1. INTRODUCTION
The runoff curve number method for the estimation of direct runoff from storm rainfall is well established in hydrologic engineering and environmental impact analyses. Its popularity is rooted in its convenience, its simplicity, its authoritative origins, and its responsiveness to four readily grasped catchment properties: soil type, land use/treatment, surface condition, and antecedent condition.
The method was developed in 1954 by the USDA Soil Conservation Service (Rallison 1980), and is described in the Soil Conservation Service (SCS) National Engineering Hand-book Section 4: Hydrology (NEH-4) (SCS 1985). The first version of the handbook containing the method was published in 1954. Subsequent revisions followed in 1956, 1964, 1965, 1971, 1972, 1985, and 1993. Since its inception, the method had the full support of a federal agency and, moreover, it filled a strategic technological niche. Thus, it quickly became established in hydrologic practice, with numerous applications in the United States and other countries. Experience with the runoff curve number continues to increase to this date (Bosznay 1989; Hjelmfelt 1991; Hawkins 1993; Steenhuis et al. 1995).
The method's credibility and acceptance has suffered, however, due to its origin as agency methodology, which effectively isolated it from the rigors of peer review. Other than the information contained in NEH-4, which was not intended to be exhaustive (Rallison and Cronshey 1979), no complete account of the method's foundations is available to date, despite some recent noteworthy attempts (Rallison 1980; Chen 1982; Miller and Cronshey 1989).
In the four decades that have elapsed since the method's inception, the increased availability of computers has led to the use of complex hydrologic models, many of which incorporate the curve number method. Thus, the question naturally arises: What is the status of the curve number method in a postulated hierarchy of hydrologic abstraction models?
(Miller and Cronshey 1989; Rallison and Miller 1982). Has
it matured into general acceptance and usage? Or, as some
of its critics suggest, is it now obsolete, a remnant of outdated
technology, and in need of overhaul or outright replacement?
(Smith and Eggert 1978; Van Mullem 1989).
An effective overhaul of the method would require a clearer
understanding of its properties than is currently available
(Woodward 1991; Woodward and Gburek 1992). An outright
replacement, if one were to be developed, is likely to forego
part or all of the extensive data on hydrologic soil groups and
land use/treatment classes that has been assembled for most
of the United States (Miller and Cronshey 1989). More than
4,000 soils in the United States have been given a hydrologic
soil group (Rallison 1980). Moreover, a replacement or overhaul
could not avoid relying on many of those same features
that are now part of the curve number method. Therefore,
it has become necessary to examine the curve number method,
to shed additional light on its foundations, and to delineate
its strengths and weaknesses, so that the method may continue
to be used by practitioners without fear of an impending
demise. Thus, the objectives of this paper are the following:
1. To critically examine the curve number method,
2. To clarify its conceptual and empirical basis,
3. To delineate its capabilities, limitations, and uses, and
4. To identify areas of research in runoff curve number
methodology.
Over the years, the conceptual basis of the curve number
method has been the object of both support and criticism. A
conceptual model shares the simplicity of empirical models
and the wider applicability of the more rigorous physically
based models (Dooge 1977). Being conceptual, the runoff
curve number method is simple, and this is at the root of its
popularity. On the other hand, it is precisely for this reason
that the runoff curve number method has not fared well among
the supporters of alternative models, which include the physically
based models (Smith 1976).
Branson et. al. (1962, 1981), among others, have argued
that the simpler conceptual models are not necessarily inferior
to the more complex physically based models. The latter may
do a good job of describing the physical processes, but this
is usually at the expense of the chemical and biological aspects. In many instances,
processes such as surface crusting, clay shrinkage and swelling, entrapped gases, root
structure and decay, and soil macro- and microfauna may be of such importance as to
largely invalidate a strictly physical approach to infiltration modeling
(Le Bissonnais and Singer 1993).
2. LUMPED VERSUS DISTRIBUTED MODELS
The curve number method is an infiltration loss model,
although it may also account for interception and surface
storage losses through its initial abstraction feature. As originally
developed, the method is not intended to account for
evaporation and evapotranspiration (long-term losses).
An infiltration loss model can be either lumped or distributed.
The lumped model aggregates spatial and temporal variations
into a calculation of the total infiltration depth for a
given storm depth and drainage area. The distributed model
describes instantaneous and/or local infiltration rates, from
which a total infiltration depth is eventually obtained by suitable
integration in time and space. The curve number method
was originally developed as a lumped model (spatial and temporal),
used to convert storm rainfall depth into direct runoff
volume. To this date, it is used primarily as a temporally
lumped model in the manner specified by the NEH-4 handbook
(SCS 1985). However, a few investigators, notably Smith
(1976), Aron et. al. (1977), Chen (1975, 1976, 1982), and
Hawkins (1978a, 1980) have developed infiltration-capacity-equivalent formulas based directly or indirectly on the curve
number method. This effectively extends the method to the
domain of distributed modeling, although the instances of
this type of use appear to be relatively few. Existing infiltration
formulas such as Green and Ampt (1911), Horton (1933),
and Philip (1957) describe instantaneous and/or local infiltration
rates, and thus are directly suited for distributed modeling.
The relative advantages of distributed modeling versus
lumped modeling are not easily determined. With regard to
infiltration capacities, the spatial and temporal variability that
prevails in almost all practical settings does not usually favor
the distributed approach, unless the nature of this variability
can be specifically incorporated into the model, which is not
a small task (Miller and Cronshey 1989). Disregarding this
variability, or not accounting for it in a realistic way, amounts
in a real sense to lumping. Therefore, the lumped models
owe their existence to our inability to properly account for
the intrinsic variability of natural phenomena. What this means
in practice is that a lumped model is not necessarily bad.
Rather, that it is a practical way to substitute for the more
complex distributed process while attempting to preserve the
main features of the prototype.
A measurement of infiltration rate, or infiltration capacity,
as accurate as it may be, can only describe the rate at the
point of measure (Miller and Cronshey 1989). Extrapolation
to a larger area is tantamount to lumping. In fact, a lumped
infiltration depth is a statement of a spatially and temporally
averaged infiltration rate (however small the sample plot),
with all the advantages and disadvantages that this implies.
The advantage is that the method preserves the average features
of the phenomena. The disadvantage is that the method
does not specifically describe the spatial and/or temporal variability.
Nevertheless, a few interpretations of the curve number
method in terms of the spatial distribution of loss depths
have been developed (Hawkins 1982; Hawkins and Cundy
1982).
In practice, an acceptable amount of lumping is a function
of problem scale. For small-scale problems, for example, plots
measured in square feet or acres (square meters or hectares),
an attempt to ascertain the spatial and temporal variability
of infiltration capacity may be justified by detailed field measurements.
However, as the scale increases to hundreds of
hectares and tens of square kilometers, the practical inability
to collect increasing amounts of infiltration data makes lumping
an absolute necessity in infiltration modeling. Sooner or
later, a certain amount of spatial averaging has to be introduced.
Furthermore, considering that spatial averaging is implicit
in the nature of rainfall data at any scale, a strong case
is made for lumping as a de facto modeling tactic.
3. CONVERSION OF RAINFALL TO RUNOFF
The conversion of rainfall to runoff is the centerpiece of
surface water modeling. An elementary expression of conservation
of mass is:
where Q = runoff; P= rainfall; and L= abstractive losses, or hydrologic abstractions.
The quantification of hydrologic abstractions can be a complex task. These fall into five categories:
Interception storage in a rural setting, by vegetation
foliage, stems, and litter and in an urban setting, by
cultural features of the landscape,
Surface storage in ponds, puddles, and other usually
small temporary storage locations,
Infiltration to the subsurface to feed and replenish soil
moisture, interflow, and ground-water flow,
Evaporation from water bodies such as lakes, reservoirs,
streams, and rivers as well as from moisture on bare ground, and
Evapotranspiration from all types of vegetation.
Of these five types of hydrologic abstractions, infiltration
is the most important for storm analysis (short term). Evaporation
and evapotranspiration are the most important for
seasonal or annual yield evaluations (long term). The remaining
two losses (interception and surface storage) are usually
of secondary importance.
The curve number method is an infiltration loss model;
therefore, its applicability is restricted to modeling storm losses.
Barring appropriate modifications, the method should not be
used to model the long-term hydrologic response of a catchment.
Nevertheless, it is recognized that the method has been
used in several long-term hydrologic simulation models developed
in the past two decades (Williams and LaSeur 1976;
Huber et. al. 1976; Knisel 1980; Soni and Mishra 1985), with
varying degrees of success (Woodward and Gburek 1992).
Since the curve number method (as developed by SCS) does
not model evaporation and evapotranspiration, its use in long-term
hydrologic simulation should be restricted to modeling
the storm losses and associated surface runoff (Boughton 1989).
Ponce and Shetty (1995) have recently developed a conceptual
model of a catchment's annual water balance. The
model accomplishes the sequential separation of (1) annual
precipitation into surface runoff and wetting; and (2) wetting
into baseflow and vaporization. Ponce and Shetty's model
draws on a concept similar to that of the runoff curve number.
However, for a given site, the value of the annual retention
parameter bears no resemblance to that of the conventional
curve number method.
4. MODES OF SURFACE RUNOFF GENERATION
To clarify the basis of the curve number method, we review
here the processes of surface runoff generation. Surface runoff
is generated by a variety of surface and near-surface flow
processes, of which some of the most important are:
Hortonian overland flow,
Saturation overland flow,
Throughflow processes,
Partial-area runoff,
Direct channel interception, and
Surface phenomena, such as crust development, hydrophobic soil layers, and frozen ground.
Hortonian overland flow describes the process that takes
place when rainfall rate exceeds infiltration capacity, usually
at the beginning of a storm (or season), when the soil profile
is likely to be on the dry side. The rate difference (rainfall
rate minus infiltration capacity) is the effective rainfall rate
that is converted to surface runoff.
Saturation overland flow describes the process that takes
place after the soil profile has become saturated, either from
antecedent rainfall events or from a sufficient volume of rainfall
within the same event. At this point, any additional rainfall,
regardless of intensity, will be converted into surface
runoff. Saturation overland flow usually occurs during an
infrequent storm, or toward the end of a particularly wet
season, when the soil is likely to be already wet from prior
storms.
Throughflow prevails in heavily vegetated areas with thick
soil covers containing less permeable layers, overlying relatively
impermeable unweathered bedrock (Kirkby and Chorley 1967).
The concept of partial-area runoff developed from the recognition
that runoff estimates were improved by assuming
that only rainfall on a small and fairly constant part of each
drainage basin is able to contribute to direct runoff (Kirkby
and Chorley 1967). Thus, partial-area runoff can be interpreted
as a combination of throughflow in the upper hillslopes
and saturation overland flow in the lower hillslopes (Chorley
1978; Branson et. al. 1981; Hawkins 1981).
Direct channel interception refers to the runoff that originates
from rainfall falling directly into the channels. This
mode of surface runoff generation may be important in dense
channel networks and certain humid bases, where direct channel
interception may be the primary source of streamflow
(Hawkins 1973).
Surface phenomena includes processes such as crust development,
hydrophobic soil layers, and frozen ground, which
render the soil surface impermeable, promoting surface runoff.
For instance, a surface crust may develop following splash
erosion in a denuded watershed, adversely affected by human
activities or a natural hazard such as fire. Under a specific
set of circumstances, including soil type and texture, the silt
entrained by splash erosion may deposit on the surface and
create a thin crust that eventually reduces the infiltration rate
to a negligible level. Thus, any additional rainfall will be
converted to surface runoff. This mode of surface runoff generation
is typical of semiarid environments, where large
amounts of surface runoff may take place even though the
underlying soil profile, below a relatively thin veneer, remains
substantially dry ("Influences" 1940;
5. HISTORICAL BACKGROUND
The origins of the curve number methodology can be traced
back to the thousands of infiltrometer tests carried out by
SCS in the late 1930s and early 1940s. The intent was to
develop basic data to evaluate the effects of watershed treatment
and soil conservation measures on the rainfall-runoff
process. A major catalyst for the development and implementation
of the runoff curve number methodology was the
passage of the Watershed Protection and Flood Prevention
Act of August 1954. Studies associated with small watershed
project planning were expected to require a substantial improvement
in hydrologic computation within SCS (Rallison 1980).
Sherman (1942, 1949) had proposed plotting direct runoff
versus storm rainfall. Building on this idea. Mockus (1949)
proposed that estimates of surface runoff for ungauged watersheds
could be based on information on soils, land use,
antecedent rainfall, storm duration, and average annual temperature.
Furthermore, he combined these factors into an
empirical parameter b characterizing the relationship between
rainfall depth P and runoff depth Q (Rallison 1980):
Andrews (unpublished report, 1954), using infiltrometer
data from Texas, Oklahoma, Arkansas, and Louisiana, developed
a graphical procedure for estimating runoff from rainfall for
several combinations of soil texture, type and amount
of cover, and conservation practices. The association was referred
to as a soil-cover complex (Miller and Cronshey1989).
Mockus empirical P-Q rainfall-runoff relationship [(2)] and
Andrews' soil-cover complex were the basics of the conceptual
rainfall-runoff relationship incorporated into the forerunner
version of NEH-4 (Hydrology 1954). The method,
since referred to as the runoff curve number, had the following
significant features:
The runoff depth Q is bounded in the range 0 ≤ Q ≤ P,
assuring its stability.
As rainfall depth P grows unbounded (P → ∞), the
actual retention (P - Q) asymptotically approaches a
constant value S. This constant value, referred to in
NEH-4 as "potential maximum retention," and here
simply as "potential retention," characterizes the watershed's
potential for abstracting and retaining storm
moisture and, therefore, its direct runoff potential.
A runoff equation relates Q to P, and a curve parameter
CN, in turn, relates to S.
Estimates of CN are based on: (1) hydrologic soil group;
(2) land use and treatment classes; (3) hydrologic surface
condition; and (4) antecedent moisture condition.
6. RUNOFF CURVE NUMBER EQUATION
The method assumes a proportionality between retention
and runoff, as follows:
in which F = P - Q = actual retention; S = potential retention;
Q = actual runoff; and P = potential runoff, that is,
total rainfall. The values of P, Q, and S are given in depth
dimensions. While the original method was developed in U.S.
customary units (in), an appropriate conversion to SI units
(cm) is possible (Ponce 1989). Rainfall P is the total depth
of storm rainfall. Runoff Q is the total depth of direct runoff
resulting from storm rainfall P. Potential retention S is the
maximum depth of storm rainfall that could potentially be
abstracted by a given site.
In a typical case, a certain amount of rainfall, referred to
as "initial abstraction," is abstracted as interception, infiltration,
and surface storage before runoff begins. In the curve number method,
this initial abstraction lα is substracted from
rainfall P in Eq. 3 to yield:
Solving for Q in Eq. 4 yields:
which is valid for P > lα, that is, after runoff begins; and
Q = 0 otherwise. With initial abstraction included in Eq. 4, the
actual retention P - Q asymptotically approaches a constant
value S + lα, as rainfall grows unbounded.
Equation 5 has two parameters: S and lα. To remove the
necessity for an independent estimation of initial abstraction, a
linear relationship between lα and S was suggested [SCS (1985),
and earlier versions]:
in which λ = initial abstraction ratio.
Equation 6 was justified on the basis of measurements in watersheds
less than 10 acres in size (SCS 1985). While there
was considerable scatter in the data, NEH-4 reported that
50% of the data points lay within the limits 0.095 ≤ λ ≤ 0.38
[SCS (1985), and earlier versions]. This led SCS to adopt a
standard value of the initial abstraction ratio λ = 0.2. However,
values varying in the range
With λ = 0.2 in Eq. 6, Eq. 5 becomes:
subject to P > 0.2S; and Q = 0 otherwise.
Equation 7 now contains only one parameter, potential retention
S, which varies in the range
where 1,000 and 10 are arbitrarily chosen constants having the same
units as S (in). Likewise:
A CN = 100 represents a condition of zero potential retention
(S = 0), that is, an impermeable watershed. Conversely,
a CN = 0 represents a theoretical upper bound to
the potential retention
Substituting Eq. 8 into Eq. 7, the equation relating direct runoff
Q to storm rainfall P is obtained, with CN as the curve
number, or curve parameter:
subject to P > (200/CN) - 2; and Q = 0 otherwise.
Equation 5 can be expanded to yield (Chen 1976; Hawkins 1978b):
This equation reveals that as potential runoff grows unbounded
(P - lα → ∞), actual retention, excluding initial
abstraction (P - lα - Q), asymptotically approaches
potential retention S. This is the basic tenet of the curve number
method, that is, the asymptotic behavior of actual retention
toward potential retention for sufficiently large values of potential
runoff. Note that this behavior properly simulates the
saturation overland flow mode of runoff generation. In this
connection, Chen (1975, 1976, 1982) has derived an infiltration
equation based on the curve number method, and related
it to the Holtan infiltration equation, which explicitly accounts
for available soil storage (Holtan et. al. 1975).
In practice, there are some situations where the storm rainfall-runoff
relationship does not follow
have been formulated (Fogel and Duckstein 1970; Hawkins
1942), but the problem remains to determine the empirical
coefficient b, preferably as a function of runoff-producing
properties.
The humble empirical beginnings of the curve number
method in no way detract from its distinctive conceptual basis.
Indeed, it is only under a conceptual modeling framework
that we are able to discern why the retention and runoff ratios
ought to be equal (Eq. 3). Equality of these ratios leads to
a conceptual model where the curve number is the only parameter
describing the process. In turn, this parameter is a
surrogate for potential retention, a measure of available subsurface storage,
that is, of the ability of a given site to abstract
storm rainfall.
7. ANTECEDENT MOISTURE/RUNOFF CONDITION
A conceptual model works in the mean, implying that there
is room for some variability.
The effect of the spatial variability of storm and watershed properties,
The effect of the temporal variability of the storm, that
is, the storm intensity,
The quality of the measured data, that is, the P - Q sets
moisture, and
The effect of antecedent rainfall and associated soil moisture.
The latter was recognized very early as the primary or
tractable source of the variability, and thus, the concept of
antecedent moisture condition (AMC) originated (SCS 1985).
More recently, the same concept has been referred to as the
antecedent runoff condition (ARC) to denote a shift of emphasis
from soil moisture to runoff ("Urban" 1986).
The original-handbook runoff curve numbers were developed
from recorded rainfall-runoff data, where hydrologic
soil group, land use/treatment class, and surface condition
were known.
To account for this variability, the P-Q plots were used to
define enveloping or near-enveloping CN values for each site.
While the theoretical bounds of curve number are CN = 0
(Q = 0) and CN = 100 (Q = P), the enveloping CN values
reduce the limits to practical values based on site experience.
These enveloping CN values are considered as the practical
upper and lower limits of expected CN variability for the given
soil-cover complex combination. Thus, antecedent moisture
condition was used as a parameter to represent the experienced
variability (Rallison and Cronshey 1979).
The curve number lying in the middle of the distribution
is the median curve number, corresponding to AMC 2 (average
runoff potential). This is the standard curve number
given in the SCS and other applicable tables (SCS 1985). The
low value is the dry curve number, of AMC 1 (lowest runoff
potential). The high value is the wet curve number, of AMC
3 (highest runoff potential).
NEH-4 contains a conversion table (Table 10.1) listing corresponding
AMC 1 and AMC 3 CN values for given AMC 2
CN values. The original values of this table, reported in the
1956 edition of NEH-4, were based on unsmoothed data. The
values in the present AMC conversion table [in SCS (1985)]
have been smoothed by fitting straight lines on normal probability
paper. Capitalizing on this fact, Sobhani (1975) and
Hawkins et. al. (1985) developed correlations between the dry
or wet potential retentions S1 and S3 and the average potential
retention S. Hawkins et. al. (1985) reported the following:
with r 2
with r 2 = 0.994, and Se = 0.088 in.These equations are applicable in the range 55 ≤ CN ≤ 95, which encompasses most estimated or experienced curve numbers. Substitution of Eq. 13 and Eq. 14 into Eq. 8 leads to:
with r 2 = 0.996, and Se = 1.0 CN, and
with r 2 = 0.994, and Se = 0.7 CN.
The one-to-one relationship between CN and S (Eqs. 8 and 9)
renders the latter intrinsically related to antecedent moisture.
Thus, potential retention is a measure of the ability of
a given site to abstract and retain storm rainfall, provided the
level of antecedent moisture has been factored into the analysis.
In other words, potential retention and its corresponding
curve number are intended to reflect not only the capacity of
a given site to abstract and retain storm rainfall, but also the following: (1)
the recent history of antecedent rainfall, or lack of it, which
may have caused the soil moisture to depart from an average
level; (2) seasonal variations in runoff properties; and In this role, site moisture per se acts as a surrogate for all other sources of variability, beyond that which could be attributed to soil, land use/treatment, and surface condition. Hjelmfelt et. al. (1982) found that the AMC conversion table described the 90% (AMC 1), 50% (AMC 2), and 10% (AMC 3) cumulative probabilities of exceedence of runoff depth for a given rainfall. In other words, they found that AMC 2 represented the central tendency, while AMC 1 and AMC 3 accounted for dispersion in the data. A similar analysis was performed by Gray et. al. (1982) using data from Indiana, Kentucky, and Tennessee, and by Hawkins (1983), using data from Arizona and Utah. Hawkins et. al. (1985) interpreted the AMC categories as "error bands" or envelopes indicating the experienced variability in rainfall-runoff data. What level of AMC should be used in a given case? For this purpose, NEH-4 (SCS 1985) shows the appropriate AMC level based on the total 5-day antecedent rainfall, for dormant and growing season (Table 4.2: "Seasonal Rainfall Limits for AMC"). This table was developed using data from an unspecified location, and subsequently was adopted for general use (Miller and Cronshey 1989). Unfortunately, the table does not account for regional differences or scale effects. An antecedent period longer than 5 days would probably be required for larger watersheds. Echoing this concern, SCS has recently deleted Table 4.2 from the new version of Chapter 4, NEH-4, released in 1993. In practice, a determination of AMC is left to the user, who must evaluate whether a certain design situation warrants either AMC 1, AMC 2, or AMC 3. It is understood that AMC 2 represents a typical design situation. A choice of AMC 1 results in lesser runoff volume, whereas greater runoff results from a choice of AMC 3. Design manuals specify the AMC choice as a function of return period, with AMC level increasing with return period. For example, the Hydrology Manual (1986) of Orange County, California, specifics AMC 1 for 2- and 5-yr storms, AMC 2 for 10-, 25-, and 50-yr storms, and AMC 3 for 100-yr storms. Likewise, the Hydrology Manual (1985) of San Diego County. California, specifies AMC values varying between 1.5 and 3.0 (in increments of 0.5) for a range of design frequencies (5-150 yr) and four climate regions: coast. foothills, mountains, and desert. While SCS does not endorse the use of fractional AMC levels (Rallison and Cronshey 1979), the practice exists and should be acknowledged. 8. RUNOFF CURVE NUMBERS EVALUATED FROM DATA Since the method's inception, several investigators have attempted to determine runoff curve numbers from small watershed rainfall-runoff data. The objective has been either to verify the CN values given in the standard tables, or to extend the methodology to soil-cover complexes and geographic locations not covered in the NEH-4 handbook. An established procedure solves for S in Eq. 7, leading to (Hawkins 1973; 1979):
For a given P and Q pair, the potential retention S is calculated with this equation, and the corresponding CN is calculated using Eq. 9.
There are several ways to select the P-Q pairs for analysis.
The standard method, referred to as the annual flood series, is to
select daily rainfall P and its corresponding runoff
volume Q (both in inches) for the annual floods at a site
(Rallison and Cronshey 1979; Springer et. al. 1980). In the absence of a long annual flood series, particularly in semiarid regions, some investigators have chosen to use less selective criteria for candidate storm events, including events of return period less than 1 yr (Woodward 1973; Hawkins 1984). This choice results in considerably more data for analysis, as well as slightly different CN values compared to those obtained using an annual flood series (Springer et. al. 1980). The choice of frequency for candidate storm events is the subject of continuing research (Woodward and Gburek 1992). Another approach to determine curve numbers from data is the frequency-matching method (Hjelmfelt 1980). The storm rainfall and direct runoff depths are sorted separately, and then realigned on a rank-order basis to form seemingly desirable P-Q pairs of equal return period. However, the individual runoff values are not necessarily associated with the causative rainfall values (Hawkins 1993). 9. OTHER EXPRESSIONS OF THE CURVE NUMBER EQUATION The SCS runoff curve number has been applied in many countries throughout the world. Therefore, its expression in SI units is necessary. Likewise, geographic and other differences may dictate that the initial abstraction ratio λ be relaxed to the range validated by local experience, say 0.0 ≤ λ ≤ 0.3. In SI units, Eq. 10 converts to:
in which P (cm) is divided by R = 2.54 (cm/in), and the result of the computation is multiplied by R, to give Q in cm. Being dimensionless, the curve number CN remains the same in both U.S. customary and SI units. Equation 18 is subject to the restriction that P > R [(200/CN) - 2]; and Q = 0 otherwise. To obtain the runoff curve number equation for a variable λ, Eqs. 6 and 8 are substituted into Eq. 5 to yield (Ponce 1989):
which is subject to the restriction that P > (1,000 λ/ CN) - 10λ; and Q = 0 otherwise. Equation 17 is applicable only for the standard value of initial abstraction λ = 0.2. For λ = 0:
In general, for λ > 0 (Chen 1982):
10. CRITIQUE OF RUNOFF CURVE NUMBER There is a growing body of literature on the curve number method (Bosznay 1989; Hjelmfelt 1991; Hawkins 1993; Steenhuis et. al. 1995). It will suffice here to enumerate the method`s advantages and disadvantages. The advantages are:
While it is theoretically possible for the its numbers to span the range 0-100, practical design values validated by experience are more likely to be in the range 40-98, with few exceptions (Van Mullem 1989). This is a significant advantage, because it restricts the method's only parameter to a relatively narrow range. Viewed in this light, it is seen that estimating a design CN is indeed an empirical exercise within a conceptual modeling framework. Such an exercise is not unlike that of estimating Chezy's C or Manning's n in open-channel flow (Hawkins 1975). Perceived disadvantages of the CN method are:
11. RUNOFF CURVE NUMBER: HAS IT REACHED MATURITY? Having reviewed its foundations, its conceptual/empirical basis, and its range of applicability, we now address the central issue of this paper: Has the runoff curve number method reached its maturity? Maturity implies usefulness, acceptance with faults acknowledged, understanding of its capabilities, and continued growth with possible eventual refinements. We believe the method has now reached maturity on these counts:
12. SUMMARY The runoff curve number method owes its popularity among hydrology practitioners to its simplicity, predictability, and stability, and to its support by a major U.S. federal agency. In the six decades that have elapsed since its inception, questions have arisen as to its nature and beginnings. Its adoption and use throughout the United States and other countries, far beyond the scope intended by its original developers, have demanded that the method be subject to close scrutiny. The method is a conceptual model of hydrologic abstraction of storm rainfall, supported by empirical data. Its objective is to estimate direct runoff volume from storm rainfall depth, based on a curve number CN. The curve number, which varies in the convenient range 100 ≥ CN ≥ 0, is a surrogate for potential retention, a conceptual parameter varying in the range 0 ≤ S ≤ ∞. The method does not take into account the spatial and temporal variability of infiltration and other abstractive losses; rather, it aggregates these into a calculation of the total depth loss for a given storm event and drainage area. The method works in the mean, by describing average trends, which precludes it from being perfectly predictive. The observed variability in curve numbers, beyond that which can be attributed to soil type, land use/treatment, and surface condition, is embodied in the concept of antecedent condition. The advantages of the method are: (1) its simplicity; (2) its predictability; (3) its stability; (4) its reliance on only one parameter; and (5) its responsiveness to major runoff-producing watershed properties. Perceived disadvantages are: (1) its marked sensitivity to the choice of curve number; (2) the absence of clear guidance on how to vary antecedent moisture; (3) the method's varying accuracy for different biomes; (4) the absence of an explicit provision for spatial scale effects; and (5) the fixing of the initial abstraction ratio at λ = 0.2, preempting a regionalization based on geologic and climatic setting.
APPENDIX I. REFERENCES
APPENDIX II. NOTATION The following symbols are used in this paper:
b = exponent in Eq. 2, coefficient in Eq. 12; CN = runoff curve number; CN1 = dry curve number (AMC 1); CN2 = average curve number (AMC 2); CN3 = wet curve number (AMC 3); F = actual retention; Iα = initial abstraction; L = abstractive losses; P = rainfall, potential runoff; P - Q = actual retention; Q = runoff, actual runoff; R = unit conversion factor; r = correlation coefficient; S = potential retention; S1 = dry potential retention; S2 = average potential retention; S3 = wet potential retention; Se = standard error of estimate; and λ = initial abstraction ratio. |
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