dc.contributor.author |
Chaibi, A
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|
dc.contributor.author |
Mafusire, C
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|
dc.contributor.author |
Forbes, A
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dc.date.accessioned |
2014-06-17T12:55:05Z |
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dc.date.available |
2014-06-17T12:55:05Z |
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dc.date.issued |
2013-09 |
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dc.identifier.citation |
Chaibi, A, Mafusire, C and Forbes, A. 2013. Propagation of orbital angular momentum carrying beams through a perturbing medium. Journal of Optics, vol. 15(10), pp |
en_US |
dc.identifier.issn |
2040-8978 |
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dc.identifier.uri |
http://iopscience.iop.org/2040-8986/15/10/105706/pdf/2040-8986_15_10_105706.pdf
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dc.identifier.uri |
http://hdl.handle.net/10204/7484
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dc.description |
Copyright: 2013 IOP Publishing. This is an ABSTRACT ONLY. The definitive version is published in Journal of Optics, vol. 15(10), pp 1- 10 |
en_US |
dc.description.abstract |
The orbital angular momentum of light has been suggested as a means of information transfer over free-space, yet the detected optical vortex is known to be sensitive to perturbation. Such effects have been studied theoretically, in particular through turbulence. Here we demonstrate a simple apparatus to introduce turbulence-like distortions to optical fields propagating over a long path. We create vortex beams and observe their propagation through a heated spinning pipe, known to mimic the two primary atmospheric aberrations, namely tip–tilt and defocus. We use a digital decomposition tool to modally resolve the distorted vortex beam into its azimuthal components to observe the impact of the medium on the detection of the encoded vortex charge. Such techniques are useful in studies of free-space optical communication with orbital angular momentum. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
IOP Publishing |
en_US |
dc.relation.ispartofseries |
Workflow;12822 |
|
dc.subject |
Orbital angular momentum |
en_US |
dc.subject |
OAM |
en_US |
dc.subject |
Turbulence |
en_US |
dc.subject |
Vortex beams |
en_US |
dc.title |
Propagation of orbital angular momentum carrying beams through a perturbing medium |
en_US |
dc.type |
Article |
en_US |
dc.identifier.apacitation |
Chaibi, A., Mafusire, C., & Forbes, A. (2013). Propagation of orbital angular momentum carrying beams through a perturbing medium. http://hdl.handle.net/10204/7484 |
en_ZA |
dc.identifier.chicagocitation |
Chaibi, A, C Mafusire, and A Forbes "Propagation of orbital angular momentum carrying beams through a perturbing medium." (2013) http://hdl.handle.net/10204/7484 |
en_ZA |
dc.identifier.vancouvercitation |
Chaibi A, Mafusire C, Forbes A. Propagation of orbital angular momentum carrying beams through a perturbing medium. 2013; http://hdl.handle.net/10204/7484. |
en_ZA |
dc.identifier.ris |
TY - Article
AU - Chaibi, A
AU - Mafusire, C
AU - Forbes, A
AB - The orbital angular momentum of light has been suggested as a means of information transfer over free-space, yet the detected optical vortex is known to be sensitive to perturbation. Such effects have been studied theoretically, in particular through turbulence. Here we demonstrate a simple apparatus to introduce turbulence-like distortions to optical fields propagating over a long path. We create vortex beams and observe their propagation through a heated spinning pipe, known to mimic the two primary atmospheric aberrations, namely tip–tilt and defocus. We use a digital decomposition tool to modally resolve the distorted vortex beam into its azimuthal components to observe the impact of the medium on the detection of the encoded vortex charge. Such techniques are useful in studies of free-space optical communication with orbital angular momentum.
DA - 2013-09
DB - ResearchSpace
DP - CSIR
KW - Orbital angular momentum
KW - OAM
KW - Turbulence
KW - Vortex beams
LK - https://researchspace.csir.co.za
PY - 2013
SM - 2040-8978
T1 - Propagation of orbital angular momentum carrying beams through a perturbing medium
TI - Propagation of orbital angular momentum carrying beams through a perturbing medium
UR - http://hdl.handle.net/10204/7484
ER -
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en_ZA |