from recent...Figure 13.2 A prototype THz instrument for exploring the atmosphere and wate...Figure 13.3 The availability of planar Schottky diodes has made it possible ...Figure 13.4 A number of different technologies can possibly be used as local...Figure 13.5 A compilation of measured output power from various multiplied s...Figure 13.6 An all‐solid‐state receiver to 1200 GHz has been demonstrated. B...Figure 13.7 A Nb SIS chip fabricated on SOI wafer and packaged in a split wa...Figure 13.8 Recent measurements on high current density SIS receiver. The br...Figure 13.9 Comparison of the frequency‐dependent loss of different supercon...Figure 13.10 Measured sensitivity of SIS, HEB, and SBD is compared along wit...Figure 13.11 Measured D/H ratios indicate a large range for comets with only...Figure 13.12 A two‐pixel 340 GHz. (a) show the full assembly with WR‐8 input...Figure 13.13 W‐band GaN power amplifiers make it possible to design 1.9 THz ...Figure 13.14 A compact 16‐pixel LO chain has been built with diagonal horns ...Figure 13.15 Nominal power requirement of 10 microwatts is demonstrated acro...Figure 13.16 A nominal block diagram for an active instrument that can measu...
Guide
1 Cover
10 Index
11 Wiley End User License Agreement
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