Submillimeter observations of planets
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference15 articles.
1. Far-infrared brightness temperature of the planets;Armstrong;Astrophys. J. (Lett.),1973
2. Absorption of infrared radiant energy by CO2 and H2O. III. Absorption by H2O between 0.5 and 36 cm−1 (278 μm–2 cm);Burch;J. Opt. Soc. Amer.,1968
3. Observations of planets, nebulae, and galaxies at 350 microns.;Harper;Astrophys. J. (Lett.),1973
4. Lunar observations at a wavelength of 1 millimeter;Low;Astrophys. J.,1965
5. Thermal models and microwave temperatures of the planet Mercury;Morrison;Smithsonian Astrophys. Obs. Spec. Rept.,1969
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1. The brightness temperature of Mercury at 150 and 240 GHz;The European Physical Journal Plus;2011-10
2. Spectrophotometry of Saturn and its rings from 60 to 180 microns;Icarus;1983-02
3. Observations of the radio emission of Venus, Jupiter, and certain galactic sources at 0.87 mm;Radiophysics and Quantum Electronics;1982-03
4. The submillimeter spectra of the planets: Narrow-band photometry;Icarus;1981-10
5. Brightness Temperatures of Saturn's Disk and Rings at 400 and 700 Micrometers;Science;1980-11-14
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