Turbopause
Template:Short description The turbopause, also called the homopause, marks the altitude in an atmosphere below which turbulent mixing dominates. Mathematically, it is defined as the point where the coefficient of Eddy diffusion is equal to the coefficient of molecular diffusion.[1] Because the molecular diffusion coefficient is dependent on both the composition of the diffusing molecule and the background gas, the turbopause altitude will be different for the different molecular species in an atmosphere. For example, in hydrogen (H2) dominated atmospheres, the helium (He) and methane (CH4) turbopause altitudes are different as a result of the different binary diffusion coefficients of helium and methane in molecular hydrogen.[1][2]
The region below the turbopause is known as the homosphere, where the atmosphere is well mixed for chemical species which have long mean residence times. Highly reactive chemicals tend to have variable concentration throughout the atmosphere, while unreactive species have more homogeneous concentrations. The region above the turbopause is the heterosphere, where molecular diffusion dominates and the chemical composition of the atmosphere varies according to chemical species and their atomic weight.
Earth's turbopause lies near the mesopause, at the intersection of the mesosphere and the thermosphere, at an altitude of roughly Template:Cvt.[3] Some other turbopauses in the Solar System that are known include Venus' turbopause at about Template:Cvt, Mars' at about Template:Cvt, Jupiter's at roughly Template:Cvt, and Titan's at around Template:Cvt.[4]
It was discovered by French scientists following the firing of two Véronique sounding rockets on 10 and 12 March 1959.[5]
References
- ^ a b Page Module:Citation/CS1/styles.css has no content.Atreya, Sushil K. (1986), "Vertical Mixing", Atmospheres and Ionospheres of the Outer Planets and Their Satellites, vol. 15, Berlin, Heidelberg: Springer Berlin Heidelberg, pp. 67–68, 74, doi:10.1007/978-3-642-71394-1_4, ISBN 978-3-642-71396-5, retrieved 2025-11-25
{{citation}}: CS1 maint: work parameter with ISBN (link) - ^ Page Module:Citation/CS1/styles.css has no content.Moses, Julianne I.; Fouchet, T.; Yelle, R. V.; Friedson, A. J.; Orton, G. S.; Bezard, B.; Drossart, P.; Gladstone, G. R.; Kostiuk, T.; Livengood, T. A. (2007). "The Stratosphere of Jupiter". In Bagenal, Fran; Dowling, Timothy E.; McKinnon, William B. (eds.). Jupiter (PDF). Cambridge University Press. p. 137.
- ^ Page Module:Citation/CS1/styles.css has no content."turbopause". AMS Glossary (glossary.ametsoc.org). American Meteorological Society. Retrieved 2019-06-01.
- ^ Page Module:Citation/CS1/styles.css has no content.Catling, David; Kasting, James (2017). Atmospheric Evolution on Inhabited and Lifeless Worlds?. Cambridge University Press. p. 6. ISBN 9780521844123.
- ^ Page Module:Citation/CS1/styles.css has no content.Varnoteaux, Philippe. "Il y a 60 ans, Véronique AGI emmenait la France dans l'espace – PARTIE 1 : La campagne de tirs" (in français). Retrieved 2019-08-31.
- Page Module:Citation/CS1/styles.css has no content."The Atmosphere". web.haystack.mit.edu. Archived from the original on 8 November 2005.
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