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Chapter 5 ....continued
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5.2.4 The plant growth module
The plant growth module models plant growth (of up to two vegetation layers) as a function of light, nutrient and water availability, grazing pressure (if livestock are present), ambient temperature and soil salinity and pH. This is done using the Integrated Rate Methodology (IRM), described by Hatton et al. (1992), Wu et al. (1994), Hatton et al. (1995), Dawes et al. (1995) and Vertessy et al. (in press). The module assumes that the actual CO2 assimilation rate is dependent on a maximum rate and the relative availability of light, water, and nutrients. It computes the carbon assimilation index (r) of (Wu et al. 1994):
r = 1 + wH + wN
1/xT xL + wH/xW + wN/xN5.16 where:
wH = the weighting of water relative to light
wN = the weighting of nutrients relative to light
xW, xN, xL are the relative resource availabilities for water, nutrition, and light, respectively, and
xT = the modifier of light availability due to temperature
Carbon assimilation (A) is calculated as:
A = r. Amax 5.17 where:
Amax = the maximum mean daily assimilation rate of CO2.
Five carbon pools are defined:
- litter
- Leaf
- Root
- live stem
- a soluble pool expressed as a fraction of leaf carbon
Maintenance respiration is calculated as a function of temperature as in Running and Coghlan (1988) and net photosynthesis is calculated as assimilation less total respiration. When daily respiration exceeds assimilation, carbon is taken from the soluble pool (if present), then from the leaf and root pools. Growth respiration is assumed to be a constant fraction of allocated carbon (Rauscher et al. 1990).
On days when assimilation exceeds respiration, a soluble carbohydrate pool is filled. When it reaches its maximum, the excess is assigned dynamically to leaves, roots and stems. Leaf carbon may not exceed a level where 95% of incoming light is intercepted, nor exceed stem carbon. These conditions recognise that once canopies capture all available light, there is little point adding more leaves, and that leaves require some minimum mechanical and hydraulic support. Carbon allocation to leaves, roots and stems is dynamic and follows the approach of Running and Gower (1991) in that the leaf:root ratio is based on the relative availabilities of above- and below-ground resources (sensu Chapin et al. 1987, Wilson 1988), in this case as calculated by the equation for r.
Increments to root carbon are distributed by dynamic allocation of carbon through the root zone. We assume that root carbon is continuous from the surface downwards, that roots are added to the wettest (most favourable) region of soil, and that roots grow downwards in search of water, if necessary. The favourability of a soil region is a function of the moisture there.
Irrespective of daily assimilation, each of the three living carbon pools suffer daily decrements, representing the turnover of leaves, bark and roots. Shedding from the two above-ground carbon pools, as well as any carbon from net negative assimilation, contributes to the litter pool. This litter pool decays as a function of temperature and moisture (Hatton et al. 1992).
5.2.5 The overland flow module
When Topog_Dynamic is run in the 'stormflow' mode with the kinematic wave overland flow option invoked, overland flow within each catchment element is computed for each timestep using the one-dimensional kinematic wave equation. It is assumed that overland flow occurs uniformly across the catchment element as sheet flow. While such flows are characterised by low depths and velocities, we assume that they are fully turbulent, owing to the effects of raindrop impact and surface obstructions such as vegetation and soil particles.
It should be noted here that the transpiration calculations are not implemented during sub-daily timestep calculations.
The Manning equation is used to relate flow velocity (v) to flow depth (h):
v = h2/3 m1/2
n5.18 where:
m = the surface slope
n = the Manning roughness coefficientFor each element, the volume of overland flow (q) at each timestep (DT) is computed as:
q = v. A. DT 5.19 where A is the element area.
Continuity is governed by:
where:
dh
dt+ dQ
dx= no 5.20
t = time
x = distance measured downslope
Q = the net flux of overland flow per unit width of element
no = the net rate of added (eg. rainfall or exfiltration) or lost (eg. infiltration) water.A backwards weighting procedure is used to ensure a smooth and stable solution.
5.2.6 The sediment transport module
For each catchment element, the sediment transport module computes :
- detachment of soil by rainfall splash
- detachment of soil by overland flow
- sediment transport capacity of overland flow
- net flux of sediment.
5.2.6.1 Splash detachment
For bare soil, the splash detachment DS is computed as:
D DS = A(e). . . S . (ND . PD2) = A(e).MR 5.21 where:
A(e) = the soil erodibility factor
e = the energy required to detach an aggregate
ND = the number of raindrops of a certain size class (diameter D) in the rainfall event
PD = the momentum of a raindrop of size D
MR = the sum of squared momenta of the raindropsThe sum of squared momenta for raindrops hitting the ground is approximated by:
MR = 2.04 x 10-8 I 1.63 for I <= 75
MR = 4.83 x 10-8 I 1.43 for I >= 75
5.22 where I = the rainfall intensity in mm/h.
For cases where there is a plant canopy, mulch or stones and water ponding on the ground, the net splash detachment rate is computed as:
DR = C1 C2 Kh cos(a) Ds 5.23 where:
C1 = the canopy factor
C2 = the fraction of area affected by splash (ie. the fraction of area not covered by plants, mulch or stones)
Kh = the water depth correction factor
a = the ground surface slope.
The canopy factor is defined as:
C1 = (1-c) MR + c Mc
MR5.24 where:
c = the area fraction of canopy cover (0-1)
MR = the sum of squared momenta of the raindrops, and
MC = the sum of squared momenta of the raindrops from canopyThe squared momenta of the raindrops from canopy is calculated by:
MC = Inet. p
6D3. rw2 . VD2 = Inet. DH 5.25 where:
Inet = the volume of water transformed to new drops (drainage from leaves)
D = the drop diameter of drops falling from leaves
rw = the density of water
VD = the velocity of rainfall drops, which is a function of drop size and fall heightFor a typical drop diameter (D = 5 - 5.5mm), the relationship between the parameter DH and canopy height is approximated by:
DH = 1.29 H for H <= 2 DH = 0.0051H3 - 0.158H2 + 1.6696H - 0.1743 for 2 < H <= 13 DH = 6.2 for H > 13 5.26 where:
H is the distance from the ground to the gravity centre of the plant canopy (in m).
A water layer on the ground will influence the ease of detachment in different ways. When the water layer reaches a certain thickness, it starts working as a shield against the forces of the incoming drops, and the viscosity of the water restricts movement of the detached aggregates. We therefore introduce a correction factor in calculating the splash detachment rate, given as:
Kh = 1.0 for h <= Dm Kh = e(1 - h/Dm) for h > Dm 5.27 where:
h = the water layer depth in mm
Dm = the mean drop diameterand Dm = 1.238 I0.182 (in mm),
where:
I = rainfall intensity in mm/h.
5.2.6.2 Transport of particles detached by rainfall splash
The splash detached soil particles are transported by overland flow. Due to gravity, the particles are deposited again a distance downslope according to their fall velocities. Neglecting the wash load, the net transport qr is expressed by:
qR = DR q
2S
ifi
wi5.28 where:
DR = the total splashed soil
q = the overland flow discharge
fi = weight percentage of size fraction i
wi = the fall velocity of size fraction i.
5.2.6.3 Entrainment of soil particles by overland flow
The flow entrainment of cohesive soils qE is described by
qE = h qT 5.29 where:
qT = the sediment transport capacity of overland flow
h = the entrainment rateIn the sediment transport module h is used as a calibration factor.
5.2.6.4 Transport capacity and total sediment load
Topog_Dynamic uses the Engelund and Hansen (1968) equation to calculate sediment transport capacity of flow for non-cohesive sediments. The formula is used for determining transport capacity of overland flow, because once detached, the soil aggregates are transported as non-cohesive sediments until they settle again. The Engelund-Hansen transport equation is based on a fundamental energy equation for transport and deposition of sediments along a movable bed. It is assumed that the gain in potential energy when a particle is lifted can be equated with the work done by the drag forces of the flow. Thus, the sediment transport capacity of overland flow is calculated by:
qT = 0.04 (Sh)3/2
(s-1)2 d50 g1/2v2 = 0.04 ( 2g
f)1/6 (Sq)5/3
(s-1)2 d50 g1/25.30 where:
qT = the amount of transported sediment (m3m-1s-1),
S = the energy slope,
s = the ratio of specific weight (or density) of sediment to the specific weight (or density) of water,
v = the flow velocity (m/s), computed as (2g/f)1/2 . (Sh)1/2 = q/h
h = the water depth (m),
f = the roughness coefficient,
d50 = the median grain diameter (m),
q = the quantity of runoff (m3m-1s-1),
g = the acceleration due to gravity (m/s2).
The total sediment load qs leaving an element is limited by the transport capacity of overland flow. Thus, if the computed transport is higher than the transport capacity, the flow entrainment and successively the net transport of splashed soil are limited to give a total sediment load equal to the transport capacity.
qs = qR + qE if qR + qE <= qT qs = qT if qR + qE >= qT 5.31 where:
qR = the net transport of splash detached soil
qE = the flow entrainment of soils
qT = the transport capacity of the overland flow.As an alternative to the Engelund-Hansen (1968) equation, Topog_Dynamic also allows the user to compute total sediment load using Yang's unit stream power theory. With this option, it is assumed that erosion is transportation capacity limited; soil detachment is considered to be non-limiting and surface cover or depression storage effects are not considered. The sediment flux is calculated by:
qs = rg
n0.6bq0.4b S1.3b 5.32 where:
qs = the sediment flux per unit width in kg m-1s-1
q = the discharge per unit width in m3m-1s-1
r = the density of water
n = Manning's surface roughness coefficient
S = the element slope
g and b constants which are functions of the median sediment size, the kinematic viscosity of the water, and the terminal fall velocity of sediment particles in water.
5.2.6.5 Estimation of net erosion and deposition
The net erosion or deposition for each element and each time step is calculated as the difference between the sediment load entering and leaving an element. The erosion/deposition rate per unit area is estimated by:
Red = qis bi - qos bo
ae5.33 where:
qis = the sediment fluxes per unit width entering the element
qos = the sediment fluxes per unit width exiting the element
bi and bo are the contour segments
ae = the area of the element.
Take me out of frames | Chapter 5 continued ....... |