The Venus spectrum: New evidence for ice
β Scribed by William T. Plummer
- Publisher
- Elsevier Science
- Year
- 1970
- Tongue
- English
- Weight
- 452 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
A spectrum from 1.2 to 2.5 Β΅m of Uranus' small satellite Miranda obtained in June 1999 reveals strong water-ice signatures. It confirms the existence of a 2.0-Β΅m water feature previously detected on Miranda and shows a strong second broad 1.5-Β΅m water-ice absorption feature. The spectra also reveal
We report a search, at wavelengths between 402 and \(850 \mathrm{~nm}\), for anomalies in the Venus polarization curve near the \(22^{\circ}\) halo scattering angle for ice crystals (phase angle \(158^{\circ}\) ). Such anomalies, if present, can be interpreted as due to halo birefringence peaks. Ano
Periodic intensity variations in the measured Compton profile anisotropies of ordinary ice I h correspond to distances of 1.8 and 3.0 A Λ, which are close to the hydrogen bond length and the nearest-neighbor O-O distance, respectively. We interpret this result as direct evidence for the covalent nat