Bibliography database of Radiophysics Laboratory (RpLab) -- Query Results

Chouvaev D, Kuzmin L, Tarasov M, Sundquist P, Willander M, Claeson T. Normal metal hot-electron microbolometer with Andreev mirrors for THz space applications. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. p. 331–5. https://db.rplab.ru/refbase/show.php?record=285
Mann CM, Matheson DN, Ellison BN, Oldfield ML, Moyna BP, Spencer JJ, et al. On the design and measurement of a 2.5 THz waveguide mixer. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. 161. https://db.rplab.ru/refbase/show.php?record=283
Yazoubov P, Kroug M, Merkel H, Kollberg E, Gol'tsman G, Lipatov A, et al. Quasioptical NbN phonon-cooled hot electron bolometric mixers with low optimal local oscillator power. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. p. 131–40. Abstract: In this paper, the noise perform.ance of NIN based phonon-cooled Hot Electron Bolometric (HEB) quasioptical mixers is investigated in the 0.55-1.1 THz frequency range. The best results of the DSB noise temperature are: 500 K at 640 GHz, 600 K at 750 GHz, 850 K at 910 GHz and 1250 K at 1.1 THz. The water vapor in the signal path causes a significant contribution to the measured noise temperature around 1.1 THz. The required LO power is typically about 60 nW. The frequency response of the spiral antenna+lens system is measured using a Fourier Transform Spectrometer with the HEB operating in a detector mode. Keywords: NbN HEB mixers https://db.rplab.ru/refbase/show.php?record=1589
Svechnikov S, Verevkin A, Voronov B, Menschikov E, Gershenzon E, Gol'tsman G. Quasioptical phonon-cooled NbN hot electron bolometer mixers at 0.5-1.1 THz. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. p. 45–51. Abstract: The noise performance of a receiver incorporating spiral antenna coupled NbN phonon-cooled superconducting hot electron bolometric mixer is measured from 450 GHz to 1200 GHz. The mixer element is thin (thickness nm) NbN 1.5 pm wide and 0.2 i.um long film fabricated by lift-off e-beam lithography on high-resistive silicon substrate. The noise of the receiver temperature is 1000 K at 800-900 GHz, 1200 K at 950 GHz, and 1600 K at 1.08 THz. The required (absorbed) local-oscillator power is —20 nW. Keywords: NbN HEB mixers https://db.rplab.ru/refbase/show.php?record=1586
Tetsu Suzuki, Chris Mann, Takanari Yasui, Hirotomo Fujishima, Koji Mizuno. Quasi–integrated planar Schottky barrier diodes for 2.5 THz receivers. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. 187. https://db.rplab.ru/refbase/show.php?record=284

Chouvaev D, Kuzmin L, Tarasov M, Sundquist P, Willander M, Claeson T. Normal metal hot-electron microbolometer with Andreev mirrors for THz space applications. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. p. 331–5.

Mann CM, Matheson DN, Ellison BN, Oldfield ML, Moyna BP, Spencer JJ, et al. On the design and measurement of a 2.5 THz waveguide mixer. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. 161.

Yazoubov P, Kroug M, Merkel H, Kollberg E, Gol'tsman G, Lipatov A, et al. Quasioptical NbN phonon-cooled hot electron bolometric mixers with low optimal local oscillator power. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. p. 131–40.

Svechnikov S, Verevkin A, Voronov B, Menschikov E, Gershenzon E, Gol'tsman G. Quasioptical phonon-cooled NbN hot electron bolometer mixers at 0.5-1.1 THz. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. p. 45–51.

Tetsu Suzuki, Chris Mann, Takanari Yasui, Hirotomo Fujishima, Koji Mizuno. Quasi–integrated planar Schottky barrier diodes for 2.5 THz receivers. In: Proc. 9^th Int. Symp. Space Terahertz Technol.; 1998. 187.