MMIC amplifier-based receivers for Earth remote sensing

We have developed amplifier based receivers using Indium Phosphide high electron mobility transistor (HEMT) monolithic microwave integrated circuit (MMIC) technology. These compact receivers are designed with atmospheric temperature and humidity sounding requirements in mind, operating at 100-125 GHz around the 118 GHz oxygen line, and at 160-185GHz near the 183 GHz water line, with average noise temperatures of 1600 and 1200K respectively. They are intended for applications where small volume and power consumption are critical. We will present laboratory data on the noise temperature of these receivers operated at room temperature and preliminary field data.

[1]  M. Barsky,et al.  A 183 GHz low noise amplifier module with 5.5 dB noise figure for the conical-scanning microwave imager sounder (CMIS) program , 2001, 2001 IEEE MTT-S International Microwave Sympsoium Digest (Cat. No.01CH37157).

[2]  Lorene Samoska,et al.  High-gain 150-215-GHz MMIC amplifier with integral waveguide transitions , 1999 .

[3]  P.M. Smith Status of InP HEMT technology for microwave receiver applications , 1996, IEEE 1996 Microwave and Millimeter-Wave Monolithic Circuits Symposium. Digest of Papers.

[4]  S. Weinreb,et al.  Full band waveguide-to-microstrip probe transitions , 1999, 1999 IEEE MTT-S International Microwave Symposium Digest (Cat. No.99CH36282).

[5]  P. Siegel,et al.  A 155-GHz monolithic low-noise amplifier , 1998 .

[6]  M. Janssen Atmospheric Remote Sensing by Microwave Radiometry , 1993 .

[7]  S. Weinreb,et al.  A monolithic HEMT diode balanced mixer for 100-140 GHz , 2001, 2001 IEEE MTT-S International Microwave Sympsoium Digest (Cat. No.01CH37157).

[8]  Aaas News,et al.  Book Reviews , 1893, Buffalo Medical and Surgical Journal.