Estimating transpiration and water flow in trees remains a major challenge for quantifying water exchange between the biosphere and the atmosphere. We develop a finite element tree crown hydrodynamics (FETCH) model that uses porous media equations for water flow in an explicit three-dimensional branching fractal tree-crown system. It also incorporates a first-order canopy-air turbulence closure model to generate the external forcing of the system. We use FETCH to conduct sensitivity analysis of transpirational dynamics to changes in canopy structure via two scaling parameters for branch thickness and conductance. We compare our results with the equivalent parameters of the commonly used resistor and resistor-capacitor representations of tree hydraulics. We show that the apparent temporal and vertical variability in these parameters strongly depends on structure. We suggest that following empirical calibration and validation, FETCH could be used as a platform for calibrating the “scaling laws” between tree structure and hydrodynamics and for surface parameterization in meteorological and hydrological models.
 However, unlike canopy radiation models, in which plant area density can be treated as a random medium (with clumping), plant hydrodynamics must resolve the plant architecture, allometry, and branching. Several factors frustrate modeling water movement within the tree system, as summarized below:
 The first factor is computational. Although it is possible to derive point equations for flow within one organ element, solving a transient nonlinear diffusion equation in high-resolution 3-D on an unstructured mesh needs a large computational resource.
 Although this study does not offer new empirical data, it makes use of published empirical parameters to derive a novel numerical model, the finite element tree crown hydrodynamics (FETCH) model. This model resolves plant hydrodynamics across a range of realistic tree structures. This model is coupled to tree microclimate through radiative transfer and simplified turbulent transport theories. Using this new framework, we explore the sensitivity of plant hydrodynamics to canopy structure via parametric variations of simple scaling laws. The goal of this study is to highlight the advantages of this new modeling approach relative to the commonly used models of plant contribution to land-surface energy balance. These advantages include better temporal description of water fluxes from a tree crown and detailed vertical distribution. We suggest that by adopting this hydrodynamic description of the plant system, it is possible to better predict nonlinear, hard-to-parameterize phenomena such as midday stomata closure and differential stomatal response along a branch and incorporate the effects of tree structure and physiology in the prediction of changes in transpiration fluxes following environmental changes such as fertilization.
 The common models of tree-water systems incorporated within meteorological land-surface models are based on equivalence to an electric circuit (Figure 1). The most simple of these water flow models are the single (1R) or multiple (2R) resistor models [Jones, 1992]. These lump all vegetation below the grid resolution to a single effective “big leaf,” or to a low number of subgrid patches. Some examples for “big leaf” resistor models include SiB2 [Sellers et al., 1996a, 1996b] and LEAF2 [Walko et al., 2000]. The resistor models take no account of water storage in the plant and therefore assume constant equilibrium between transpiration and the energy gradients between the soil and the atmosphere (see Figure 1). The resistance-capacitance (RC) models are another type of electric circuit equivalence model developed to account for water storage (or “charge capacitance”), which is presumably important in tall forested ecosystems [Jones, 1992; Schulte and Costa, 1996; Phillips et al., 1997]. The resistance and capacitance are empirical properties often calibrated to match observations. It is possible to represent a crown structure using a RC model, but that would require branch level or crown/canopy-layer level empirical calibration [Jones, 1992].
 A more physically based approach is to combine the continuity equation with a physical transport law applied to an elemental organ, which leads to a nonlinear partial differential equation (PDE) resembling Richards' equation for soil water movement including sources and sinks. In essence, this approach assumes that water movement through a collection of interconnected tracheids in the hydroactive xylem (typical to conifers) resembles porous media flow [Siau, 1983; Früh and Kurth, 1999; Kumagai, 2001; Chuang et al., 2005]. This view is perhaps indirectly supported by the wealth of hydraulic cavitation curves collected for various plant organs that are analogous to hydraulic losses in porous media (e.g., Sperry  and review by Feild et al. ). As discussed by Chuang et al. , the mathematical properties (and boundary conditions) of the resulting porous-media PDEs may significantly diverge from RC models whose mathematical properties are first-order ordinary differential equations for the water flux.
 Treating sap flow in wood as porous media flow to apply Darcy's law was first suggested by Siau . Arbogast et al.  developed a Richards-type equation as a way to numerically solve water movement in lateral roots as part of a soil water system. A branch system was suggested by Früh and Kurth , who generated a splitting-branch tree-grid system and solved it using finite differences. A similar but somewhat simplified approach was also developed by Kumagai  and later adopted by Chuang et al. , who revised it to include nonlinear terms for the conductance and capacitance. All of the above require specified transpiration from each branch as a model input. The stem systems in the latter two studies were limited to a single stem without branching (see Figure 1).
 An even more complete model of the tree transport system was suggested by Aumann and Ford [2002a, 2002b]. They observed that a tracheid-level model could lead to a better representation of the flow in nonsaturated stages, for example, when recovering from cavitations. The need, though, for many cell-level parameters and explicit cell-structure element construction makes it less attractive as a general simulation tool. Furthermore, none of the above models considers interaction between the tree and its microclimate.
 Here we adopt the formulation of Chuang et al.  and adjust it to handle a nonvertical branching system, similar to that proposed by Früh and Kurth . We also added a multiple-layer canopy microclimate model using leaf-level physiological, radiative transfer, and canopy drag properties as discussed by Lai et al. [2000a] with a first-order turbulent closure scheme [Poggi et al., 2004], and add a stomatal response that links pressure in the branches to stomatal resistance. The resulting FETCH model simulates the hydrodynamics of a branching pipe system, constructed in a manner to be consistent with the plant area density. The model also utilizes the “aorta” or “fully coupled” tree transport system formulation [McCulloh et al., 2003; Schulte and Brooks, 2003]. This approach assumes free flow along the radial axis of the branches.
 By using such a physically based plant-atmosphere-hydraulics model with explicit three-dimensional (3-D) representation of the tree structure, we can confront the question of how the variability in crown architecture (i.e., interspecific, age, or ecosystem dependent structure) would lead to different transpiration responses. We compare the results from such a detailed model with the equivalent resistance and capacitance parameters that would have been obtained by 2R and RC models (see Figure 1). This comparison is used to test the sensitivity of the tree system to structure and its consequent effects on 2R or RC parameterizations that do not and in most cases cannot include structural aspects of the tree.
2. Materials and Methods
2.1. Governing Equations
 Upon horizontal averaging a cross-sectional plane that includes a collection of tracheids, we can adopt a porous media analogy using a 1-D Richards equation for the water pressure along the hydraulic path length l:
In a vertical branch segment (l = z), the total water potential (Ψ) is related to the water pressure (Φ) by the equation Ψ = Φ + ρgl. The capacity C(Φ) and xylem conductivity k(Φ) are nonlinear functions of Φ. Snk represents all water sinks and sources including water loss by transpiration. A key assumption in equation (1) is that water transport is driven primarily by pressure and gravitational potential differences and not dominated by other forcing such as solute potential differences. Units and descriptions for the symbols used in this and all other equations below appear in Table 1.
 The system we use to represent a tree is an assortment of 1-D branches, but the nonvertical branches add volume to the system and thus turn it to a 3-D rather than a 1-D system. For further computational efficiency, we obtain a strict 1-D representation of this 3-D structure by using a conversion term, cos(α), for the hydrostatic pressure to correct for the angle between the branch element and zenith (α) in nonvertical branches (where the path length l is longer than its vertical component z). This yields the following PDE system:
 This representation allows expressing the coordinates system only in the vertical direction (z, positive above the ground). We neglect all other sources or sinks of water other than transpiration (EV). We assume Dirichlet boundary conditions at the bottom of the trunk (i.e., the “stem-root interface”). When soil is saturated, pressure at the top of the root system can be assumed constant and near saturation. Thus we treat the pressure at this boundary as surrogate for soil water pressure (Ψs). In the current simulations, Ψs was kept constant and near saturation. Theoretically, in drying soil it would be possible to fit a decreasing pressure curve to this boundary that would simulate the roots' diminishing ability to extract water from the soil. At the top boundaries (i.e., at the end of branches), we set Neumann no-flux conditions, meaning water only exits the leaf-supporting branch elements via the transpiration sink term. Initial conditions are hydrostatic pressure equilibrium throughout the tree system.
 The equations for the hydraulic properties of the xylem system (the capacity and conductivity) can be derived and calibrated from empirical observations of wood properties [Sperry et al., 1988; Alder et al., 1997]. Trees' conductive systems, whether conifers or broadleaf, may be approximated by an anisotropic porous medium if capacitance and conductance are a priori calibrated. It is not our intent to diagnose those equations; instead, we use empirically fitted Weibull-shaped equations (equations (3) and (4)) to describe these hydraulic properties. These Weibull-shaped equations for xylem vulnerability were observed for many species including conifers and broadleaf [e.g., Tyree and Sperry, 1989; Sperry et al., 1994; Alder et al., 1997]. Following Chuang et al. , we define the capacitance and conductance as
Az and Aaz are the physical and effective hydraulic cross-sectional areas of the branch (see equation (9) for definition), and c1, c2, kmax, θsat, Φ0, and p are empirical coefficients for the hydraulic system (see Table 1 for definitions and values). The FETCH model, as any other land-surface model, requires parameterization in order to correctly describe different species and biomes. Our model parameters c1, c2, kmax, θsat, Φ0, and p can be determined by fitting the model's hydraulic parameters (in equations (3) and (4)) using sap-flux and atmospheric flux measurements.
 Unlike previous work in porous media flow in plants that solved the system using the finite difference approach [Früh and Kurth, 1999; Kumagai, 2001; Aumann and Ford, 2002a; Chuang et al., 2005], the FETCH model uses the finite element method (FE). FE has a particular advantage with the “aorta” branching pipe system because of the simplicity with which it handles the branching of the tree system in the element assembly process without the need to explicitly represent the structure of the junction in the element level formulation. The FE approach results in linearized 1-D element level equation system with a sparse diagonally banded tangent matrix that can be readily solved as described in Appendix A.
2.2. Maximum and Actual Transpiration
 For the vertical variation of maximal potential transpiration (EV,max) we use a multiple-layer coupled radiative-transfer, plant physiological, and turbulent transport model. This is used to calculate the relevant maximal potential transpiration that determined the water sink forcing of the tree system assuming maximal stomatal conductance is regulated by photosynthesis and thus controlled only by CO2 concentration (Ca), photosynthetically active radiation (PAR) and vapor pressure deficit (VPD) at a given level in the canopy. Our approach assumes that the plant would maximize its carbon gain as long as plant hydraulics pose no limitation [Katul et al., 2003].
(See Table 1 for definitions, sources, and values of the coefficients used in this equation set.) The maximum “leaf level” transpiration (El,max) represents the transpiration water sink regardless of hydrological limitations, and is given by
where kb is the boundary layer conductance (which varies with mean wind speed at a given level within the canopy), and β′ is a constant for unit conversions (Table 1). Branch-level maximal transpiration (EV,max) depends on El,max, total leaf area, and the leaf area density distribution (LAD).
 To compute PAR at each level within the canopy, an exponential extinction for a spherical leaf angle distribution with considerations for leaf clumping is employed [Campbell and Norman, 1998]. For this study, only beam radiation was considered, though it is possible to revise this formulation and include penumbral effects [Stenberg, 1995]. The model is forced by canopy-top values of PAR, air temperature, mean wind speed, and mean above canopy VPD. These values are updated every 15 min. To compute kb, the wind speed at each level must be known. We used the mixing length and the turbulent closure model of Poggi et al.  to compute the mean wind speed at each level within the canopy using the mean wind speed above the canopy. The calculations assume initially ambient scalar profiles of air temperature and relative humidity. It also assumes CO2 concentration is equal to the canopy top value. As CO2 uptake and water emissions occur, these profiles are then adjusted iteratively as described by Lai et al. [2000a, 2000b]. A sample vertical profile of El,max is shown in Figure 1 for noontime conditions. Note that while there is no foliage at the base of the tree, a finite El,max exists; however, this finite El,max does not contribute to the potential canopy transpiration when scaled with LAD.
 The actual transpiration water sink (EV) depends on the stomatal response to “upstream xylem pressure” even when soil is saturated [Oren et al., 1999b; Brodribb and Holbrook, 2004]. This is represented in our model by the branch pressure at the transpiring element. Highly negative water pressure can lead to cavitation and loss of conductivity. Stomata have therefore evolved to reduce the water flux by increasing the leaf resistance to water loss (i.e., by closing the guard cells) when pressure is low [Sperry et al., 1998; Oren et al., 1999a; Hubbard et al., 2001; Cruiziat et al., 2002]. The stomatal response is typically not instantaneous [Sperry et al., 2003]. Therefore, using the pressure at the previous time step (i.e., a 1-s lag) is justifiable. We expressed the evaporation water sink term as
2.3. Constructing the Model Trees: Scaling Structure
Equations (1)–(7) have dealt with water flow and sinks at either the element or the crown level. Integrating these equations to the tree scale requires detailed representation of the tree architecture, which considers its branching geometry and architecture structural allometry. One of the popular models for branching-tree systems is based on the so-called L-system [Lindenmayer, 1968, 1971]. L-system has been successfully used to model a variety of plants at different stages of their growth, providing a convenient theoretical and programming framework for the architectural modeling of plants [Prusinkiewicz and Lindenmayer, 1990; Prusinkiewicz et al., 1997].
 Here we adopt the “turtle interpretation” [Szilard and Quinton, 1979] to construct the L-system. According to the “turtle interpretation,” a single set of instructions specifies a core series of “steps and turns,” each step adding a single element. This core series is repeated recursively to construct the full “tree.” The complexity level (set in this case to 2) controls the number of recursive iterations. The size and direction of each additional element (relative to the previous element) are controlled by two “structural” rules. The first rule controls the number and direction of additional branch elements at each branch junction (set in this study to 4 branches at 65° to the main axis). The second rule controls the branch cross-sectional area (see equation (8) for the formulation of this rule). An example application of these rules, representing the simplified “spruce” we used in our simulations, is shown in Figure 1.
 The cross-sectional area of branches emanating from any axis was represented by a linear function, decreasing with height:
where Azi, Abi are the physical cross-sectional area of a main and a side branch, respectively, at height level i, NB is the number of side branches at each split, and c4 is an empirical “branch thinning” coefficient (Table 1). EB is referred to here as the “extra-branch” coefficient. EB represents the allometry of cross-sectional area distribution between the main stem and branches. It is expressed as the proportional coefficient between the cross-sectional areas, which are added to the tree by adding side branches, relative to the area lost by the narrowing of the main stem since the previous junction. It is a measure for the structural (carbon) cost of added conductive area.
EB values can represent a wide range of hydraulic structures from the EB = 1 case, which is in essence, the “da Vinci scaling law” [Leonardo da Vinci, 1970], to more efficient structures specified by “Murray's law” [Murray, 1926]. This law states that the optimal system should preserve the total volume, Atot ∝ Σr3, were r is the pipe radius, in the conductive pipes, and can be applied with some adjustments to vascular systems of plants, especially when accepting an aorta-like pipe system model [McCulloh et al., 2003]. Murray's law predicts that the total cross-sectional area of the plant hydraulic system would increase along the aboveground flow pathway in a tree as the radius of individual branches decrease. Values ranging significantly between Σr2 and Σr4.5 (note that Σr2 is equivalent to the da Vinci scaling law) in several tree species were observed by McCulloh et al. . An observed mean value for EB in Picea abies (L.) Karst (Norway spruce) is 1.75 [Oren et al., 1986].
 A plant stem or branch is not an empty pipe, and the cross-sectional area includes tissues that do not participate in axial water transport (e.g., bark, heartwood) and poorly conductive structural tissue (e.g., compression and tension wood). This implies that adding more cross-sectional area to existing branches can be more hydraulically efficient than adding a new thin branch. This leads to a functional relationship between the effective cross-sectional area of the branch and its conductivity. In an “empty-pipe,” the conductivity (k) is proportional to the cross-sectional area and scales with the diameter (d) to the second power, i.e., k ∝ dED where ED = 2. For a tree system not following an empty pipe model, ED, defined as the exponent order of conductivity, may exceed 2. ED smaller than 2 is also possible where heartwood exists in the thicker stem areas. Thus it is convenient to define an “effective hydraulic cross-sectional area” at level i (Aazi) as
Note that if ED = 2, then Aaz = Az. ED would be high in fast growing species because they grow by adding large, and thus hydraulically efficient, xylem elements and tracheids. ED would be low in drought-resistant plants that maximize cavitation resilience over hydraulic efficiency, and thus add narrow thick walled xylem elements and tracheids [Tyree, 2003]. Observations in several species found that ED values range between 2.41 and 2.79 [Cruiziat et al., 2002]. An observed ED for Norway spruce is 2.44 [Cruiziat et al., 2002].
 In summary, the combination of ED (a measure of the hydraulic efficiency gained by adding cross-sectional area) and EB (an architectural scaling law for the branch thickness) serves as a logical surrogate to evaluate the effects of crown architecture on its hydrodynamics in a virtual range of possible tree physiologies, representing different growth stages, environmental adaptations, and species.
2.4. Experimental Settings
 In this investigation we use a tree with four side branches, symmetrically splitting from the main branch or stem at each branch junction (Figure 1). End branches include the last members of each branch and all branch elements that are the sixth or farther from the bottom of the main stem (Figure 1). Only end branches carry leaves and lose water by transpiration. To roughly match a Norway spruce tree, we set the tree to be 12 m high (above the forest floor) with a branching angle of 65° and with 114 elements (branches and stem) of 1.2 m each. The base of the stem diameter is 0.25 m, tapering linearly up to 0.5 cm at the top. Leaf area index (LAI) is 6, and the total ground projection area for the crown (Acan) is 5.56 m2, based on a Norway spruce stand [Ewers et al., 2001], scaled to twice the height. We set the conductance coefficients c1 and c2 so that 50% xylem conductivity is lost when pressure reaches −4.2 MPa [Mayr et al., 2003], and we set the stomatal curve fitting coefficients (Φσ and c3) accordingly. We follow the rule that stomatal conductance would reduce 90% in response to 10% loss of xylem conductivity [Cruiziat et al., 2002]. Hence stomata of our model trees commence closure at branch pressure of −1.5 MPa and follow a Weibull reduction curve with reduced pressure until full closure at −2.5 MPa, as often reported for spruce [Cruiziat et al., 2002]. Calibration of the hydraulic coefficients (kmax, θsat, Φ0, and p) was based on the work of Chuang et al.  that empirically calibrated the dimensionless ratio (kmax Φ0 θsat−1p−1) based on sap-flux measurements at the same Norway spruce stand [Ewers et al., 2001; Phillips et al., 2004]. We kept this dimensionless ratio constant, and fixed θsat to its physically based value, and calibrated the other three coefficients. This calibration was done assuming that trees are naturally selected for “optimal transpiration,” and thus we fitted the coefficients to allow the natural tree to arbitrarily transpire about 90% of the maximal transpiration (3.66 mm/d [Phillips et al., 2001, 2004]) and to fully recharge before 0500 LT (see Table 1 for coefficient values and units).
2.5. Comparing to Resistor and Resistor Capacitor Models
 To address the study objectives, we seek a connection between variations in ED and EB and the resulting time-dependent resistors and capacitors of the electric circuit analogy (Figure 1). The 2R model system can be represented by the following set of equations:
where Esf is sap flux, Φl, Φs, and Φa are the liquid water pressure at the leaf petiole (i.e., at the ends of branches), the base of the stem (represents “soil” pressure), and in the air, respectively. Rs, Rl are “per tree” stem (i.e., all woody parts) and leaf resistance, Rl,min is the minimal “per tree” leaf resistance when stomata are fully open. Note that sap flux is equal to transpiration because the 2R model assumes no storage. By substituting the system in equation (10) into (7), we can obtain a solution for the equivalent leaf pressure:
The equivalent values of the two resistors are calculated as
 Another version of electric equivalence model is the resistor-capacitor analogy (RC) (see Figure 1), defined with a time constant (τ = RpC) that determines the time it takes to empty 63% of the capacitor [Jones, 1992]. Here Rp is the total aboveground resistance of the tree. To compute the equivalent capacitance from our model, we first determine the storage of the whole tree (Stot):
where Nel is the total number of branch elements, zibase and zitop are the height at the base and top of each element, and θzi is the local water content. Tree level capacitance (Ctot) and sap flux Esf through the base of the stem at each time step can be calculated through the water mass balance:
where Φtot is a tree level pressure calculated by volume averaging Φ. LAI and Acan are used to convert the capacitance to consistent units with the “per-tree” resistance terms [Jones, 1992].
 Hence the effects of canopy architecture and allometry (i.e., EB and ED) on the electric-circuit-analogy models (Figure 1) can be directly assessed. As a first step, we focus on fully hydrated soil conditions (i.e., water pressure at base of stem held constant in time and close to saturation) to explore the effects of aboveground plant hydraulics on transpiration and storage.
3. Results and Discussion
 To address the study objectives, we simulated a total of 88 trees, with all combinations of ED and EB for a wide range of values between 1.0 and 3.0 (see Table 1). For reference, we define a “natural tree” with the scaling-parameter values EB = 1.75 and ED = 2.44, which were observed for Norway spruce. We will first show the temporal response of the “natural tree” to the canopy top meteorological forcing and relate the diurnal dynamics of the departure between actual transpiration and EV,max to the pressure distribution and storage within various areas of the crown. Finally, we discuss the effects of crown architecture, through EB and ED, on the equivalent parameters of the 2R and RC circuit models (Figure 1).
3.1. Daily Dynamics of Evaporation and Sap Flux
 We simulated a period of 40 hours from 0500 LT of 1 August to 2100 LT the next day. The environmental conditions we use were smoothed long-term averages for that day over the Duke forest. The “natural tree” case was calibrated so that total daily transpiration would reach about 90% of the maximum transpiration that was reported by Chuang et al.  and that storage would be restored to 99% of the initial conditions at 0400 LT of the second day (Figure 2). Our “natural tree” system displayed a daily transpiration and sap-flux cycle with a maximal transpiration peak at about 1130 LT and a sap flux peak lagging approximately 2.5 hours (Figure 2).
 Actual measurements of sap flux differ widely between trees in the daily total amount of water transported. There are large differences between species, between sites, and between days within same trees, depending on the trees structure, soil moisture, and environmental conditions [e.g., Oren et al., 1996; Phillips et al., 1996; Oren et al., 1998; Oren et al., 1999a; Phillips et al., 1999; Pataki et al., 2000]. Typical transpiration and sap flux time series are much noisier than the smooth curves our model predicted. This is probably because our light function did not include shading effects by clouds, other trees, and branches and because our tree's structure was simple and symmetric.
 Although we do not have the structural, environmental, and water flux data needed to fully calibrate and validate the model's performance in comparison to a real tree in a particular day, qualitative comparisons can still be discussed. For example, early onset of the transpiration peak in Norway spruce in saturated soil was observed by Zweifel et al. . The length and strength of the lag between transpiration and sap flux are in agreement with values measured in Norway spruce trees by Herzog et al. , and within the range of sap-flux-derived observations in other species, although in many examples it tends to be shorter than the one our model simulated [e.g., Goldstein et al., 1998; Schäfer et al., 2002; Meinzer et al., 2003].
 Trees lost water from storage during the day and recovered to full storage at night (for the “natural tree,” see Figure 2). Figure 3 describes the time series of water pressure in different branches. The middle column shows results for structural parameters close to the “natural tree” settings. When pressure drops below −1.5 MPa, stomata start closing. The model predicted earlier onset of midday closure of stomata on higher branches. These dynamics of midday stomatal closure are well documented, even in saturated soils (e.g., in spruce [Herzog et al., 1998; Oren et al., 2001; Zweifel et al., 2002; Brodribb and Holbrook, 2004]), though they are not necessarily observed in all occasions. Our model also predicted the afternoon reopening of some of the stomata in the intermediate and high branches (Figure 3), consistent with Zweifel et al.  who observed stomata reopening in upper branches.
3.2. Effect of Tree Structure
 For an analysis of the effects of EB and ED, we use only 13 hours of each simulation (i.e., 0600–1900 LT of 2 August). This is done to avoid artificial effects from the initial conditions. We focus primarily on the water pressure dynamics at various levels within the canopy because of their controls on leaf stomata.
 It is clear from Figures 3 and 4 that EB and ED affect the plant hydrodynamics in a nonlinear manner despite the hydrated soil conditions, the identical meteorological conditions above the canopy, and the identical leaf area and leaf-level physiological properties across the simulations. In all trees, pressure in the higher branches dropped faster than in the lower branches or those closer to the tree's core (Figure 3). There are large differences, though, between trees with different structure (i.e., different values of ED and EB). In trees with thinner branches (lower EB) the branch pressure drops faster and reaches the limiting pressure of −1.5 MPa earlier in the day, compared with branches at the same height in trees with thicker branches (Figure 3). These strongly negative pressures are the reason for the midday stomatal closure despite saturated soils. Trees with high conductive efficiency (i.e., high ED) are able to maintain higher levels of equilibrium water flow and therefore maintain less negative noontime branch pressures relative to branches of the same height in trees with lower ED. They also recover faster in the afternoon from the noontime pressure lows and are more likely to reopen stomata in higher branches (Figure 3).
 The structurally imposed differences in branch pressure and storage lead to different stomatal dynamics and thus change the daily transpiration and sap-flux dynamics (Figure 4). Trees with high EB draw more water from storage and their transpiration rate does not drop below the potential maximal transpiration for a long period throughout the day when compared with trees with low EB (see, in particular, Figure 4, middle column, where ED = 2.8). This effect was observed in a range of tropical tree species [Goldstein et al., 1998]. Thus the simulation results demonstrate that total daily amounts of transpiration and change of storage are highly affected by tree structure: Although sap flux at the stem base is hardly affected by differences in EB, the transpiration peak can increase with EB due to water supplied from storage. Conversely, ED controls the maximal rate of sapflux: Low ED leads to lower sap flux and longer lag time between maximal transpiration and maximal sap flux (Figure 4).
3.3. Equivalence to Electric Circuit Models
 On the basis of the simulations, crown architecture (simulated in this case through ED and EB) can inject different spatial and temporal responses in the equivalent parameters of 2R and RC circuit models. These models are currently the common parameterization approaches for determining the daily hydrodynamics of canopies. The notion of independent and constant values for capacitance and resistance (within a given set of external conditions such as soil moisture, VPD, temperature, and light intensity) is inherent in the electric equivalence models but cannot represent the tree hydraulic system. For example, the “capacitor discharge” of a branch not only reduces the available water storage but also increases the resistance of the drier branch and inhibits further discharge or recharge of the branch.
 In the 2R model, the main control on diurnal transpiration is the leaf resistance, while stem resistance, which accounts for the resistance of all woody parts of the tree, is either ignored, assumed to be constant, or assumed proportional to leaf resistance. Furthermore, leaf resistance is assumed to vary only as a function of external variables (e.g., VPD, soil moisture, temperature). With such parameterization, this approach cannot predict diurnal time lags between changes in water demand and dynamic pressure in the stem [Phillips et al., 2004]. The numerical results reported here suggest that none of these three representations are reasonable. Stem resistance was smaller than leaf resistance but still important (Rs/Rl = 2–40%, Figure 5). Both stem and leaf resistances were highly affected by ED. With low ED, the leaf resistance increased rapidly throughout the day with a late afternoon peak (gray curves, Figure 5, top right panel). With high ED, leaf resistance was lower and less variable (black curves, Figure 5, top right). Stem resistance was relatively constant throughout the day with high ED (black curves, Figure 5, top left). With low ED, though, stem resistance was higher and had a rapid increase in the afternoon (gray curves, Figure 5, top left). The response of increased resistance at the afternoon for both leaf and stem was more pronounced for a tree with lower EB (solid curves, Figure 5, top panels). The relative size of stem resistance was larger with low ED (gray curves, Figure 5, lower left).
 In reality, leaf resistance is nonlinearly dependent on stem resistance. Plant stomata have evolved to regulate the stem pressure in order to prevent cavitation and respond to low stem pressure by closing the guard cells and increasing their resistance [Sperry et al., 1998; Hubbard et al., 2001; Oren et al., 2001; Cruiziat et al., 2002; Sperry et al., 2003]. This dependence might lead to different dynamic responses of leaf resistance in trees of different structures and in different environmental and climatic conditions that would be hard to calibrate empirically when using the common electric equivalence resistor models (other than a “per case” calibration).
 RC models are more flexible in their ability to represent different dynamic cycles and responses to environmental forcing. Owing to the addition of an empirical time constant, they can represent the time lag between transpiration and sap-flux response. Typically, the resistor and capacitor coefficients are assumed constant in a given set of environmental conditions. By the definition of the capacitance in a porous media system, it is clear that C is a nonlinear function of the pressure, but the “working assumption” is that the diurnal variability in C is small and it can be averaged to a single capacitor constant [Jones, 1992; Phillips et al., 1997]. Our simulations show that this is a good approximation when the branches are very thin (EB = 1, solid curves, Figure 5, bottom right) but not when branches are thick (EB = 3, dotted curves, Figure 5, bottom right). Branch structure (through EB) affects the capacitance more than the conductive efficiency (ED). Trees with high EB have up to a manyfold higher capacitance and tend to increase the capacitance more rapidly throughout the day (Figure 5, bottom right) when compared with their low EB counterpart. High ED tends to increase the capacitance but only in the thicker branches (Figure 5, bottom right). The range of C values estimated here is similar to the reported range for Norway spruce (∼0.2 × 10−7 [Phillips et al., 2004]).
 Another advantage of RC models over 2R models is that they can be extended to represent a vertical canopy structure by including many independently calibrated capacitors. However, obtaining a realistically detailed description of a tree crown or a canopy system from such a multi-RC model requires specific empirical parameterization at the branch level or canopy-layer level that is very laborious and can rarely be practical. In addition, such parameterization can only be site specific and is not consistent among species, growth stages, and even seasons, because trees change their structure and their transpiration dynamics [e.g., Tyree and Ewers, 1991; Borchert, 1994; Ryan et al., 2000; Köstner, 2001]. Our simulations show that structural differences lead to marked differences in electric-equivalent parameters (Figures 5 and 6). Differences in conductance due to crown structure were observed in spruce trees [Herzog et al., 1998; Rayment et al., 2000].
 Typically, RC models do not operate at a branch level and thus lump all branches into a single- or multiple-layer representation. This approach is consistent with the atmospheric model representation of a horizontally layered grid but ignores the tree vertical structure. The result is a tree level time constant (τ). We find from our model calculations that τ is highly variable between trees with different crown structure (Figure 6). Here τ increases with higher EB but is also negatively affected by ED because τ is a product of resistance and capacitance and thus affected by both the conductive efficiency, which mostly modifies Rp, and the branch thickness, which mostly controls C. Trees with low conductance (high Rp) and thick branches (high C) have the longest τ. In the “natural tree,” τ = 15.33 min, but depending on ED and EB, τ can vary from a few seconds to about 60 min. Phillips et al.  showed that the RC model could be developed in a way that allows empirical calibration but requires introducing two different τ terms: a tree-level τ and a branch-level τ. They reported values of 5.4–6.4 min for the branch level and 48 min for the tree level in a Norway spruce. Our calculations of the time constant are mostly affected by the fluxes at the end branches, but also include the tree level C and therefore represent an intermediate term between the tree and the branch level. This problem of ill-defined time constant (i.e., which part of the tree is considered in the discharge calculations) may explain why the reported τ varies appreciably among studies. For example, Rayment et al.  reported a branch τ that ranges between 0.5 and 2 hours depending on the height. Also, Chuang et al.  demonstrated that stem tapering can lead to significant changes in τ and reported an estimate of 1.25 hours from their model calculations, but their τ represented the time constant for nighttime recharge and not an RC equivalent daytime discharge. When these findings are all taken together, τ is likely to vary significantly with organ size, height, and structure, and throughout the day; hence the constant capacitance is an unrealistic representation of storage dynamics in the tree.
3.4. Scaling the Structure Effects in Time
 By integrating the transpiration rate over time, we can compare the total amounts of water transpired throughout the day by trees with different crown structure. In cases where the trees are fully replenished after a 24-hour cycle, this is also the amount of water that the tree transferred from the soil to the atmosphere. Trees with low ED or intermediate ED and low EB transpire much less than the maximal potential transpiration (as low as 20%), while trees with high ED reach 95% or more of the maximal potential transpiration (Figure 7). This response is due to pressure limitation that forces stomata to close in trees with suboptimal structure. At about 95% of potential, this response saturates and very little additional transpirational gain is achieved for an additional increase of ED or EB. Such an increase must have a cost in terms of carbon allocation (bigger branches) or tradeoff with other functions of the branch (e.g., structural strength may be compromised to gain higher conductance for a given branch diameter), hinting at some optimization of conductive costs versus reduced transpiration and thus carbon gain. Combined with our findings about conductance, our model suggests that trees might adopt different structural strategies for different hydrological adaptations. Drought-resistant trees should have high storage and low conductance [Tyree, 2003], and thus hydraulic structural properties typical to the upper left corner of our virtual structural plane (Figures 6 and 7) would be selectively preferred in a drought-resistant tree. Trees that optimize growth (and with it, transpiration rate) would be most efficient along the 95% contour of relative transpiration rate (Figure 7).
 We demonstrated that tree structure (through ED and EB) significantly impacts transpiration. This impact is apparent in the temporal and spatial (and in particular vertical) pattern of water fluxes from the canopy to the air. We also showed that this impact accumulates to generate large differences in the total diurnal water flux from the soil to tree to atmosphere.
 That tree structure affects its hydraulic function and total daily transpiration is not new [Tyree and Ewers, 1991]. Differences in daily transpiration dynamics and totals were shown to be the result of structural differences due to fertilization [Ewers et al., 2001], soil physical properties [Hacke et al., 2000], seasonal phenology [Borchert, 1994], and different biomass allocation due to climate in different habitats [Maherali and DeLucia, 2001]. Tree age and height were shown to cause consistent differences in total transpirational flux [Ryan et al., 2000; Schäfer et al., 2000; Köstner, 2001; Addington et al., 2004]. In particular, taller (older) trees were found to have lower daily transpiration rates per leaf area. As can be predicted from the model results, this is probably an effect of higher hydraulic stress in higher branches. Furthermore, on the basis of simulations, trees with higher stem capacitances are able to sustain higher transpiration throughout the day and in particular during noontime [Goldstein et al., 1998; Meinzer et al., 2003]. The consistency between the model results and observations suggests that this modeling approach offers a direct method to predict the structural effects on crown hydrodynamics via parameterization of scaling laws of crown structure and wood conductance. With further work, these effects could be scaled to represent the canopy on temporal and spatial scales that are relevant for regional meteorological and hydrological modeling.
4. Practical Considerations and Future Applications
 We proposed an organ-level hydrodynamic model with properties that can be independently derived. Given that the model uses conservation of mass and porous-media transport equations, it can be readily generalized to any woody species. Furthermore, unlike a laminar-flow pipe system, this approach preserves the nonlinear nature of the capacitance-conductance relationship through the structural allometry and hydraulic properties of the wood.
 FETCH is built as a modular combination of three independent modules: the porous media FEM solver, the fractal tree generator, and the turbulence-closure forcing module. The tree generator could be readily used to generate various structures that approximate observed crown scaling laws in order to study the ecological and evolutionary effects, and could also be replaced by actual tree measurements to link sap flux with transpiration in monitored sites. The meteorological forcing that now uses observations above the canopy could be replaced by a regional meteorological model such as RAMS [Pielke et al., 1992]. Information about canopy morphology is becoming widely available, given the advancements in both canopy lidar measurements that can resolve the “coarse-tree branching” [see Lefsky et al., 2002, Figure 9] and IKONOS imagery that can resolve crown width [Tanaka and Sugimura, 2001]. The fractal tree generator can readily incorporate such data to construct realistic trees.
 While several practical and theoretical difficulties remain, such as the applicability of Darcy's law to water flow in xylems, and root dynamics and their relationship to soil moisture, the proposed approach is timely because it provides a framework for confronting the challenges to modeling water flow in the plant-atmosphere system. We showed that the simplification achieved by the assembly of 1-D porous media pipes as a representation of the 3-D tree hydraulic system and the sparse banded symmetric structure of the tangent FE-solution matrix resulted in high computational efficiency. Hence the computational overhead of adding such a model (vis-à-vis the common models) in regional atmospheric, hydrologic, and ecological models is not high. Some examples of current models that link plant transpiration and atmospheric simulations and might benefit from an integrated FETCH approach, include LEAF [Walko et al., 2000], VIC [Wood et al., 1992; Liang et al., 1994], SIB2 [Sellers et al., 1996a, 1996b], and inference of water flux from the NOAA advanced very high resolution radiometer (AVHRR) instrument on board MODIS [Nishida et al., 2003].
 In terms of relevance to ecohydrology, FETCH can account for the effects of forest structure on plant hydrodynamics, with subsequent effects on forest hydrology and carbon uptake [Schäfer et al., 2000; Katul et al., 2003]. Height was rarely considered in resistor-capacitor models that at best use calibrated static parameters with stand height. Following a rigorous phase of model validation, and given the potential availability and improvements in canopy lidar measurements, a FE porous media pipe system, such as FETCH, could replace current representations of plant hydrodynamics (e.g., 2R-big leaf, resistor-capacitor) and further contribute to the “greening” of climate models.
Appendix A: Development of the Finite Element Solution
 The strong form of the problem can be stated as follows:Find Φ(z, t): Ω×R+ → R such that
 Multiplying (A1a) by a weighting function ω, and integrating by parts over the domain of interest Ω, we obtain
Defining the function spaces
where H1(Ω) denotes the Hilbert space whose member functions, and their first-order derivatives, are square-integrable on Ω, we can state the weak form of the problem as follows:Find Φ ∈ ℘ such that, for all ω ∈ ν,
It is noted that (A3a) ensures that the Dirichlet boundary condition (A1b) is satisfied. It is also noted that the boundary integral in (A2) does not appear in the weak form as the integrand vanishes on Γg, by virtue of (A3b), as well as on Γh, to satisfy the Neumann boundary condition (A1c).
 The domain is discretized into nel element domains, denoted by Ωe. Within an element with nen nodal points, the trial solution and weighting function are approximated by their finite-dimensional counterparts, given by
Here( )h is used to denote a finite-dimensional function; Ni, di, and ci are the shape function, the unknown nodal value of Φh, and the arbitrary nodal value of ωh, respectively, belonging to node i. The Galerkin weak form can then be expressed as a summation of integrals over the individual elements:
 Substituting (A5) into (A6) leads to a matrix equation of the form
where ∂d/∂t and d are the vectors of nodal unknowns of ∂Φ/∂t and Φ, respectively. The “mass” matrix M and the “stiffness” matrix K are given by
and the internal and external “force” vectors, Fint and Fext, are given by
 Recalling from equations (3) and (4) that the conductance k and the capacitance C are both dependent on Φ, we note that the time-dependent matrix equation (A7) is nonlinear. Its linearized form is derived below. The Newton-Raphson method is then used to iteratively find the solution at each time step, and the backward-Euler scheme is used to step the solution forward in time.
 As a first step in the linearization process, we define the residual vector,
It is obvious that R = 0 if and only if (A7) is satisfied. For the purpose of linearization, we denote by d(n+1)(p+1) the unknown solution being sought in iteration p + 1 of time step n + 1, and by d(n+1)(p) the known solution obtained at the end of the preceding iteration of the same time step, and we write
Accordingly, a truncated Taylor-series expansion of R(d(n+1)(p+1)) gives
The right side of (A12) is made to vanish by solving
where the vector S and the tangent matrix T are defined as
and obtained via the usual assembly process [see Hughes, 2000] from the corresponding element arrays, s and t, respectively. These are given by
where for compactness, C(n+1)(p) denotes C(d(n+1)(p)) and k(n+1)(p) denotes k(d(n+1)(p)).
 The authors thank Michiaki Sugita and three anonymous referees for their helpful comments. We acknowledge the comments and assistance we received from Yao Li Chuang. We also thank Tea Yeon Kim, Eui Joong Kim, Ilinca Stanciulescu, and Huidi Ji for assistance in the model development, Mathieu Therezien and Kristen Goris for additional simulations, and Robert Walko, Amilcare Porporato, Edoardo Daly, Kivanc Ekici, Gary Ybarra, Stacy Tantum, and Zbigniew Kabala for assistance and advice. This research was supported by the Office of Science (BER), U.S. Department of Energy, through the Terrestrial Carbon Processes Program (TCP), grant DE-FG02-00ER63015 and grant DE-FG02-95ER62083; by the BER's Southeast Regional Center (SERC) of the National Institute for Global Environmental Change (NIGEC) under Cooperative Agreement DEFC02-03ER63613; by the National Oceanic and Atmospheric Administration (NOAA), grant NA96GP0479; and by the National Science Foundation (NSF), grant DEB-0453296. The views expressed herein are those of the authors and do not necessarily reflect the views of these agencies.