24 August 1992 Adaptive acousto-optical processor for observations of radio emission from pulsars
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Abstract
The paper considers the possibility of using acousto-optic devices for compensation of interstellar dispersion influence in observations of radio emission from pulsars. The principle of operation in an adaptive acousto-optical processor using a CCD-line photodetector in the shift-and-add mode is discussed. An adaption is fulfilled by control CCD scan rate. Results are reported for experimental investigations in the laboratory breadboard setup.
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Nelly A. Esepkina, Nelly A. Esepkina, Alexander P. Lavrov, Alexander P. Lavrov, Michail N. Ananyev, Michail N. Ananyev, Nickolay N. Evtikhiev, Nickolay N. Evtikhiev, } "Adaptive acousto-optical processor for observations of radio emission from pulsars", Proc. SPIE 1704, Advances in Optical Information Processing V, (24 August 1992); doi: 10.1117/12.139909; https://doi.org/10.1117/12.139909
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