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Proceedings of the Royal Society B: Biological Sciences logoLink to Proceedings of the Royal Society B: Biological Sciences
. 2022 May 11;289(1974):20220202. doi: 10.1098/rspb.2022.0202

Increasing temporal variance leads to stable species range limits

John W Benning 1,, Ruth A Hufbauer 2, Christopher Weiss-Lehman 1
PMCID: PMC9091838  PMID: 35538777

Abstract

What prevents populations of a species from adapting to the novel environments outside the species' geographic distribution? Previous models highlighted how gene flow across spatial environmental gradients determines species expansion versus extinction and the location of species range limits. However, space is only one of two axes of environmental variation—environments also vary in time, and we know temporal environmental variation has important consequences for population demography and evolution. We used analytical and individual-based evolutionary models to explore how temporal variation in environmental conditions influences the spread of populations across a spatial environmental gradient. We find that temporal variation greatly alters our predictions for range dynamics compared to temporally static environments. When temporal variance is equal across the landscape, the fate of species (expansion versus extinction) is determined by the interaction between the degree of temporal autocorrelation in environmental fluctuations and the steepness of the spatial environmental gradient. When the magnitude of temporal variance changes across the landscape, stable range limits form where this variance increases maladaptation sufficiently to prevent local persistence. These results illustrate the pivotal influence of temporal variation on the likelihood of populations colonizing novel habitats and the location of species range limits.

Keywords: species range limits, temporal stochasticity, adaptation, geographic distributions, invasion, fluctuating selection

1. Introduction

The limits of species' geographic distributions have long puzzled biologists [1,2]. The causes of distribution, or range, limits fit into two broad categories—either populations have not colonized suitable areas outside their current range margin (a distribution limited by dispersal) or the environment outside that margin is unsuitable, keeping population growth below replacement (a distribution limited by adaptation). The latter case begs the question of why populations do not simply adapt to the novel environmental conditions beyond their range edge. This question is especially perplexing as this exact process—adaptation to novel environments—presumably gave rise to the species' current distribution.

Spatial gradients in the environment clearly play a major role in determining range limits—as the environment changes across space, so do the observed flora and fauna. Climbing a mountain slope, one can readily observe how community composition changes with elevation. But within species, there is ample evidence for populations successfully adapting to all sorts of abiotic and biotic environmental gradients [38]. What causes this adaptive process to cease and a range limit to form? Theory has shed light on the mechanisms underlying the relationship between spatial environmental gradients, local adaptation, and species distributions. For a species occupying a landscape with a spatial gradient (e.g. in soil pH, precipitation, etc.), theory tells us that several mechanisms may constrain adaptation, and subsequently, expansion at the edge of a range. Steep environmental gradients and high gene flow can swamp adaptation at the range edge to create stable range limits ([9], but see [10]). Metapopulation dynamics [11] and biotic interactions [12,13] also can enforce range limits. Recent simulation approaches have highlighted how demography, genetic drift, expansion load and not only the slope but the shape (e.g. linear versus nonlinear) of the environmental gradient influence adaptation, range expansion and the formation of stable range limits [1417]. In all of these theoretical treatments, the spatial environmental gradient, which is modelled as a spatial gradient in phenotypic optima, is key to understanding when populations can expand and when stable range limits form.

However, habitats vary not only in space but also in time. Indeed, in nature, temporal variation in the environment is the rule rather than the exception [1820]. Variation in weather within and between years provides the most obvious illustration of abiotic temporal variation. Biotic environments also fluctuate (stochastically or regularly) through time as populations of predators, mutualists, pathogens and competitors wax and wane. Both theoretical and empirical work demonstrate that temporal variation has important consequences for population demography [2124, reviewed in 25] and evolution [20,2631]. Demographic models have illustrated that a population's extinction risk generally increases as temporal variation increases [23,32], and experimental work has supported these theoretical predictions [24,33]. Viewed through an evolutionary lens, temporal variation can generate fluctuating selection due to phenotypic optima changing through time [34]. These changes in phenotypic optima can lower expected individual fitness via increases in genetic load, i.e. the reduction in fitness due to an individual's deviation from an optimal phenotype [35]. With phenotypic optima changing through time, even a phenotype perfectly adapted to the long-term mean optimum will experience fitness costs due to genetic load [36,37]. In microcosm experiments, temporally fluctuating environments have also been shown to impede adaptation to directional environmental changes, presumably due to relaxed selection during benign periods [30]. However, Holt et al. [38] showed how temporal environmental fluctuations can have positive effects and facilitate adaptation in sink habitats if the sink environment becomes more benign long enough to increase population growth and adaptation. Similarly, positive effects of temporal variation were observed in an experiment exposing diatoms to increasing temperatures [31], where increased population sizes during benign periods resulted in more effective selection. Though our understanding of the prevalence of fluctuating selection in natural populations is still incomplete and plagued by sampling error [39,40], several recent rigorous studies do show strong temporal fluctuations in selection (e.g. [34,41,42]), implying fluctuating phenotypic optima through time.

Because temporal variation can influence key aspects of population demography and evolution, there is reason to expect that it influences species range dynamics, as well [43]. However, most range limit models to date assume temporally constant environments. Yet in nature, the environment will always vary in both space and time, and it is easy to imagine myriad ways that temporal variation might affect the fate of populations spreading across a spatial gradient. If the environment is changing directionally through time (e.g. glacial advance, warming temperatures), theory has shown how the rate of environmental change, the amount of genetic variance and the steepness of an underlying spatial gradient all influence population persistence [44,45]. Recent work by Holt et al. [43] provided some of the first insights into the influence of non-directional temporal variation on range dynamics, showing how temporal variation in competition can modulate the size of an established species' range, and that temporal variation in immigration increases the probability of establishment in sink habitats. However, we lack range limit models exploring the spread of a species across continuous spatial gradients with non-directional temporal variation in environmental conditions. Such temporal variation in the environment could slow adaptation along a spatial gradient via fluctuating selection. Alternatively, positive demographic effects of temporal variation, such as high fecundity in a relatively favourable year, could boost population sizes and increase range expansion and the efficacy of natural selection [38]. Temporal variation will directly affect extinction probabilities via demography [23], and could further influence adaptation by effecting levels of genetic variation [46]. Importantly, just as environmental variation through space can manifest with different patterns (e.g. linear/nonlinear gradients), environments can vary through time in different ways. First, environmental variation can exhibit temporal autocorrelation patterns that are negative (e.g. dry years tend to be followed by wet years and vice versa), positive (e.g. dry years tend to be followed by another dry year) or reflect uncorrelated random noise [47]. Second, temporal variance may not be equal across space. For instance, positive relationships between demographic variability and distance from the centre of a species' range suggest that habitats on the edge of the range may sometimes be more temporally variable than habitats in the core [48,49].

The theoretical and empirical work above indicate that there exists much potential for temporal variation to influence species' range dynamics. In this paper, we use analytical and simulation models to ask how temporal variation in the environment influences population expansion and the formation of range limits across spatial gradients. In our models, temporal variation manifests as temporal stochasticity in phenotypic optima, with optima fluctuating generation to generation around the patch's long-term mean optimum. We explore two geographic modes of temporal variation (figure 1):

  • (1)

    Varying intercept: all points in space experience environmental change equally through time. This would be the case if, say, temperatures or precipitation changed across a landscape by a similar magnitude and direction year to year (e.g. a landscape-wide drought). It manifests as stochasticity in the intercept of the spatial gradient in phenotypic optima, fluctuating around the long-term mean spatial gradient (figure 1b)

  • (2)

    Varying slope: the magnitude of environmental change through time increases away from the landscape centre. This would be the case if, say, there were increased temporal variation in inundation at the edge of a wetland compared to the centre, or increased temporal variation in rainfall as one goes from mesic to arid habitat. It manifests as stochasticity in the slope of the spatial gradient in phenotypic optima, with a constant intercept at the range centre. Thus, the phenotypic optimum displays larger fluctuations around the long-term average with increasing distance from the range centre (figure 1c).

Figure 1.

Figure 1.

Conceptual diagram illustrating how temporal variation is incorporated in the model. (a) Illustration of how spatial environmental variation is modelled in existing range limit models, with a temporally constant spatial gradient in phenotypic optima. In our model, there is intergenerational change in phenotypic optima around the mean optimum at each point in space, according to two ‘geographical modes' of temporal variation. In the ‘varying intercept’ scenario (b), the intercept of the spatial phenotypic optimum gradient fluctuates such that all patches experience the same magnitude and direction of deviation from the mean optimum each generation. In the ‘varying slope’ scenario (c), the slope of the spatial gradient fluctuates stochastically around the mean slope each generation. The gradient is ‘anchored’ at the centre of the landscape, thus, the magnitude of temporal variance increases with distance from the landscape centre. The blue dots (b,c) represent the initial founding population in the simulation, which then spreads (or does not spread) across the landscape. Black arrows indicate the magnitude of temporal variance at that point on the landscape [equal at all points in ‘varying intercept’ and increasing with distance from the landscape centre in ‘varying slope’].

We first derive an analytical model to describe how, under these two different geographic modes, temporal environmental variation imposes genetic load on individuals across a landscape. This model, while simple, helps us build our intuitions regarding the role temporal variation can play in determining individual and population-level fitness. We then explore the influence of temporal environmental variation on range expansion and dynamics using an individual-based, forward-in-time genetic simulation model. In the model, a single population colonizes the centre of a spatial environmental gradient, and we track the demography, evolution and spread of populations across the landscape with the environment varying in space and time. We vary both the steepness of the underlying spatial environmental gradient and the geographical mode of temporal variation as defined above. We also vary the temporal correlation pattern of the environment from negative to positive autocorrelation.

2. Material and methods

(a) . Expected genetic load due to temporal variation

We first present a simple analytical model to describe how our two geographic modes of temporal environmental variation (varying intercept and varying slope) affect expected individual fitness. This is not a dynamical model, but serves to help us build our intuition regarding how temporal variation in the environment may lead to fitness costs for populations at equilibrium. Consider a species distributed across a landscape, with populations occupying discrete patches. The environment varies across space (x), producing a spatial gradient in phenotypic optima with slope b (figure 1). Each population comprises individuals perfectly adapted to the long-term mean phenotypic optimum at that point (patch x) in space. As the environment varies stochastically through time, mismatches arise between individuals' phenotypes and the current phenotypic optimum, even though these individuals are perfectly adapted to the long-term mean phenotypic optimum within their patch. We model this mismatch as genetic load, which is the fitness cost incurred by an individual due to deviation from the phenotypic optimum [35]. As in Lande and Shannon [36], under a model of Gaussian stabilizing selection, we define genetic load for an individual i as

L(zi,θx,t)=s2(ziθx,t)2, 2.1

where θx,t is the phenotypic optimum in patch x at time t, s is the strength of stabilizing selection and zi is the individual's phenotype. In our varying intercept scenario (figure 1b), θx,t = εt + bx, while in our varying slope scenario (figure 1c), θx,t = (εt+b)x. In both cases, b is the slope of the gradient in phenotypic optima, x is the patch position along the gradient and εt is a normally distributed random variable defining the stochastic deviation in either the intercept or slope of the spatial environmental gradient. For now, we assume uncorrelated temporal fluctuations with a fixed variance of τ (i.e. εtN(0,τ)). For an individual perfectly adapted to the expected phenotypic optimum (i.e. zi = bx), genetic load in the varying intercept scenario becomes

L(zi,θx,t)=s2εt2, 2.2

Since εt is normally distributed, the expected genetic load in this scenario can be shown to be

E[L]=sτ2. 2.3

Similarly, genetic load for an individual with zi = bx in the varying slope scenario is

L(zi,θx,t)=s2(εtx)2, 2.4

and the expected genetic load is E[L] = sx2τ/2. Therefore, expected genetic load increases with spatial position (x) in the varying slope scenario, but is constant in space in the varying intercept scenario.

(b) . Effects of temporal variation on range dynamics

The analytical model above describes individuals' expected genetic load due to temporal stochasticity in phenotypic optima in our two landscape scenarios. However, the model does not account for gene flow, density dependence, genetic drift, demographic stochasticity, varying patterns of temporal autocorrelation, or range colonization dynamics. To explore these factors, we used SLiM [50], a forward-in-time population genetic modelling software, to build a complex, individual-based simulation of species range dynamics in a spatially and temporally varying environment. SLiM has recently come to the fore as a flexible, fast and powerful tool to model individual genomes under a wide variety of spatially and temporally explicit evolutionary scenarios. Our simulation model builds most directly on the modelling frameworks of Polechová & Barton [14] and Bridle et al. [16], which explored the role of spatial environmental gradients in range dynamics. We build on the insights from those models by asking how temporal variation in the environment influences population spread and the formation of range limits.

(i) . Genetics and mutation

In our simulations, individuals were diploid and either male or female, with obligate sexual reproduction, and a single chromosome 100 000 bp long. There were two mutation types: (1) neutral mutations and (2) mutations that contributed additively to a quantitative trait (i.e. biallelic quantitative trait loci (QTL) with no dominance). The overall mutation rate was set to 1 × 10−7 mutations per base position on a gamete per generation (electronic supplementary material, table S1) and mutations were 10 times more likely to be neutral than QTLs. QTL effect size was drawn from a standard normal distribution (i.e. N(0, 1)). Recombination rate was set to 1 × 10−5 (probability of a cross-over event between any two adjacent bases per genome per generation).

(ii) . Mating and population dynamics

The simulated landscape comprised a one-dimensional array of 201 patches. This is most analogous to a natural landscape that approximates one dimension, like a river, river corridor, mountain ridge or valley. Each patch hosted a local population subject to density-dependent regulation, with carrying capacity (for a perfectly adapted population) constant across the landscape (here, K = 50). Following Bridle et al. [16], individual fitness was calculated using

Wi=2+2r(1NxK)L, 2.5

where r is the population maximum rate of increase (set to r = 0.8; electronic supplementary material, table S1), Nx is the number of individuals in population x, K is the carrying capacity of each patch (set to K = 50) and L defines the genetic load as defined in the analytical model above (equation (2.1)). Note that L, as defined by equation (2.1), is a function of both an individual's phenotype (zi) and current location along the spatial gradient (θx,t), but from here on we simply write it as L for simplicity. Thus, the first part of equation (2.5) describes standard logistic growth and the second part introduces the fitness cost proportional to the deviation of an individual's phenotypic value from the local optimum (i.e. genetic load) under a model of Gaussian stabilizing selection. The maximum attainable Wi thus decreases with increasing maladaptation, L. For females, Wi defined the mean of a Poisson distribution for the number of offspring that female produced (female fecundity); for males, Wi defined the likelihood of a male mating (Wi corresponded to a male's weight in a weighted draw from the pool of available males in a population). Males could mate multiple times. Any Wi < 0 was set to Wi = 0.00001 (as the mean for a Poisson distribution in SLiM must be greater than zero). After mating occurred within a population, offspring dispersed according to a Poisson dispersal kernel with mean (m) = 0.8. The direction of dispersal (left or right along the gradient) was unbiased and random. Individuals set to disperse beyond the edges of the landscape were instead routed to the most distal patch in that direction. To avoid any potential edge effects, one end condition for our simulations (see below) was if the population of either of the most distal patches reached half the carrying capacity or more. It is important to note that dispersal (m) and carrying capacity (K) are both hard to estimate and highly variable in natural populations; for our main simulations we use values for these parameters near the mode of their distributions as estimated by Polechová & Barton [14]. We explored the sensitivity of our results to varying m and K in electronic supplementary material, S1.

(iii) . Environmental variation

Environmental variation manifested as changes in the optimum phenotype of the quantitative trait across space and time. The slope of the spatial environmental gradient (b) represents the change in phenotypic optima across the landscape (figure 1a). To illustrate how b manifests as a fitness cost of dispersal (i.e. genetic load due to spatial variation in optima), let us assume s = 0.125 (used throughout; electronic supplementary material, table S1). Then the genetic load incurred by dispersal to patch x + 1 for an individual perfectly adapted to patch x is

L=0.125b22. 2.6

Thus if b = 1, a female perfectly adapted to patch x will experience a fitness cost of L = 0.0625 upon migration to patch x + 1, or a fitness decrease of approximately 3.125%.

Temporal environmental variation was implemented as intergenerational stochasticity in the intercept or slope of the spatial gradient in patch phenotypic optima using the same equations presented for the analytical model above. To incorporate temporal autocorrelation, the random deviations in intercept or slope were defined as:

εt=aεt1+dϕt, 2.7

where ε0 = 0, d scales the magnitude of noise Φt ∼ Normal(0, τ) and a represents the degree of temporal autocorrelation. When a = 0 and d = 1, equation (2.7) is equivalent to the distribution of stochastic deviations in phenotypic optima used in the analytical model above. Temporal autocorrelation could be positive (0 < a ≤ 1), negative (−0.99 ≤ a < 0), or uncorrelated (a = 0) temporal stochasticity, with autocorrelation lag equal to one generation (electronic supplementary material, figure S1). (We prevented a from going all the way to −1 because, due to ε0 = 0, this would be identical to a = 1). We set d = (1 − a2)0.5 so that Var(ε) over the full time series used in our simulations was approximately equal for all values of a.

τ differed between the two geographical modes of temporal variation. For the ‘varying intercept’ scenario we set τintercept = 4. This resulted in temporal variation in selection gradients, quantified as σβ ≈ 0.14, being within the range of estimates from natural populations (median σβ = 0.099 in de Villemeruil et al. [42], averaging across birds and mammals; full derivation of σβ presented in electronic supplementary material S2). For the ‘varying slope’ scenario, we set τslope = 0.0025, which resulted in patch conditions mimicking the ‘varying intercept’ scenario at 40 patches away from the landscape centre (figure 2). We also ran simulations with the intercept and slope varying simultaneously; in this ‘varying intercept and slope’ scenario, respective τ values remained the same (τintercept = 4 and τslope = 0.0025).

Figure 2.

Figure 2.

Results of the analytical model estimating expected genetic load across space due to temporal stochasticity in phenotypic optima, for the varying intercept (black; figure 1b) and varying slope (gray; figure 1c) scenarios. Solid lines represent lower magnitude of temporal variance (τintercept = 4 and τslope = 0.0025); dashed lines represent higher magnitude of temporal variance (τintercept = 6 and τslope = 0.005).

(iv) . Simulation process

Burn-in

Each simulation began with a burn-in period of 20 000 generations. At the start of the burn-in, 100 genetically homogeneous, perfectly adapted, founding individuals were initiated in the central patch of the landscape. Mating and dispersal happened as described above, but the landscape was limited to 21 patches wide (10 patches on either side of the founding patch). Carrying capacity in each patch was 100 individuals (thus, landscape-wide K = 2100). There was a modest spatial environmental gradient in optima across these 21 patches (b = 0.5), and modest, uncorrelated temporal fluctuations in the intercept of the spatial gradient in optima [deviations drawn from Normal (0,1)]. The goal of this burn-in period was to generate independent replicates of genetically variable source populations that had evolved in landscapes of similar spatial and temporal heterogeneity for each simulation run, while allowing enough time for the different simulation burnins to converge on similar levels of genetic diversity. During the burn-in, mean heterozygosity of neutral mutations (π) in the central population usually reached an equilibrium by 10 000 generations (electronic supplementary material, figure S2). At generation 20 000, a random subset of 50 individuals was selected from the 21-patch landscape and migrated to the central patch for the ‘founding event’. All other individuals were then removed from the simulation.

Main simulation

After the burn-in period, the main simulation began with the prescribed parameters and the available landscape expanded to 201 patches, with 50 individuals in the founding central patch. Simulations ended after 20 000 generations, or if all populations went extinct, or if at least one of the most peripheral landscape patches reached a population size of at least half the carrying capacity (i.e. the species had filled the entire landscape). We ran 1000 simulations for each of the three temporal variation scenarios (varying intercept, varying slope, varying intercept and slope), with parameter values pulled randomly from uniform distributions: b[0–3], aintercept[−0.99–1], aslope[−0.99–1]. To compare our model with the model of Polechová & Barton [14], we also ran 200 simulations, varying b but with aintercept = 1 and aslope = 1 (i.e. a temporally constant environment) and compared our results to results predicted from that model (electronic supplementary material S3).

3. Results

(a) . Analytical model

As previous work has shown [29,36,38], temporal variation in phenotypic optima results in a genetic load on individuals (figure 2). In our varying intercept scenario, this load is constant across space, while in the varying slope scenario, load increases nonlinearly with distance from the landscape centre. Genetic load increases with the magnitude of temporal variance (τ) and the strength of stabilizing selection (s).

(b) . Simulation model

With a temporally constant environment (i.e. a = 1), expansion was prevented where the spatial gradient slope (b) was greater than approximately 2.5, somewhat steeper than the threshold predicted from the model of Polechová & Barton [14], b ≳ 1.96 (electronic supplementary material S3).

(c) . Varying intercept

When temporal variation in the environment was equal in all patches on the landscape (‘varying intercept’ scenario; figure 1b), a clear relationship emerged between the degree of temporal autocorrelation (a) and the slope of the underlying spatial gradient (b) in determining whether populations spread across the landscape or went extinct (figure 3). Range expansion was favoured when temporal variation was more positively autocorrelated and spatial gradients were shallow. The ultimate fate of the species in each simulation was either eventual extinction or continual expansion; stable range limits did not form, though the rate of range expansion slowed as spatial gradients steepened (light blue points in figure 3). (Here and below we use ‘species' to describe the group of populations on the landscape.)

Figure 3.

Figure 3.

Range dynamics under the ‘varying intercept’ scenario. (a) When temporal variation manifests identically across the landscape, range expansion is favoured when temporal variation ((a), x-axis) is more positively autocorrelated and spatial gradients ((b), y-axis) are shallow. (A temporal autocorrelation of 1 is a temporally static environment, as modelled in previous range limit models.) Each point represents a simulation (N = 1000). No stable range limits formed in this scenario; species either continually expanded or went extinct. All blue points are simulations where species were able to spread, and red/orange points are simulations where species went extinct; points are coloured by how quickly they expanded or went extinct. (bd) Details of one simulation (marked with crosshairs in panel (a)) prior to extinction. Panels track (b) temporal changes in patch phenotypic optima, (c) landscape-wide population abundance and (d) median population genetic variance (for the trait conferring adaptation to the gradient) across generations prior to extinction (grey dashed lines).

As in previous models, steep spatial gradients introduced a strong fitness cost of dispersal, allowing drift to overpower selection and stymie adaptation. Temporal variation exacerbated the negative effects of dispersal by introducing a fitness cost even for individuals well-adapted to their patch's long-term mean optimum; i.e. temporal fluctuations in optima meant that no genotype could completely escape maladaptation across generations. In environments with temporal variation, populations were often able to adapt to the underlying spatial gradient if it was not too steep. However, a large deviation from the mean optimum in a generation had large negative demographic consequences due to individuals being strongly maladapted in most patches. If the following generation then experienced a strongly different optimum, which is more likely as temporal autocorrelation becomes more negative, extinction risk was high (figure 3b,c). Thus, temporal variation introduced an extinction risk due to fluctuating phenotypic optima that had strong effects on mean fitness (e.g. [29,36,38]).

(d) . Varying slope

When the magnitude of temporal variance increased away from the landscape centre (‘varying slope’ scenario), stable range limits formed (figure 4). The exact location of the range limit fluctuated over time as extinction/colonization dynamics played out at the range edge; thus, we define stable range limits as the most distal patches on either side of the founding patch that did not go extinct for at least 950 of the 1000 generations before the end of the simulation (which lasted 20 000 generations). Range limits formed where increasing temporal variance resulted in increasing genetic load (figure 2), causing populations to fail to adapt to the optimum of edge patches because temporal fluctuations in optima caused populations in those patches to often go extinct (or close enough to extinction to strongly undermine genetic variance and adaptive potential).

Figure 4.

Figure 4.

Range dynamics under the ‘varying slope’ scenario. When temporal variance increases away from the landscape centre, stable range limits form where temporal variance is too high to allow further adaptation and persistence. (a) Effects of the spatial gradient slope (x-axis) and degree of temporal autocorrelation (point colour) on a species' ultimate range width (y-axis). (Range width is the number of patches between the species' two stable range limits.) Each point represents a simulation (N = 1000) at the end of 20 000 generations. Open points near the top of the y-axis are simulations where the species reached at least one edge of the landscape. (b) Abundance, (c) temporal variation in optima, (d) genetic variance and (e) mean phenotype of populations in a single simulation (b = 0.17, a = 0.48; marked with crosshairs in panel (a)) after formation of stable range limits (dashed red lines), averaging over the final 1000 generations of the simulation. We define stable range limits as the most distal patches that did not go extinct for at least 950 of the 1000 generations prior to the end of the simulation. (c) The standard deviation of the temporal changes in phenotypic optima, illustrating how temporal variance increases away from the landscape centre. In (e), black points show the mean phenotype and the solid blue line indicates the underlying mean spatial gradient in phenotypic optima.

Range width (distance between range limits) remained relatively constant across a wide range of spatial gradient slopes, but then began to decrease with steeper spatial gradients (figure 4a). The high fitness costs of dispersal across steep gradients (due to maladaptation) combined with the negative fitness effects of temporally fluctuating optima to increase extinction risk more quickly as populations moved away from the centre. This led to narrower range widths than for species spreading across shallower gradients. When temporal variation was positively autocorrelated, range width generally increased. If that positive autocorrelation was particularly strong (a ≈ 1), sometimes the landscape filled completely, especially when the spatial gradient was shallow (open points in figure 4). Because environmental conditions at the landscape core were stable, species usually only went extinct with very steep spatial gradients.

The results presented above for the varying intercept and varying slope scenarios were qualitatively robust to changes in carrying capacity (K) and dispersal (m) (electronic supplementary material S1). In general, larger carrying capacities decrease the parameter space where populations go extinct, likely due to lower demographic stochasticity (e.g. [51]) and more efficient selection (e.g. [52]). By contrast, higher dispersal lowered the maximum spatial gradient slope where expansion was possible, likely because this introduced a higher mean fitness cost of dispersal (e.g. [14]).

When both the slope and the intercept of the spatial gradient varied through time, there was a contraction in the parameter space where range expansion was possible (electronic supplementary material, S4; figures S8, S9, S10). In general, species persistence and range expansion required positive temporal autocorrelation in the gradient intercept (i.e. aintercept >0). Range width was overall smaller and more variable when the spatial gradient intercept varied along with the slope (compare figure 4a and electronic supplementary material, figure S8b).

4. Discussion

Our model results show that, for the parameter space explored here, temporal variation in the environment substantially alters our predictions for range dynamics across spatially variable landscapes. When environmental conditions change from generation to generation similarly across the landscape (‘varying intercept’ scenario), the ultimate fate of species is determined by the interaction between the degree of temporal autocorrelation in environmental fluctuations and the slope of the spatial environmental gradient. As found in previous results [14], species extinction becomes more likely as the slope of the environmental gradient increases. However, positive autocorrelation of temporal variation can allow populations to expand along even very steep gradients. Negative autocorrelation, though, increases demographic fluctuations and increases extinction risk due to fluctuating phenotypic optima resulting in frequent maladaptation and high genetic load. When temporal variation in the environment increases toward the periphery of a landscape (‘varying slope’ scenario), stable range limits form. Populations persist where temporal variance is modest, but where temporal variance becomes too large, the associated genetic load reduces fitness such that population adaptation and persistence are not possible. The ultimate width of the species' range is primarily a function of the underlying spatial environmental gradient. When spatial gradients vary in both intercept and slope through time, range expansion overall becomes less likely. Together these results illustrate how temporal variation in the environment can have a pivotal influence on the likelihood of a species colonizing a new landscape and the location of a taxon's range limit.

When temporal variance has no spatial structure (varying intercept), we can clearly delineate the parameter space where colonizing populations go extinct, versus where they expand across the landscape. When the underlying spatial gradient is shallow, expansion can occur across a wide range of temporal correlation patterns, but increasingly positive autocorrelation is required for expansion as the spatial gradient steepens. Environmental noise in nature seems to largely range from random to positively autocorrelated [47]. Indeed, these simulations indicate that if environmental conditions were strongly negatively autocorrelated through time, colonization and expansion would be very rare. Increasing temporal variability is one predicted (and observed) consequence of contemporary climate change [53], and our simulations suggest that this increased variability could reduce the probability that populations will be able to successfully track climatic changes via shifting spatial distributions. For example, the upslope colonization process of an alpine plant due to warming could be stymied if temporal variation is augmented by climate change. Our model suggests that increased temporal environmental variation due to climate change could further reduce fitness of edge populations, potentially hampering their ability to track or adapt to changing mean conditions. Furthermore, if a species' current range limit is due in part to increased temporal environmental variation, then models forecasting future distributions built solely using the mean, and not variance, of predicted climate will likely be inadequate.

The biogeographic fact that all species have limited distributions is often at odds with the ability of evolutionary range limit models to produce stable range limits. For instance, when Barton [10] adjusted Kirkpatrick and Barton's foundational work [9] to allow genetic variance to evolve, range expansion was continuous and limits failed to form. Polechova & Barton [14] provided a solution to this conundrum by incorporating genetic drift and demographic stochasticity in their models but still found that stable limits only formed with nonlinear spatial gradients (see also [15,16]). Similarly, in our model there are no stable range limits when there is no spatial trend in temporal variance (i.e. varying intercept scenario). However, we do see stable range limits form when there is a spatial gradient in the magnitude of temporal variance—i.e. temporal variance, and the resulting genetic load, increase nonlinearly with distance from the centre of the landscape (varying slope scenario)—even across linear spatial gradients. When viewed collectively, our results and those of Polechová & Barton [14], Polechová [15], and Bridle et al. [16] highlight how nonlinear spatio-temporal trends may be key in generating stable range limits. This work indicates that we should perhaps expect qualitatively different patterns in how environments change through time and space at the edge versus the core of a species' range.

Our results suggest that there is a critical threshold at which temporal variation in the environment can stop range expansion and enforce a stable range limit. Do we find evidence for such a pattern in nature? The idea that environments at the edge of species' ranges tend to be more temporally variable has been assumed more often than empirically shown, but some demographic studies do suggest range edge habitats to be more temporally variable than range core habitats [48,49,5457]. Beyond indirect inference of temporal environmental variation via demographic data, there are surprisingly few direct measurements of temporal environmental variability across species ranges. One exception is Eckhart et al. [58], who showed that for the California annual plant Clarkia xantiana ssp. xantiana, interannual variability in precipitation increased toward the subspecies' eastern range margin. Our model supports the notion that increased variability in precipitation could contribute to the stable range limit observed in this species.

These results lead to several testable predictions. First, does temporal variation in the environment increase toward species range edges? For climatic variables this would be fairly straightforward to test, as we have excellent data for both species distributions and long-term weather. With such data, we could also ask whether, looking across species distributions, we see a positive relationship between the steepness of putatively important spatial gradients across a species range and the temporal autocorrelation in that environmental variable. Figure 3 would suggest this relationship—colonization across steep spatial gradients should only be possible in fairly stable environments (i.e. environments with positive temporal correlation). For example, we might expect to observe that species with populations distributed across steep altitudinal gradients experience more positively correlated temporal variation than species spread across more shallow spatial gradients (e.g. a primarily latitudinal rather than altitudinal gradient). Extensions of our model incorporating other ecological and evolutionary processes would help refine our predictions for range dynamics in nature (electronic supplementary material, Model extensions).

Species range limits are as ubiquitous as they are puzzling. What prevents adaptation from allowing species distributions to continually grow by ‘accretion like the rings of a tree’ [59]? Recent theory highlights the importance of genetic drift and nonlinear spatial gradients in controlling range dynamics and the location of stable range limits [1416]. Here we showed how temporal variation in the environment, an ever-present feature of natural systems, strongly contributes to determining whether a population will expand into novel habitat or go extinct, and can readily enforce stable range limits. By expanding range dynamics models to the temporal dimension, we gain more realistic, comprehensive insight into the mechanisms and processes underlying biogeographic patterns, insights of great relevance to invasion biology, the limits to adaptation, and the fate of populations with environmental change.

Supplementary Material

Acknowledgements

We thank three anonymous reviewers for their insightful comments that greatly improved the manuscript.

Data accessibility

All SLiM and R code, simulation parameters and the simulation results needed to reproduce the figures in this manuscript are archived on FigShare (https://doi.org/10.6084/m9.figshare.c.5552028).

The data are provided in the electronic supplementary material [60].

Authors' contributions

J.W.B.: conceptualization, data curation, formal analysis, funding acquisition, investigation, methodology, project administration, visualization, writing—original draft, writing—review and editing; R.A.H.: conceptualization, methodology, supervision, writing—review and editing; C.W.-L.: conceptualization, formal analysis, investigation, methodology, supervision, writing—review and editing.

All authors gave final approval for publication and agreed to be held accountable for the work performed therein.

Conflict of interest declaration

We declare we have no competing interests.

Funding

This work was supported by grants from the National Science Foundation (DBI-2010892 to J.W.B., EPS-2019528 to C.W.-L. and DEB-2121980 to R.A.H.). Any opinions, findings and conclusions expressed in this material are those of the authors and do not necessarily reflect the views of the National Science Foundation.

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Associated Data

This section collects any data citations, data availability statements, or supplementary materials included in this article.

Supplementary Materials

Data Availability Statement

All SLiM and R code, simulation parameters and the simulation results needed to reproduce the figures in this manuscript are archived on FigShare (https://doi.org/10.6084/m9.figshare.c.5552028).

The data are provided in the electronic supplementary material [60].


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