Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Cynthia A. Hyde"'
Publikováno v:
Optics Communications. 133:381-392
Atmospheric turbulence limits the resolution of astronomical optical imaging systems. Speckle imaging and deconvolution from wavefront sensing (DWFS) are two post-detection image processing methods for overcoming some turbulence effects which do not
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e087fad40311dbb9fd31694c8af21312
https://doi.org/10.1016/s0030-4018(96)00261-1
https://doi.org/10.1016/s0030-4018(96)00261-1
Autor:
Cynthia S, Hyde
Publikováno v:
Journal of AHIMA. 79(11)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::9b0ba2c29e337c80062cc6ec5f61a414
https://pubmed.ncbi.nlm.nih.gov/19115731
https://pubmed.ncbi.nlm.nih.gov/19115731
Publikováno v:
Adaptive Optics.
Many techniques for overcoming the optical effects of turbulence have been studied. These correction techniques include post detection image processing, such as speckle imaging (SI) [1] and deconvolution from wavefront sensing (DWFS) [2]. The post de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::32fadeadb78af681eb549267c1b3ce43
https://doi.org/10.1364/adop.1996.awa.2
https://doi.org/10.1364/adop.1996.awa.2
Publikováno v:
SPIE Proceedings.
Simulating the effects of atmospheric turbulence on optical imaging systems is an important aspect of understanding the performance of these systems. Methods exist for making random draws of phase screens which arise from the Kolmogorov spectrum. In
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9991ee0fc638c5c098daf0d573c9bfca
https://doi.org/10.1117/12.217762
https://doi.org/10.1117/12.217762
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