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Cosmic background radiation at 408 Mc/s

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dc.contributor.authorPrice, Richard Marcusen_AU
dc.date.accessioned2017-12-18T01:24:55Z
dc.date.available2017-12-18T01:24:55Z
dc.date.copyright1965
dc.date.issued1965
dc.date.updated2017-11-22T22:44:43Z
dc.description.abstractContinuum cosmic radio emission can be completely described by three observable parameters, (1) the brightness distribution, (2) spectrum, and (3) polarization of the radiation. The purpose of the present investigation is to discuss the "background" component of the observed radio emission, its brightness distribution, absolute brightness temperature, and origins. For the purpose of this thesis, the background radiation is defined as the nearly isotropic component of the emission on which are superimposed strong discrete radio sources, radiation from the disk, or plane, of our own Galaxy, and contributions from within our own solar system.en_AU
dc.format.extent1 v
dc.identifier.otherb1217782
dc.identifier.urihttp://hdl.handle.net/1885/138299
dc.language.isoenen_AU
dc.subject.lcshCosmic rays
dc.titleCosmic background radiation at 408 Mc/sen_AU
dc.typeThesis (PhD)en_AU
dcterms.valid1965en_AU
local.contributor.affiliationThe Australian National Universityen_AU
local.description.notesThesis (Ph.D.)--Australian National University, 1965. This thesis has been made available through exception 200AB to the Copyright Act.en_AU
local.identifier.doi10.25911/5d6fa08725d93
local.identifier.proquestYes
local.mintdoimint
local.type.degreeDoctor of Philosophy (PhD)en_AU

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