Thermal IR spectroscopy of Saturn's A and B rings in the 8to 13-µm range reveals a smooth, Planck-like continuum with no spectral structure that could be attributed to optically thin water ice or silicate dust. The brightness temperatures of the A and B rings obtained by fitting a Planck function to
The 2–4-μm spectrum of Saturn's rings
✍ Scribed by Richard C. Puetter; Ray W. Russell
- Publisher
- Elsevier Science
- Year
- 1977
- Tongue
- English
- Weight
- 257 KB
- Volume
- 32
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
The overtone spectrum of H2S has been recorded by intracavity laser spectroscopy in the 14100-14400 cm-1 spectral region. The rovibrational analysis was performed allowing one to assign not only lines involving the pair of interacting states {(402), (303)} ({(60(+), 0), (60(-), 0)} in local mode not
We report the detection of the (H 2 ) 2 dimer in the atmospheres 2. Observations and data reduction. The observations were obtained of Saturn and Neptune based on spectra of the fundamental on UT June 13 and 14, 1995 using the CGS4 Cassegrain spectrograph S 1 (1) collision-induced band of H 2 . The