Tipping points in open systems: bifurcation, noise-induced and rate-dependent examples in the climate system

Peter Ashwin , Sebastian Wieczorek , Renato Vitolo , Peter Cox


Tipping points associated with bifurcations (B-tipping) or induced by noise (N-tipping) are recognized mechanisms that may potentially lead to sudden climate change. We focus here on a novel class of tipping points, where a sufficiently rapid change to an input or parameter of a system may cause the system to ‘tip’ or move away from a branch of attractors. Such rate-dependent tipping, or R-tipping, need not be associated with either bifurcations or noise. We present an example of all three types of tipping in a simple global energy balance model of the climate system, illustrating the possibility of dangerous rates of change even in the absence of noise and of bifurcations in the underlying quasi-static system.

1. Tipping points: not just bifurcations

In the last few years, the idea of ‘tipping points’ has caught the imagination in climate science with the possibility, also indicated by both palaeoclimate data and global climate models, that the climate system may abruptly ‘tip’ from one regime to another in a comparatively short time.

This recent interest in tipping points is related to a long-standing question in climate science: to understand whether climate fluctuations and transitions between different ‘states’ are due to external causes (such as variations in the insolation or orbital parameters of the Earth) or to internal mechanisms (such as oceanic and atmospheric feedbacks acting on different time scales). A famous example is the Milankovich theory, according to which these transitions are forced by an external cause, namely the periodic variations in the Earth's orbital parameters [1]. Remarkably, the evidence in favour of the Milankovich theory still remains controversial [2].

Hasselmann [3] was one of the first to tackle this question through simple climate models obtained as stochastically perturbed dynamical systems. He argued that the climate system can be conceptually divided into a fast component (the ‘weather’, essentially corresponding to the evolution of the atmosphere) and a slow component (the ‘climate’, i.e. the ocean, cryosphere, land vegetation, etc.). The ‘weather’ would act as an essentially random forcing exciting the response of the slow ‘climate’. In this way, short-time-scale phenomena, modelled as stochastic perturbations, can be thought of as driving long-term climate variations. This is what we refer to as noise-induced tipping.

Sutera [4] studied noise-induced tipping in a simple global energy balance model previously derived by Fraedrich [5]. Sutera's results indicate a characteristic time of 105 year for the random transitions between the ‘warm’ and the ‘cold’ climate states, which matches well with the observed average value. One shortcoming is that this analysis leaves open the question as to the periodicity of such transitions indicated by the power spectral analysis [6, fig. 7].

There is a considerable literature on noise-induced escape from attractors in stochastic models [7]. These have successfully been used for modelling changes in climate phenomena [8], although authors do not always use the word ‘tipping’ and other aspects have been examined. For example, Kondepudi et al. [9] considered the combined effect of noise and parameter changes on the related problem of ‘attractor selection’ in a noisy system.

More recently, bifurcation-driven tipping points or dynamic bifurcations [10] have been suggested as an important mechanism by which sudden changes in the behaviour of a system may come about. For example, Lenton et al. [11,12] conceptualized this as an open system Embedded Image 1.1 where λ(t) is in general a time-varying input. In the case that λ is constant, we refer to (1.1) as the parametrized system with parameter λ, and to its stable solution as the quasi-static attractor. If λ(t) passes through a bifurcation point of the parametrized system where a quasi-static attractor (such as an equilibrium point Embedded Image) loses stability, it is intuitively clear that a system may ‘tip’ directly as a result of varying that parameter, though in certain circumstances the effect may be delayed because of well-documented slow passage through bifurcation effects [13]. Related to this, Dakos et al. [14] have proposed that tipping points are recognizable and to some extent predictable. They propose a method to de-trend signals and then, examining the correlation of fluctuations in the de-trended signal, they find a signature of bifurcation-induced tipping points. These papers have concentrated on systems where equilibrium solutions for the parametrized system lose stability, although recent work of Kuehn [15] considered tipping effects in general two time-scale systems as occasions when there is a bifurcation of the fast dynamics.

The explanation of climate tipping as a phenomenon purely induced by bifurcations has been called into question. For example, Ditlevsen & Johnsen [16] suggested that the predictive techniques to forecast a forthcoming tipping point [14] are not always reliable. Indeed, noise alone can drive a system to tipping without any bifurcation. Nonetheless, it seems that the ideas of bifurcation-induced tipping can give practically useful predictions; for example, in detecting potential ecosystem population collapses [17].

In their review paper, Thompson & Sieber [18] discussed bifurcation- and noise-induced mechanisms for tipping. They examined stochastically forced systems Embedded Image 1.2 where W represents a Brownian motion. Using generic bifurcation theory, they distinguished between safe bifurcations (where an attracting state loses stability but is replaced by another ‘nearby’ attractor), explosive bifurcations (where the attractor dynamics explores more of phase space but still returns to near the old attractor) and dangerous bifurcations (where the attractor dynamics after bifurcation are unrelated to what has gone before). Thompson & Sieber [19] clarified that a time-series analysis of a bifurcation-induced tipping point near a quasi-static equilibrium (QSE) relies on a separation of time scales Embedded Image 1.3 where κdrift is the average drift rate of parameters, κcrit is the decay rate for the slowest decaying mode of the QSE and κstab are the remaining (faster decaying) modes. However, it is not easy to define κdrift in general (especially in a coordinate-independent manner) and there is no a priori reason for inequality (1.3) to hold for a given system.

Rate-dependent tipping has not previously been discussed in detail, but it has been identified in Wieczorek et al. [20] as an important tipping mechanism that cannot be explained by previously proposed mechanisms (i.e. noise or bifurcations of a quasi-static attractor). This paper aims to better understand the phenomenon of rate-dependent tipping by introducing a linear model with a tipping radius and discussing three basic examples where this type of tipping appears.

We suggest that tipping effects in open systems can be usefully split into three categories:

  • — ‘B-tipping’, in which the output from an open system changes abruptly or qualitatively owing to a bifurcation of a quasi-static attractor.

  • — ‘N-tipping’, in which noisy fluctuations result in the system departing from a neighbourhood of a quasi-static attractor.

  • — ‘R-tipping’, in which the system fails to track a continuously changing quasi-static attractor.

We demonstrate that each mechanism on its own can produce a tipping response. Furthermore, any open system may exhibit tipping phenomena that result from a combination of several of the above.

This paper is organized as follows: in the remainder of this section, we discuss a setting for open systems, allowing discussion of the three types of tipping phenomena. In §2, we formulate a criterion for R-tipping. In §3, we discuss three illustrative low-dimensional examples of R-tipping; two related to bifurcation normal forms and one for a slow–fast system. Section 4 gives an illustrative example of all three types of tipping for an energy-balance model of the global climate for different parameter regimes. Section 5 concludes with a discussion and some open questions.

(a) Towards a general theory of tipping in open systems

Dynamical systems theory has developed a wide-ranging corpus of results concentrated on the behaviour of autonomous finite-dimensional deterministic systems—often called closed systems, because their future time trajectories depend only on the current state of the system. If the systems have inputs that can change the fate of system trajectories then we say the system is open. Real-world systems are never closed except to some degree of approximation, and a range of methods have been developed to cope with the fact that they are open: (i) one can view external perturbations as time variation of parameters that would be fixed for a closed system; (ii) there are various theoretical approaches to stochasticity in systems, either intrinsic or external; and (iii) control theory allows one to design inputs to control a system's outputs in a desired way, given (possibly imperfect) knowledge of the system.

In figure 1a, we illustrate an arbitrary high-dimensional system where we have identified a low-dimensional subsystem that we wish to check for ‘tipping effects’. We do this by analysing the response of an open system (1.1) in figure 1b to possible time-varying inputs λ(t). Figure 2 shows some possible candidates for the input λ(t); we are interested in classifying those inputs that lead to a sudden change in x. This ‘tipping’ may depend on details of the noise (N-tipping), may involve passing through a critical value of λ(t) corresponding to a bifurcation (B-tipping) of the parametrized subsystem or may depend on the rate of change of λ(t) along some path in parameter space (R-tipping).

Figure 1.

The system (x,y) in (a) represents a (high dimensional) open system with inputs ξ(t). We identify a low-dimensional but nonlinear subsystem x forced by some ‘observables’ λ(y) from the high-dimensional system. The behaviour of x in (a) can be partially understood by examining the open subsystem (b) for a suitable class of temporal forcing λ(t).

Figure 2.

Candidate inputs λ(t) in the subsystem (1.1). These may include noise- and signal-like components as in (a), or purely deterministic smooth inputs/parameter variations as in (b,c). Tipping responses in the subsystem may occur in response to noise fluctuations (N-tipping), to passing through a bifurcation point for the parametrized subsystem λ=λ0 (B-tipping) or as a result of too rapid variation (R-tipping).

2. R-tipping: a linear model

We use a simple model to explore R-tipping and to give sufficient conditions such that R-tipping does/does not occur. Suppose that the system (1.1) for Embedded Image and parameter λ has a QSE Embedded Image with a tipping radius R>0. For some initial x0 with Embedded Image, we assume that the evolution of x with time is given by Embedded Image 2.1 where M is a fixed stable linear operator (i.e. Embedded Image as Embedded Image). More generally, we consider a time-varying parameter, λ(t), that represents the input to the subsystem. If Embedded Image then we say that x(t) tracks (or adiabatically follows) the QSE Embedded Image. If there is a t0 such that Embedded Image then we say the solution tips (adiabatic approximation fails) at t0 and regard the model as unphysical beyond this point in time. The tipping radius may be related to the basin of attraction boundary for the nonlinear problem (1.1), as is the case in §3a,b, but it need not be, as is the case in §3c and in Wieczorek et al. [20]. System (2.1) shows only R-tipping—because M is fixed there is no bifurcation in the system and no noise is present. Clearly, the model can be generalized to include M and R that vary with λ(t), and/or nonlinear terms. Equation (2.1) can be solved with initial condition x(0)=x0 to give Embedded Image If we assume that the solution is modelled by the linear system near the QSE for an arbitrarily long past and set u=ts, then the dependence on initial value decays to give Embedded Image 2.2 Assuming that M is invertible and exponentially stable (more precisely, we assume that Embedded Image as Embedded Image for k=1,2) and that the rate of motion of the QSE and parameter are bounded (more precisely, the derivatives Embedded Image and dlλ/dtl for l=1,2 are bounded in time) then (2.2) can be integrated by parts to give Embedded Image and so Embedded Image 2.3 Integrating again by parts gives Embedded Image The linear instantaneous lag is Embedded Image 2.4 If we define the drift of the QSE to be the rate of change Embedded Image 2.5 then the linear instantaneous lag is Embedded Image 2.6 The error to the linear instantaneous lag is Embedded Image which includes historical information. This can also be expressed as Embedded Image To summarize, the solution of (2.1) follows the QSE Embedded Image with a linear instantaneous lag term L(t) and a history-dependent term E(t).

(a) A criterion for R-tipping with steady drift

If Embedded Image is constant in time then we say the system has steady drift and (2.3) simplifies to Embedded Image. In other words, one can verify that E(t)=0 and that Embedded Image 2.7 On writing the matrix norm Embedded Image, we note that for any r≠0 and invertible M we have Embedded Image We can avoid R-tipping if Embedded Image, and hence a sufficient condition on the rate of parameter variation to avoid R-tipping is that Embedded Image 2.8 while a sufficient condition for R-tipping to occur in this model is that Embedded Image In the intermediate case, the path of parameter variation will determine whether or not there is any R-tipping.

(b) General criteria for R-tipping

In the more general case where r(t) varies, we can use (2.3) to note that Embedded Image If we define Embedded Image then, noting that Embedded Image, we can guarantee that (2.1) avoids R-tipping up to time t if Embedded Image 2.9 Conversely, there will be an R-tipping by time t if Embedded Image 2.10

One can define a natural time scale for the motion of the QSE as Embedded Image note that, in general, combinations of Embedded Image and dλ/dt do not give time scales in units per second. For an R-tipping to occur, this natural time scale may be comparable to the slowest time scale (e.g. the reciprocal of the leading eigenvalue of M) of the parametrized system. The three examples in §3 have Embedded Image and R≈1 so we expect R-tipping when |dλ/dt|≈∥M∥. However, if Embedded Image, then clearly we can have R-tipping even when |dλ/dt|≈ϵM∥.

It is possible to think of more general tipping problems by analogy with the ‘linear system and tipping radius’ model discussed here. For example, for an open nonlinear system, we consider an ‘effective tipping radius’ that corresponds to how far the linearized system needs to be from a branch of QSE to ensure that the nonlinear system tips. There is however no exact analogy possible—the effective tipping radius may depend on the shape of the local basin of attraction, the nonlinearities present and the exact path taken in parameter space.

3. R-tipping: model examples

We give three illustrative examples of R-tipping. The first two are based on normal forms for the two basic co-dimension one bifurcations that are generic for dissipative systems: the saddle–node and the Hopf bifurcation. The third is an example that uses a fast–slow system to show that R-tipping can occur even in cases where there is a single attractor that is globally asymptotically stable.

(a) Saddle–node normal form with steady drift

We consider the example system for Embedded Image with parameter Embedded Image and drift r, Embedded Image 3.1 and Embedded Image 3.2 with fixed μ>0. In the (x,λ) phase plane of (3.1)–(3.2), there are two dx/dt=0 isoclines given by Embedded Image and Embedded Image that correspond to two QSE: a stable node and a saddle, respectively, for (3.1). Furthermore, if μ>r there are two invariant lines, one attracting Embedded Image and one repelling Embedded Image both with a constant slope dλ/dx=−1 (figure 3). The stability manifests itself as an exponential decay (growth) of small perturbations about A(μ,r) (B(μ,r)).

Figure 3.

Phase portraits of (3.1) for (a) 0<r<μ, (b) r=μ, and (c) r>μ, including the two quasi-static equilibria, Embedded Image and Embedded Image, and the two invariant lines, A and B.

If 0<r<μ then B(μ,r) defines a tipping threshold. Initial conditions below B(μ,r) converge to A(μ,r), whereas initial conditions above B(μ,r) give rise to solutions Embedded Image as Embedded Image. If r=μ then A(μ,r) and B(μ,r) coalesce into a neutrally stable invariant line AB (figure 3b) that disappears for r>μ (figure 3c). Hence, for r>μ there is no tipping threshold, meaning that trajectories for all initial conditions become unbounded as Embedded Image.

Let us assume that the system is at (x0,λ0) at time t=0. If the initial condition (x0,λ0) lies between λ=−x and Embedded Image, then the critical rate rc is the value of r at which the r-dependent tipping threshold B(μ,r) crosses (x0,λ0). If the initial condition lies on or below the line λ=−x then the critical rate rc is the value of r at which B(μ,r) and A(μ,r) meet and disappear. This gives a precise value for the critical rate as the following function of initial conditions: Embedded Image 3.3

We can approximate this result using the simple linear model (2.1) with the linearization at the QSE as Embedded Image so that Embedded Image. Clearly, the linear model with Embedded Image given by Embedded Image (basin boundary for Embedded Image) overestimates rc because the linear attraction weakens on moving away from the stable QSE in the nonlinear problem. This can be overcome by choosing an effective tipping radius Rc. Comparing with (2.8), the system avoids tipping if Embedded Image which, for rc=μ, suggests an effective tipping radius Embedded Image. Finally, owing to steady drift, this problem can be reduced to a saddle–node bifurcation at r=μ in a co-moving coordinate system y=x+λ.

(b) A subcritical Hopf normal form

As a second example, we consider Embedded Image 3.4 where Embedded Image. For the subcritical Hopf normal form with frequency ω, we choose Embedded Image Note that the system (3.4) has only one QSE at Embedded Image. Two cases of R-tipping that we consider are with steady drift (these can be reduced to a bifurcation problem in another coordinate system) and with unsteady drift (where there is no straightforward simplification to a bifurcation problem).

(i) Hopf normal form with steady drift

Consider (3.4) with a uniform drift of the QSE along the real axis, at a rate r (which must be real): dλ/dt=r. There is a critical rate rc at which the system moves away from the stable QSE. We can find this rc analytically by changing to the co-moving system for w=zλ, Embedded Image 3.5 where a stable equilibrium represents the ability to track the QSE in the original system. Setting w=|w| eiθ and rewriting equation (3.5) in terms of d|w|/dt and dθ/dt gives an equilibrium at (|we|,θe) that satisfies Embedded Image 3.6 In the (r,ω) parameter plane, there is a saddle–node bifurcation curve (S in figure 4a) whose different branches are given by equation (3.6) with Embedded Image 3.7 and join at cusp points at (r,ω)=(±(2/3)3/2,±(1/3)1/2) (not marked in figure 4a). Linearizing about the stable equilibrium (|we|,θe) reveals that the characteristic polynomial Embedded Image has a pair of pure imaginary roots, indicating a Hopf bifurcation when |we|2=1/2 and ω2>1/4. In the (r,ω) parameter plane, (disjoint) Hopf bifurcation curves (H) originate from Bogdanov–Takens bifurcation points (BT) at (r,ω)=(±1/2,±1/2), and are given by Embedded Image 3.8 which follows from equation (3.6) with |we|2=1/2. At BT, saddle–node bifurcation changes from super (solid) to subcritical (dashed). It turns out that the stable equilibrium for (3.5), indicating the ability to track the QSE in the original system, disappears in a supercritical saddle–node bifurcation when ω2<1/4 and becomes unstable in a subcritical Hopf bifurcation when ω2>1/4. Hence, for initial conditions within the basin boundary of this equilibrium, the critical rate is given by Embedded Image 3.9

Figure 4.

(a) Solid curves in a two-parameter tipping diagram for (3.4) with steady drift indicate the critical rate rc(ω). The stable equilibrium for the co-moving system (3.5), or the ability to track the QSE in the original system (3.4), (b) disappears in a saddle–node bifurcation or (c) destabilizes in a subcritical Hopf bifurcation when r=rc(ω).

Again, we can approximate this result using the simple linear model (2.1) with the linearization at the QSE as M=(−1,5;−5,−1) so that ∥M−1∥=∥M−1=0.1961. Clearly, the linear model with a tipping radius R=1 given by the unstable periodic orbit (basin boundary for Embedded Image) does not account for nonlinear attraction away from the QSE and for the spiralling shape of trajectories when ω≠0. Therefore, we choose an effective tipping radius Rc. Comparing with (2.8), the system avoids tipping if Embedded Image which suggests an ω-dependent effective tipping radius Rc(ω)=rc(ω)/5.099.

R-tipping that reduces to a bifurcation problem in a co-moving system should not be confused with B-tipping: observe that the bifurcation parameter r does not vary in time, and it is ‘the ability to track the QSE’, rather than the QSE itself, that bifurcates.

(ii) Hopf normal form with unsteady drift

We now consider (3.4) where we include a smooth shift of QSE between asymptotically steady positions at z=0 to z=Δ, according to Embedded Image 3.10 where ρ>0 parametrizes the maximum rate of the shift, Δ>0 is the amplitude of the shift and t0 is the time when the rate of change is largest. Integrating (3.10) gives Embedded Image 3.11 which implies the following parameter dependence on time: Embedded Image Near t=t0 this describes a smooth shift between the location of an asymptotically stable equilibrium from z=0 to z=Δ, and the maximum rate of the shift is Δ2ρ/4 at t=t0. Observe that there is no change in stability or basin size of the QSE as t changes. Figure 5 shows typical trajectories starting at an arbitrary initial condition within the basin of attraction using fixed Δ and two values of ρ. As shown in the diagram, there is a critical value ρc such that for ρ<ρc the system can track the QSE while for ρ>ρc a tipping occurs near t=t0.

Figure 5.

R-tipping for (3.5)–(3.10) for Δ=8 showing time evolution for (a) ρ=4.76 and (bρ=4.8 (recall that ρ scales the maximum rate of change) from an initial condition (x,y,λ)=(0.4,0.5,0.0001). For ρ>ρc=4.78, we find that system trajectories no longer follow the stable QSE (shown by the dashed line) as they meet its basin boundary.

J. Sieber (2010, personal observation) has pointed out that this case may still be quantifiable by numerical approximation of the ρc that gives a heteroclinic connection from an (initial) saddle equilibrium at (z,λ)=(0,0) to a saddle periodic orbit at (|z−Δ|,λ)=(1,Δ) for the extended system (3.4) and (3.10). Such a connection indicates ρc for which the (initial) saddle equilibrium moves away from the basin boundary of the stable equilibrium at (z,λ)=(Δ,Δ).

(c) A fast–slow system with R-tipping

A particularly interesting case of R-tipping can occur in slow–fast systems that have a (unique, globally stable) QSE near a locally folded critical (slow) manifold, of which the recently studied compost-bomb instability is a representative [20,21]. Here, we consider a simple example Embedded Image 3.12 and Embedded Image 3.13 with odd N, fast variable Embedded Image, slow variable Embedded Image, and small parameter 0<ϵ≪1. A unique equilibrium for (3.12)–(3.13)Embedded Image, is asymptotically stable for any fixed value of λ, and globally asymptotically stable if N≥5. The slow dynamics is approximated by the one-dimensional critical (slow) manifold, Embedded Image, that has a fold, Embedded Image, tangent to the fast x1 direction. If N≥5, the fold defines a tipping threshold that is not associated with any basin boundary. Here, S(λ) is partitioned into the attracting part, Sa(λ) for Embedded Image, fold L(λ) for Embedded Image, and repelling part, Sr(λ) for Embedded Image.

(i) The slow–fast system with steady drift

Consider (3.12)–(3.13) with a uniform drift of the QSE, Embedded Image, in the negative x2 direction at a constant rate Embedded Image 3.14 so that λ becomes the second slow variable. There is a critical rate, rc, at which (3.12)–(3.14) is destabilized, meaning that trajectories diverge away from the QSE for r>rc. We can find this critical rate in the singular limit, Embedded Image, by setting ϵ=0 in (3.12), differentiating the resulting algebraic equation with respect to t, and studying the projected reduced system [22], Embedded Image 3.15 and Embedded Image 3.16 that approximates the slow dynamics for (3.12)–(3.14) on the two-dimensional critical manifold, Embedded Image (grey surface in figure 6). Although (3.15)–(3.16) is typically singular at the one-dimensional fold, Embedded Image, its phase portrait can be constructed by rescaling time Embedded Image

Figure 6.

R-tipping in slow–fast systems with a unique QSE, Embedded Image, and (grey surface) locally folded critical (slow) manifold, S=SaLSr, for (a) the steady drift problem (3.12)–(3.14) and (b) the unsteady drift problem (3.12)–(3.13) and (3.20), where ϵ=0.01 and N=1. In (a), equation (3.19) gives Embedded Image and shown are trajectories for r=0.4<rc and r=0.6>rc. In (b), equation (3.23) gives ρc≈0.99 for the initial condition at the origin (black dot) and shown are trajectories for ρ=0.7<ρc and ρ=1>ρc.

producing the phase portrait for the desingularized system [23] Embedded Image 3.17 and Embedded Image 3.18 and then reversing the direction of time on the repelling part of the critical manifold, Sr. In this way, we find that for Embedded Image trajectories for all initial conditions within Sa converge to a stable invariant line that is defined by a constant x1 satisfying Embedded Image, meaning that trajectories remain close to the QSE, Embedded Image, for all time [r<rc] in figure 6a. However, for Embedded Image, trajectories for all initial conditions within Sa reach the fold, L, where they ‘slip off’ the critical manifold and diverge away from the QSE in the fast x1 direction [r>rc] in figure 6a. Hence, system (3.12)–(3.14) exhibits R-tipping and, for Embedded Image, the critical rate is Embedded Image 3.19

(ii) The slow–fast system with unsteady drift

We now consider (3.12)–(3.13) with a non-uniform drift Embedded Image 3.20 that is a logarithmic growth, Embedded Image, where we assume ρ>0. Again, there is a critical rate, ρc, at which system (3.12)–(3.13) and (3.20) is destabilized. The key difference from the steady drift problem is that ρc depends on the initial condition within Sa. This is because the desingularized system Embedded Image 3.21 and Embedded Image 3.22 has a saddle equilibrium for all ρ>0, corresponding to a folded saddle singularity [24,25], Embedded Image for the projected reduced system. One can use the theory developed in Wieczorek et al. [20], §4 to approximate the critical value, ρc. Given F, the eigenvector Embedded Image corresponding to the stable eigendirection of the saddle F for (3.21)–(3.22), an initial condition (x1,0,λ0) within Sa, and as far as Embedded Image, the critical rate can be calculated using Wieczorek et al. [20], eqn (4.12) to give Embedded Image 3.23 where Embedded Image, Embedded Image. Below the critical rate, the trajectory misses the fold, L, and approaches the QSE, Embedded Image, as time tends to infinity [ρ<ρc] in figure 6b. Above the critical rate, the trajectory reaches L and diverges from the QSE in the fast x1 direction [ρ>ρc] in figure 6b. Note that, in this example, the critical rate of parameter variation is of the same order as the slow dynamics—only when the parameter variation is very slow with respect to the slow variable and there are three time scales is tracking guaranteed. In this sense, the rate-dependent tipping occurs when the slow and very slow time scales are no longer separable.

4. B-, N- and R-tipping examples in a simple climate model

We present a simple climate model that independently shows, under differing circumstances, all three types of tipping. In its deterministic version, this is a ‘zero-dimensional’ global energy balance model originally introduced by Fraedrich [5], Embedded Image 4.1 The state variable T represents an average surface temperature of an ocean on a spherical planet subject to radiative heating. Equation (4.1) is a deterministic energy conservation law where the constant c represents the thermal capacity of a well-mixed ocean layer of depth 30 m covering 70.8 per cent of the Earth's surface. The incoming solar radiation R↓ and outgoing radiation R↑ are modelled as Embedded Image Here I0 is the solar constant and the parameter μ allows for variations in the planetary orbit, or in the solar constant. An ice–albedo feedback is introduced to link variations in temperature with changes of ice and thus of albedo αp: Fraedrich [5] used a quadratic relation Embedded Image 4.2 where the parameters a2>1 and b2 control the albedo magnitude and slope of the albedo–temperature relation. The outgoing radiation term is obtained by the Stefan–Boltzmann law, where eSA is the effective emissivity and σ is the Stefan–Boltzmann constant. With these choices (4.1) is written as [5], eqn 4.1 Embedded Image 4.3 Table 1 shows the values of constants and parameters for the system at equilibrium. Sutera [4] reformulated Fraedrich's model to incorporate stochastic forcing: Embedded Image 4.4 with f(T) as in (4.3), where dW is a normalized Wiener (white noise) process such that (dW)2 has dimension of time t, ν has dimension of 1/t and the variance of Embedded Image per unit time is ν.

View this table:
Table 1.

Values of the constants and parameters for equation (4.3).

For μ larger than a critical value 0<μc<1, the deterministic system (4.3) has two equilibria, T+ (stable) and T (unstable). A saddle–node bifurcation takes place at some μ=μc with 0<μc<1, where the two equilibria T± merge and disappear. Sutera [4] studied N-tipping in the stochastically forced system (4.4) for μ>μc, as a function of the distance μμc from the bifurcation value. Namely, they computed the exit time such that the process jumps over the ‘potential barrier’ T and falls irreversibly to ‘ice-covered Earth’.

We illustrate in figure 7 three situations where the Sutera–Fraedrich model exhibits ‘pure’ B-, N- and R-tipping independently; parameter values are detailed in table 2. In table 2, (ab) shows an example of R-tipping, (c) of N-tipping and (d) of B-tipping. For case (ab), we evolve the dimensionless parameter λ according to the ODE dλ/dt=ρλ(1−λ) and set Embedded Image—for this figure, we use initial values λ=106 and T=290 K. The value of a2 is calculated to ensure that Embedded Image is held constant for the parameter groups defined in (4.3). The constant ρ can be thought of as simply scaling the rate of passage from the initial to the final values given in the table.

Figure 7.

Illustrations of trajectories for the Sutera–Fraedrich model (4.4) showing the presence of all three tipping types for parameters in table 2—horizontal axis, years; vertical axis, Kelvin. The solid lines show system trajectories while the dashed lines show the location of the QSE—the branch T+ is stable while the branch T is unstable in this model. (a,b) R-tipping for a smooth change of parameters between two steady states. (a) The system returns to the QSE after a transient (ρ=0.18). (b) The system becomes unbounded, indicating a critical value ρc≈0.185 yr−1 (ρ=0.19). (c) An example of N-tipping in the presence of noise of amplitude ν=1.0 yr−1; (d) shows an example of B-tipping on decreasing μ uniformly from 1 at a constant rate. Note that in case (d) the two QSE coalesce at a saddle–node bifurcation.

View this table:
Table 2.

Parameter values for simulations shown in figure 7. For case (ab), we interpolate between the values given along the curve such that Embedded Image is constant at a rate proportional to ρ. In case (c), all parameters are fixed but noise is added, while, in case (d), we impose a steady drift of the parameter μ downwards.

5. Summary and conclusions

It is of great practical importance to understand the theoretical mechanisms behind tipping phenomena in the climate system as well as other systems. We have proposed here that such mechanisms can be effectively divided into three distinct categories: bifurcation-induced, noise-induced and rate-dependent tipping, respectively denoted as B-, N- and R-tipping. In particular, we describe R-tipping, a mechanism that may be exhibited by (subsystems of) the climate system independently of the presence or absence of the other types of tipping.

In realistic models, tipping effects may be associated with a combination of the three mechanisms, and it will be a challenge to understand this more general case. For example, B-tipping, usually associated with slow changes in a parameter, may turn into R-tipping upon increasing the rate of change for the parameters. However, as illustrated in figure 8, completely new mechanisms may appear on increasing the rate, including the possibility that B-tipping may be suppressed for fast enough variation of parameters. Alternatively, the B-tipping may persist but an R-tipping mechanism may come into play before the B-tipping is reached.

Figure 8.

Different possible system behaviours on ramping the parameter λ at differing rates (dashed arrows) through the region λ∈[0,1]. (a) Example where there is a B-tipping for low rates (quasi-static) that disappears for high enough rates. (b) An example where there is no tipping for small enough rates but R-tipping for large enough rates. (c) Both B- and R-tipping, but there is a range of rates where no instability appears.

We emphasize that neither N-tipping nor R-tipping require any change of stability. Hence there is no reason to assume that the techniques of Dakos et al. [14], based on a de-trended autoregressive model for B-tipping, should deliver useful predictions in such cases—as noted by Ditlevsen & Johnsen [16], N-tipping is intrinsically unpredictable. We are investigating whether any novel predictive technique may be developed for R-tipping. Those cases of R-tipping that can be reduced to a local bifurcation in a co-moving system may be expected to be predictable using similar methods; this includes the examples in §3a,b(i) with steady drift. In more complex cases, ρc may still be quantifiable by global heteroclinic bifurcations for an extended system, for example (3.1) and (3.10) or (3.4) and (3.10) in §3b(ii).

The classification proposed here may be applicable to a wide range of open systems under the influence of noise and/or parameter changes. Recent work of Nene & Zaikin [26] suggested that there may be interesting applications of rate-dependent bifurcation theory to determine cell fate. There are potentially many other application areas, from mechanics and ecology to economics and social sciences, where tipping points are of interest. We suggest that this will be an area of significant mathematical development in the coming years.


The authors thank the Isaac Newton Institute for hosting the programme ‘Mathematical and Statistical Approaches to Climate Modelling and Prediction’ in autumn 2010, where this topic was initially discussed, and are indebted to Alexei Zaikin and Jan Sieber for stimulating conversations in relation to this work.



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