Published in SPIE Proceedings Vol. 4008:
Optical and IR Telescope Instrumentation and Detectors
Masanori Iye; Alan F. M. Moorwood, Editor(s)

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