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Decagon Devices, 950 NE Nelson Ct., Pullman, WA 99163 and Washington State Univ., Pullman, WA 99164
* Corresponding author (gaylon{at}decagon.com).
Received for publication August 26, 2002.
| ABSTRACT |
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| INTRODUCTION |
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| EQUATIONS FOR SENSIBLE AND LATENT HEAT FLUX |
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![]() | [1] |
is the molar density of air (mol m-3), cp is the molar specific heat of air (J mol-1 K-1), KH is an appropriate diffusivity (m2 s-1), T (°C) is temperature, and z (m) is distance.
The transport of latent heat is similarly described by
![]() | [2] |
Here
(J mol-1) is the latent heat of vaporization for water, E (mol m-2 s-1) is the flux density of water vapor, Kv is a vapor diffusivity (molecular or eddy diffusivity, depending on location), p is atmospheric pressure (kPa), and e is the vapor pressure (kPa).
From the definition of relative humidity, h, the vapor pressure in Eq. [2] can be rewritten as the product esh, where es is the saturation vapor pressure at air temperature. Substituting this product for e in Eq. [2] and using the product rule from calculus gives:
![]() | [3] |
The derivative in the first term on the right can be rewritten as
dT/dz, where
= des/dT is the slope of the saturation vapor pressure function (kPa °C-1). The derivative in the second term in Eq. [3] can also be transformed by defining a vapor deficit as D = es(1 - h). The derivative of the vapor deficit is dD = -esdh. Substituting these into Eq. [4] gives
![]() | [4] |
The second term on the right of Eq. [4] is defined as the isothermal latent heat flux density,
Ei.
![]() | [5] |
While it arises from mathematical expediency, isothermal latent heat flux is sometimes used to approximate actual latent heat flux, such as when evaporation is assumed proportional to a gradient in relative humidity. In an isothermal system, such an assumption would be correct, but in nonisothermal systems, an additional component of evaporation is due to the temperature difference (Eq. [4]).
Equations 1, 4, and 5 can now be combined to give
![]() | [6] |
The apparent psychrometer constant
* =
KH/Kv, where the thermodynamic psychrometer constant
= cp/
(K-1). When KH = Kv,
* =
. The slope of the saturation mole fraction function s =
/p (K-1).
The sum of the sensible and latent heat fluxes is the enthalpy flux:
![]() | [7] |
Combining Eq. [6] and [7] to eliminate C gives
![]() | [8] |
When H = Rn - G (Rn is net radiation; G is the rate of heat storage), Eq. [8] is the form of the PenmanMonteith equation given by Monteith (1980) for surfaces that are not saturated. A complementary equation for C is derived by eliminating
E between Eq. [6] and [7]:
![]() | [9] |
This equation is similar to one given by Monteith (1973), except here the humidity of the evaporating surface is included in the denominator while Monteith's original equation assumed evaporation from a saturated surface.
| DECOUPLING THE HEAT AND VAPOR TRANSPORT EQUATIONS |
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E. One combination is given in Eq. [7] and is the enthalpy flux. When Eq. [8] and [9] are added, the terms dependent on D add to zero, leaving just the enthalpy flux term. The driving force for this flux is shown by Monteith (1973) to be the equivalent temperature:
![]() | [10] |
It is derived by adding Eq. [1] and [2] and combining the derivatives. When Kv = KH, as is the case for eddy transport within and above the canopy,
* =
and
* =
.
A second combination is
E - (hs/
*)C. When Eq. [8] and [9] are combined in this way, the enthalpy terms add to zero, and only the isothermal latent heat flux,
Ei, remains. The driving force for this flux is the vapor deficit gradient, dD, as shown in Eq. [5]. Chen (1984) chose a different combination of H and
E. He defined a saturation heat flux density as J = C - (
/s)
E. This choice does decouple the equations but does not eliminate H from the second set of equations, resulting in a more complicated analysis and a flux that is less intuitive than the isothermal latent heat flux density. There are, of course, many linear combinations of C and
E that result in sets of decoupled equations for canopy transport. The set chosen here is thought preferable to Chen's because of its simplicity. As previously mentioned, it has some physical meaning in that it is the evaporation rate in systems with negligible temperature gradients.
| APPLICATION TO TRANSPORT IN PLANT AND RESIDUE CANOPIES |
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z/
Kv and rH =
z/
KH. Since KH and Kv are assumed equal for turbulent transport within the canopy (Campbell and Norman, 1998), the resistances for heat and vapor transport between canopy layers are equal. Resistances shown as r' in Fig. 1 are the boundary-layer resistances for canopy elements. The resistances between canopy elements and the air for vapor can be quite different from those for heat. When water evaporates from substomatal cavities, then r'v is the sum of a stomatal resistance and a boundary-layer resistance for the leaf. When the leaf surface is wet, the resistance is just the vapor boundary-layer resistance of the canopy element, which is about 10% smaller than the corresponding value for r'H (Campbell and Norman, 1998).
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Figure 2
shows the decoupled electrical analogs for the flux of enthalpy and isothermal latent heat. Boundary conditions are
a and Da for the air above the canopy and
o and Do at the soil surface. Values for
a, Da,
o, and Do are computed from known temperatures and relative humidities of the atmosphere and the soil surface. If boundary conditions and resistances are known, then all other values of
and D can be computed. Once these are known, T and e can be found from the definitions of equivalent temperature and vapor deficit.
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| CALCULATION OF THE THEVENIN EQUIVALENT POTENTIALS AND RESISTANCES |
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![]() | [11] |
![]() | [12] |
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The method for calculating the Thevenin equivalent potentials and resistances is straightforward. The circuit is broken at points AA' (Fig. 2 and 3). The Thevenin resistance is the resistance of the circuit with batteries shorted and current sources open-circuited. The Thevenin potential is the open circuit potential, or the potential measured at AA' when nothing is connected. For the enthalpy circuit
![]() | [13] |
![]() | [14] |
a is the equivalent temperature of the air above the canopy.
The potential and resistance for the vapor and isothermal latent heat flux calculation are obtained similarly. The Thevenin potential is
![]() | [15] |
is the product operator and Ri is calculated from the recursive relationship
![]() | [16] |
![]() | [17] |
| THEVENIN EQUIVALENT CIRCUITS AS BOUNDARY CONDITIONS FOR THE SOIL PROBLEM |
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![]() | [18] |
![]() | [19] |
These are obtained by substituting Eq. [11] and [12] into [8] and [9] and taking derivatives.
| IMPLEMENTATION |
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and D and then for T and e. Iteration may be required at several points, especially for long time steps. For example, as soil water is depleted, stomatal resistance increases due to decreasing leaf water potential. There is therefore a link between steps 1 and 3. Also, the temperature profile influences atmospheric stability, which influences transport resistance. Steps 4 and 1 are therefore linked.
| GAPS AND UNRESOLVED ISSUES |
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Once the canopy saturates, the rate of evaporation or condensation of layer j can be computed from Eq. [8], modified to account for evaporation from a saturated surface:
![]() | [20] |
If the value is negative, condensation is occurring. The value for H is known for each layer (Rn j - Gj), but a value for Di is needed to make the calculation.
A serious shortcoming of the present model is an implicit use of K-theory to describe turbulent transport within the canopy. New solutions to the Lagrangian description of scalar transport in canopies have recently become available (Raupach, 1989; Warland and Thurtell, 2000). These typically are used for heat, water vapor, or CO2, but presumably would also work for enthalpy and vapor deficit. This is a clear opportunity for further development.
| APPENDIX: |
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D, kPa water vapor pressure deficit, es (1 - h) or es - e
E, mol m-2 s-1 flux density of water vapor
Ei, mol m-2 s-1isothermal flux density of water vapor
G, W m-2 soil heat flux density or rate of heat storage
H, W m-2 enthalpy flux density
KH, m2 s-1 molecular or eddy diffusivity for heat
Kv, m2 s-1 molecular or eddy diffusivity for vapor
Rn, W m-2 net radiation
T, °C temperature
cp, J mol-1 K-1 specific heat of air
e, kPa water vapor pressure
es, kPa saturation vapor pressure at air temperature
h, relative humidity
p, Pa atmospheric pressure
rH, m2 s mol-1 resistance to heat transport between canopy layers
rv, m2 s mol-1 resistance to vapor transport between canopy layers
r'H, m2 s mol-1 leaf or residue boundary layer resistance for heat transport
r'v, m2 s mol-1 leaf or residue boundary layer and surface resistance for vapor transport
rHT, m2 s mol-1 Thevenin equivalent resistance for heat transport
rvT, m2 s mol-1 Thevenin equivalent resistance for vapor transport
s, °C-1 slope of the saturation mole fraction function,
/p
z, m distance
, kPa °C-1 des/dT, slope of the saturation vapor pressure function
, product operator (successive terms multiplied together)
, °C-1 psychrometer constant, cp/
*, °C-1 apparent psychrometer constant,
KH/Kv
, J mol-1 latent heat of vaporization for water
, mol m-3 molar density of air
*, °C equivalent temperature
a, °C equivalent temperature of air above canopy
o, °C equivalent temperature of soil surface
T, °C Thevenin equivalent temperature
| REFERENCES |
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This article has been cited by other articles:
![]() |
V. S. Manoranjan, A. R. Kemanian, R. L. Orozco, and G. S. Campbell Comment on "Modeling Sensible and Latent Heat Transport in Crop and Residue Canopies" by G.S. Campbell. Agron. J. 95:1388-1392 (2003). Agron. J., October 31, 2006; 98(6): 1664 - 1664. [Full Text] [PDF] |
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