Title :
Receiver measurements at 1267 GHz using a diffusion-cooled superconducting transition-edge bolometer
Author :
Skalare, A. ; McGrath, W.R. ; Bumble, B. ; LeDuc, H.G.
Author_Institution :
Center for Space Microelectron. Technol., California Inst. of Technol., Pasadena, CA, USA
fDate :
6/1/1997 12:00:00 AM
Abstract :
We report receiver noise temperature measurements using a quasioptically coupled diffusion-cooled hot-electron bolometer mixer at a local oscillator frequency of 1267 GHz, and an intermediate frequency of 1.4 GHz. A best double-sideband (DSB) receiver noise temperature of 1880 K was measured, with an estimated mixer noise of 945 K (DSB), and a conversion efficiency including coupling losses of -19 dB (DSB). The coupled local oscillator power requirement for this device is estimated at roughly 6 nW. The mixer noise temperature is less than twice that measured earlier in a waveguide receiver at 530 GHz, which shows that the sensitivity of this type of mixer does not degrade sharply with increasing frequency in this regime.
Keywords :
bolometers; niobium; submillimetre wave mixers; submillimetre wave receivers; superconducting device noise; superconducting device testing; superconducting microbridges; superconducting microwave devices; 1.4 GHz; 1267 GHz; 6 nW; Nb; Nb microbridge; conversion efficiency; coupled local oscillator power requirement; coupling losses; diffusion-cooled superconducting transition-edge bolometer; double-sideband receiver noise temperature; intermediate frequency; local oscillator frequency; mixer noise temperature; quasioptically coupled diffusion-cooled hot-electron bolometer mixer; receiver noise temperature measurements; sensitivity; Bolometers; Electrons; Extraterrestrial measurements; Frequency; Lenses; Niobium; Phonons; Space technology; Superconducting device noise; Temperature;
Journal_Title :
Applied Superconductivity, IEEE Transactions on