High power compatible internally sensed optical phased array
| dc.contributor.author | Roberts, Lyle | |
| dc.contributor.author | Ward, Robert | |
| dc.contributor.author | Francis, Samuel | |
| dc.contributor.author | Sibley, Paul | |
| dc.contributor.author | Fleddermann, Roland | |
| dc.contributor.author | Sutton, Andrew | |
| dc.contributor.author | Smith, Craig | |
| dc.contributor.author | McClelland, David | |
| dc.contributor.author | Shaddock, Daniel | |
| dc.date.accessioned | 2018-11-29T22:54:44Z | |
| dc.date.available | 2018-11-29T22:54:44Z | |
| dc.date.issued | 2016 | |
| dc.date.updated | 2018-11-29T08:02:10Z | |
| dc.description.abstract | The technical embodiment of the Huygens-Fresnel principle, an optical phased array (OPA) is an arrangement of optical emitters with relative phases controlled to create a desired beam profile after propagation. One important application of an OPA is coherent beam combining (CBC), which can be used to create beams of higher power than is possible with a single laser source, especially for narrow linewidth sources. Here we present an all-fiber architecture that stabilizes the relative output phase by inferring the relative path length differences between lasers using the small fraction of light that is back-reflected into the fiber at the OPA’s glass-air interface, without the need for any external sampling optics. This architecture is compatible with high power continuous wave laser sources (e.g., fiber amplifiers) up to 100 W per channel. The high-power compatible internally sensed OPA was implemented experimentally using commercial 15 W fiber amplifiers, demonstrating an output RMS phase stability of λ/194, and the ability to steer the beam at up to 10 kHz | |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 1094-4087 | |
| dc.identifier.uri | http://hdl.handle.net/1885/152901 | |
| dc.publisher | Optical Society of America | |
| dc.source | Optics Express | |
| dc.title | High power compatible internally sensed optical phased array | |
| dc.type | Journal article | |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.issue | 12 | |
| local.contributor.affiliation | Roberts, Lyle, College of Science, ANU | |
| local.contributor.affiliation | Ward, Robert, College of Science, ANU | |
| local.contributor.affiliation | Francis, Samuel, College of Science, ANU | |
| local.contributor.affiliation | Sibley, Paul, College of Science, ANU | |
| local.contributor.affiliation | Fleddermann, Roland, College of Science, ANU | |
| local.contributor.affiliation | Sutton, Andrew, College of Science, ANU | |
| local.contributor.affiliation | Smith, Craig, RMIT / EOS Space Systems Pty Ltd | |
| local.contributor.affiliation | McClelland, David, College of Science, ANU | |
| local.contributor.affiliation | Shaddock, Daniel, College of Science, ANU | |
| local.contributor.authoruid | Roberts, Lyle, u4403794 | |
| local.contributor.authoruid | Ward, Robert, u5088188 | |
| local.contributor.authoruid | Francis, Samuel, u4526962 | |
| local.contributor.authoruid | Sibley, Paul, u5987805 | |
| local.contributor.authoruid | Fleddermann, Roland, u5088176 | |
| local.contributor.authoruid | Sutton, Andrew, u2548624 | |
| local.contributor.authoruid | McClelland, David, u8802403 | |
| local.contributor.authoruid | Shaddock, Daniel, u9701638 | |
| local.description.notes | Imported from ARIES | |
| local.identifier.absfor | 020100 - ASTRONOMICAL AND SPACE SCIENCES | |
| local.identifier.absfor | 090504 - Earthquake Engineering | |
| local.identifier.absfor | 090606 - Photonics and Electro-Optical Engineering (excl. Communications) | |
| local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | |
| local.identifier.ariespublication | U3488905xPUB24329 | |
| local.identifier.citationvolume | 24 | |
| local.identifier.doi | 10.1364/OE.24.013467 | |
| local.identifier.scopusID | 2-s2.0-84979032067 | |
| local.identifier.thomsonID | 000378298400098 | |
| local.type.status | Published Version |
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