✦ LIBER ✦

Sulfur dioxide at the Venus cloud tops, 1978–1986

✍ Scribed by Esposito, Larry W.; Copley, M.; Eckert, R.; Gates, L.; Stewart, A. I. F.; Worden, H.

Book ID: 119721071
Publisher: American Geophysical Union
Year: 1988
Tongue: English
Weight: 765 KB
Volume: 93
Category: Article
ISSN: 0148-0227
DOI: 10.1029/jd093id05p05267

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Water vapor and sulfur dioxide abundance

Water vapor and sulfur dioxide abundances at the Venus cloud tops from the Venera-15 infrared spectrometry data

✍ V.I. Moroz; D. Spänkuch; D.V. Titov; K. Schäfer; A.V. Dyachkov; W. Dohler; L.V. 📂 Article 📅 1990 🏛 Elsevier Science 🌐 English ⚖ 437 KB

Variations of sulphur dioxide at the clo

Variations of sulphur dioxide at the cloud top of Venus’s dynamic atmosphere

✍ Marcq, Emmanuel; Bertaux, Jean-Loup; Montmessin, Franck; Belyaev, Denis 📂 Article 📅 2012 🏛 Nature Publishing Group 🌐 English ⚖ 317 KB

The abundance of sulfur dioxide below th

The abundance of sulfur dioxide below the clouds of Venus

✍ Bézard, Bruno; de Bergh, Catherine; Fegley, Bruce; Maillard, Jean-Pierre; Crisp, 📂 Article 📅 1993 🏛 American Geophysical Union 🌐 English ⚖ 359 KB

Global-Scale Winds at the Venus Cloud-To

Global-Scale Winds at the Venus Cloud-Top Inferred from Cloud Streak Orientations

✍ Michael D. Smith; Peter J. Gierasch 📂 Article 📅 1996 🏛 Elsevier Science 🌐 English ⚖ 358 KB

Spatially-resolved high-resolution spect

Spatially-resolved high-resolution spectroscopy of Venus 2. Variations of HDO, OCS, and SO2 at the cloud tops

✍ Vladimir A. Krasnopolsky 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 649 KB

While CO, HCl, and HF, that were considered in the first part of this work, have distinct absorption lines in high-resolution spectra and were detected four decades ago, the lines of HDO, OCS, and SO 2 are either very weak or blended by the telluric lines and have not been observed previously by gro

Sulfur dioxide and other cloud-related g

Sulfur dioxide and other cloud-related gases as the source of the microwave opacity of the middle atmosphere of Venus

✍ Paul G. Steffes; Von R. Eshleman 📂 Article 📅 1981 🏛 Elsevier Science 🌐 English ⚖ 389 KB