Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

High power compatible internally sensed optical phased array

dc.contributor.authorRoberts, Lyle
dc.contributor.authorWard, Robert
dc.contributor.authorFrancis, Samuel
dc.contributor.authorSibley, Paul
dc.contributor.authorFleddermann, Roland
dc.contributor.authorSutton, Andrew
dc.contributor.authorSmith, Craig
dc.contributor.authorMcClelland, David
dc.contributor.authorShaddock, Daniel
dc.date.accessioned2018-11-29T22:54:44Z
dc.date.available2018-11-29T22:54:44Z
dc.date.issued2016
dc.date.updated2018-11-29T08:02:10Z
dc.description.abstractThe 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.mimetypeapplication/pdfen_AU
dc.identifier.issn1094-4087
dc.identifier.urihttp://hdl.handle.net/1885/152901
dc.publisherOptical Society of America
dc.sourceOptics Express
dc.titleHigh power compatible internally sensed optical phased array
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue12
local.contributor.affiliationRoberts, Lyle, College of Science, ANU
local.contributor.affiliationWard, Robert, College of Science, ANU
local.contributor.affiliationFrancis, Samuel, College of Science, ANU
local.contributor.affiliationSibley, Paul, College of Science, ANU
local.contributor.affiliationFleddermann, Roland, College of Science, ANU
local.contributor.affiliationSutton, Andrew, College of Science, ANU
local.contributor.affiliationSmith, Craig, RMIT / EOS Space Systems Pty Ltd
local.contributor.affiliationMcClelland, David, College of Science, ANU
local.contributor.affiliationShaddock, Daniel, College of Science, ANU
local.contributor.authoruidRoberts, Lyle, u4403794
local.contributor.authoruidWard, Robert, u5088188
local.contributor.authoruidFrancis, Samuel, u4526962
local.contributor.authoruidSibley, Paul, u5987805
local.contributor.authoruidFleddermann, Roland, u5088176
local.contributor.authoruidSutton, Andrew, u2548624
local.contributor.authoruidMcClelland, David, u8802403
local.contributor.authoruidShaddock, Daniel, u9701638
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absfor090504 - Earthquake Engineering
local.identifier.absfor090606 - Photonics and Electro-Optical Engineering (excl. Communications)
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB24329
local.identifier.citationvolume24
local.identifier.doi10.1364/OE.24.013467
local.identifier.scopusID2-s2.0-84979032067
local.identifier.thomsonID000378298400098
local.type.statusPublished Version

Downloads

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
01_Roberts_High_power_compatible_2016.pdf
Size:
5.46 MB
Format:
Adobe Portable Document Format