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 (S 11 < -10 dB, S 22 < -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.
Original language | English |
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Article number | 025001 |
Journal | Journal of Semiconductors |
Volume | 33 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Feb 2012 |
Keywords
- HEMT
- InGaAs
- InP
- LNA
- SKADS
- telescope