Estimate of characteristic scales of atmospheric turbulence by thin beams: Comparison between the von karman and hill-andrews models

Journal of Modern Optics

Volumn 51, Issue 3, 2004, Pages 333-342

  Innocenti, C ^a   Consortini, A ^a  

^a UNIVERSITY OF FLORENCE   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

ATMOSPHERIC TURBULENCE; CORRELATION METHODS; FUNCTIONS; LIGHT PROPAGATION; MATHEMATICAL MODELS; NUMERICAL METHODS;

CORRELATION FUNCTIONS; HILL ANDREWS MODELS; VON KARMAN MODELS;

ATMOSPHERIC OPTICS;

EID: 1242332932     PISSN: 09500340     EISSN: 13623044     Source Type: Journal    
DOI: 10.1080/09500340408235527     Document Type: Article

References (7)

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2. Lukin, V. P., Nosov, E. V., and Fortes, B. V., 1997. Atmos. Oceanic Opt., 10:100
3. Hill, R. J., 1996. “ Trends in Optics:Research ”. In Developments and Applications, Edited by:Consortini, A., 337–349. New York:Academic Press.
4. Consortini, A., and O'Donnell, K. A., 1991. Waves in Random Media, 1:S11
5. Consortini, A., and O'Donnell, K. A., 1993. Waves in Random Media, 3:85
6. Consortini, A., Innocenti, C., and Paoli, G., 2002. Opt. Commun., 214:9
7. Andrews, L. C., 1992. J. Mod. Optics, 39:1849