The thermal structure and energy balance of the Uranian upper atmosphere

Energy sources of the upper atmosphere

✍ V.I. Krassovsky 📂 Article 📅 1959 🏛 Elsevier Science 🌐 English ⚖ 712 KB

Non-Maxwellian Characteristics of the En

Non-Maxwellian Characteristics of the Energy Distribution of Thermal Electrons in the Upper Atmosphere

✍ H. Amemiya 📂 Article 📅 1985 🏛 John Wiley and Sons 🌐 English ⚖ 677 KB

Handbook of Atmospheric Science || Atmos

Handbook of Atmospheric Science || Atmospheric Energy and the Structure of the Atmosphere

✍ Hewitt, C.N.; Jackson, Andrea V. 📂 Article 📅 2003 🏛 Blackwell Science Ltd ⚖ 450 KB 👁 2 views

Thermal Physics of the Atmosphere (Ambau

Thermal Physics of the Atmosphere (Ambaum/Thermal Physics of the Atmosphere) || Vertical Structure of the Moist Atmosphere

✍ Ambaum, Maarten H. P. 📂 Article 📅 2010 🏛 John Wiley & Sons, Ltd 🌐 English ⚖ 189 KB 👁 1 views

*Thermal Physics of the Atmosphere* offers a concise and thorough introduction on how basic thermodynamics naturally leads on to advanced topics in atmospheric physics. The book starts by covering the basics of thermodynamics and its applications in atmospheric science. The later chapters describe

Thermal Physics of the Atmosphere (Ambau

Thermal Physics of the Atmosphere (Ambaum/Thermal Physics of the Atmosphere) || Appendix D: Relationship between Energy Density and Energy Flux

✍ Ambaum, Maarten H. P. 📂 Article 📅 2010 🏛 John Wiley & Sons, Ltd 🌐 English ⚖ 65 KB

*Thermal Physics of the Atmosphere* offers a concise and thorough introduction on how basic thermodynamics naturally leads on to advanced topics in atmospheric physics. The book starts by covering the basics of thermodynamics and its applications in atmospheric science. The later chapters describe

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