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dc.contributor.authorRobertson, Duncan A.
dc.date.accessioned2018-09-05T13:30:05Z
dc.date.available2018-09-05T13:30:05Z
dc.date.issued2018-06-20
dc.identifier255732512
dc.identifier2ba54324-89b7-42c4-9ab7-af70d06c4d1d
dc.identifier85053639546
dc.identifier.citationRobertson , D A 2018 , Enabling technologies for high performance millimetre and aub-millimetre wave radar . in 2018 19th International Radar Symposium (IRS) . , 8448180 , IEEE , 2018 19th International Radar Symposium (IRS) , Bonn , North Rhine-Westphalia , Germany , 20/06/18 . https://doi.org/10.23919/IRS.2018.8448180en
dc.identifier.citationconferenceen
dc.identifier.isbn9781538612699
dc.identifier.isbn9783736995451
dc.identifier.othercrossref: 10.23919/IRS.2018.8448180
dc.identifier.otherORCID: /0000-0002-4042-2772/work/48131844
dc.identifier.urihttps://hdl.handle.net/10023/15969
dc.description.abstractThe successful realisation of high performance millimetre and sub-millimetre wave radars requires key enabling technologies, many of which are not yet commercially available. This paper illustrates some of the key enabling technologies developed to address radar system requirements including chirp generation, feedhorns, duplexing and non-mechanical beam steering. The type of high performance radar system which can be achieved using these technologies is illustrated with the examples of the ‘T-220’ 94 GHz FMCW Doppler radar used for high sensitivity target and clutter phenomenology studies and the ‘CONSORTIS’ 340 GHz 3D imaging radar developed for concealed object detection as required for next generation aviation security screening.
dc.format.extent10
dc.format.extent1423170
dc.language.isoeng
dc.publisherIEEE
dc.relation.ispartof2018 19th International Radar Symposium (IRS)en
dc.subjectQC Physicsen
dc.subjectT Technologyen
dc.subjectT-NDASen
dc.subject.lccQCen
dc.subject.lccTen
dc.titleEnabling technologies for high performance millimetre and aub-millimetre wave radaren
dc.typeConference itemen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.23919/IRS.2018.8448180


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