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http://archives.univ-biskra.dz/handle/123456789/2332
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DC Field | Value | Language |
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dc.contributor.author | Z. Hamaizia | - |
dc.contributor.author | N. Sengouga | - |
dc.contributor.author | M. C. E. Yagoub | - |
dc.contributor.author | M. Missous | - |
dc.date.accessioned | 2014-04-18T11:00:26Z | - |
dc.date.available | 2014-04-18T11:00:26Z | - |
dc.date.issued | 2014-04-18 | - |
dc.identifier.uri | http://archives.univ-biskra.dz/handle/123456789/2332 | - |
dc.description.abstract | This 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/1674-4926/33/2/025001 | en_US |
dc.language.iso | en | en_US |
dc.subject | HEMT; InGaAs; InP; SKADS; telescope; LNA | en_US |
dc.title | S-band low noise amplifier using 1 μm InGaAs/InAlAs/InP pHEMT | en_US |
dc.type | Article | en_US |
Appears in Collections: | Publications Internationales |
Files in This Item:
File | Description | Size | Format | |
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S-band low noise amplifier using 1 µm InGaAs_InAlAs_InP pHEMT.pdf | 37,45 kB | Adobe PDF | View/Open |
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