Neptune's microwave spectrum from 1 mm to 20 cm
Description
Total flux densities and disk-averaged brightness temperatures have been tabulated on the basis of VLA observations of Neptune at 1.3, 2, 6, and 20 cm wavelengths; a recalibration is also conducted of previous observations in order to accurately ascertain the spectral shape of this planet, which is found to have increasing brightness temperature with increasing wavelength, in contrast with that of Uranus. If all the detected emission is atmospheric thermal radiation, ammonia abundance must either be a factor of about 50 lower than the solar N value throughout the Neptune atmosphere, or the planet must emit about 0.3-0.5 mJy synchrotron radiation at 20 cm; the latter possibility is consistent with a planetary magnetic field strength of about 0.5 G at the surface. 39 refs
Additional details
Publishing Information
- Journal Title
- Icarus
- Journal Volume
- 80
- Series
- Icarus.
- Journal Page Range
- 1-13
- ISSN
- 0019-1035
- CODEN
- ICRSA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21016770
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AMMONIA; BRIGHTNESS; FLUX DENSITY; MAGNETIC FIELDS; MATHEMATICAL MODELS; MICROWAVE SPECTRA; NEPTUNE PLANET; RADIATION FLUX; SYNCHROTRON RADIATION; THERMAL RADIATION; URANUS PLANET
- Descriptors DEC
- BREMSSTRAHLUNG; ELECTROMAGNETIC RADIATION; HYDRIDES; HYDROGEN COMPOUNDS; NITROGEN COMPOUNDS; NITROGEN HYDRIDES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; PLANETS; POLAR SOLVENTS; RADIATIONS; SOLVENTS; SPECTRA