Models of the millimeter-centimeter spectra of the giant planets

Icarus

Volumn 62, Issue 1, 1985, Pages 143-171

  De Pater, Imke ^a   Massie, Steven T ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000450382     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(85)90177-0     Document Type: Article

References (67)

1. Radio observations of some minor and major planets
2. Inhomogenous models of the atmosphere of Jupiter
3. Interpretation of the 68189-Å Methane feature observed on Jupiter Saturn and Uranus
4. Planetary observations with the Tidbinbilla interferometer
5. Transition from resonant to nonresonant line shape in microwave absorption
6. Impact broadening of microwave spectra
7. Earth-based radio observations of Jupiter: Millimeter to meter wavelengths
8. 2S in Jupiter
9. 2He Collisions
10. 2He spectrum
11. A method for the determination of abundance ratios in the outer planets—Application to Jupiter
12. Observations of giant planets at 1.4 mm and consequences on the effective temperatures
13. The submillimeter spectra of the planets Narrow-band photometry
14. 21 cm maps of Jupiter's radiation belts from all rotational aspects
15. A comparison of radio data and model calculations of Jupiter's synchrotron radiation I The high energy electron distribution in Jupiter's inner magnetosphere
16. Jupiter's radiation belts and atmosphere
17. Comparison of the thermal and non-thermal-radiation characteristics of Jupiter at 6 11 and 21 cm with model calculations
18. The rotation inversion spectrum of ammonia
19. 15N Jovian ratios: A tentative determination from infrared observations
20. Models of Jupiter's Atmosphere
21. The rotation of Uranus.
22. A Review of the Millimeter and Centimeter Observations of Uranus
23. Evidence for the depletion of ammonia in the Uranus atmosphere
24. Uranus Variability of the microwave spectrum
25. Thermal radio emission from Jupiter and Saturn
26. Interior structure of Saturn inferred from Pioneer 11 gravity data
27. Jupiter's atmosphere Observations and interpretation of the microwave spectrum near 125 cm wavelenght
28. Saturn's microwave spectrum: Implications for the atmosphere and the rings
29. Radio astronomical studies of Venus
30. Detection of water vapor on Jupiter
31. On the observability of HCN in the microwave spectrum of Jupiter
32. The atmosphere of Jupiter An analysis of the Voyager Radio-Occultation measurements
33. Ammonia vertical density profiles in Jupiter and Saturn from their radio electric and infrared emissivities
34. Study of the ammonia ice cloud layer in the equatorial region of Jupiter from the infrared interferometric experiment on Voyager
35. Conversion of para and ortho Hydrogen in the Jovian Planets
36. Microwave radiation from Uranus and Neptune
37. Microwave absorption by gas mixtures at pressures up to several hundred bars
38. Thermal infrared constraints on ammonia ice particles as candidates for clouds in the atmosphere of Saturn
39. Far-infrared through millimeter observations of Uranus and Neptune
40. Observational constraints on the atmospheres of Uranus and Neptune from new measurements near 10 μm
41. Millimeter measurements of Uranus and Neptune
42. Infrared optical properties of graphite
43. 3
44. Chemistry and spectroscopy of the Jovian atmosphere
45. The infrared spectrum of Jupiter
46. High-resolution maps of the 15 GHz emission from Jupiter's disk and radiation belts
47. 3 from 50–7000 cm
48. Origin and structure of Jupiter and its satellites
49. The detection of HCN on Jupiter
50. High spatial and spectral resolution 10-μm observations of Jupiter
51. New observational constraints on the temperature inversions of Uranus and Neptune
52. Photometry and polarimetry of Jupiter
53. Model atmospheres of the major planets
54. The aerosol distribution in Uranus' atmosphere Interpretation of the hydrogen spectrum
55. Absolute brightness temperature measurements at 21 mm wavelength
56. Millimeter-continuum wavelength calibration sources
57. Planetary observations at a wavelength of 132 mm
58. The Jovian ammonia abundance from interferometric observations of limb darkening at 34 mm
59. The structure of the Uranus atmosphere
60. Atmosphere and cloud structure of the Jovian planets
61. One millimeter brightness temperatures of the planets
62. The spectrum of Jupiter at millimeter wavelengths
63. Physics of Planetary Interiors