|
Pozdeeva, E. V., Botaki, A. A., & Ul'anov V. L. (1978). Low-temperature measurement of linear thermal-expansion coefficient of electroceramic materials. Steklo i Keramika, (4), 30–31.
|
|
|
Boreman, G. D. (1997). Infrared microantennas. SPIE, 3110, 882–885.
Abstract: We present results of mesurments of the polarization response of asymetric spiral antennas coupled Ni-NiO-Ni diodes, over the wavelength range 10.2 to 10.7 μm. The feed structure of the antenna imposes an elliptical polarization singature that is different from the circular polarization expected from a symmetric spiral. We develop a lossy-transmission-line model yielding the measured polarization response. A combination of a balanced and an unbalanced mode is required. Reflected current waves from the arm ends are significant.
|
|
|
Doi, Y., Wang, Z., Ueda, T., Nickels, P., Komiyama, S., Patrashin, M., et al. (2009). CSIP – a novel photon-counting detector applicable for the SPICA far-infrared instrument. SPICA, (SPICA Workshop 2009).
Abstract: We describe a novel GaAs/AlGaAs double-quantumwell device for the infrared photon detection, called ChargeSensitive Infrared Phototransistor (CSIP). The principle of CSIP detector is the photo-excitation of an intersubband transition in a QW as an charge integrating gate and the signal ampli<ef><ac><81>cation by another QW as a channel with very high gain, which provides us with extremely high responsivity (104 – 106 A/W). It has been demonstrated that the CSIP designed for the mid-infrared wavelength (14.7 μm) has an excellent sensitivity; the noise equivalent power (NEP) of 7 × 10-19 W/ with the quantum effciency of ~ 2%. Advantages of the CSIP against the other highly sensitive detectors are, huge dynamic range of > 106, low output impedance of 103 – 104 Ohms, and relatively high operation temperature (> 2 K). We discuss possible applications of the CSIP to FIR photon detection covering 35 – 60 μm waveband, which is a gap uncovered with presently available photoconductors.
|
|
|
Mumma, M., Kostiuk, T., Cohen, S., Bühl, D., & Von Thuna, P. C. (1975). Heterodyne spectroscopy of astronomical and laboratory sources at 8.5 μm using diode laser local oscillators. Space Science Reviews, 17(5), 661–667.
|
|
|
Encrenaz, T. (2005). Neutral Atmospheres of the Giant Planets: An Overview of Composition Measurements. Space Sci Rev, 116(1-2), 99–119.
|
|