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dc.contributor.authorJiwani, Aziz Mohamed Husein
dc.contributor.supervisorProf. Peter Hall
dc.contributor.supervisorProf. Anathkrishnan
dc.contributor.supervisorDr Adrian Sutinjo
dc.contributor.supervisorDr Shantanu Padhi
dc.date.accessioned2017-01-30T09:47:06Z
dc.date.available2017-01-30T09:47:06Z
dc.date.created2014-05-20T05:39:54Z
dc.date.issued2013
dc.identifier.urihttp://hdl.handle.net/20.500.11937/200
dc.description.abstract

The Square Kilometre Array is a next-generation radio telescope originally slated to operate at 70 – 450 MHz frequency in its lowest band (SKA-low). This thesis examines aspects of SKA-low station design and finds that two-stage beamforming produces acceptable performance. Additionally, single- and dual-polarised conical spirals are evaluated as candidate SKA-low elements. Though neither versions are strong candidates for SKA, the single-polarised spiral is an excellent antenna for use in Global Epoch of Reionisation experiments.

dc.languageen
dc.publisherCurtin University
dc.titleConical spiral antennas for the Square Kilometre Array - a feasibility study
dc.typeThesis
dcterms.educationLevelMPhil
curtin.departmentSchool of Electrical and Computer Engineering, Curtin Institute of Radio Astronomy
curtin.accessStatusOpen access


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