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Volumn , Issue , 2010, Pages

Thermal Physics of the Atmosphere

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EID: 84891583960     PISSN: None     EISSN: None     Source Type: Book    
DOI: 10.1002/9780470710364     Document Type: Book
Times cited : (69)

References (68)
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    • SI stands for Systéme International d'Unitès, the internationally agreed system of units for physical quantities
    • SI stands for Systéme International d'Unitès, the internationally agreed system of units for physical quantities.
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    • The number N of thermodynamic variables required to define the state of any system is given by the Gibbs' phase rule, N = 2 + C-P, with C the number of independent constituents and P the number of coexisting phases (gas, liquid, solid) in the system
    • The number N of thermodynamic variables required to define the state of any system is given by the Gibbs' phase rule, N = 2 + C-P, with C the number of independent constituents and P the number of coexisting phases (gas, liquid, solid) in the system.
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    • Not all available degrees are necessarily accessible. Quantization of energy levels implies that there is a minimum energy required to excite any degree of freedom
    • Not all available degrees are necessarily accessible. Quantization of energy levels implies that there is a minimum energy required to excite any degree of freedom.
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    • In a more formal treatment of thermodynamics, temperature is defined to be the quantity that indicates the direction of spontaneous heat flow; so heat will flow by definition from high to low temperatures. See Baierlein, R. (1999) Thermal Physics. Cambridge University Press, Cambridge.
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    • Although the expansion is not a reversible process, we can in principle link the initial and final state with a reversible process and thus calculate the change in state variables between the initial and final states
    • Although the expansion is not a reversible process, we can in principle link the initial and final state with a reversible process and thus calculate the change in state variables between the initial and final states.
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    • This problem is solved in quantum mechanics, where the phase space available to molecules is made up of elementary volumes with a size equal to Planck's constant, h
    • This problem is solved in quantum mechanics, where the phase space available to molecules is made up of elementary volumes with a size equal to Planck's constant, h.
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    • Bell System Technical Journal
    • The configuration freedom of a system can be quantified by its information entropy, as defined by Claude Shannon. Edwin Jaynes showed how Shannon's information entropy maps onto the thermodynamic entropy we use here. See
    • The configuration freedom of a system can be quantified by its information entropy, as defined by Claude Shannon. Edwin Jaynes showed how Shannon's information entropy maps onto the thermodynamic entropy we use here. See Shannon, C. E. (1948) Bell System Technical Journal 27, 379-423, 623-656
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    • See also Problem 4.8.
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    • A monoatomic molecule is made of one atom and a diatomic molecule is made of two atoms
    • A monoatomic molecule is made of one atom and a diatomic molecule is made of two atoms.
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    • Thermal physics
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    • The expression Uρh is really a flux density, that is, a flux per unit area. Here, and throughout the rest of this book, we will use the term 'flux' to mean either 'total flux' or 'flux density', depending on the context.
    • The expression Uρh is really a flux density, that is, a flux per unit area. Here, and throughout the rest of this book, we will use the term 'flux' to mean either 'total flux' or 'flux density', depending on the context.
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    • For moist air, we need to replace the temperature in these equations by the virtual temperature, see Section 1.3.
    • For moist air, we need to replace the temperature in these equations by the virtual temperature, see Section 1.3.
  • 21
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    • Because in dynamic meteorology applications only gradients of the Montgomery function play a role, we normally use the dry static energy, Eq. 4.51, instead of the generalized enthalpy to define the Montgomery function for the atmosphere
    • Because in dynamic meteorology applications only gradients of the Montgomery function play a role, we normally use the dry static energy, Eq. 4.51, instead of the generalized enthalpy to define the Montgomery function for the atmosphere.
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    • This requires the cylinder to be below the critical temperature, the temperature above which the gas and liquid phases become indistinguishable and no phase separation can occur no matter how high the pressure is. The critical temperature for water is 647 K
    • This requires the cylinder to be below the critical temperature, the temperature above which the gas and liquid phases become indistinguishable and no phase separation can occur no matter how high the pressure is. The critical temperature for water is 647 K.
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    • This version of Tetens' formula was published in
    • This version of Tetens' formula was published in Bolton, D. (1980) Mon. Wea. Rev. 108, 1046-1053.
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    • The effects of global warming on water vapour and the hydrological cycle are discussed in Boer, G. J. (1993) Clim. Dynam. 8, 225-239; Allen, M. R. & Ingram, W. J. (2002) Nature 419, 224-232; Held, I. M. & Soden, B. J (2006) J. Clim. 19, 5686-5699.
    • The effects of global warming on water vapour and the hydrological cycle are discussed in Boer, G. J. (1993) Clim. Dynam. 8, 225-239; Allen, M. R. & Ingram, W. J. (2002) Nature 419, 224-232; Held, I. M. & Soden, B. J (2006) J. Clim. 19, 5686-5699.
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    • Pseudo-adiabatic processes are somewhat artificial for descending parcels: this would require the external provision of just enough liquid water at the right temperature to keep the parcel saturated
    • Pseudo-adiabatic processes are somewhat artificial for descending parcels: this would require the external provision of just enough liquid water at the right temperature to keep the parcel saturated.
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    • For accurate expressions for the wet-bulb potential temperature see Bolton, D. (1980) Mon. Wea. Rev. 108, 1046-1053.
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    • In these arguments we use virtual temperature, but note that the tephigram only shows temperatures
    • In these arguments we use virtual temperature, but note that the tephigram only shows temperatures.
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    • The Kóhler curve itself is a weak function of temperature. However, this does not change the main argument here
    • The Kóhler curve itself is a weak function of temperature. However, this does not change the main argument here.
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    • There is an asymmetry between positively charged ions and negatively charged ions: positively charged ions require a relative humidity of about 600%; this is presumably due to the geometry of water molecules. See Wilson, C. T. R. (1899) Proc. Roy. Soc. London 65, 289-290.
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    • There are quite a few specialized texts on atmospheric radiation. Notable examples are Goody R. M. & Yung, Y. L. (1989) Atmospheric radiation. Theoretical basis, 2nd edn. Oxford University Press Oxford;
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    • Optical depth is also often given the symbol
    • Optical depth is also often given the symbol.
  • 45
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    • The default choice of 1Wm-2 misrepresents the scatter in the data
    • The value of the reference irradiance Sr does not modify the outcome of the fit but does change the graphical representation of the data, it is better to choose Sr to be similar to S0 or typical values of Sb
    • The value of the reference irradiance Sr does not modify the outcome of the fit but does change the graphical representation of the data. The default choice of 1Wm-2 misrepresents the scatter in the data; it is better to choose Sr to be similar to S0 or typical values of Sb.
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    • The present derivation is partly based on , Equilibrium thermodynamics, 3rd edn. Cambridge University Press, Cambridge
    • The present derivation is partly based on Adkins, C. J. (1983) Equilibrium thermodynamics, 3rd edn. Cambridge University Press, Cambridge.
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    • We can add a constant S0 to the total entropy S by adding S0/V to the entropy density s̃ and still satisfy Eq. 9.87. By the third law, this constant is zero
    • We can add a constant S0 to the total entropy S by adding S0/V to the entropy density s̃ and still satisfy Eq. 9.87. By the third law, this constant is zero.
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    • We have assumed that the radiation remains black during the compression
    • We have assumed that the radiation remains black during the compression.
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    • For further reading see , Thermal physics 2nd edn. W. H. Freeman, New York
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    • The argument presented here is not complete in quantum mechanics as we ignore the ground level of each wave mode. However, this does not change the phase space density gK, which is the purpose of the quantization presented here
    • The argument presented here is not complete in quantum mechanics as we ignore the ground level of each wave mode. However, this does not change the phase space density gK, which is the purpose of the quantization presented here.
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    • Here we restrict ourselves to atmospheric applications. More general treatments can be found in De Groot, S. R. &
    • Here we restrict ourselves to atmospheric applications. More general treatments can be found in De Groot, S. R. &
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    • Bull. Amer. Meteor. Soc
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    • There are various synonyms for exergy, The most commonly encountered synonym is availability, hence the symbol A
    • There are various synonyms for exergy. The most commonly encountered synonym is availability, hence the symbol A.
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    • Accurate equations used to construct pseudo-adiabats are given in
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