Abstract
We have constructed a very reliable SIS receiver on the base of the Nb/A1Ox/Nb junction and the 4-K closed-cycle helium refrigerator. Six SIS receivers are now successfully used in the 45-m telescope and in the Nobeyama Millimeter Array(NMA) for 35–50 GHz and 85–115 GHz.
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References
J.Inatani,T.Kasuga,A.Sakamoto,H.Iwashita and S.Kodaira: IEEE Trans., MAG-23, 1037(1987)
M.Tsuboi,J.Inatani,T.Kasuga,R.Kawabe,A.Sakamoto,H.Iwashita and K.Miyazawa: Int.J.Infrared Millimeter Waves, 8, 1 (1987)
M.Tsuboi,J.Inatani,T.Kasuga and S.Kodaira: ISEC’87, 293(1987)
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© 1990 Springer Science+Business Media Dordrecht
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Inatani, J. et al. (1990). SIS Receiver Development at Nobeyama Radio Observatory. In: Watt, G.D., Webster, A.S. (eds) Submillimetre Astronomy. Astrophysics and Space Science Library, vol 158. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-6850-0_28
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DOI: https://doi.org/10.1007/978-94-015-6850-0_28
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