Shapes and functions of species–area curves: a review of possible models
Abstract
Aim This paper reviews possible candidate models that may be used in theoretical modelling and empirical studies of species–area relationships (SARs). The SAR is an important and well‐proven tool in ecology. The power and the exponential functions are by far the models that are best known and most frequently applied to species–area data, but they might not be the most appropriate. Recent work indicates that the shape of species–area curves in arithmetic space is often not convex but sigmoid and also has an upper asymptote.
Methods Characteristics of six convex and eight sigmoid models are discussed and interpretations of different parameters summarized. The convex models include the power, exponential, Monod, negative exponential, asymptotic regression and rational functions, and the sigmoid models include the logistic, Gompertz, extreme value, Morgan–Mercer–Flodin, Hill, Michaelis–Menten, Lomolino and Chapman–Richards functions plus the cumulative Weibull and beta‐P distributions.
Conclusions There are two main types of species–area curves: sample curves that are inherently convex and isolate curves, which are sigmoid. Both types may have an upper asymptote. A few have attempted to fit convex asymptotic and/or sigmoid models to species–area data instead of the power or exponential models. Some of these or other models reviewed in this paper should be useful, especially if species–area models are to be based more on biological processes and patterns in nature than mere curve fitting. The negative exponential function is an example of a convex model and the cumulative Weibull distribution an example of a sigmoid model that should prove useful. A location parameter may be added to these two and some of the other models to simulate absolute minimum area requirements.
Introduction
The species–area relationship (SAR) is one of the most important tools available in the study of species diversity, conservation biology and landscape ecology (see e.g. Schoener, 1976; Lomolino, 1989, 2000a; Palmer & White, 1994; Rosenzweig, 1995). It is one of the oldest and most well‐proven patterns in ecology. The shapes of species–area curves have been discussed extensively, sometimes even fiercely, for most of the last century (e.g. Arrhenius, 1921; Gleason, 1922, 1925; Connor & McCoy, 1979; Sugihara, 1981; Connor et al., 1983; Lomolino, 2000a, 2002; Williamson et al., 2001).
As the shape of the curve has been extensively debated over the years, the best known and most commonly applied curves are the two convex upward shaped curves: the exponential curve (Gleason, 1922, 1925; Fisher et al., 1943) and the power curve (Arrhenius, 1921; Preston, 1962a,b), whereof the power (log–log) model is the most frequently encountered in recent literature. Both curves are convex but not asymptotic. The power function goes through the origin of axes, but the exponential function does not. They are usually transformed into log–log and log‐linear space, respectively.
They are perhaps the most cited functions, but by no means the only plausible models (Connor & McCoy, 1979). It is argued that we may be using the wrong model, or at least an overly simplistic one (Lomolino, 2000a). Several authors (e.g. Williamson, 1981; Legendre & He, 1996; Rosenzweig & Ziv, 1999) have argued that the power model is best suited for, i.e. will produce straight lines in log–log space for, intermediate and larger sampling areas, and the exponential model is best and will produce straight lines in log‐linear space for smaller sampling areas. It is probable that the success of the power model and the exponential model is due to the fact that they are used for data within a restricted scale, and these curves are most useful at these scales. They might not be fitted successfully to data from very small or very large areas.
It is important to note that the species–area curve was originally intended to describe the increase in species number found as the size of the sampling area increases. These sample areas (census‐patches) are pieces of some large unbounded universe. When MacArthur & Wilson (1967) presented their theory of island biogeography, they treated the species–area curve as the result of bounded areas, or islands. Within the tradition of landscape ecology, nature consists of mosaics of isolates that can be treated more or less as islands. Species–area curves from sample areas, from isolates and from large continuous areas should differ in shape and other properties (Tjørve & Turner, unpubl. data.).
In the discussions of the shape of species–area curves, one should therefore bear in mind that historically the aim has been to fit empirical data (i.e. observed patterns). The Preston and the Arrhenius functions were chosen out of convenience and not from biological causes. As fitted curves they lack biological explanatory power. Only later have SARs become part of theories of species diversity (e.g. Preston, 1962a,b; MacArthur & Wilson, 1967; May, 1975).
The shapes of species–area curves
Why is it so important to know the shape of the species–area curve? Based on the curve shape, one may estimate total species diversity or species pools from counted numbers of samples or isolates, or estimate species extinction as a result of habitat loss and fragmentation. We also need to discuss the shape of species–area curves to be able to address more complex models or theories of SARs within landscape patterns and at different scales.
Both the power and the exponential functions have convex upward shapes and lack upper asymptotes. These models are usually indiscriminately used on isolate (island and habitat‐patch) data, without considering other possible models. Several authors have tried to find alternatives to the power function. A few have advocated convex upward models that have an asymptote (Holdridge et al., 1971; Miller & Wiegert, 1989). Lately, an increasing number of authors have argued that some SARs are perhaps best represented by functions that are sigmoid in arithmetic space (e.g. Williams, 1995, 1996; Legendre & He, 1996; Lomolino, 2000a,b, 2001). There are also a number of recent studies where sigmoid models have been fitted to empirical data (see Williams, 1995; Flather, 1996; Burbidge et al., 1997; Lomolino, 2000a; Veech, 2000; Belant & Van Stappen, 2002).
Many have fitted data that show sigmoid shapes in log‐linear space or discussed sigmoid shapes in log‐linear space (e.g. Archibald, 1949; Vestal, 1949; Hopkins, 1955; Coleman et al., 1982; Palmer & White, 1994; He et al., 1996; Legendre & He, 1996; Plotkin et al., 2000). Unfortunately, a sigmoid shape in log‐linear space does not imply a sigmoid shape in arithmetic space (and vice versa). Neither are sigmoid shapes in log–log space always sigmoid also in arithmetic space. Sigmoid species–area curves in log–log space are rarely found in the literature. Some have appeared in some modelling papers (e.g. Durrett & Levin, 1996; Leitner & Rosenzweig, 1997; Ney‐Nifle & Mangel, 1999). The sigmoid log–log space curves (covering many orders of magnitude of area) found in Preston (1960) and Williams (1964) go from decreasing slope to increasing slope, contrary to the models discussed here.
Thus, discussions of biological explanations for sigmoid SARs (in arithmetic space) do not necessarily apply to and cannot be supported by sigmoid shapes in log‐linear or log–log space. This has led to some confusion in the literature, as one often does not discern between different types of space. One always needs to be careful and aware of what type of space is used, when discussing the possibility of sigmoid species–area curves. I believe biological explanations and patterns that shape species–area curves are best discussed in arithmetic space.
Two kinds of small‐scale species–area curves, the sample curve and the isolate curve, have been distinguished (Preston, 1962a; Tjørve & Turner, in prep.). The sample curve is the result of species diversity of census patches (sample) of different sizes within an expanse of habitat with boundaries defined by the survey design, and is expected to be convex upward. The isolate curve is the result of species diversity within different sizes of habitat patches or islands (isolates) of the same type. One key distinction among functions may be their ability to fit data compiled from samples vs. data compiled from isolates, which should produce quantitatively different SARs (Rosenzweig, 1995; Tjørve & Turner, in prep.). The sample curve is expected to be convex upward and the isolate curve sigmoid. The failure to distinguish between these two patterns has produced considerable confusion in the literature.
There is a need to discuss the biological causes of SARs further and to evaluate possible species–area models that may coincide better with the way biological processes generate SARs. One should a priori be able to predict biological patterns in nature as the shapes of species–area curves. Failure to implicate these biological patterns while continuing to just indulge in mere curve fitting will hamper future understanding of these systems.
Aims
This paper reviews functions that in the literature have been fitted to species–area or species–accumulation data in the past. These functions will be evaluated and classified by curve shape, number of parameters and how parameters affect shape. Looking at both asymptotic convex upward shaped models and sigmoid models, model characteristics are systemized and discussed with respect to their behaviour in arithmetic space. Six convex and eight sigmoid models are reviewed. Other important characteristics are asymptotes, inflection‐points, symmetry and zero values. The relationship between different models is also discussed, with some models treated just as reductions of more complex models.
Sigmoid curve models should be expected to fit isolate (habitat‐patch or island) data, and convex models should fit sample area (census patch) data. Convex shapes should also fit isolate type data where no data are present from the lower convex downward (j‐shaped) part of the curve. Therefore strictly concave upward models can also be used successfully if only data from medium and large sized habitats or islands are included. One way to circumvent this problem has been by using different power line segments for different ranges, as is often performed to deal with the small island or minimum area effect. The minimum area effect is here defined as the effect of species minimum area requirements on species–area curves. That species have minimum area requirements is well known, but these have not been estimated empirically for most species (Gurd et al., 2001).
The different models (Tables 1 and 3) are reviewed to see how their parameters behave (Tables 2 and 4). The behaviour of these parameters may provide an indication of which function type will give us a curve that coincides with biological explanations, arguments as the existence of species pools and the minimum area effect. The nomenclature of these models is standardized so that x represents the independent variable (in this case area) and the parameters (constants) are named consecutively from ‘a’ to ‘d’, as no model has more than four parameters.
| Curve name | Model | Parameters (asymptote) | Source |
|---|---|---|---|
| Power | ax b | 2 (no) | Arrhenius (1921) , Preston (1962a,b) |
| Exponential | a + b log (x) | 2 (no) | Gleason (1922, 1925), Fisher et al. (1943) |
| Monod | a(x/(b + x)) | 2 (yes) | Monod (1950), de Caprariis et al. (1976), Clench (1979) |
| Negative exponential | a(1 − exp (−bx)) | 2 (yes) | Holdridge et al. (1971), Miller & Wiegert (1989), Ratkowsky (1990) |
| Asymptotic regression | a − bc−x | 3 (yes) | Ratkowsky (1983) |
| Rational function | (a + bx)/(1 + cx) | 3 (yes) | Ratkowsky (1990) |
| Curve name | Model | Parameter (when y = 0) | Source |
|---|---|---|---|
| Logistic function | a/(1 + exp (−bx + c)) | 3 (x = −∞) | Ratkowsky (1990) |
| Gompertz model | a exp (− exp (−bx + c)) | 3 (x = −∞) | Ratkowsky (1990) |
| Extreme value function | a(1 − exp (− exp (bx + c))) | 3 (x = −∞) | Williams (1995, 1996), Burbidge et al. (1997) |
| Morgan–Mercer–Flodin (Hill‐function) | a xc/(b + xc) | 3 (x = 0) | Morgan et al. (1975) |
| Lomolino funcion | a/1 + (b log (c/x)) | 3 (x = 0) | Lomolino (2000a) |
| Chapman–Richards | a(1− exp (−bx))c | 3 (x = 0) | Ratkowsky (1990) |
| Cumulative Weibull distribution | a(1− exp (−bxc)) | 3 (x = 0 and c = 0) | Weibull (1951), Reid (1978), Yang et al. (1978), Brown & Mayer (1988), Rørslett (1991), Flather (1996) |
| Cumulative beta‐P distribution | a(1−(1 + (x/c)d)−b) | 4 (x = 0) | Mielke & Johnson (1974) |
| Curve name | First parameter | Second parameter | Third parameter | Curve through origin of axis |
|---|---|---|---|---|
| Power | Curve shape | Shape* | Yes | |
| Exponential | Curve shape | Shape* | No | |
| Monod | Upper asymptote | Shape* | Depends on parameters | |
| Negative exponential | Upper asymptote | Shape | Yes | |
| Asymptotic regression | Upper asymptote + y‐axis intersection | Shape + y‐axis intersection | Shape* | Depends on parameters |
| Rational function | Shape + y‐axis intersection | Curve shape + upper asymptote | Shape + upper asymptote | Depends on parameters |
| Name curve | First parameter | Second parameter | Third parameter | Fourth parameter |
|---|---|---|---|---|
| Logistic function | Upper asymptote + y‐axis intersection | Shape + y‐axis intersection | Shape + y‐axis intersection | |
| Gomperitz model | Upper asymptote + y‐axis intersection | Shape + y‐axis intersection | Shape + y‐axis intersection | |
| Extreme value function | Upper asymptote + y‐axis intersection | Shape + y‐axis intersection | Shape + y‐axis intersection | |
| Morgan–Mercer–Flodin | Upper asymptote | Shape | Shape | |
| Lomolino function | Upper asymptote | Shape | Shape | |
| Chapman–Richards | Upper asymptote | Shape | Shape | |
| Cumulative Weibull distribution | Upper asymptote | Shape | Shape | |
| Cumulative beta‐P distribution | Upper asymptote | Shape | Shape | Shape |
Possible convex models
Neither of the two most commonly used models, the power and the exponential models, have an upper asymptote. This means that the total number of species (i.e. the species pool) is infinite. As long as one does not need an upper asymptote or the lower j‐shaped part of the curve (i.e. sigmoid shape), these are proven models that perform well. If one wants convex upward shaped SAR‐models, then there are several possible functions (Table 1). All of the models except for the power and the exponential have upper asymptotes. The asymptote of a fitted curve may serve as an estimate of the species pool or the total number of species.
The Monod function (Monod, 1950) is also called the two‐parameter hyperbola. It is one of several versatile models. The curve has an upper asymptote, but does not always go through the origin of axes. The first parameter represents the upper asymptote, while the other parameter affects curve shape (Table 2). The curve always goes through a point in space given by x = 0, f(x) = a − b. Flather (1996) reported that the Monod function did not perform well with his bird census data. Clench (1979) and de Caprariis et al. (1976) successfully used the Monod model to produce species–accumulation curves from samples of number of individuals or some measure of effort.
The negative exponential function (Ratkowsky, 1990) is a very simple two‐parameter model (Table 1) that always passes through the origin. It produces an ordinary convex upward curve with an upper asymptote. It is, contrary to the power and exponential functions, convex upward in space for all positive values of both parameters. More than 30 years ago Holdridge et al. (1971) used this function to fit tree species data from sample plots in Costa Rica. Miller & Wiegert (1989) fitted the negative exponential function to cumulative plots of number of rare plant species to area, and reported a close agreement between the model curve and the data. Flather (1996), on the other hand, reported that the model performed poorly relative to all other candidate models he tested. The negative exponential function should also be useful on species–accumulation data (Sorberon & Llorente, 1993; Colwell & Coddington, 1994).
The asymptotic regression (Ratkowsky, 1983) has an upper asymptote but does not always go through the origin of axes. The three‐parameter model is not as easy to handle as the Monod and the negative exponential functions. This is because two of the parameters in the asymptotic regression affect more than one curve trait at the same time (shape, upper asymptote and y‐axis intersection). Flather (1996) tested the asymptotic regression but found it did not perform well on his bird survey data.
The rational function (Ratkowsky, 1990) also has an upper asymptote but does not always go through the origin. This three‐parameter function is perhaps also more difficult to handle than the other convex upward models. This is again because each parameter in the model affects more than one curve trait at the same time (shape, upper asymptote and y‐axis intersection). It is only convex with positive values of x and f(x) only for some values of the two parameters. Flather (1996) also tested the rational function and reported that of the convex upward models it fit his data best, better than the power and the exponential functions, which performed second and third best of the models he tested (see Table 5).
| Author | Model fitted | Type of areas | Taxonomic group |
|---|---|---|---|
| Holdridge et al. (1971) | Negative exponential | Sample | Trees |
| Miller & Wiegert (1989) | Negative exponential | Hypothetical sample | Plants |
| Rørslett (1991) | Weibull distribution | Isolate | Plants |
| Williams (1995) | Extreme value function | Isolate | Birds, mammals |
| Legendre & He (1996) | Hill‐function | Sample | Trees, birds |
| Flather (1996) | Monod, negative exponential, asymptotic regression, rational function, Chapman–Richards, Weibull distribution and cumulative beta‐P distribution | Sample | Birds |
| Burbidge et al. (1997) | Extreme value function | Isolate | Mammals |
| Natuhara & Imai (1999) | Logistic | Isolate | Birds |
| Veech (2000) | Extreme value function | Sample | Many |
| Belant & Van Stappen (2002) | Extreme value function | Isolate | Mammals |
| Matter et al. (2002) | Extreme value function | Isolate | Birds, mammals |
Possible sigmoid models
A number of sigmoid mathematical functions have recently been suggested as alternatives to the power and exponential functions (Williams, 1995, 1996; Flather, 1996; Legendre & He, 1996; Lomolino, 2000a). Of the several functions proposed to describe sigmoid growth rates in biology, eight different candidate sigmoid functions are shown in Table 3. The functions treated here are perhaps the most relevant, but other functions (e.g. Ratkowsky, 1983, 1990), may also be used to describe SARs. All sigmoid functions reviewed have upper asymptotes. A basic distinction between different types of sigmoid functions is that some are symmetrical on each side of the inflection point, whereas others are not.
By adding parameters, one may get increased possibilities to manipulate curve shape, inflection point, axis intersection and asymptotes. The effect caused by manipulation of the different parameters is shown in Table 4. The upper asymptote is given by a parameter value that constitutes the total species pool. The value for the upper asymptote can of course be set to one if one wants the model to describe the cumulative expected probability of occurrence of a given species with increasing area (species incidence curve) (see e.g. Schoener & Adler, 1991; Williams, 1995; Ney‐Nifle & Mangel, 1999; Nupp & Swihart, 2000; Bartha & Ittzes, 2001).
The logistic function (Ratkowsky, 1990) is the only function considered here that is symmetrical about the inflection point. This property makes the function less flexible than other sigmoid models, which may limit its ability to fit data well. But the logistic function is still one of the most useful models for fitting sigmoid responses (Ratkowsky, 1990). The logistic function as presented here has three parameters (Table 3). The first represents the upper asymptote. The two other parameters alter the curve shape. The curve has a lower asymptote of zero, and the intersection with the y‐axis depends on all three parameters. Thus it never goes through the origin, which should not be a major problem when fitted to empirical data, but may pose problems if used in a model type approach. Natuhara & Imai (1999) compared the logistic curve with the power and the exponential functions and reported that bird data from urban wood remnants were better fitted by the power function. The logistic function is seldom fitted to species–area plots, but is in common use for multiple regressions where the explanatory power of several parameters in addition to area is assessed (e.g. Schoener & Adler, 1991; Morrison, 1997; Miller & Cale, 2000). Where area or other parameters are evaluated to explain species number, some papers may also present graphs or results where the logistic function is fitted to show species incidence (single‐species probability–area) curves (e.g. Schoener & Adler, 1991; Nupp & Swihart, 2000). Some confusion results when the term ‘logistic curve’ is used interchangeably with ‘sigmoid’. In fact, the logistic function is only one of many models producing sigmoid curves.
The Gompertz model (Ratkowsky, 1990) is related to and behaves somewhat similar to the logistic function. It is also presented with three parameters but it is not symmetrical about the inflection point. It has a lower asymptote of zero and all three parameters affect the intersection with the y‐axis.
The extreme value function (Williams, 1995, 1996) also has three parameters and behaves quite similarly to the logistic and Gompertz models. The extreme value function has one parameter that gives the upper asymptote and two that affect shape. It also has a lower asymptote of zero and thus never goes through the origin.
Williams (1995) used Coleman's (1981) model and showed that if individuals are randomly distributed over area, then the cumulative extreme value function is an appropriate model for the species incidence curve. He showed the appropriate log‐transformation that linearizes the extreme value function. He claimed that this function is superior to the logistic function and that the parameters have biologically meaningful interpretations. Williams also demonstrated that it is an appropriate model even when the assumption of random distribution is severely violated. The extreme value function has later been fitted to empirical species–area data by several authors (Burbidge et al., 1997; Veech, 2000; Belant & Van Stappen, 2002; Matter et al., 2002) (see Table 5).
The Morgan–Mercer–Flodin function (Morgan et al., 1975), with three parameters, has an upper asymptote and goes through the origin of axes. The Morgan–Mercer–Flodin model can be reduced to the familiar Hill (Hill, 1913) and the Michaelis–Menten (Michaelis & Menten, 1913 functions, or to the simplified Hill‐function used by Legendre & He (1996). It is also possible to add more parameters to the Morgan–Mercer–Flodin, e.g. to change the y‐axis intersection.
The Chapman–Richard function (Ratkowsky, 1990) is a modification of the negative exponential function used by Miller & Wiegert (1989). It is yet another three‐parameter model that behaves similarly to the Morgan–Mercer–Flodin, has an upper asymptote and goes through the origin. Flather (1996) also tested this model on his bird survey data and found that it performed well.
The Lomolino function (Lomolino, 2000a) differs from the Morgan–Mercer–Flodin and the Chapman–Richard functions in that the second parameter (b) changes the inflection point. Lomolino called his function a Hill function, but it is not. He only used it on a hypothetical data set.
The cumulative Weibull distribution (Weibull, 1951) is here shown with three parameters. It also has an upper asymptote and goes through the origin of axes. The Weibull is probably the most versatile sigmoid model presented here. It is flexible enough to accommodate most biological growth curves (see e.g. Reid, 1978; Yang et al., 1978), and it has also been shown to fit empirical species–area data well (Flather, 1996). Flather (1996) reported that the Weibull fitted his data better than the other models. He compared nine candidate models (see Table 5), both sigmoid and non‐sigmoid models, by fitting them to data of bird species numbers in different regions of North America. Rørslett (1991) found the Weibull useful for multiple regressions on plant diversity data from lakes.
The cumulative beta‐P distribution behaves similarly to the Weibull distribution, but has four parameters instead of three. The beta‐P distribuion also possesses very desirable computional properties (Mielke & Johnson, 1974), as it is very flexible and has a great ability to fit data sets closely. The only investigator who tried to fit this model to species–area plots was Flather (1996). It performed well, but not as well as the cumulative Weibull distribution. The Weibull is probably just as flexible as the beta‐P distribution and may be preferable because it has one less parameter than the beta‐P.
Which model to choose?
The power function and the exponential function dominate the literature, but there are, as we see, a handful of papers where other species–area models are fitted to empirical data (Table 5). Sigmoid models have been fitted to both sample area data and isolate type data. However, the better fit of sigmoid curves, such as the Weibull distribution, does not necessarily prove sigmoid relationships. The better fit may be just the result of the flexibility of the model.
The sigmoid species–area models could nevertheless be more appropriate for isolates. But one should bear in mind that convex models may be sufficient, e.g. at scales above a possible inflection point or if the inflection point is so close to the lower end of the curve that the convex downward part of the curve becomes very small compared with the rest of the curve. This should be the case if the minimum area requirements of the organisms studied are very small compared with the scale in question.
Convex or sigmoid models?
It is important to distinguish between sample areas (census patches) on one hand and isolates (habitat patches or islands) on the other. One should not expect the same species–area models to be the best for both sample area data sets and isolate data sets, or across scales of communities, habitats, regions or provinces. If one takes known biological patterns, as the effect of minimum area requirements and species pools, into consideration, then the theoretically correct choice for sample curves seems to be a convex upward model with an upper asymptote, and for isolates a sigmoid model with an upper asymptote. These expected shapes do not conflict with the fact that one may find other shapes that fit a given set of data better.
If one wants a function just for theoretical models, then one should look for the simplest possible model that will fit the biological arguments for the shape of the curve. If one can only argue that the curve should be convex upward, then the traditional power function or the exponential function will do. But if an upper asymptote is inferred, then the negative exponential function would be the simplest model to conform to that condition. Such a convex asymptotic model allows one to estimate species pools from sample areas (Colwell & Coddington, 1994). Convex asymptotic function should also be useful for upper parts of isolate curves. For modelling purposes the negative exponential is recommended for isolate data as a result of its simplicity and ease of handling. However it may not fit empirical data as well as the asymptotic regression or the rational function with three parameters.
For isolates, the Weibull distribution should be a very versatile and desirable model. It can be used in a simple form with only two parameters (a(1− exp (−xb))) for modelling situations, and with three parameters (Table 3) it easily fits most empirical data sets requiring a sigmoid shape. If one wants a curve that is symmetrical on each side of the inflection point, then the logistic function is a possibility. If manipulation of inflection points is important, then the Lomolino function may also be considered. The extreme value function should also be considered as a possible sigmoid model.
Adding a location parameter
(1)
(2)These two models should be both relatively simple and flexible candidates for asymptotical, convex shaped species–area curves and sigmoid curves, respectively. Figure 1A shows the negative exponential model with and without a location parameter (c = 3), and Fig. 1B shows the cumulative Weibull distribution with and without a location parameter (d = 3).

(A) Negative exponential function. The dashed line shows the function without and the unbroken line with a location parameter. The curves are 8(1 − exp (−0.5x)) and 8(1 − exp (−0.5(x − 3))), respectively. (B) Weibull distribution. The dashed line shows the function without and the unbroken line with a location parameter. The curves are 8(1 − exp (−0.1x2)) and 8(1− exp (−0.1(x − 3)2)), respectively. For the last curve, values of x < 3 are not shown.
The start point at the x‐axis for this Weibull distribution (2) is actually a curve minimum. In order for the model to make sense as a species–area curve, one must disregard values of x < d. This parameter (d) locates where the minimum of the curve touches the x‐axis. The negative exponential and the Weibull models are closely related, as the Weibull can easily be reduced to the negative exponential. In conclusion, models that allow a start‐point at the x‐axis should be particularly desirable when absolute minimums are needed.
Concluding remarks
Several authors have discussed alternative species–area models, but most only discussed one or a few function types. Flather (1996) is the exception, as his paper reviewed nine candidate models and tested their fit to empirical data. The overwhelming majority of authors only tried to fit either the power function or the exponential function to their data. Different possible models have been reviewed in this paper. The behaviour of model parameters and implications for theoretical discussions or mathematical modeling of more complex SARs was also discussed.
Biology suggests that the SARs represent convex curves in some cases and sigmoid curves in other cases. On the other hand, the choice of model has in the past been based on what has fit the data and less on what should be expected from a biological understanding of the system under study. This highlights shortcomings in our understanding of biological processes and the manner in which these generate SARs. The selection of species–area models should be based on the recognition of biology rather than statistics, by incorporating biological patterns found in nature into our models. Examples of factors that may affect curve shape are species minimum area or resource requirements, competition, predation and species pools. Basic curve fitting will not further our biological understanding. The basis for the two most used models, the power and the exponential functions, is phenomenological, not biological. If we see the need to include biological interpretations into our models, several of the other models reviewed in this paper should be useful or appropriate alternatives both in theoretical modeling and in fitting empirical data.
References
Biosketch
Even Tjørve is Associate Professor at Lillehammer University College. His research interests are in biogeography, landscape ecology and macroecology with emphasis on the effect of spatial patterns on species diversity and abundance. Other interests include bird migration and landscape history. He is currently working with theoretical models on species diversity in multi‐habitat environments, based on species–area curves. He is also currently involved in the writing of the Norwegian Bird Banding Atlas (Norsk ringmerkingsatlas), which will be published in two volumes.
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