光学
光谱成像
天文台
极化(电化学)
旋光法
成像光谱学
物理
遥感
光谱特征
高光谱成像
天文
地质学
化学
物理化学
散射
作者
David A. Glenar,J. J. Hillman,Babak Saif,Jay T. Bergstralh
出处
期刊:Applied optics-OT
[Optica Publishing Group]
日期:1994-11-01
卷期号:33 (31): 7412-7412
被引量:147
摘要
We review the operating principles of noncollinear acousto-optic tunable filters (AOTF's), emphasizing the use of two orthogonally polarized beams for narrow-band imaging. Spectral characterization and spectral broadening measurements of commercially available AOTF's agree with theoretical predictions and reveal difficulties associated with imaging noncollimated light. An AOTF imaging spectropolarimeter for ground-based astronomy that uses CCD's has been constructed at NASA Goddard Space Flight Center. It uses a TeO(2) noncollinear AOTF and a simple optical relay assembly to produce side-by-side orthogonally polarized spectral images. We summarize the instrument design and initial performance tests. We include sample spectral images acquired at the Goddard Geophysical and Astronomical Observatory.
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