SINIS Detectors: 30 Years of Achievements and Delusions

Tarasov, M. A.; Gunbina, A. A.; Chekushkin, Artem; Yusupov, R. A.; Édelman, V. S.; Vdovin, V. F.

doi:10.1109/rmc55984.2022.10079692

Cited by 1 publication

(3 citation statements)

References 17 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“… Simulation results of the spectral response of an array of annular antennas with integrated 90 GHz SINIS detectors: irradiation from the substrate ( a ) and irradiation from the antennas ( b ). Figure from [ 48 ]. …”

Section: Figurementioning

confidence: 99%

“…As noted above, for primary test studies, the 90 GHz range is assumed, which is the most convenient from the point of view of astroclimate conditions (observations can be carried out at any time of the year). Publication [48] presents the results of modeling arrays of receiving annular antennas in the 90 GHz range with irradiation from the sub- As noted above, for primary test studies, the 90 GHz range is assumed, which is the most convenient from the point of view of astroclimate conditions (observations can be carried out at any time of the year). Publication [48] presents the results of modeling arrays of receiving annular antennas in the 90 GHz range with irradiation from the substrate side and from the antenna side (Figure 14).…”

Section: Detecting Devicementioning

confidence: 99%

“…Publication [48] presents the results of modeling arrays of receiving annular antennas in the 90 GHz range with irradiation from the sub- As noted above, for primary test studies, the 90 GHz range is assumed, which is the most convenient from the point of view of astroclimate conditions (observations can be carried out at any time of the year). Publication [48] presents the results of modeling arrays of receiving annular antennas in the 90 GHz range with irradiation from the substrate side and from the antenna side (Figure 14). The topology of such a structure was developed with two types of connection of array elements (serial and parallel) (Figure 15).…”

Section: Detecting Devicementioning

confidence: 99%

See 2 more Smart Citations

Microwave Receiving System Based on Cryogenic Sensors for the Optical Big Telescope Alt-Azimuth

Balega,

Bubnov,

Chekushkin

et al. 2024

Sensors

Self Cite

View full text Add to dashboard Cite

This article presents the results of evaluating the possibility of conducting radio astronomy studies in the windows of atmospheric transparency ~100, ~230, and ~350 GHz using the optical Big Telescope Alt-Azimuthal (BTA) of the Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS). A list of some promising astronomical tasks is proposed. The astroclimat conditions at the BTA site and possible optical, cryogenic, and mechanical interfaces for mounting a superconducting radio receiver at the focus of the optical telescope are considered. As a receiving system, arrays of detectors cooled to ~0.3 K based on the superconductor–insulator–normal metal–insulator–superconductor (SINIS) structure are proposed. The implementation of the project will make it possible to use the BTA site of the SAO RAS not only to solve some astronomical problems (it is possible to consider the implementation of a single observatory, the VLBI (very-long-baseline interferometry) mode in the Suffa, EHT (Event Horizon Telescope), and Millimetron projects), but it will also be used to test various cryogenic detectors in a real observatory.

show abstract

Section: Figurementioning

confidence: 99%

Section: Detecting Devicementioning

confidence: 99%