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Convergence of Rain Process Models to Point Processes

Scott Hottovy Department of Mathematics, United States Naval Academy, Annapolis, Maryland    Samuel N. Stechmann Department of Mathematics, and Department of Atmospheric and Oceanic Sciences, University of Wisconsin–Madison, Madison, Wisconsin
Abstract

A moisture process with dynamics that switch after hitting a threshold gives rise to a rainfall process. This rainfall process is characterized by its random holding times for dry and wet periods. On average, the holding times for the wet periods are much shorter than the dry. Here convergence is shown for the rain fall process to a point process that is a spike train. The underlying moisture process for the point process is a threshold model with a teleporting boundary condition. This approximation allows simplification of the model with many exact formulas for statistics. The convergence is shown by a Fokker-Planck derivation, convergence in mean-square with respect to continuous functions, of the moisture process, and convergence in mean-square with respect to generalized functions, of the rain process.

I Introduction

Rain processes are often studied and tested as single column models in the atmosphere Betts and Miller, (1986); Frierson et al., (2004). These single column models are used to “trigger” a transition to convection or rainfall. Furthermore, these rainfall models are simple and have uses in global climate models (GCMs) Lin and Neelin, (2000); Suhas and Zhang, (2014); Bergemann et al., (2017). One type of rainfall model that has been successful is a Renewal process (Bernardara et al., (2007); Foufoula-Georgiou and Lettenmaier, (1987); Green, (1964); Schmitt et al., (1998)). A renewal process is a continuous-time Markov process that is defined by its holding times Cox, (1962). For example, a simple rain renewal process, σ(t)\sigma(t), may be defined by its holding times τd\tau^{d} when σ(t)=0\sigma(t)=0, defined to be that the column of air is dry, and τr\tau^{r} when σ(t)=1\sigma(t)=1, defined to be that the column of air is raining. Thus a dry (or rain) event will last τd\tau^{d} (or τr\tau^{r}) time where the distribution of the (possibly) random times are given.

The model presented here was previously studied in Stechmann and Neelin, (2011, 2014); Hottovy and Stechmann, (2015); Abbott et al., (2016). The underlying process is a one dimensional continuous-time stochastic process modeling the moisture q(t)(,)q(t)\in(-\infty,\infty) for t0t\geq 0, typically in cm, for a parcel of air. This quantity is vertically integrated and averaged over a square domain to give the units of length. Here the rain process is modeled as σ(t)\sigma(t) an indicator function for rain. One choice of process for q(t)q(t) is the hysteresis dynamics studied in Hottovy and Stechmann, (2015). There the q(t)q(t) process is governed by the stochastic differential equations (SDE)

dq(t)={mdt+D0dWtfor σ(t)=0rdt+D1dWtfor σ(t)=1,q(0)=0,σ(0)=0,dq(t)=\left\{\begin{array}[]{lr}m\;dt+D_{0}\;dW_{t}&\mbox{for }\sigma(t)=0\\ -r\;dt+D_{1}\;dW_{t}&\mbox{for }\sigma(t)=1\end{array}\right.,\quad q(0)=0,\quad\sigma(0)=0, (1)

where mm and rr are the moistening and rain rates respectively, and D0D_{0} and D1D_{1} are the fluctuations of moisture during the respective states. The dynamics of σ(t)\sigma(t) switch from 0 to 1 when q(t)q(t) reaches a fixed threshold bb. That is (q(0),σ(0))=(0,0)(q(0),\sigma(0))=(0,0) and σ(t)=1\sigma(t)=1 for t=inf{t0,q(t)=b}t=\inf\{t\geq 0,q(t)=b\}. Then σ(t)\sigma(t) switches back to zero when q(t)q(t) reaches the threshold q(t)=0q(t)=0. This model is referred to as the deterministic trigger, two threshold (D2) model in Hottovy and Stechmann, (2015). A realization of the processes q(t)q(t) and σ(t)\sigma(t) are shown in Figure 1. In a renewal process perspective, σ(t)\sigma(t) is modeled by the holding times τd\tau_{d} and τr\tau_{r}. These times are the first passage times for Brownian motion with drift to travel a distance of bb units.

Models of triggering precipitation are used for convective parameterizations. Convective parameterizations are useful in global climate and circulation models (GCMs). In GCMs, the models are run for long times to examine potential effects, for example, of climate change. In long times, the model (2) was studied in Abbott et al., (2016). In a long time view, the dry events dominate the rain events. In Figure 2 the top panel shows σ(t)\sigma(t) process is plotted up to time T=T=..., and in the bottom panel an example of the rain process in observations (OBS DETAILS). Thus for long times, rr is a much larger rate than mm, and σ(t)\sigma(t) resembles a point process.

Refer to captionRefer to caption
Figure 1: Sample precipitation time series from observations at (a) Manus Island and (b) Nauru Island reproduced from Fig 3. of Abbott et al., (2016) with permission from the authors. Panels (c) and (d) are realizations of the model of the rain rate process σϵ(t)\sigma^{\epsilon}(t) with finite rain rate rr and σ(t)\sigma(t) the point process, respectively.

The main result of the paper is to define and show convergence of the threshold model above as rr\to\infty. For example, on the level of renewal processes, τr0\tau^{r}\to 0 and thus σ(t)\sigma(t) converges to a process that is zero everywhere and has spikes at infinity at random times τd\tau^{d}. However, σ(t)\sigma(t) is right continuous and has left hand limits, where as the spike train is not. Thus the mode of convergence is not clear. For q(t)q(t) the limit is also unclear, but will be redefined in a way to show convergence with respect to the topology on continuous functions with the uniform metric. In this study, the limiting processes are define (in Section II) and convergence is shown both heuristically (for the Fokker-Planck equation) and rigorously.

There are many novel aspects of this work. The limit jump process q(t)q(t) has an associated Fokker-Planck equation that is derived using a matched asymptotic method. The resulting Fokker-Planck equation has a peculiar boundary flux condition which defines a “teleporting” boundary condition of q(t)q(t). The processes are decoupled into evaporating and precipitating processes. Only after this decoupling can convergence of the evaporation processes be shown rigorously with respect to the uniform metric on the space of continuous functions. Finally, the rain process σ(t)\sigma(t) is shown to converge rigorously with respect to the the generalized function space. This proof shows convergence of a renewal process to a delta process. Further more, the proof shows what kinds of bounds the rain event times τr\tau^{r} need in order for integrated convergence to hold.

The convergence results shown here have the potential to impact various other fields. Many fields of study use similar renewal processes to model phenomena. The connections to rain models was made above. In addition, there has been much work in queuing theory to approximate point processes with renewal processes (e.g. Whitt, (1982); Bhat, (1994)), and using threshold triggers in financial models Lejay and Pigato, (2019). The strongest connection is with neuron stochastic integrate and fire models (see Sacerdote and Giraudo, (2013) for a review). The moisture process with a finite rain rate is similar to a Wiener Process model of a single Neuron with refractoriness. A similar model was studied in Albano et al., (2008) where the refractory time was constant. Here, the refractory time is random and coincides with the rain duration time τr\tau^{r}. Thus the work here is applicable to understanding the differences in using a model without refractoriness versus a model with a short, possible random, refractory time. The structure of the paper is as follows. The processes for moisture and rain are defined in Section II. The modes of convergence are discussed in Section III. The heuristic derivation of the Fokker-Planck equation is shown in Section III.1. Rigorous convergence of the moistening process EϵE^{\epsilon} to EE is shown with respect to L2L^{2} in Section III.2 and the rain process σϵ\sigma^{\epsilon} is shown to converge to the sum of delta distributions σ\sigma with respect to generalized functions in Section III.3. The results are summarized in Section IV.

II Model Description

In this section the moisture and precipitation processes are defined. First the underlying moisture process of the renewal rain process is defined. The processes are defined with a small parameter ϵ\epsilon with the limit as ϵ0\epsilon\to 0 in mind.

The moisture process qϵ(t)q^{\epsilon}(t)\in\mathbb{R} is defined as the solution to the stochastic differential equation (SDE),

dqϵ(t)={mdt+D0dWtfor σϵ(t)=0rϵdt+D1dWtfor σϵ(t)=1,q(0)=0,σϵ(0)=0,dq^{\epsilon}(t)=\left\{\begin{array}[]{lr}m\;dt+D_{0}\;dW_{t}&\mbox{for }\sigma^{\epsilon}(t)=0\\ -\frac{r}{\epsilon}\;dt+D_{1}\;dW_{t}&\mbox{for }\sigma^{\epsilon}(t)=1\end{array}\right.,\quad q(0)=0,\quad\sigma^{\epsilon}(0)=0, (2)

where mm and r/ϵr/\epsilon are the moistening and rain rates, and 0<D0D10<D_{0}\leq D_{1} are the fluctuations of moisture during the respective states. The rain process, σϵ(t){0,r/ϵ}\sigma^{\epsilon}(t)\in\{0,r/\epsilon\} are as follows: since σϵ(0)=0\sigma^{\epsilon}(0)=0, let τ1d,ϵinf{t>0|qϵ(t)=b}\tau_{1}^{d,\epsilon}\equiv\inf\{t>0|q^{\epsilon}(t)=b\}. Then σϵ(t)=0\sigma^{\epsilon}(t)=0 for t[0,τ1d)t\in[0,\tau_{1}^{d}). Next let τ1rinf{t>τ1d|qϵ(t)=0}\tau_{1}^{r}\equiv\inf\{t>\tau_{1}^{d}|q^{\epsilon}(t)=0\}, and σϵ(t)=r/ϵ\sigma^{\epsilon}(t)=r/\epsilon for t[τ1d,τ1r)t\in[\tau_{1}^{d},\tau_{1}^{r}). This process repeats up to an arbitrary final time TT.

The associated processes, as ϵ0\epsilon\to 0, are defined as q(t)q(t) and σ(t)\sigma(t) for the moisture and rain processes. The moisture process is the solution to the SDE,

dq(t)=mdt+D0dWt,q<b,q(0)=0,dq(t)=m\;dt+D_{0}\;dW_{t},\quad q<b,\quad q(0)=0, (3)

with the unusual boundary condition as follows: Let the usual stopping time be as follows τ1d=inf{t>0|q(t)=b}\tau_{1}^{d}=\inf\{t>0|q(t)=b\}. Then at time t>τ1dt>\tau_{1}^{d} the process q(t)q(t) jumps or “teleports” to q=0q=0. Thus

limt(τ1d)q(t)=b,limt(τ1d)+q(t)=0,q(τ1d)=b.\lim_{t\rightarrow(\tau_{1}^{d})^{-}}q(t)=b,\quad\lim_{t\rightarrow(\tau_{1}^{d})^{+}}q(t)=0,\quad q(\tau_{1}^{d})=b. (4)

Then the process starts over using the dynamics of (3) until τ2d=inf{t>τ1d|q(t)=b}\tau_{2}^{d}=\inf\{t>\tau_{1}^{d}|q(t)=b\}, and the process repeats. The stopping times τid\tau_{i}^{d} are the dry event times of the process. These dynamics arise from the heuristic Fokker-Planck derivation in the next section (see Section III.1).

Examples of the processes are shown in Figure 2. The processes with finite rain rate r/ϵr/\epsilon for ϵ>0\epsilon>0 are shown in panels (a) and (b). Panel (a) is the moisture process qϵ(t)q^{\epsilon}(t) defined is equation (2). The rain rate process is shown in (d) and takes value r/ϵr/\epsilon when qϵ(t)q^{\epsilon}(t) reaches level bb for the first time (panel (a) in black) and resets to zero when qϵ(t)q^{\epsilon}(t) reaches zero (panel (a) in gray). This process repeats. The limiting processes are shown in panels (c) and (d). Panel (c) shows the limiting moisture process q(t)q(t) defined in equation (3) and panel (d) shows the rain process defined in equation (5). The moisture process is a Brownian motion with positive drift until reaching level bb. When q(t)=0q(t)=0, the process σ(t)\sigma(t) takes an infinite value and the moisture process is reset at zero.

Refer to caption
Figure 2: Realizations are plotted of the processes (a) qϵ(t)q^{\epsilon}(t), (b) σϵ(t)\sigma^{\epsilon}(t) for rain rate r/ϵr/\epsilon defined in equation (2) with ϵ>0\epsilon>0 and (c) q(t)q(t) and (d) σ(t)\sigma(t) defined in equation (3) and (5) respectively.

From the definition of τid\tau_{i}^{d} above, the rain point process σ(t)\sigma(t) is defined as

σ(t)=bi=1𝒩(T)δ(tτid),\sigma(t)=b\sum_{i=1}^{\mathcal{N}(T)}\delta(t-\tau_{i}^{d}), (5)

where 𝒩(T)\mathcal{N}(T) is the random variable of the number of times the process q(t)q(t) reaches bb in time TT. The quantity bb arises because the moisture process qϵq^{\epsilon} loses moisture at a rate of r/ϵr/\epsilon per time, on average. The moisture process q(t)q(t) loses all the moisture built up (bb) instantaneously.

Note that qϵ(t)q^{\epsilon}(t) has continuous paths while q(t)q(t) has jump discontinuities. Thus any mode of convergence between qϵq^{\epsilon} and qq with an associated metric (e.g. uniform or Skorohod) will fail. There is another way to define both qϵq^{\epsilon} and qq in which convergence with respect to L2L^{2} with the uniform metric on the space of continuous functions (𝒞[0,T]\mathcal{C}[0,T]) can be shown. To do so, qϵ(t)q^{\epsilon}(t) is decomposed into an evaporation process, Eϵ(t)E^{\epsilon}(t), and precipitating process Pϵ(t)P^{\epsilon}(t). These processes are defined as,

dEtϵ={mdt+D0dWtfor σtϵ=00for σtϵ=1, and dPtϵ={0for σtϵ=0rϵdt+D0dWtfor σtϵ=1.dE_{t}^{\epsilon}=\left\{\begin{array}[]{lr}m\;dt+D_{0}dW_{t}&\mbox{for }\sigma_{t}^{\epsilon}=0\\ 0&\mbox{for }\sigma_{t}^{\epsilon}=1\end{array}\right.,\quad\mbox{ and }\quad dP_{t}^{\epsilon}=\left\{\begin{array}[]{lr}0&\mbox{for }\sigma_{t}^{\epsilon}=0\\ -\frac{r}{\epsilon}\;dt+D_{0}dW_{t}&\mbox{for }\sigma_{t}^{\epsilon}=1\end{array}\right.. (6)

Thus the moisture process qϵ(t)q^{\epsilon}(t) is written as

qϵ(t)=Eϵ(t)+Pϵ(t).q^{\epsilon}(t)=E^{\epsilon}(t)+P^{\epsilon}(t).

In the limit, the jumps will be captured in the PϵP^{\epsilon} process. In the following section it will be shown (see Section III.2) that EϵEE^{\epsilon}\rightarrow E, where E(t)E(t) is defined as the solution to the SDE

dE(t)=mdt+D0dWt,E(0)=0.dE(t)=m\;dt+D_{0}\;dW_{t},\quad E(0)=0. (7)

Furthermore, the σ\sigma process is defined as above in (5) where τid=inf{t>0|E(t)=kb,k}\tau_{i}^{d}=\inf\{t>0|E(t)=kb,\;k\in\mathbb{N}\}, i.e. the first passage time of Brownian motion with drift to kbkb.

III Convergence to a Point Process

In this section convergence is shown both heuristically (e.g. Section III.1) and rigorously (e.g. Sections III.3 and III.2).

Note that the simplest ideas of convergence break down when considering path-wise convergence of qϵq^{\epsilon} to qq and σϵ\sigma^{\epsilon} to σ\sigma. This is because qϵq^{\epsilon} is a continuous process (σϵ\sigma^{\epsilon} is left continuous and has right hand limits) for all ϵ>0\epsilon>0 and qq is a process with jumps (σ\sigma no longer is left continuous). Thus, there is no topology with associated metric dd such that qϵqq^{\epsilon}\rightarrow q with respect to dd. However, one can show that qϵq^{\epsilon} converges in a notion weaker than the Skorohod topology. See Kurtz, (1991) for these conditions. This convergence happens in a topology which does not have an associated metric (see Jakubowski et al., (1997)). This is not done here as it is technical and does not give any insight to the model or approximation.

The following three subsections prove convergence of the various processes introduced in Section II. In Section III.1 the Fokker-Planck equation for qϵq^{\epsilon} is shown to converge (formally) to a Fokker-Planck equation for qq. This derivation gives rise to an interesting partial differential equation (PDE) with unusual “teleporting” boundary conditions. In Section III.2 convergence in paths is shown for EϵE^{\epsilon} to EE with respect to the uniform metric for continuous functions on [0,T][0,T]. In Section III.3 convergence is shown for σϵ\sigma^{\epsilon} to σ\sigma with respect to generalized functions. This norm is necessary because σ\sigma is a sum of dirac delta functions. In addition, this convergence is the “natural” convergence to consider when analyzing the errors between using σϵ\sigma^{\epsilon} and a point process (σ\sigma) in, for example, a GCM.

III.1 Fokker-Planck Equation

In this section, the derivation for the Fokker-Planck equation of equation (3) is shown.

The Fokker-Planck equation for the (D2) process (see Hottovy and Stechmann, (2015)) is composed of two densities. These densities are denoted ρ0\rho_{0} and ρ1\rho_{1} for the dry and rain states respectively. These densities follow the following Fokker-Planck equations

tρ0=\displaystyle\partial_{t}\rho_{0}= mqρ0+D022q2ρ0δ(q)f1|q=0,<q<b,t0,\displaystyle-m\partial_{q}\rho_{0}+\left.\frac{D_{0}^{2}}{2}\partial_{q}^{2}\rho_{0}-\delta(q)f_{1}\right|_{q=0},\quad-\infty<q<b,t\geq 0, (8)
tρ1=\displaystyle\partial_{t}\rho_{1}= rϵqρ1+D122q2ρ1+δ(qb)f0|q=b,0<q<,t0,\displaystyle\frac{r}{\epsilon}\partial_{q}\rho_{1}+\left.\frac{D_{1}^{2}}{2}\partial_{q}^{2}\rho_{1}+\delta(q-b)f_{0}\right|_{q=b},\quad 0<q<\infty,t\geq 0, (9)

where the fluxes fif_{i} are defined as

f0(q,t)\displaystyle f_{0}(q,t) =mρ0(q,t)D022qρ0(q,t)\displaystyle=-m\rho_{0}(q,t)-\frac{D_{0}^{2}}{2}\partial_{q}\rho_{0}(q,t) (10a)
f1(q,t)\displaystyle f_{1}(q,t) =rϵρ1(q,t)D122qρ1(q,t)m,\displaystyle=\frac{r}{\epsilon}\rho_{1}(q,t)-\frac{D_{1}^{2}}{2}\partial_{q}\rho_{1}(q,t)m, (10b)

and with the following conditions,

ρ0(b)=ρ1(0)\displaystyle\rho_{0}(b)=\rho_{1}(0) =0\displaystyle=0 (11)
ρ0(q,t)+ρ1(q,t)dq\displaystyle\int_{-\infty}^{\infty}\rho_{0}(q,t)+\rho_{1}(q,t)\;dq =1,t0.\displaystyle=1,\quad t\geq 0. (12)

The proposed limit as ϵ0\epsilon\to 0 for the Fokker-Planck equation is

tρ0=\displaystyle\partial_{t}\rho_{0}= mqρ0+D022q2ρ0+δ(q)f0|q=b,<q<b,t0,\displaystyle-m\partial_{q}\rho_{0}+\left.\frac{D_{0}^{2}}{2}\partial_{q}^{2}\rho_{0}+\delta(q)f_{0}\right|_{q=b},\quad-\infty<q<b,t\geq 0, (13)
ρ1=\displaystyle\rho_{1}= 0.\displaystyle 0. (14)

with the following conditions,

ρ0(b)\displaystyle\rho_{0}(b) =0\displaystyle=0 (15)
bρ0(q,t)𝑑q\displaystyle\int_{-\infty}^{b}\rho_{0}(q,t)\;dq =1.\displaystyle=1. (16)

The analysis follows asymptotic matching conditions from Bender and Orszag, (2013) (Chpt. 9). Consider two regions [0,ϵ][0,\epsilon] and [ϵ,)[\epsilon,\infty). Let ρ1,B\rho_{1,B} be the density in the first, boundary layer region. For this equation, define the rescaled variable q~=1ϵq\tilde{q}=\frac{1}{\epsilon}q. This yields the equation

tρ1,B=rϵ2q~ρ1,B+D122ϵ2q~2ρ1,B\partial_{t}\rho_{1,B}=\frac{r}{\epsilon^{2}}\partial_{\tilde{q}}\rho_{1,B}+\frac{D_{1}^{2}}{2\epsilon^{2}}\partial_{\tilde{q}}^{2}\rho_{1,B} (17)

Let ρ1,B\rho_{1,B} have the asymptotic expansion of the form,

ρ1,B=ρ1,B0+ϵρ1,B1+O(ϵ2).\rho_{1,B}=\rho_{1,B}^{0}+\epsilon\rho_{1,B}^{1}+O(\epsilon^{2}).

Substituting this expansion into equation (17) yields the order ϵ2\epsilon^{-2} terms

O(ϵ2): 0\displaystyle O(\epsilon^{-2}):\;0 =rq~ρ1,B0+D122q2ρ1,B0\displaystyle=r\partial_{\tilde{q}}\rho_{1,B}^{0}+\frac{D_{1}^{2}}{2}\partial^{2}_{q}\rho_{1,B}^{0} (18a)
O(ϵ1): 0\displaystyle O(\epsilon^{-1}):\;0 =rq~ρ1,B1+D122q2ρ1,B1\displaystyle=r\partial_{\tilde{q}}\rho_{1,B}^{1}+\frac{D_{1}^{2}}{2}\partial^{2}_{q}\rho_{1,B}^{1} (18b)

The solution to the order ϵ2\epsilon^{-2} equation (18a)and applying the absorbing boundary condition at q~=0\tilde{q}=0 yields

ρ1,B0=C1(t)(1exp[2rD12q~]).\rho_{1,B}^{0}=C_{1}(t)\left(1-\exp\left[-\frac{2r}{D_{1}^{2}}\tilde{q}\right]\right). (19)

The order ϵ1\epsilon^{-1} equation (18b) has the same solution as above, after applying the absorbing boundary,

ρ1,B1=C2(t)(1exp[2rD12q~]).\rho_{1,B}^{1}=C_{2}(t)\left(1-\exp\left[-\frac{2r}{D_{1}^{2}}\tilde{q}\right]\right). (20)

Now consider the interval away from the boundary [O(ϵ),)[O(\epsilon),\infty). Let ρ1,A\rho_{1,A} be the density in this region. The equation in this region is

tρ1,A=rϵqρ1,A+D122q2ρ1,A+δ(qb)f0(b,t).\partial_{t}\rho_{1,A}=\frac{r}{\epsilon}\partial_{q}\rho_{1,A}+\frac{D_{1}^{2}}{2}\partial_{q}^{2}\rho_{1,A}+\delta(q-b)f_{0}(b,t). (21)

Let ρ1,A\rho_{1,A} have the asymptotic expansion

ρ1,A=ρ1,A0+ϵρ1,A1+O(ϵ2).\rho_{1,A}=\rho_{1,A}^{0}+\epsilon\rho_{1,A}^{1}+O(\epsilon^{2}).

Note that the δ\delta term acts on f0f_{0} which is a function of ρ0\rho_{0}. The asymptotic analysis is for ρ1\rho_{1} only, thus the density ρ0\rho_{0} is an order one term. Substituting the expansion into equation (21) gives the following equations, separated into their orders of ϵ\epsilon,

O(ϵ1):0\displaystyle O(\epsilon^{-1}):0 =rqρ1,A0\displaystyle=r\partial_{q}\rho_{1,A}^{0} (22a)
O(1):tρ1,A0\displaystyle O(1):\partial_{t}\rho_{1,A}^{0} =rqρ1,A1+D122q2ρ1,A0+δ(qb)f0(b,t).\displaystyle=r\partial_{q}\rho_{1,A}^{1}+\frac{D_{1}^{2}}{2}\partial^{2}_{q}\rho_{1,A}^{0}+\delta(q-b)f_{0}(b,t). (22b)

The order ϵ1\epsilon^{-1} equation (22a) has the solution

ρ1,A0=C3(t).\rho_{1,A}^{0}=C_{3}(t). (23)

Note that ρ1,A\rho_{1,A} is a density and thus ρ1,A0\rho_{1,A}^{0} must be integrable on [O(ϵ),)[O(\epsilon),\infty). Thus C3(t)=0C_{3}(t)=0 and

ρ1,A0=0.\rho_{1,A}^{0}=0. (24)

The order one equation (22b), by substituting in ρ1,A0=0\rho_{1,A}^{0}=0, gives the solution,

ρ1,A1={C4(t)forO(ϵ)q<bC4(t)1rf0(b,t),forqb\rho_{1,A}^{1}=\left\{\begin{array}[]{lcr}C_{4}(t)&\mbox{for}&O(\epsilon)\leq q<b\\ C_{4}(t)-\frac{1}{r}f_{0}(b,t),&\mbox{for}&q\geq b\end{array}\right. (25)

Note that the constant of integration in each interval of bb must be the same. Otherwise, the magnitude of the δ\delta function in (22b) would not be correct. The density ρ1,A1\rho_{1,A}^{1} must be integrable which implies that

C4(t)=1rf0(b,t).C_{4}(t)=\frac{1}{r}f_{0}(b,t). (26)

It is assumed that the matching between the AA and BB solutions must occur at the left most edge of the region [0,O(ϵ)][0,O(\epsilon)]. That is, for values of q=O(ϵ1/2)q=O(\epsilon^{1/2}),

ρ1,B0(O(ϵ1/2),t)=ρ1,A0(O(ϵ1/2),t)\rho_{1,B}^{0}(O(\epsilon^{1/2}),t)=\rho_{1,A}^{0}(O(\epsilon^{1/2}),t)

and

ρ1,B1(O(ϵ1/2),t)=ρ1,A1(O(ϵ1/2),t).\rho_{1,B}^{1}(O(\epsilon^{1/2}),t)=\rho_{1,A}^{1}(O(\epsilon^{1/2}),t).

The first equation implies that C1(t)=0C_{1}(t)=0 and ρ1,B0=ρ1,A0=0\rho_{1,B}^{0}=\rho_{1,A}^{0}=0. In the limit as ϵ0\epsilon\to 0 the second equation yields

C2(t)=1rf0(b,t).C_{2}(t)=\frac{1}{r}f_{0}(b,t). (27)

Thus the densities are

ρ10=0\rho_{1}^{0}=0 (28)

and

ρ11={1rf0(b,t)(1exp[2rD12qϵ])0qO(ϵ)1rf0(b,t)O(ϵ)qb0b<q.\rho_{1}^{1}=\left\{\begin{array}[]{lr}\frac{1}{r}f_{0}(b,t)\left(1-\exp\left[-\frac{2r}{D_{1}^{2}}\frac{q}{\epsilon}\right]\right)&0\leq q\leq O(\epsilon)\\ \frac{1}{r}f_{0}(b,t)&O(\epsilon)\leq q\leq b\\ 0&b<q\par\end{array}\right.. (29)

Note the flux of ρ1\rho_{1} at q=0q=0 is,

f1(0,t)=rρ1(0,t)+D122qρ1|(0,t).f_{1}(0,t)=r\rho_{1}(0,t)+\frac{D_{1}^{2}}{2}\partial_{q}\left.\rho_{1}\right|_{(0,t)}. (30)

Using the asymptotic expansion yields,

f1(0,t)=D122ϵ{1rf0(b,t)(2rD12ϵ)}=f0(b,t).f_{1}(0,t)=\frac{D_{1}^{2}}{2}\epsilon\left\{\frac{1}{r}f_{0}(b,t)\left(-\frac{2r}{D_{1}^{2}\epsilon}\right)\right\}=f_{0}(b,t). (31)

Thus the Fokker-Planck type equation for q(t)q(t) is

tρ0=\displaystyle\partial_{t}\rho_{0}= mqρ0+D022q2ρ0+δ(q)f0|q=b,<q<b,t0,\displaystyle-m\partial_{q}\rho_{0}+\left.\frac{D_{0}^{2}}{2}\partial_{q}^{2}\rho_{0}+\delta(q)f_{0}\right|_{q=b},\quad-\infty<q<b,t\geq 0, (32)
ρ1=\displaystyle\rho_{1}= 0.\displaystyle 0. (33)

with the following conditions,

ρ0(b)\displaystyle\rho_{0}(b) =0\displaystyle=0 (34)
ρ0(q,t)𝑑q\displaystyle\int_{-\infty}^{\infty}\rho_{0}(q,t)\;dq =1.\displaystyle=1. (35)

III.2 Pathwise Convergence

For this section and next, a useful lemma is first stated and proved.

Lemma 1.

Let 𝒩ϵ(T)\mathcal{N}_{\epsilon}(T) be the number of rain events for the qϵq^{\epsilon} process defined in (3). The probability of that the number of events is nn decays exponentially as nn tends to infinity, i.e. for 0<s<min{rb/ϵD22,mb/D12}0<s<\min\{rb/\epsilon D_{2}^{2},mb/D_{1}^{2}\}

P(𝒩ϵ(T)=N)exp{sTNmbD12(1+2D12sm21)}.P(\mathcal{N}_{\epsilon}(T)=N)\leq\exp\left\{sT-\frac{Nmb}{D_{1}^{2}}\left(\sqrt{1+\frac{2D_{1}^{2}s}{m^{2}}}-1\right)\right\}.
Proof.

Note that the process 𝒩ϵ(T)\mathcal{N}_{\epsilon}(T) is a renewal process. It is defined by the interarrival times,

Sn=τnd,ϵ+τnr,ϵ,n1,S_{n}=\tau_{n}^{d,\epsilon}+\tau_{n}^{r,\epsilon},\quad n\geq 1, (36)

where τid,ϵ(τir,ϵ)\tau_{i}^{d,\epsilon}\;(\tau_{i}^{r,\epsilon}) is the duration for the iith dry (rain) event of the σϵ\sigma^{\epsilon} process. The distributions of τid\tau_{i}^{d} and τid,ϵ\tau_{i}^{d,\epsilon} are the same independent of ϵ\epsilon, while τir,ϵ\tau_{i}^{r,\epsilon} depends on epsilon. To estimate the sum in (53), the probability of having NN rain events in time TT is estimated using the Central Limit Theorem. Consider the probability

P(𝒩ϵ(T)=N)=P(S1+S2+SNT,S1+S2++SN+SN+1>T).P\left(\mathcal{N}^{\epsilon}(T)=N\right)=P\left(S_{1}+S_{2}+\cdots S_{N}\leq T,\quad S_{1}+S_{2}+\cdots+S_{N}+S_{N+1}>T\right). (37)

The probability on the right hand side is estimated crudely by only considering one of the two events. Note that S1,S2,S3,,SnS_{1},S_{2},S_{3},...,S_{n} are IID random variables with E[S1]=E[τd,ϵ+τr,ϵ]E[S_{1}]=E[\tau^{d,\epsilon}+\tau^{r,\epsilon}], and σ2=Var(S1)<\sigma^{2}=\mbox{Var}(S_{1})<\infty, thus

P(𝒩ϵ(T)=N)P(S1+S2++SNT).\displaystyle P(\mathcal{N}^{\epsilon}(T)=N)\leq P\left(S_{1}+S_{2}+\cdots+S_{N}\leq T\right). (38)

The above probability is estimated by using a variant of the Chernoff bound Hoeffding, (1994). That is,

P(S1+S2+SNT)exp(sT)i=0nE[esSi],P\left(S_{1}+S_{2}+\cdots S_{N}\leq T\right)\leq\exp(sT)\prod_{i=0}^{n}E[e^{-sS_{i}}], (39)

for s>0s>0, where E[esSi]=MSi(s)E[e^{-sS_{i}}]=M_{S_{i}}(s) is the moment generating function for the random variable SiS_{i}. The moment generating function factors due to independence of τir,ϵ\tau_{i}^{r,\epsilon} and τid,ϵ\tau_{i}^{d,\epsilon},

MSi(s)=Mτir,ϵ(s)Mτid,ϵ(s).M_{S_{i}}(s)=M_{\tau_{i}^{r,\epsilon}}(s)M_{\tau_{i}^{d,\epsilon}}(s).

These moment generating functions are computed explicitly from the distributions found in Hottovy and Stechmann, (2015). They are,

Mτir,ϵ\displaystyle M_{\tau_{i}^{r,\epsilon}} =0estρr(t)𝑑t=exp{rbϵD22(1+2D22sϵ2r21)}\displaystyle=\int_{0}^{\infty}e^{-st}\rho_{r}(t)\;dt=\exp\left\{\frac{-rb}{\epsilon D_{2}^{2}}\left(\sqrt{1+\frac{2D_{2}^{2}s\epsilon^{2}}{r^{2}}}-1\right)\right\} (40)
Mτid,ϵ\displaystyle M_{\tau_{i}^{d,\epsilon}} =0estρd(t)𝑑t=exp{mbD12(1+2D12sm21)}.\displaystyle=\int_{0}^{\infty}e^{-st}\rho_{d}(t)\;dt=\exp\left\{\frac{-mb}{D_{1}^{2}}\left(\sqrt{1+\frac{2D_{1}^{2}s}{m^{2}}}-1\right)\right\}. (41)

where s<min{rb/ϵD22,mb/D12}s<\min\{rb/\epsilon D_{2}^{2},mb/D_{1}^{2}\}. Thus Chernoff’s bound yields,

P(𝒩ϵ(T)=N)\displaystyle P(\mathcal{N}_{\epsilon}(T)=N) P(S1+S2+SnT)\displaystyle\leq P\left(S_{1}+S_{2}+\cdots S_{n}\leq T\right) (42)
exp(sT)i=0NE[esSi]\displaystyle\leq\exp(sT)\prod_{i=0}^{N}E[e^{-sS_{i}}] (43)
=exp{sTNrbϵD22(1+2D22ϵ2sr21)NmbD12(1+2D12sm21)}\displaystyle=\exp\left\{sT-\frac{Nrb}{\epsilon D_{2}^{2}}\left(\sqrt{1+\frac{2D_{2}^{2}\epsilon^{2}s}{r^{2}}}-1\right)-\frac{Nmb}{D_{1}^{2}}\left(\sqrt{1+\frac{2D_{1}^{2}s}{m^{2}}}-1\right)\right\} (44)
exp{sTNmbD12(1+2D12sm21)}.\displaystyle\leq\exp\left\{sT-\frac{Nmb}{D_{1}^{2}}\left(\sqrt{1+\frac{2D_{1}^{2}s}{m^{2}}}-1\right)\right\}. (45)

With this lemma, convergence from EϵE^{\epsilon} to EE is shown in L2(Ω)L^{2}(\Omega) with respect to the uniform metric on the space of continuous functions C[0,T]C[0,T].

Theorem 1.

Let qtϵq_{t}^{\epsilon} be defined as

qtϵ=Etϵ+Ptϵq_{t}^{\epsilon}=E_{t}^{\epsilon}+P_{t}^{\epsilon}

where Et,PtE_{t},P_{t} are solutions to the SDEs in (6). Furthermore let EtE_{t} be defined as the solution to (7). Then

limϵ0E[(sup0tT|EtϵEt|)2]=0.\lim_{\epsilon\to 0}E\left[\left(\sup_{0\leq t\leq T}|E_{t}^{\epsilon}-E_{t}|\right)^{2}\right]=0. (46)
Proof.

To begin, note that the SDEs for EϵE^{\epsilon} and EE (see (6)) only differ when σϵ(t)=1\sigma^{\epsilon}(t)=1. Thus, the solutions to the SDEs give the formula

|Eϵ(t)E(t)|=|i=1Nϵ(t)τidτid+τirm𝑑t+τidτid+τirD0𝑑Wt|,\left|E^{\epsilon}(t)-E(t)\right|=\left|\sum_{i=1}^{N^{\epsilon}(t)}\int_{\tau_{i}^{d}}^{\tau_{i}^{d}+\tau_{i}^{r}}m\;dt+\int_{\tau_{i}^{d}}^{\tau_{i}^{d}+\tau_{i}^{r}}D_{0}\;dW_{t}\right|, (47)

where 𝒩ϵ(T)\mathcal{N}^{\epsilon}(T) is the number of rain events for T<T<\infty and ϵ>0\epsilon>0 fixed. The number of rain events is conditioned to be NN. By Lemma 1, the sum in (53) converges due to the fast decay of P(𝒩ϵ(T)=N)P(\mathcal{N}_{\epsilon}(T)=N) as NN\to\infty. Note that m>0m>0 and the stochastic integral is a martingale and Doob’s maximal inequality yields,

E[(sup0tT|Eϵ(t)E(t)|)2]N=14E[|i=1Nτidτid+τirm𝑑t+τidτid+τirD0𝑑Wt|2|Nϵ(T)=n]P(𝒩ϵ(T)=n).E\left[\left(\sup_{0\leq t\leq T}\left|E^{\epsilon}(t)-E(t)\right|\right)^{2}\right]\leq\sum_{N=1}^{\infty}4E\left[\left.\left|\sum_{i=1}^{N}\int_{\tau_{i}^{d}}^{\tau_{i}^{d}+\tau_{i}^{r}}m\;dt+\int_{\tau_{i}^{d}}^{\tau_{i}^{d}+\tau_{i}^{r}}D_{0}\;dW_{t}\right|^{2}\right|N^{\epsilon}(T)=n\right]P(\mathcal{N}^{\epsilon}(T)=n). (48)

Applying the Cauchy-Schwarz inequality to the sum and the Itô isometry to the stochastic integral yields

E[(sup0tT|Eϵ(t)E(t)|)2]n=1CnE[m|τr|2+D02|τr||Nϵ(T)=n]P(Nϵ(T)=n).E\left[\left(\sup_{0\leq t\leq T}\left|E^{\epsilon}(t)-E(t)\right|\right)^{2}\right]\leq\sum_{n=1}^{\infty}C_{n}E\left[\left.m|\tau^{r}|^{2}+D_{0}^{2}|\tau^{r}|\right|N^{\epsilon}(T)=n\right]P(N^{\epsilon}(T)=n). (49)

This sum converges due to the fast decay of P(Nϵ(T)=n)P(N_{\epsilon}(T)=n) as shown in Eq.(45). Tonelli’s theorem allows the limit as ϵ0\epsilon\to 0 to exchange with the infinite sum.

To finish the theorem the following moments of τir,ϵ\tau_{i}^{r,\epsilon} are used. The integrals can be computed exactly using the densities for τir,ϵ\tau_{i}^{r,\epsilon} found in Hottovy and Stechmann, (2015). They are

E[τir,ϵ]=bϵr,E[|τir,ϵ|2]=bD2ϵ3r3+b2ϵ2r2.E[\tau_{i}^{r,\epsilon}]=\frac{b\epsilon}{r},\quad E[|\tau_{i}^{r,\epsilon}|^{2}]=\frac{bD^{2}\epsilon^{3}}{r^{3}}+\frac{b^{2}\epsilon^{2}}{r^{2}}. (50)

III.3 Distributional Convergence

In this subsection L2(Ω)L^{2}(\Omega) of σϵ\sigma^{\epsilon} to σ\sigma is shown with respect to a generalized function norm. This norm is the one considered due to the nature of the delta function. It is also a natural norm to consider as it is an integrated error. That is, this norm considers the accumulation of errors after running the model for time T>0T>0.

Theorem 2.

Let ϕ:[0,)\phi:[0,\infty)\to\mathbb{R} be a test function in Cc(0,)C^{\infty}_{c}(0,\infty). Let σ(t)\sigma(t) and σϵ(t)\sigma^{\epsilon}(t) be defined in (5). Then

limϵ0E[(|σϵ(t),ϕ(t)σ(t),ϕ(t)|)2]=0,\lim_{\epsilon\to 0}E[\left(|\langle\sigma^{\epsilon}(t),\phi(t)\rangle-\langle\sigma(t),\phi(t)\rangle|\right)^{2}]=0, (51)

where

f(t),g(t)=0f(t)g(t)𝑑t.\langle f(t),g(t)\rangle=\int_{0}^{\infty}f(t)g(t)\;dt. (52)
Proof.

To prove the theorem, the expectation is conditioned on the number of events 𝒩ϵ(t)\mathcal{N}^{\epsilon}(t), as is done in the previous section. Thus the expectation is

E[|σϵ(t)σ(t)|,ϕ(t)2]\displaystyle E[\langle|\sigma^{\epsilon}(t)-\sigma(t)|,\phi(t)\rangle^{2}] (53)
=\displaystyle= N=1E[(i=1Nτid,ϵτid,ϵ+τir,ϵσϵ(t)ϕ(t)dt\displaystyle\sum_{N=1}^{\infty}E\left[\left.\left(\sum_{i=1}^{N}\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\sigma^{\epsilon}(t)\phi(t)\;dt\right.\right.\right. (54)
\displaystyle- 0Tbδ(tτid)ϕ(t)dti=N𝒩(T)0Tσ(t)ϕ(t)dt)2|𝒩ϵ(T)=N]P(𝒩ϵ(T)=N)\displaystyle\left.\left.\left.\int_{0}^{T}b\delta(t-\tau_{i}^{d})\phi(t)\;dt-\sum_{i=N}^{\mathcal{N}(T)}\int_{0}^{T}\sigma(t)\phi(t)\;dt\right)^{2}\right|\mathcal{N}^{\epsilon}(T)=N\right]P(\mathcal{N}^{\epsilon}(T)=N) (55)

where 𝒩(T)\mathcal{N}(T) is the number of dry events for the σ(t)\sigma(t) process up to time TT. Again, because of the decay of P(𝒩ϵ(T)=N)P(\mathcal{N}^{\epsilon}(T)=N) as NN\to\infty given in Lemma 1, the infinite sum converges.

To estimate the quantity in (53), one rain event is considered and the Cauchy-Schwarz bound will be used. Consider the iith rain event,

τid,ϵτid,ϵ+τir,ϵσϵ(t)ϕ(t)𝑑tbϕ(τid)\displaystyle\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\sigma^{\epsilon}(t)\phi(t)\;dt-b\phi(\tau_{i}^{d}) =τid,ϵτid,ϵ+τir,ϵrϵϕ(t)rϵϕ(τ1d,ϵ)+rϵϕ(τid,ϵ)dt+bϕ(τid,ϵ)bϕ(τid,ϵ)bϕ(τid)\displaystyle=\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\frac{r}{\epsilon}\phi(t)-\frac{r}{\epsilon}\phi(\tau_{1}^{d,\epsilon})+\frac{r}{\epsilon}\phi(\tau_{i}^{d,\epsilon})\;dt+b\phi(\tau_{i}^{d,\epsilon})-b\phi(\tau_{i}^{d,\epsilon})-b\phi(\tau_{i}^{d}) (56)
=\displaystyle= τid,ϵτid,ϵ+τir,ϵrϵ(ϕ(t)ϕ(τid,ϵ))𝑑t+(rϵτir,ϵb)ϕ(τid,ϵ)+b(ϕ(τid,ϵ)ϕ(τid)).\displaystyle\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\frac{r}{\epsilon}\left(\phi(t)-\phi(\tau_{i}^{d,\epsilon})\right)\;dt+\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}-b\right)\phi(\tau_{i}^{d,\epsilon})+b(\phi(\tau_{i}^{d,\epsilon})-\phi(\tau_{i}^{d})). (57)

The function ϕ(t)\phi(t) is smooth on [0,T][0,T] and thus is locally Lipschitz. Let the Lipschitz constant be K>0K>0. Then, along with the Cauchy-Schwarz inequality,

|τid,ϵτid,ϵ+τir,ϵσϵ(t)ϕ(t)𝑑tbϕ(τid)|\displaystyle\left|\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\sigma^{\epsilon}(t)\phi(t)\;dt-b\phi(\tau_{i}^{d})\right| (58)
\displaystyle\leq Cτid,ϵτid,ϵ+τir,ϵrϵK|tτid,ϵ|dt+C|(rϵτir,ϵb)ϕ(τid,ϵ)|+C|ϕ(τid,ϵϕ(τid)|\displaystyle C\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\frac{r}{\epsilon}K\left|t-\tau_{i}^{d,\epsilon}\right|\;dt+C\left|\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}-b\right)\phi(\tau_{i}^{d,\epsilon})\right|+C|\phi(\tau_{i}^{d,\epsilon}-\phi(\tau_{i}^{d})| (59)
\displaystyle\leq CrϵK|τir|2+C|(rϵτir,ϵb)ϕ(τid,ϵ)|+C|ϕ(τid,ϵ)ϕ(τid)|.\displaystyle C\frac{r}{\epsilon}K|\tau_{i}^{r}|^{2}+C\left|\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}-b\right)\phi(\tau_{i}^{d,\epsilon})\right|+C|\phi(\tau_{i}^{d,\epsilon})-\phi(\tau_{i}^{d})|. (60)

With the last inequality resulting from tτid,ϵt-\tau_{i}^{d,\epsilon} being an increasing function on [τid,ϵ,τid,ϵ+τir,ϵ][\tau_{i}^{d,\epsilon},\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}].

Using the inequality above, along with the Cauchy-Schwarz inequality, the quantity in (53) is bounded by

N=1\displaystyle\sum_{N=1}^{\infty} E[(i=1Nτid,ϵτid,ϵ+τir,ϵσϵ(t)ϕ(t)dt\displaystyle E\left[\left.\left(\sum_{i=1}^{N}\int_{\tau_{i}^{d,\epsilon}}^{\tau_{i}^{d,\epsilon}+\tau_{i}^{r,\epsilon}}\sigma^{\epsilon}(t)\phi(t)\;dt\right.\right.\right. (61)
\displaystyle- 0Tbδ(tτid)ϕ(t)dti=N𝒩(T)0Tσ(t)ϕ(t)dt)2|𝒩ϵ(T)=N]P(𝒩ϵ(T)=N)\displaystyle\left.\left.\left.\int_{0}^{T}b\delta(t-\tau_{i}^{d})\phi(t)\;dt-\sum_{i=N}^{\mathcal{N}(T)}\int_{0}^{T}\sigma(t)\phi(t)\;dt\right)^{2}\right|\mathcal{N}^{\epsilon}(T)=N\right]P(\mathcal{N}^{\epsilon}(T)=N) (62)
\displaystyle\leq N=1i=1N(C(rϵ)2E[|τir|4]+CE[|(rϵτir,ϵb)ϕ(τid,ϵ)|2]+CE[|ϕ(τid,ϵ)ϕ(τid)|2])P(𝒩ϵ(T)=N)\displaystyle\sum_{N=1}^{\infty}\sum_{i=1}^{N}\left(C\left(\frac{r}{\epsilon}\right)^{2}E[|\tau_{i}^{r}|^{4}]+CE\left[\left|\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}-b\right)\phi(\tau_{i}^{d,\epsilon})\right|^{2}\right]+CE\left[|\phi(\tau_{i}^{d,\epsilon})-\phi(\tau_{i}^{d})|^{2}\right]\right)P(\mathcal{N}^{\epsilon}(T)=N) (63)
+\displaystyle+ N=1CE[(i=N+1𝒩(T)0Tσ(t)ϕ(t)𝑑t)2]P(𝒩ϵ(T)=N),\displaystyle\sum_{N=1}^{\infty}CE\left[\left(\sum_{i=N+1}^{\mathcal{N}(T)}\int_{0}^{T}\sigma(t)\phi(t)\;dt\right)^{2}\right]P(\mathcal{N}^{\epsilon}(T)=N), (64)

where all expectations are conditional on 𝒩ϵ(T)=N\mathcal{N}^{\epsilon}(T)=N.

To finish the theorem the following moments of τir,ϵ\tau_{i}^{r,\epsilon} are used

E[τir,ϵ]=bϵr,E[|τir,ϵ|2]=bD2ϵ3r3+b2ϵ2r2,E[|τir,ϵ|4]=b4ϵ4r4+6b3D12ϵ5r5+15b2D14ϵ6r6+15bD16ϵ7r7.E[\tau_{i}^{r,\epsilon}]=\frac{b\epsilon}{r},\quad E[|\tau_{i}^{r,\epsilon}|^{2}]=\frac{bD^{2}\epsilon^{3}}{r^{3}}+\frac{b^{2}\epsilon^{2}}{r^{2}},\quad E[|\tau_{i}^{r,\epsilon}|^{4}]=\frac{b^{4}\epsilon^{4}}{r^{4}}+6\frac{b^{3}D_{1}^{2}\epsilon^{5}}{r^{5}}+15\frac{b^{2}D_{1}^{4}\epsilon^{6}}{r^{6}}+15\frac{bD_{1}^{6}\epsilon^{7}}{r^{7}}. (65)

Thus the first term in (64) is

(rϵ)2E[|τir|4]=O(ϵ2).\left(\frac{r}{\epsilon}\right)^{2}E[|\tau_{i}^{r}|^{4}]=O(\epsilon^{2}). (66)

The second term in (64) is

E[|(rϵτir,ϵb)ϕ(τid,ϵ)|2]=\displaystyle E\left[\left|\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}-b\right)\phi(\tau_{i}^{d,\epsilon})\right|^{2}\right]= E[(rϵτir,ϵb)2]E[ϕ(τid,ϵ)2]\displaystyle E\left[\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}-b\right)^{2}\right]E\left[\phi(\tau_{i}^{d,\epsilon})^{2}\right] (67)
=\displaystyle= E[((rϵτir,ϵ)22brϵτir,ϵ+b2)]E[ϕ(τid,ϵ)2]\displaystyle E\left[\left(\left(\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}\right)^{2}-2b\frac{r}{\epsilon}\tau_{i}^{r,\epsilon}+b^{2}\right)\right]E\left[\phi(\tau_{i}^{d,\epsilon})^{2}\right] (68)
=\displaystyle= O(ϵ3)\displaystyle O(\epsilon^{3}) (69)

where the expectation turns into a product because τir,ϵ\tau_{i}^{r,\epsilon} and τid,ϵ\tau_{i}^{d,\epsilon} are independent. The third term of (64), E[|ϕ(τid,ϵ)ϕ(τid)|2]E\left[|\phi(\tau_{i}^{d,\epsilon})-\phi(\tau_{i}^{d})|^{2}\right], is zero because τid,ϵ\tau_{i}^{d,\epsilon} and τid\tau_{i}^{d} have the same distribution.

For the last “remainder” term, it is written as a comparison between 𝒩(T)\mathcal{N}(T) and 𝒩ϵ(T)\mathcal{N}^{\epsilon}(T),

N=1\displaystyle\sum_{N=1}^{\infty} CE[(i=N+1𝒩(T)0Tσ(t)ϕ(t)𝑑t)2|𝒩ϵ(T)=N]P(𝒩ϵ(T)=N)\displaystyle CE\left[\left.\left(\sum_{i=N+1}^{\mathcal{N}(T)}\int_{0}^{T}\sigma(t)\phi(t)\;dt\right)^{2}\right|\mathcal{N}^{\epsilon}(T)=N\right]P(\mathcal{N}^{\epsilon}(T)=N) (70)
=\displaystyle= CE[(i=𝒩ϵ(T)+1𝒩(T)0Tσ(t)ϕ(t)𝑑t)2]\displaystyle CE\left[\left(\sum_{i=\mathcal{N}^{\epsilon}(T)+1}^{\mathcal{N}(T)}\int_{0}^{T}\sigma(t)\phi(t)\;dt\right)^{2}\right] (71)
=\displaystyle= N<ME[(i=N+1M0Tσ(t)ϕ(t)𝑑t)2|𝒩ϵ(T)=N<𝒩(T)=M]P(𝒩ϵ(T)<𝒩(T))\displaystyle\sum_{N<M}E\left[\left.\left(\sum_{i=N+1}^{M}\int_{0}^{T}\sigma(t)\phi(t)\;dt\right)^{2}\right|\mathcal{N}^{\epsilon}(T)=N<\mathcal{N}(T)=M\right]P(\mathcal{N}^{\epsilon}(T)<\mathcal{N}(T)) (72)

If 𝒩ϵ(T)<𝒩(T)\mathcal{N}^{\epsilon}(T)<\mathcal{N}(T), then the processes EtϵE_{t}^{\epsilon} and EtE_{t} must be at least bb units apart. Thus

P(𝒩ϵ(T)<𝒩(T))P(|Eϵ(t)E(t)|>b).P(\mathcal{N}^{\epsilon}(T)<\mathcal{N}(T))\leq P(|E^{\epsilon}(t)-E(t)|>b). (73)

From theorem 1, this quantity tends to zero as ϵ0\epsilon\to 0.

Thus, the sum in (53) converges due to the fast decay of P(Nϵ(T)=n)P(N_{\epsilon}(T)=n) as shown in Eq.(45). Tonelli’s theorem allows the limit as ϵ0\epsilon\to 0 to exchange with the infinite sum. This along with Theorem 1 completes the proof. ∎

IV Conclusions

In this paper a threshold model for moisture and rain was shown to converge to interesting processes for various modes of convergence. The original threshold model processes, defined in equation (2), originated from Stechmann and Neelin, (2014) and were studied in Hottovy and Stechmann, (2015). There, exact formulas were derived for various quantities of interest such as stationary distributions and expected rainfall. In Abbott et al., (2016) a connection was made between the rain process from the threshold model and the point process defined in equation (5). Here convergence for the moisture processes were defined and shown for the Fokker-Planck equation as well as the paths of the processes. Furthermore, the convergence of the rain process were shown in mean square difference with respect to the space of generalized functions.

Using a point process to approximate rainfall allows simplification for computation and exact formulas. For example, the autocorrelation function is known exactly in the case of point processes as shown in Abbott et al., (2016). Furthermore, point processes have been studied extensively in the neural science literature Sacerdote and Giraudo, (2013) and many statistics have been derived.

The proofs shown here are revealing on their own. The Fokker-Planck derivation in Section III.1 shows the density for the moisture in the rain state tends to zero while the flux term remains allowing for the “teleporting” boundary condition that arises for limiting moisture process. For the convergence of paths of moisture shown in Theorem 1 the moisture process must first be decoupled into a moistening and precipitating process. Then the moistening process is shown to converge (Theorem 1) while the precipitating process contains all of the discontinuities. Finally, the proof of convergence of the rain processes in Theorem 2 gives estimates that would be useful for determining the error rates for using the point process approximation.


Acknowledgements. The research of author Hottovy is partially supported by the National Science Foundation under Grant DMS-1815061.

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