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  1. Atreya, S. K., A. S. Wong, K. H. Baines, M. H. Wong, and T. C. Owen (2005), Jupiter's ammonia clouds—localized or ubiquitous?, Planet. Space Sci., 53(5), 498–507, doi:10.1016/j.pss.2004.04.002.
  2. Bergin, E. A., E. Lellouch, M. Harwit, M. A. Gurwell, G. J. Melnick, M. L. N. Ashby, G. Chin, N. R. Erickson, P. F. Goldsmith, J. E. Howe, S. C. Kleiner, D. G. Koch, D. A. Neufeld, B. M. Patten, R. Plume, R. Schieder, R. L. Snell, J. R. Stauffer, V. Tolls, Z. Wang, G. Winnewisser, and Y. F. Zhang (2000), Submillimeter Wave Astronomy Satellite Observations of Jupiter and Saturn: Detection of 557 GHz Water Emission from the Upper Atmosphere, Astrophys. J. Lett., 539, L147.
  3. Bézard, B., J. P. Balatueau, and A. Marten (1983), Study of the Deep Cloud Structure in the Equatorial Region of Jupiter from Voyager Infrared and Visible Data, Icarus, 54(3), 434–455.
  4. Burgdorf, M. J., Th. Encrenaz, H. Feuchtgruber, G. R. Davis, Th. Fouchet, D. Gautier, E. Lellouch, G. S. Orton, and S. D. Sidher (2001), IS0 Far-infrared Spectroscopic Observations of Jupiter, In: ESA SP-460.
  5. Carly, J. A., R. W. Carlson, G. J. Irwin, and S. B. Calcutt (2007), Optical constants of ammonium hydrosulfide ice and ammonia ice, J. Optical Soc. o. Am. B, 24(1), 126–136, doi:10.1364/JOSAB.24.000126.
  6. Cavalié, T., F. Billebaud, N. Biver, M. Dobrijevic, E. Lellouch, J. Brillet, A. Lecacheux, Å. Hjalmarson, Aa. Sandqvist, U. Frisk, M. Olberg, and E. A. Bergin (2008), Observation of water vapor in the stratosphere of Jupiter with the Odin space telescope, Planet. Space Sci., 56, 1573–1584, doi:10.1016/j.pss.2008.04.013.
  7. Cavalié, T., N. Biver, P. Hartogh, M. Dobrijevic, F. Billebaud, E. Lellouch, Aa. Sandqvist, J. Brillet, A. Lecacheux, Å. Hjalmarson, U. Frisk, and M. Olberg (2012), Odin space telescope monitoring of water vapor in the stratosphere of Jupiter, Planet. Space Sci., 61, 3–14, doi:10.1016/j.pss.2011.04.001.
  8. Clapp, M. L. and R. E. Miller (1996), Complex Refractive Indices of Crystalline Hydrazine from Aerosol Extinction Spectra, Icarus, 123(2), 396–403, doi:10.1006/icar.1996.0166.
  9. Cunningham, C. T., P. A. R. Ade, E. I. Robson, I. G. Nolt, and J. V. Radostitz (1981), The submillimeter spectra of the planets: Narrow-band photometry, Icarus, 48, 127–139, doi:10.1016/0019-1035(81)90158-5.
  10. de Pater, I. and S. T. Massie (1985), Models of the Millimeter-Centimeter Spectra of the Giant Planets, Icarus, 62(1), 143–171, doi:10.1016/0019-1035(85)90177-0.
  11. Devaraj, K., P. G. Steffes, and B. M. Karpowicz (2011), Reconciling the centimeter- and millimeter-wavelength ammonia absorption spectra under jovian conditions: Extensive millimeter-wavelength measurements and a consistent model, Icarus, 212(1), 224–235, doi:10.1016/j.icarus.2010.12.010.
  12. Encrenaz, Th. and R. Moreno (2002), The microwave spectra of planets, In: AIP Conference Proceedings – EXPERIMENTAL COSMOLOGY AT MILLIMETRE WAVELENGTHS: 2K1BC Workshop, pp. 330–337, doi:10.1063/1.1475653.
  13. Ferraro, J. R., G. Sill, and U. Fink (1980), Infrared Intensity Measurements of Cryodeposited Thin Films of NH3, NH4HS, H2S, and Assignments of Absorption Bands, Am. Sci., 34(5), 525–533.
  14. Fouchet, Th., G. Orton, P. G. J. Irwin, S. B. Calcutt, and C. A. Nixon (2004), Upper limits on hydrogen halides in Jupiter from Cassini/CIRS observations, Icarus, 170, 237–241, doi:10.1016/j.icarus.2004.03.013.
  15. Griffin, M. J., P. A. R. Ade, G. S. Orton, E. I. Robson, W. K. Gear, I. G. Nolt, and J. V. Radostitz (1986), Submillimeter and millimeter observations of Jupiter, Icarus, 65, 244–256, doi:10.1016/0019-1035(86)90137-5.
  16. Hagen, W., A. G. G. M. Tielens, and J. M. Greenberg (1983), A laboratory study of the infrared spectra of interstellar ices, Astronomy & Astrophysics Suppl. S., 51, 389–416.
  17. Hildebrand, R. H., R. F. Loewenstein, D. A. Harper, G. S. Orton, J. Keene, and S. E. Whitcomb (1985), Far-infrared and submillimeter brightness temperatures of the giant planets, Icarus, 64, 64–87, doi:10.1016/0019-1035(85)90039-9.
  18. Joiner, J. and P. G. Steffes (1991), Modeling of Jupiter's millimeter wave emission utilizing laboratory measurements of ammonia (NH3) opacity, J. Geophys. Res., 96(E2), 17463–17470, doi:10.1029/91JE01740.
  19. Karpowicz, B. M. and P. G. Steffes (2011), In search of water vapor on Jupiter: Laboratory measurements of the microwave properties of water vapor under simulated jovian conditions, Icarus, 212(1), 210–223, doi:10.1016/j.icarus.2010.11.035.
  20. Kunde, V., R. Hanel, W. Maguire, D. Gautier, J. P. Baluteau, A. Marten, A. Chedin, N. Husson, and N. Scott (1982), The tropospheric gas composition of Jupiter's north equatorial belt (NH3, PH3, GeH4, H2O) and the Jovian D/H isotopic ratio, Astrophys. J., 263, 443–467.
  21. Lellouch, E., B. Bézard, J. I. Moses, G. R. Davis, P. Drossart, H. Feuchtgruber, E. A. Bergin, R. Moreno, and Th. Encrenaz (2002), The Origin of Water Vapor and Carbon Dioxide in Jupiter's Stratosphere, Icarus, 159, 112–131, doi:10.1006/icar.2002.6929.
  22. Lellouch, E., T. Encrenaz, F. Combes, and P. Drossart (1984), The observability of HCN on Jupiter in the millimeter range, A&A, 135, 365–370.
  23. Li, L., K. H. Baines, M. A. Smith, R. A. West, S. Pérez-Hoyos, H. J. Trammell, A. A. Simon-Miller, B. J. Conrath, P. J. Gierasch, G. S. Orton, C. A. Nixon, G. Filacchione, P. M. Fry, and T. W. Momary (2012), Emitted power of Jupiter based on Cassini CIRS and VIMS observations, J. Geophys. Res., 117(E11), doi:10.1029/2012JE004191.
  24. Lorenz, R. D. and S. E. Shandera (2001), Physical properties of ammonia-rich ice: Application to Titan, Geophys. Res. Lett., 28(2), 215–218, doi:10.1029/2000GL01219.
  25. Marten, A., D. Rouan, J. P. Baluteau, D. Gautier, B. J. Conrath, R. A. Hanel, V. Kunde, R. Samuelson, A. Chedin, and N. Scott (1981), Study of the Ammonia Ice Cloud Layer in the Equatorial Region of Jupiter from the Infrared Interferometric Experiment on Voyager, Icarus, 46, 233–248.
  26. Martonchik, J. V., G. S. Orton, and J. F. Appleby (1984), Optical properties of NH3 ice from the far infrared to the near ultraviolet, Appl. Opt., 23(4), 541–547, doi:10.1364/AO.23.000541.
  27. Moreno, R., A. Marten, Y. Biraud, B. Bézard, E. Lellouch, G. Paubert, and W. Wild (2001), Jovian stratospheric temperature during the two months following the impacts of comet Shoemaker–Levy 9, Planet. Space Sci., 49, 473–486, doi:10.1016/S0032-0633(00)00139-.
  28. Mukai, T. and W. Krätschmer (1986), Optical constants of the mixture of ices, Earth, Moon and Planets, 36(2), 145–155.
  29. Roux, J. A. and B. E. Wood (1983), Infrared optical properties of solid monomethyl hydrazine, N2O4, and N2H4 at cryogenic temperatures, J. Optical Soc. o. Am., 73(9), 1181–1188, doi:10.1364/JOSA.73.001181.
  30. Sagawa, H., P. Hartogh, M. Rengel, A. de Lange, and Th. Cavalié (2010), Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS, Planet. Space Sci., 58, 1692–1698, doi:10.1016/j.pss.2010.05.011.
  31. Sill, G. and U. Fink (1980), Absorption coefficients of solid NH3 from 50 to 7000 cm-1, J. Optical Soc. o. Am., 70(6), 724–739, doi:10.1364/JOSA.70.000724.
  32. Sill, G., U. Fink, and J. R. Ferraro (1981), The infrared spectrum of ammonia hydrate: Explanation for a reported ammonia phase, J. Chem. Phys., 74(2), 997–1000, doi:10.1063/1.441157.
  33. Ulich, B.L., J.R. Cogdell, and J.H. Davis (1973), Planetary brightness temperature measurements at 8.6 mm and 3.1 mm wavelengths, Icarus, 19, 59–82, doi:10.1016/0019-1035(73)90139-5.
  34. Ward, D. B., G. E. Gull, and M. Harwit (1977), Far-infrared spectral observations of Venus, Mars, and Jupiter, Icarus, 30, 295–300, doi:10.1016/0019-1035(77)90162-2.
  35. West, R. A., K. H. Baines, A. J. Friedson, D. Banfield, B. Ragent, and F. W. Taylor (2004), Jupiter: The Planet, Satellites and Magnetosphere, chap. Jovian Clouds and Haze, Cambridge University Press, ISBN 978-0521035453.
  36. Whitcomb, S. E., R. H. Hildebrand, J. Keene, R. F. Stiening, and D. A. Harper (1979), Submillimeter brightness temperatures of Venus, Jupiter, Uranus, and Neptune, Icarus, 38, 75–80, doi:10.1016/0019-1035(79)90086-1.