dc.creatorYacoub, MD
dc.date2000
dc.dateFEB
dc.date2014-12-02T16:25:25Z
dc.date2015-11-26T17:22:19Z
dc.date2014-12-02T16:25:25Z
dc.date2015-11-26T17:22:19Z
dc.date.accessioned2018-03-29T00:09:47Z
dc.date.available2018-03-29T00:09:47Z
dc.identifierIeee Antennas And Propagation Magazine. Ieee-inst Electrical Electronics Engineers Inc, v. 42, n. 1, n. 150, n. 159, 2000.
dc.identifier1045-9243
dc.identifierWOS:000085881800020
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/66724
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/66724
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/66724
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1283578
dc.descriptionThis paper describes the physical models behind the various fading distributions applicable in wireless-communications systems, and presents the probability density functions, both for the signal envelope and for the power of the mobile radio signal. It addresses the problem of the co-channel interference in terms of its mean value, for macrocellular and microcellular structures, and illustrates how the outage probability is influenced by a series of factors such as reuse pattern, modulation scheme, traffic load, and others.
dc.description42
dc.description1
dc.description150
dc.description159
dc.languageen
dc.publisherIeee-inst Electrical Electronics Engineers Inc
dc.publisherNew York
dc.publisherEUA
dc.relationIeee Antennas And Propagation Magazine
dc.relationIEEE Antennas Propag. Mag.
dc.rightsfechado
dc.rightshttp://www.ieee.org/publications_standards/publications/rights/rights_policies.html
dc.sourceWeb of Science
dc.subjectland mobile radio cellular systems
dc.subjectelectromagnetic propagation
dc.subjectUHF propagation
dc.subjectmicrowave propagation
dc.subjectco-channel interference, reuse pattern, fading distributions, outage probability
dc.subjectUrban
dc.subjectRadio
dc.subjectModel
dc.titleFading distributions and co-channel interference in wireless systems
dc.typeArtículos de revistas


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