Please use this identifier to cite or link to this item: http://archives.univ-biskra.dz/handle/123456789/2332
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dc.contributor.authorZ. Hamaizia-
dc.contributor.authorN. Sengouga-
dc.contributor.authorM. C. E. Yagoub-
dc.contributor.authorM. Missous-
dc.date.accessioned2014-04-18T11:00:26Z-
dc.date.available2014-04-18T11:00:26Z-
dc.date.issued2014-04-18-
dc.identifier.urihttp://archives.univ-biskra.dz/handle/123456789/2332-
dc.description.abstractThis paper discusses the design of a wideband low noise amplifier (LNA) in which specific architecture decisions were made in consideration of system-on-chip implementation for radio-astronomy applications. The LNA design is based on a novel ultra-low noise InGaAs/InAlAs/InP pHEMT Linear and non-linear modelling of this pHEMT has been used to design an LNA operating from 2 to 4 GHz. A common-drain in cascade with a common source inductive degeneration, broadband LNA topology is proposed for wideband applications. The proposed configuration achieved a maximum gain of 27 dB and a noise figure of 0.3 dB with a good input and output return loss (S11 < −10 dB, S22 < −11 dB). This LNA exhibits an input 1-dB compression point of −18 dBm, a third order input intercept point of 0 dBm and consumes 85 mW of power from a 1.8 V supply. Link http://iopscience.iop.org/1674-4926/33/2/025001en_US
dc.language.isoenen_US
dc.subjectHEMT; InGaAs; InP; SKADS; telescope; LNAen_US
dc.titleS-band low noise amplifier using 1 μm InGaAs/InAlAs/InP pHEMTen_US
dc.typeArticleen_US
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