𝔖 Bobbio Scriptorium
✦   LIBER   ✦

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


8- to 13-μm Spectra of Saturn's A and B
✍ David K. Lynch; Ann L. Mazuk; Ray W. Russell; John A. Hackwell; Martha S. Hanner 📂 Article 📅 2000 🏛 Elsevier Science 🌐 English ⚖ 66 KB

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 H2S Spectrum around 0.7 μm
✍ J.-M. Flaud; O. Vaittinen; A. Campargue 📂 Article 📅 1998 🏛 Elsevier Science 🌐 English ⚖ 187 KB

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

Hydrogen Dimer Features in the 2-μm Spec
✍ Laurence M. Trafton; Sang J. Kim; Thomas R. Geballe; Steven Miller 📂 Article 📅 1997 🏛 Elsevier Science 🌐 English ⚖ 254 KB

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