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dc.contributor.author Mabena, Chemist M
dc.contributor.author Roux, FS
dc.date.accessioned 2019-04-11T06:44:52Z
dc.date.available 2019-04-11T06:44:52Z
dc.date.issued 2019-01
dc.identifier.citation Mabena, C.M. and Roux, F.S. 2019. Optical orbital angular momentum under strong scintillation. Physical Review A, Vol 99(1), pp. 1-8 en_US
dc.identifier.issn 2469-9926
dc.identifier.issn 2469-9934
dc.identifier.uri DOI: 10.1103/PhysRevA.99.013828
dc.identifier.uri https://journals.aps.org/pra/abstract/10.1103/PhysRevA.99.013828
dc.identifier.uri http://hdl.handle.net/10204/10949
dc.description Copyright: 2019 American Physical Society en_US
dc.description.abstract The evolution of classical optical fields propagating through atmospheric turbulence is investigated under arbitrary conditions. We use the single-phase screen (SPS) method and the infinitesimal propagation equation (IPE), a multiphase screen (MPS) method, to compute the optical power fractions retained in an input Laguerre-Gauss (LG) mode or transferred to higher-order LG modes. Although they show the same trend while the scintillation is weak, the IPE and SPS predictions deviate when the strength of scintillation passes a certain threshold. These predictions are compared with numerical simulations of optical fields propagating through turbulence. The simulations are performed using an MPS model, based on the Kolmogorov theory of turbulence, for different turbulence conditions to allow comparison in both weak and strong scintillation. The numerical results agree well with the IPE results in all conditions, but they deviate from the SPS results for strong scintillation. en_US
dc.language.iso en en_US
dc.publisher American Physical Society en_US
dc.relation.ispartofseries Workflow;21967
dc.subject Angular momentum of light en_US
dc.subject Optical orbital angular en_US
dc.subject Scintillation en_US
dc.title Optical orbital angular momentum under strong scintillation en_US
dc.type Article en_US


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