1 July 1990 Objective prism speckle spectroscopy and wideband projection speckle spectroscopy
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Proceedings Volume 1319, Optics in Complex Systems; (1990); doi: 10.1117/12.34795
Event: 15th International Optics in Complex Systems, 1990, Garmisch, Germany
Abstract
The angular resolution of conventional astronomical spectroscopy is limited to about 1 aresec by the turbulent atmosphere. Much higher resolution can be obtained by (a) objective prism speckle spectroscopy1, which yields diffraction-limited objective prism spectra, and by (b) wideband projection speckle spectroscopy1, which yields spectrally dispersed 1-dimensional projections of the object, i. e., object/spectrum reconstructions O(x,X) or O(x,y,X).
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
F. Griegor, Gerd Weigelt, "Objective prism speckle spectroscopy and wideband projection speckle spectroscopy", Proc. SPIE 1319, Optics in Complex Systems, (1 July 1990); doi: 10.1117/12.34795; https://doi.org/10.1117/12.34795
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