Abstract
A new heterodyne receiver has been developed for the submillimeter wavelength region. The mixing element is liquid helium cooled bulk n-InSb in a quantizing magnetic field. The value of the magnetic induction is such that the detector photoresponse is dominated by cyclotron-resonance absorption. Laboratory tests have yielded double-sideband receiver noise temperatures of 250 K at 492 GHz, 350 K at 625 GHz and 510 K at 812 GHz. The magnetic induction for these tests was ≈2.5 KG and the mixer operating temperature was ≈1.6 K.
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Elliott R. Brown, M.J. Wengler and T.G. Phillips, J. Appl. Phys., in press.
H.P. Röser, R. Wattenbach and P. van der Wal, “A 150 micron to 500 micron heterodyne spectrmeter for airborne astronomy”, Airborne Astronomy Symposium, NASA Conference Publication 2353 (1984).
D. Buhl, inGalactic and Extragalactic Infrared Spectroscopy, edited by M.F. Kessler and J.P. Phillips (D. Reidel Publishing Co., Boston, 1984). Vol. 108, pp. 221–231.
R.L. Foynter and H.M. Pickett,Submillimeter, Millimeter and Microwave Spectral Line Catalog, JPL Pub. 80-23 (1981).
T.G. Phillips, P.J. Huggins, T.B.H. Kuiper and R.E. Miller, Ap. J. (Letters),238, L103 (1980).
Jocelyn Keene, G.A. Blake and T.G. Phillips, Ap. J. (Letters),271, L27 (1983).
T.G. Phillips, G.A. Blake, Jocelyn Keene, R. Claude Woods and E. Churchwell, Ap. J. (Letters), in press
G.A. Blake, J. Keene and T.G. Phillips, Ap. J. (letters), in press.
E.R. Brown, J. App. Phys.,57, 2361 (1985).
M.A.C.S. Brown and M.F. Kimmitt, Brit. Comm. and Elect.,10, 608 (1963).
J. Besson and B. Phillippeau, L'Onde Electrique,45, 107 (1965).
Junya Yamamoto, H. Yoshinaga and S. Kon, Jap. J. App. Phys.8, 242 (1969).
E.J. Johnson and D.H. Dickey, Phys. Rev. B.1, 2676 (1970).
M. Hass and B.W. Henvis J. Phys. Chem. Solids,23, 1099 (1962).
R. Bowers and Y. Yafet, Phys. Rev.,115, 1165 (1959).
L.D. Landau and E.M. Lifshitz,Quantum Mechanics (Pergamon Press, New York, 1977), Sec. 112.
Y. Yafet, R.W. Keyes and E.N. Adams, J. Phys. Chem. Solids,1, 137 (1956).
R.F. Wallis and H.J. Bowlden, J. Phys. Chem. Solids,7, 78 (1958).
R. Kaplan, J. Appl. Opt.,6, 685 (1967).
R. Kaplan, Phys. Rev.,181, 1154 (1969).
M.I. Dyakanov, A.L. Efros, and D.L. Mitchell, Phys. Rev.,180, 813 (1969).
F. Kuchar, E. Fantner and G. Bauer, J. Phys. C: Solid State Phys.,10, 3577 (1977).
T. Murotani and Y. Nisida, J. Phys. Soc. Jap.,32, 986 (1972).
Elliott R. Brown, Ph. D. dissertation, California Institute of Technology (1985).
E.H. Putley inSemiconductors and Semimetals, edited by R.K. Willardson and A.C. Beer (Academic, New York, 1966), Vol. 2, Chap. 9.
M.V. Schneider and T.G. Phillips, Int. J. of Infrared and Millimeter Waves,2, 15 (1981).
E. Otsuka inInfrared and Millimeter Waves, edited by K.J. Button (Academic Press, New York, 1980), Vol. 3, p. 347.
E. Gornik, T.Y. Chang, T.J. Bridges, V.T. Nguyen, J.D. McGee and W. Muller, Phys. Rev. Lett.,40, 1151 (1978).
Elliott R. Brown, Electronics Letters,21, 417 (1985).
Jam Farhoomand, G. A. Blake, M.A. Frerking and H.M. Pickett, J. Appl. Phys.,57, 1763 (1985).
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Brown, E.R., Keene, J. & Phillips, T.G. A heterodyne receiver for the submillimeter wavelength region based on cyclotron resonance in InSb at low temperatures. Int J Infrared Milli Waves 6, 1121–1138 (1985). https://doi.org/10.1007/BF01019856
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DOI: https://doi.org/10.1007/BF01019856