Superconductor bolometers such as transition edge sensors, hotelectron bolometers, bolometers on the kinetic inductance of a superconductor, and cold� electron bolometers are the most sensitive receivers for the submillimeter band. The radiation power in such bolometers is absorbed in an absorber made of a thin normalmetal film connected to superconductor- insulator-normal metal (SIN) tunnel junctions. These SIN junctions serve for electron cooling (simi� larly to the Peltier effect in semiconductors) and the output signal proportional to the absorbed power is measured on them. The maximum electron cooling and maximum current response are observed in a bias region somewhat lower than the energy gap of the superconductor in the region of the maximum nonlin� earity of the current-voltage characteristic. Electron cooling makes it possible not only to improve the sen� sitivity, but also to expand the dynamic range due to an increase in the saturation power, because the absorbed power is removed from the absorber by a cooling cur� rent. However, for applications in atmospheric radio astronomy, the power of cosmic microwave back� ground radiation is usually higher than the saturation power of a single bolometer of a superconductor- insulator-normal metal-insulator-superconductor (SINIS) structure, where the normal metal is an absorber film at whose edges SIN junctions are formed. When arrays of such structures are used, the signal power is distributed between individual bolom� eters; this makes it possible to expand the dynamic range in proportion to the number of bolometers in an array. To improve electron cooling, expand the dynamic range, and match the input and output impedances, series/parallel arrays of coldele ctron bolometers have been developed, manufactured, and measured at temperatures from 50 to 350 mK. The bolometers are integrated into crossslot antennas to analyze the polarization of cosmic microwave background radiation at a frequency of 345 GHz. The maximum tem� perature response is 6.5 µV/mK. The noiseequivalent electric powe r at a temperature of 300 mK is 1.2 × 10 -17 W/Hz 1/2 .
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