
JORGE A. RAMIREZ
Associate Professor
Water Resources, Hydrologic and Environmental Sciences
Civil Engineering Department
Fort Collins, CO 80523-1372
Evapotranspiration
Energy Budget Methods.
Energy budget methods are based on the direct application of the energy
budget equation, or some approximation thereof. The energy budget equation for a control volume including a
transpiring canopy and a thin layer of surface soil can be written as,
(2)
or
(3)
where LvE
is the latent heat flux or energy flux used in evaporation; H is the sensible heat flux (i.e.,
diffusive heat exchange between the land surface and the atmosphere); and Qn
is the available energy flux density. Qn
includes contributions from radiative, advective, and diffusive processes, and
energy storage changes. Over land
surfaces, the available energy flux density can be expressed as,
(4)
where Rn is the net radiation flux density at the
surface; Ah is energy
added to the system by advection; dW/dt
is the change in energy storage of the system; G is the net diffusive ground heat flux out of the soil layer; and LpFp is energy use
in photosynthesis. The contributions to
the net radiation flux density at the surface are the incident short wave
radiation, Rs; the short wave radiation reflected back
into the atmosphere, asRs; the net long wave radiation from the
atmosphere absorbed by the surface, Rld; and the long wave radiation emitted by
the surface, Rlu. Thus,
(5)
The energy advected Ah is made up of contributions by precipitation, net
streamflow, seepage, and evaporation fluxes.
The available energy flux density at the surface is partitioned into
energy for evaporation and energy for sensible heating as expressed in equation
3.
In aplications of the energy budget
method, Qn is often
approximated as Rn – G, or
as Rn only. However, care
must be taken to ensure that such approximations are valid.
Standard
Energy Budget Method.
Among the many applications of the energy budget methods, one of the most
widely used is the Bowen Ratio Method.
The Bowen Ratio, Bo,
defined as the ratio of sensible heat to latent heat,
(6)
can be determined from data on specific
humidity and temperature in the dynamic sublayer of the atmospheric boundary
layer as,
(7)
where Cp is the specific heat of air at constant
pressure; p is the surface pressure; Lv
is the latent heat of evaporation; e is the ratio of the gas constant for dry air, Rd to that of water vapor, Rv, and numerically e = 0.622; e2 and e1 are the actual vapor pressures at elevations z2 and z1 within the dynamic sublayer; T2 and T1
are the corresponding temperatures. The constant g is
(8)
and it is known as the psychrometric constant. Equation 7 above was obtained after invoking similarity arguments for the distributions (i.e., profiles) of specific humidity, velocity, and temperature within the dynamic sublayer of the atmospheric boundary layer.
If the Bowen ratio is known, then the energy budget equation leads to the following equation for the evaporation rate,
(9a)
In order to account for the energy
advected out of the system by the water as it evaporates into the atmosphere,
Equations 3, 4, and 6 lead to a modified EBBR expresion as follows,
(9b)
where Cpw is the specific heat of water, and Te
is the temperature of the evaporated water.
Potential
Evaporation. Evaporation
is a mass transport process that results from gradients in the distribution of
water vapor mass concentration (i.e.,
a gradient of specific humidity). Potential evaporation refers to the rate of
evaporation from any large uniform surface which is sufficiently moist or wet,
so that air immediately in contact with it is fully saturated, thus leading to
the largest possible local gradient of specific humidity, and consequently the
maximum rate of evaporation for the given conditions. Some of the simplified
methods introduced below are sometimes used as measures of potential
evaporation.
Simplified
Methods for Wet Surfaces.
When the surface is wet, it can be assumed that the surface specific humidity
is the saturation specific humidity at the surface temperature. This allows an
approximation, first proposed by Penman, that eliminates the need for
measurements at two levels (i.e.,
levels at z1 and z2), as required by the
standard energy budget method, or the so called profile methods (i.e., those based on similarity profiles
in the boundary layer presented later in this section.) Penman equation is,
(10)
where g=pCp/(0.622Lv) is the psychrometric constant at surface
pressure p, and where D=(des/dT) is the slope of the saturation water vapor pressure curve.
Penman equation assumes that D can be approximated as,
(11)
EA is sometimes referred to as the drying
power of the air. It is of the general form,
(12)
where
f() is the so-called wind function and es2 and e2 refer to saturation water vapor
pressure, and actual water vapor pressure of the air at elevation z2, respectively. A
particular form of the drying power of the air is the so-called aerodynamic
method or Thornthwaite-Holzmann equation,
(13)
where zo
is the roughness length of the surface, and k
is von Karman’s constant (k = 0.4).
Penman (1948) suggested the following
form for EA
(14)
where u2
is in m/s and the vapor pressures are
in mb yielding EA in units of mm/day.
Equilibrium Evaporation. When overpassing air has been in contact with a wet surface over a long fetch, it may tend to become vapor saturated (under conditions of no advection). Thus, the drying power of the air should tend to vanish. Therefore, in this limit, Penman equation yields a lower limit to the evaporation rate from moist surfaces, known as the equilibrium evaporation rate, and given by,
(15)
Partial Equilibrium Evaporation. However, equilibrium conditions are encountered only rarely, as air in the boundary layer is continually responding to large-scale weather patterns which tend to maintain a vapor deficit even over the oceans. Thus, there is always some degree of advection. Priestley and Taylor (1972) took the concept of equilibrium evaporation as the basis for an empirical equation giving evaporation from a wet surface under conditions of minimal advection, the so-called Priestley and Taylor equation for partial equilibrium evaporation,
(16)
Priestley and Taylor concluded that the
best estimate of ae is ae = 1.26.
Empirical
Equations. Jensen and
Haise (1963) proposed the following
empirical equation for the estimation of evapotranspiration for agricultural
purposes.
(17)
where a
and b are calibration constants, Ta is the air temperature in
degrees Celcius, and Rse
is the incident solar radiation expressed in equivalent units of evaporated
water. That is,
(18)
Observe that this equation has a form
similar to the equilibrium evaporation equation above. The linear function of
temperature of the equation proposed by Jensen and Haise can be justified by
the quasi-linear dependence on temperature of the factor D/(D
+ g) as shown in the figure below.

In
addition, the net short wave radiation is strongly correlated with the net
radiation Rn,
which is the most important component of the available energy, Qn,
over daily periods or longer. However,
the equation needs to be calibrated to the specific region. Based on more than
1000 measurements of consumptive use in the western U.S. representing means over
periods longer than 5 days, Jensen and Haise obtained the following values for
the constants, a = 0.025 oC-1 and b = 0.078, with a correlation coefficient r = 0.86.
Modified
Penman Equation for Vegetated Surfaces.
Vegetated surfaces, even when the vegetation is well supplied with water, can
not be considered wet, except after rainfall or dew formation. Thus, the
specific humidity at the surface of the foliage is likely to be smaller than
the saturation value at the corresponding temperature. Therefore, Penman
equation is no longer applicable. Introducing a resistance formulation for
evaporation such that,
(19)
where q1,
q2 are specific humidity
at elevation z1 and z2, and r1,2 is a resistance parameter characterizing the
transfer between points at elevation z1
and z2, a modified Penman
equation, the so called Penman-Monteith equation, can be derived. In order to
do so, two resistance parameters must be defined, one characterizing the
transfer between the vapor saturated stomatal cavities and the surface of the
leaf, and another characterizing the vapor transfer between the leaf surface
and the ambient air within the dynamic sublayer. The former resistance is known
as the stomatal resistance, rst,
and the latter as the aerodynaimc resistance, rav.
The aerodynamic resistance parameter has
the following form,
(20)
The modified Penman equation is,
(21)
Mass Transfer Methods.
Based on arguments about similarity profiles within the fully turbulent
dynamic sublayer of the ABL, the following expression was obtained for the
water vapor tranfer as a result of gradients of specific humidity in the
dynamic sublayer,
(22)
where u*
is the so-called friction velocity,
(23)
In the expression for friction velocity, to is the surface shear stress.
From similarity arguments in the ABL, the vertical profile of horizontal velocity in the dynamic sublayer is given by,
(24)
where k
is von Karman’s constant, k = 0.4.
Using analogous arguments of similarity
profiles in the dynamic sublayer, the vertical transfer of sensible heat is
given by,
(25)