✦ LIBER ✦

Twilight ozone measurement by solar occultation from AE 5

✍ Scribed by Guenther, B.; Dasgupta, Ranjit; Heath, Donald

Book ID: 119704975
Publisher: American Geophysical Union
Year: 1977
Tongue: English
Weight: 275 KB
Volume: 4
Category: Article
ISSN: 1944-8007
DOI: 10.1029/gl004i010p00434

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Mesospheric ozone densities deduced from

Mesospheric ozone densities deduced from solar occultation measurements

✍ K.H. Ohle; G. Sonnemann; B. Fichtelmann 📂 Article 📅 1984 🏛 Elsevier Science 🌐 English ⚖ 251 KB

Ozone and nitrogen dioxide vertical dist

Ozone and nitrogen dioxide vertical distributions by UV-visible solar occultation from balloons

✍ Pommereau, Jean-Pierre; Piquard, Jacques 📂 Article 📅 1994 🏛 American Geophysical Union 🌐 English ⚖ 392 KB

First Detection of Ozone in the Middle A

First Detection of Ozone in the Middle Atmosphere of Mars from Solar Occultation Measurements

✍ J.E. Blamont; E. Chassefière 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 596 KB

Improved Limb Atmospheric Spectrometer (

Improved Limb Atmospheric Spectrometer (ILAS) for stratospheric ozone layer measurements by solar occultation technique

✍ Sasano, Yasuhiro; Suzuki, Makoto; Yokota, Tatsuya; Kanzawa, Hiroshi 📂 Article 📅 1999 🏛 American Geophysical Union 🌐 English ⚖ 537 KB

Vertical profiles of dust and ozone in t

Vertical profiles of dust and ozone in the martian atmosphere deduced from solar occultation measurements

✍ Blamont, J. E.; Chassefiere, E.; Goutail, J. P.; Mege, B.; Nunes-Pinharanda, M.; 📂 Article 📅 1989 🏛 Nature Publishing Group 🌐 English ⚖ 401 KB

Vertical Structure of Martian Dust Measu

Vertical Structure of Martian Dust Measured by Solar Infrared Occultations from the Phobos Spacecraft

✍ O.I. Korablev; V.A. Krasnopolsky; A.V. Rodin; E. Chassefière 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 649 KB

Solar occultation observations of the Martian atmosphere from the Phobos spacecraft resulted in nine vertical profiles of volume extinction coefficient at 3.7 and \(1.9 \mu \mathrm{m}\) in the altitude range of 12-35 km. Interpretation of the profiles in terms of the Mie scattering theory, with the