Abstract
A 3 mm low noise beam-lead Schottky diode mixer has been developed. At cryogenic temperatures the conversion loss is ∼ 6.3 dB, and the DSB mixer noise temperature is ∼75 K, respectively. The mixer was installed into the cooled receiver for radioastronomical observations at the Metsähovi 13.7-m radio telescope. Total DSB noise temperature of the cooled receiver with an ultra low noise HEMT IF amplifier was ∼ 110 K at 103 GHz. The tuning range of the mixer mount was from ∼ 70 GHz to ∼ 115 GHz.
Similar content being viewed by others
References
Räisänen A., Lehto A., Tiuri M., Lamb J., 1983, Electronics. Lett.19, 892
Crowe T.W., Mattauch R.J., 1986, IEEE Trans.MTT–34, 753
Bozhkov V.G., Kurkan K.I., Genneberg V.A. et al., 1990, Diodes for converters and integrated converters for 3 mm wavelength. Digest, 5 Celostatni Konference o Microvlune Technice.-MITECO 90. Sbornik Prepnasek — Dil 2, Pardubice, 24 –26 Dubna 1990, p.89–97
Frost W. (ed.) Heat transfer at low temperatures. The Univers.of Tenn. Space Instit., Plenum Press., N.Y., 1975
Goronina K.A., Dryagin Y.A., 1990, Measurements of mixing diode's performances, Preprint of IAP of Acad.of Sci. USSR, N 254, Gorky (in Russian)
Predmore C.R., Räisänen A.V., Ericson N.R., Goldsmith P.F., Marero J.L., 1984, IEEE Trans. MTT–32, 498
Zinchenko I., Forsstiöm V., Lapinov A., Mattila K., 1994, Astron. Astrophys., in press
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Dryagin, Y., Lapkin, I., Vdovin, V. et al. Low noise beam-lead diode mixer for the 3 mm radio astronomical receiver at the metsähovi radio research station. Exp Astron 5, 279–287 (1994). https://doi.org/10.1007/BF01583701
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF01583701