✦ LIBER ✦

Ion properties of the high-latitude middle atmosphere

✍ Scribed by C. Li; J.D. Mitchell; R.D. Brink; C.L. Croskey; L.C. Hale

Publisher: Elsevier Science
Year: 1994
Tongue: English
Weight: 368 KB
Volume: 14
Category: Article
ISSN: 0273-1177
DOI: 10.1016/0273-1177(94)90130-9

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

N2+ ions in the nocturnal upper atmosphe

N2+ ions in the nocturnal upper atmosphere at middle latitudes

✍ Yano Kyo 📂 Article 📅 1966 🏛 Elsevier Science 🌐 English ⚖ 760 KB

Electrical properties of the middle atmo

Electrical properties of the middle atmosphere

✍ John D. Mitchell 📂 Article 📅 1990 🏛 Elsevier Science 🌐 English ⚖ 862 KB

The structure of the venusian atmosphere

The structure of the venusian atmosphere at high latitudes

✍ L.V. Zasova 📂 Article 📅 1995 🏛 Elsevier Science 🌐 English ⚖ 788 KB

High-latitude plasma densities in the mi

High-latitude plasma densities in the middle atmosphere and characteristics of precipitating electrons during an auroral absorption substorm

✍ A. Osepian; V. Vlaskov; H. Ranta; A. Ranta; E. Turunen 📂 Article 📅 1993 🏛 Elsevier Science 🌐 English ⚖ 444 KB

Middle atmosphere measurements of small-

Middle atmosphere measurements of small-scale electron density irregularities and ion properties during the MAC/Epsilon Campaign

✍ S.P. Blood; J.D. Mitchell; C.L. Croskey 📂 Article 📅 1990 🏛 Elsevier Science 🌐 English ⚖ 276 KB

The Thermal Structure of Triton's Middle

The Thermal Structure of Triton's Middle Atmosphere

✍ J.L. Elliot; D.F. Strobel; X. Zhu; J.A. Stansberry; L.H. Wasserman; O.G. Franz 📂 Article 📅 2000 🏛 Elsevier Science 🌐 English ⚖ 61 KB

The atmospheric structure of Triton in the altitude range 25-150 km shows an unexpectedly steep thermal gradient of 0.26 K km -1 above 50 km altitude, with a nearly isothermal profile below. The upper part of the profile can be explained by downward conduction of heat deposited by magnetospheric ele