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16 Apr 2019

16 Apr 2019

Fitting a stochastic fire spread model to data

^{1}Dept. of Statistics, University of British Columbia, Kelowna, BC, Canada V1V 1V7^{2}Dept. of Statistical and Actuarial Sciences, University of Western Ontario, London, Ontario, Canada N6A 5B7

^{1}Dept. of Statistics, University of British Columbia, Kelowna, BC, Canada V1V 1V7^{2}Dept. of Statistical and Actuarial Sciences, University of Western Ontario, London, Ontario, Canada N6A 5B7

Abstract

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As the climate changes, it is important to understand the effects on the environment. Changes in wildland fire risk are an important example. A stochastic lattice-based wildland fire spread model was proposed by Boychuk et al. (2007), followed by a more realistic variant (Braun and Woolford, 2013). Fitting such a model to data from remotely sensed images could be used to provide accurate fire spread risk maps, but an intermediate step on the path to that goal is to verify the model on data collected under experimentally controlled conditions. This paper presents the analysis of data from small-scale experimental fires that were digitally video-recorded. Data extraction and processing methods and issues are discussed, along with an estimation methodology that uses differential equations for the moments of certain statistics that can be derived from a sequential set of photographs from a fire. The interaction between model variability and raster resolution is discussed and an argument for partial validation of the model is provided. Visual diagnostics show that the model is doing well at capturing the distribution of key statistics recorded during observed fires.

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How to cite.

Wang, X. J., Thompson, J. R. J., Braun, W. J., and Woolford, D. G.: Fitting a stochastic fire spread model to data, Adv. Stat. Clim. Meteorol. Oceanogr., 5, 57-66, https://doi.org/10.5194/ascmo-5-57-2019, 2019.

1 Introduction

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The risk of large catastrophic wildland fires appears to be increasing in many countries as evidenced by recent high-profile wildfire events including the 2016 Fort McMurray fire in Canada and the “Black Saturday” bushfires of 2009 in Australia. Of heightened concern are climate change impacts on wildland fires. Weber and Stocks (1998) postulated that increasing temperatures could lead to an increased number of wildland fire ignitions, a longer fire season, and/or an increased number of days with severe fire weather. In regions of Canada, fire seasons are getting longer (Albert-Green et al., 2012) and fire risk has been shown to be increasing (Woolford et al., 2010, 2014). Annual area burned has increased and has been connected to human-induced climate change (Gillett et al., 2004). Studies that analyzed data output from climate model scenarios have suggested increased severity ratings (Flannigan and Van Wagner, 1991), area burned (Flannigan et al., 2005), ignitions (Wotton et al., 2010), and a longer fire season (Wotton and Flannigan, 1993).

Consequently, the development of accurate, spatially explicit fire spread models is of crucial importance for understanding aspects of fire behaviour and forecasting whether and how a wildland fire may spread. Many fire spread models are deterministic and although there have been some efforts to incorporate randomness into such models, there is also a strong need to develop stochastic fire spread models along with the statistical methodology for calibrating such models to data so that the uncertainty associated with where and when a fire might spread can be determined. A well-calibrated fire spread model can be used at the incident level for individual fire management or be coupled to fire occurrence and fire duration models in a simulation-based approach for longer-term strategic planning by wildland fire management agencies.

Taylor et al. (2013; Sect. 3) provided a detailed review of fire growth, discussing the physical process of fire growth, fire spread rate models, and spatially explicit fire growth models, including a discussion of deterministic fire spread models, such as Prometheus (Tymstra, 2005) and FARSITE (Finney, 2004), which play important roles in operational fire spread modelling by fire management agencies. Although these simulators are well established and used frequently in Canada, the United States, and in several other countries, their chief weakness is that they are not stochastic. Fire managers would benefit from probability maps to indicate where a currently burning fire may spread.

Burn-P3 (e.g. Parisien et al., 2005) used the deterministic Prometheus fire spread model in an ensemble-type simulation procedure which randomizes weather sequences in order to induce randomness to produce “burn probability maps”, typically a gridded map of the susceptibility of the landscape to be burned by wildfire over a large study area over the course of a year. We note that this kind of procedure may be more appropriate for studying fire risk on large temporal and spatial scales, such as producing an annual burn probability map for a region or district where wildland fires are managed. However, modelling at the incident level, namely quantifying whether or not a given fire may spread and where it may spread to along with estimating the uncertainty associated with the spread of a single fire, requires a different approach.

We note that deterministic models, such as Prometheus, can and are used at the incident level to model the spread of a single fire given local conditions. We also note that there has been some work to incorporate randomness into the Prometheus fire growth engine. For example, Garcia et al. (2008) attempted to introduce stochasticity to the Prometheus model via a block bootstrap procedure, and Han and Braun (2014) incorporated uncertainty through introducing an error component into the underlying model for rate of spread (ROS), as a parametric bootstrap. Nevertheless, much work remains to be done in order to make these procedures operational.

In the meantime, several other models have been considered by several other authors, including the stochastic lattice-spread model of Boychuk et al. (2007) that was studied by Braun and Woolford (2013), who also introduced an interesting variant of that lattice-spread model in their paper. This modified Boychuk model is used in our study herein where we address some statistical issues, studying the model from the point of view of data analysis not through operational implementation, which we illustrate through the analysis of some small experimental fires or “microfires”. We purposely restrict our analysis to such microfire data in order to study the model on data collected under controlled experimental conditions.

We study the modified version of the Boychuk et al. (2007) model as described
in Braun and Woolford (2013). In its simplest special case one assumes the
landscape to be flat with a fuel type and density that is homogeneous, the
weather conditions to be constant, and no wind. On this landscape we impose a
regular square *n*×*m* lattice. Each of the grid cells can be in one of
three possible states: unburned fuel (F), burning fuel (B),
or burnt out (O). Transitions between these states occur as follows:
initially (i.e. at time *t*=0), the grid cell at some location (*i*,*j*) is
in state B, while all other cells are in state F. The fire
burning in cell (*i*,*j*) will spread to each of its four nearest neighbours
(i.e. north, south, east, and west) in random amounts of time ${T}_{\mathrm{0},\mathrm{1}},{T}_{\mathrm{0},-\mathrm{1}},{T}_{\mathrm{1},\mathrm{0}},$ and ${T}_{-\mathrm{1},\mathrm{0}}$, provided it does not burn out first.
Specifically, at time *T*_{0,1}, the cell at $(i,j+\mathrm{1})$ makes the transition
from state F to B, if the cell is not already in state
B. Similar transitions are made by cell $(i,j-\mathrm{1})$ at ${T}_{\mathrm{0},-\mathrm{1}}$,
cell $(i+\mathrm{1},\mathrm{0})$ at *T*_{1,0}, and cell $(i-\mathrm{1},\mathrm{0})$ at ${T}_{-\mathrm{1},\mathrm{0}}$. These times
are assumed to be independent and exponentially distributed with a mean of
1∕*λ*. Once a cell has made a transition to state B, fire
spreads from that cell to the sites of its nearest neighbourhood at a new set
of independent exponential random times. The time until the next burning cell
burns out is exponentially distributed with rate *μ**n*, where *n* is the
current number of burning cells. At that time, the cell that has been in
state B longest makes the transition to state O. Once in
state O, a grid cell will make no further transitions.

We note that the Boychuk model and its variant are much more general than described above. Nonhomogeneous conditions, due to changing weather, variations in fuel type, moisture content, and topography can be handled. These issues are described in detail in the Boychuk et al. (2007) paper.

The purpose of the current paper is to study the modified Boychuk model from the point of view of data analysis. In particular, we assume we have video data from a burning wildfire and investigate the following two questions. First, is it possible to fit the model to the data? And secondly, is it possible to carry out model assessment? We will argue in this paper that it is possible to show that the parameters for the simplest case of this model can be estimated from a sequence of pictures of a single fire. As in Zhang et al. (1992), we are studying the characteristics of the modified Boychuk model in the context of data collected on a tiny fire burned under very controlled conditions. Although Zhang et al. (1992) burned ordinary paper, we have chosen to use waxed paper in our experiment because it burns more cleanly. In an earlier paper (Braun and Woolford, 2013), we showed that the lattice grid cell size can be calibrated using given data, and we studied particular ways to assess the appropriateness of the model, but a general parameter estimation scheme was not proposed in that paper.

The rest of this paper proceeds as follows. In the next section, we describe our burning experiments and how we extract data from a video clip of a microfire. In Sect. 3, we describe a method to estimate the two parameters of the basic interacting particle model using data on numbers of burning grid sites and numbers of neighbouring unburned sites. We next summarize the results from the experiments and then provide specific tools to assess the fit of the model to the data. We conclude the paper with our observations and our ideas about future work on related problems.

We note that work has been carried out in incorporating fire rate of spread variability using variations in weather streams (e.g. Anderson et al., 2007); here, our focus is on what statisticians refer to as “unexplained” variation.

2 Microfire experiments

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Data for testing the usefulness of the grid-based fire spread model were
obtained from a set of small-scale experimental fires. The experiments were
conducted under a fume hood in a laboratory, at a temperature of
20 ^{∘}C where wind was absent and slope and aspect effects were
negligible. In each experimental run, the material used for fuel was a
25.4 cm × 38.1 cm sheet of dry waxed paper, which had been soaked
for 1 h in an aqueous solution of potassium nitrate (as in Zhang et al.,
1992) and dried for 1 h on a hot plate set to 60 ^{∘}C. The
concentration of the solution was 0.1 g KNO_{3} mL^{−1}. The
sheet was suspended, horizontally, 2.54 cm above the base of the pan to
permit airflow. The paper was ignited, from below, at a point near its
center, and an Olympus Stylus^{®} 600 camera,
which was suspended on a tripod approximately 48 cm above the paper, was
used to digitally record the experimental fire until most of the paper was
consumed.

The potassium nitrate treatment protocol was adopted for two reasons. First, it prevented flaming and, in fact, induced smouldering combustion. This was important from a lab safety standpoint. Second, flames tend to obscure the pattern of combustion, and this leads to additional image processing issues when extracting the data from the video footage. To further simplify the image processing methodology, these experimental runs were conducted in darkness. This resulted in video footage in which only burning sites were visible; for example, see the screenshots from one of the experimental runs that are displayed in Fig. 1.

A total of 10 microfires were obtained, but only six were retained for further study, due to issues deemed to be unrelated to the study. These issues had to do with difficulties in processing the images from the video streams, due to the presence of fire-spotting, which produced small fires outside the perimeter of the original fire, and due to accidental changes in lighting, which interacted with the reflectivity of the waxed paper. In both cases, this rendered data that will be studied in the future, but which were not amenable to the very quick and simple data extraction and image segmentation procedures that will be described later. In future work, we plan to develop new image segmentation methodology to handle these situations, but as our real focus here is on applying a stochastic model to real data, we feel this is beyond the scope of the current paper.

The open-source program ffmpeg (Libav, 2010–2013) was used to freeze-frame each movie at approximately half-second intervals to obtain clear image captures with timestamps. These captured images were then saved as JPEG files, readable in the R system (R Core Team, 2018). For illustrative purposes, the images for the third experimental run are shown in Fig. 1 (the images for the remaining five microfires can be found in the Supplement submitted along with this paper). The original images were a combination of several colours: yellow, red, grey, black, etc. In order to convert the image matrices into a usable form, conversion to three colours, red (burning), green (fuel), and black (burnt out), was necessary.

This image segmentation problem was greatly simplified because of the use of darkness in the experimental setup. Each grid cell is unburned until it burns (and is lit up in the video footage) and is burnt out for all remaining time. Therefore, the time(s) at which each grid cell burns can be identified from the time series of the red, green, and blue (rgb) measurements. The series corresponding to red is most useful for this purpose. Prior to burning, the values are at or near 0; thus all images corresponding to these times can be set to “green”. After burning, the values are again at or near 0; these can be set to “black”. The values at the time(s) of burning can be set to “red”. The resulting patterns, corresponding to the images in Fig. 1 are displayed in Fig. 2.

Finally, the colour-coded images were converted to a numeric matrix corresponding to the green, red, and black pixels of the image array. We assigned the colour green to the value 0, red to the value 1, and black to the value 2. The numbers of 0, 1, and 2 were counted, which gave the numbers of unburned fuel sites, the number of burning sites, and the number of burnt-out sites. In addition, the number of fuel sites neighbouring burning sites at each time point were also counted. To illustrate, the counts for each of these statistics during the first 30 s are listed in Table 1 for the third microfire. The detailed smoldering experiment data for all the microfires are provided in the Supplement.

3 Model fitting

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We now develop the methodology required to fit the grid-based fire spread
model to the data extracted from a sequence of images of a growing fire.
Referring to data such as in Table 1, let *X*(*t*) denote the
number of burning sites at time *t* and *Y*(*t*) denote the number of sites
that are burnt out by time *t*. In addition, let *B*_{ℓ}(*t*), *B*_{r}(*t*),
*B*_{u}(*t*), and *B*_{d}(*t*) denote the number of burning sites with unburnt fuel in
the site immediately on their left (west), right (east), above (north/up),
or below (south/down), respectively. Also, let

$$\begin{array}{ll}{\displaystyle}& {\displaystyle}x\left(t\right)=E\left[X\right(t\left)\right],\\ {\displaystyle}& {\displaystyle}y\left(t\right)=E\left[Y\right(t\left)\right],\\ {\displaystyle}& {\displaystyle}{b}_{\mathrm{\ell}}\left(t\right)=E\left[{B}_{\mathrm{\ell}}\right(t\left)\right],\\ {\displaystyle}& {\displaystyle}{b}_{\mathrm{r}}\left(t\right)=E\left[{B}_{\mathrm{r}}\right(t\left)\right],\\ {\displaystyle}& {\displaystyle}{b}_{\mathrm{u}}\left(t\right)=E\left[{B}_{\mathrm{u}}\right(t\left)\right],\end{array}$$

and

$$}{b}_{\mathrm{d}}\left(t\right)=E\left[{B}_{\mathrm{d}}\right(t\left)\right].$$

According to the model rules and arguing as in Braun and Kulperger (1993), we have the relations

$$\begin{array}{}\text{(1)}& {\displaystyle}& {\displaystyle}{y}^{\prime}\left(t\right)=\mathit{\mu}x\left(t\right),\text{(2)}& {\displaystyle}& {\displaystyle}{x}^{\prime}\left(t\right)=-\mathit{\mu}x\left(t\right)+\mathit{\lambda}\left({b}_{\mathrm{\ell}}\left(t\right)+{b}_{\mathrm{r}}\left(t\right)+{b}_{\mathrm{u}}\left(t\right)+{b}_{\mathrm{d}}\left(t\right)\right),\end{array}$$

and initial conditions of *y*(0)=0 and *x*(0)=1.

These equations hold for both the original Boychuk model as well as the variant introduced by Braun and Woolford (2013). This result seems surprising since the Braun and Woolford variant is non-Markovian, while the Boychuk model is. However, it is important to note that the differential equations are for population level quantities. They are also only a partial description of the process dynamics. However, they contain enough process information to allow for construction of moment estimators for the process parameters as we now demonstrate.

The notation in the ensuing discussion can be simplified by making the substitution

$$}g\left(t\right)={b}_{\mathrm{\ell}}\left(t\right)+{b}_{\mathrm{r}}\left(t\right)+{b}_{\mathrm{u}}\left(t\right)+{b}_{\mathrm{d}}\left(t\right).$$

Then

$$\begin{array}{}\text{(3)}& {x}^{\prime}\left(t\right)=-\mathit{\mu}x\left(t\right)+\mathit{\lambda}g\left(t\right).\end{array}$$

By adding Eqs. (1) and (1), we obtain:

$$\begin{array}{}\text{(4)}& {x}^{\prime}\left(t\right)+{y}^{\prime}\left(t\right)=\mathit{\lambda}g\left(t\right).\end{array}$$

We can estimate the functions *x*(*t*) and *y*(*t*) using *X*(*t*) and *Y*(*t*),
respectively. In fact, improved estimates of these functions can be obtained
by applying a local linear kernel smoother to the (*t*,*X*(*t*)) data and (*t*,*Y*(*t*)) data respectively. Similarly, estimates of *g*(*t*) can be improved by a
local constant smoother. We used the locpoly function in the
KernSmooth package (Wand, 2015) with an automatically selected
smoothing parameter. The software also allows for estimation of the first
derivatives *x*^{′}(*t*) and *y*^{′}(*t*) from the same data sets (see Wand and Jones,
1995, for example).

Substituting these local linear kernel-smoothing-based estimates
${\widehat{y}}^{\prime}\left(t\right)$ and $\widehat{x}\left(t\right)$ into Eq. (1),
continuous least squares can then be applied to estimate *μ*. That is,

$$\widehat{\mathit{\mu}}=\mathrm{arg}\underset{\mathit{\mu}}{min}\underset{{t}_{\mathrm{1}}}{\overset{{t}_{n}}{\int}}\left({\widehat{y}}^{\prime}\right(t)-\mathit{\mu}\widehat{x}(t){)}^{\mathrm{2}}\mathrm{d}t,$$

where ${\widehat{y}}^{\prime}\left(t\right)$ and $\widehat{x}\left(t\right)$ are the smoothed estimates described in the preceding paragraph.

An estimator for *λ* can be obtained from the estimated version of
Eq. (2) similarly:

$$\widehat{\mathit{\lambda}}=\mathrm{arg}\underset{\mathit{\lambda}}{min}\underset{{t}_{\mathrm{1}}}{\overset{{t}_{n}}{\int}}\left({\widehat{x}}^{\prime}\right(t)+{\widehat{y}}^{\prime}(t)-\mathit{\lambda}\widehat{g}(t){)}^{\mathrm{2}}\mathrm{d}t.$$

It is important to note that the pixel size induced by the camera specifications has nothing to do with the size of the grid cells imposed on the lattice underlying the stochastic spread model. Thus, a scale parameter must be selected, which is used to expand or contract the default pixel sizes so that the spread model process can be used as a realistic approximation for the actual data. Specifically, we adjust the scale factor until the range of the observed data matches the range of the simulated data by using the estimated parameters.

In this paper, slightly different amounts of scaling are used for six replicates of the dark smouldering experiment in order to match the pixel size for the camera and the grid cell size on the lattice. The scale factors for all replicates are listed in Table 2. Note that these scale factors are estimated specifically for our microfire data only. One can reproduce the same results by using this fire spread model, based on the same microfire data.

4 Results

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As noted earlier, the sequence of fire images is displayed in Fig. 1 for one of the microfires. The corresponding thresholded images are displayed in Fig. 2. Based on these images, counts of the various statistics (as listed in Sect. 3) were taken, at a number of different grid resolutions (as discussed in Sect. 3.2). Table 1 displays the counts at one of the resolutions, and the third row of Table 2 contains the resulting parameter estimates and the amount of scaling performed to increase the pixel size.

The remaining rows of Table 2 contain the parameter estimates
and scalings required for the other five microfires. We see that the fires
required different amounts of scaling, and the estimates of *μ* range from
0.34 grid cells per second to 0.49 grid cells per second. The estimates of
*λ* range from 0.28 to 0.40. In all cases, the burn out parameter
exceeds the spread rate parameter, which suggests a subcritical process. Thus,
the fires would be expected to ultimately die out with probability 1.

By simulating from the fitted model and re-estimating the parameters, it is
possible to assess bias and variability of the parameter estimates. We have
chosen to display the results of this assessment for the third microfire in
Fig. 5 using box plots to graphically summarize the
distribution of the estimates *μ* and *λ* for the simulated data
sets. Horizontal lines have been drawn to indicate the locations of *μ*
(solid) and *λ* (dashed). What is immediately evident from the graphs
is that both *μ* and *λ* appear to be underestimated in the
simulations: the medians of the estimates from the simulated data are both
about 0.02 less than the values used to produce the simulated data.

The box plots also show that the distributions of the parameter estimates are approximately symmetric, and the amount of variability is of the same order as the bias. That is, if these simulations were viewed as a parametric bootstrap, the standard errors for the two estimators are approximately 0.01. Thus, the bias dominates the MSE, and the root-MSE is approximately 0.022 for both estimators.

Box plots for the other five fires (not shown) are quite similar to what appears
in Fig. 5. All six fires exhibit the same degree and
direction of bias. Table 2 contains information on the
medians for the estimates of *λ* and *μ* from simulations of each of
the fitted models. In all cases, the medians of the parameter estimates from
the simulated data are slightly below the parameter values used in the
simulations.

To assess the adequacy of the grid-based fire spread model for this particular data set, we again simulated realizations of fire spread at the estimated parameter values, using the chosen grid resolution. The results are the sequence of pictures in Fig. 3. The images have been plotted at approximately 5 s intervals. We see from these pictures that the fire size and the thickness of the fire perimeter are similar to the analogous quantities for the thresholded images at corresponding times. The boundary is somewhat less smooth in the simulation pictures than in the actual fire, but the overall shapes are fairly similar. The simulated fire appears to have grown somewhat larger than the observed fire. However, Fig. 4 shows the results of another simulation run where similar qualitative behaviour is evident but where the fire sizes tend to be somewhat smaller than observed.

Such plots are limited in their usefulness. In this case, we can see that there are differences between the simulated pictures and the actual data, but it is difficult to tell if these differences are due to the variability we are trying to model or if these are failures of the model itself.

As another check on the appropriateness of the model, we can compare the burning cell counts, burnt-out cell counts, and nearest-neighbour statistics for the original data with simulated data from the fitted model (using data from the third microfire only). Figure 6 shows the results of 100 simulated realizations (plotted in grey) with the observed counts for all the other fires (plotted in blue) against time; the observed data for the third microfire are plotted in black.

What is evident from this set of plots is that the range and distribution of
simulated counts of burning sites (based on the observed data from one fire)
match the observed range and distribution of burning sites for other fires
very well. Except for a location shift in the distribution of simulated burnt-out sites and neighbourhood statistics, we also see similarities in the range
and distribution in these cases. The location shift is likely due to the
estimation bias discussed earlier. Note that by increasing both *μ* and
*λ* slightly, we will not see much change in the total number of
burning sites over time, but we will see many more burnt-out sites, for
example. It is also noteworthy that for one of the actual fires, there were
instances of flaming which distorted the camera images at two time points,
reflected in the anomalous spikes in Fig. 6.

These observations provide strong evidence that the model is doing well at capturing distributional behaviour in these dimensions. Further assessment of model goodness of fit is provided in the Supplement submitted along with this paper.

5 Conclusions and further work

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This work is part of an ongoing investigation into the suitability of a simple grid-based interacting particle system for stochastically modelling forest fire spread. Ultimately, we wish to fit such a model to sequences of satellite-based photographs of wildfires. Then, simulations of the model could be used to produce the maps of fire spread risk that are in demand by forest fire managers. Before this can happen, experiments under other conditions on slope and different kinds of fuel and wind conditions must be carried out. This paper represents the analysis of one such set of experiments, and the results appear promising.

What can be firmly concluded is that the parameters for the simplest case of the model can be estimated from a sequential set of photographs from a fire, using differential equations for the moments of certain statistics derivable from a video clip of a fire. A critical element of this estimation is that of scale. We have shown that the “natural” grid cell size can be determined, at least crudely, from a characteristic of the fire: the ratio of burnt-out area to the square of the burning area. Information about the scale is also likely related to the variability of the fire spread; this is an issue that can be addressed by studying an ensemble of experimental fires conducted under the same conditions. It should be noted that we have thresholded individual images; other methods taking account of the time sequence at each pixel (and at neighbouring pixels) may lead to more accurate counts of neighbourhood statistics and burning and burnt-out sites, given that flames and/or smoke cause distortions. The paper by Fang et al. (2007) indicates another possible approach that could be adopted.

We have developed some goodness-of-fit methods. A simple visual assessment based on comparing burn patterns simulated from the fitted model with the observed pattern is a useful, if limited, first step. This method of assessment gives some assurance that the model appears to reasonably fit the data. However, such a comparison is highly subjective and will not necessarily generalize to cases where, for example, the assumption of isotropy is invalid. The very nature of a stochastic model leads to different possible patterns under the same conditions. Hence, the following question arises: how different can the patterns be from the observed pattern before one might conclude that the model has failed?

What is needed, in general, is a metric for scoring spatial burn pattern maps that evolve over time in terms of their shape and boundary characteristics. In this paper, we have proposed the four nearest-neighbourhood statistics as belonging to such a set of measures. On the basis of an informal bootstrap procedure applied to these statistics, we have a fair degree of confidence that the model is capturing some of the stochastic behaviour of the actual fire.

Data availability

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Data availability.

For the purposes of reproducible research, we have uploaded the data (frozen video frames) and R code to the Open Science Framework repository. See Braun et al. (2018). The frozen video frames can be downloaded and unzipped, and then the file called MainDriver.R can be run in R to process the data as carried out in this paper.

Supplement

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Supplement.

The supplement related to this article is available online at: https://doi.org/10.5194/ascmo-5-57-2019-supplement.

Author contributions

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Author contributions.

DGW and WJB developed the modelling methodology and under their direction, XJW and JRJT designed and carried out the experiments. XJW and WJB designed and carried out the simulation experiments that were used to assess the model.

Competing interests

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Competing interests.

The authors declare that they have no conflict of interest.

Acknowledgements

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Acknowledgements.

The authors gratefully acknowledge support from the Natural Sciences and Engineering Research Council of Canada through individual Discovery Grants to W. John Braun and Douglas G. Woolford and the Canadian Statistical Sciences Institute through its Collaborative Research Team funding program. The authors are also grateful to Andrew Jirasek for facilitating access to his laboratory where the experiments were conducted.

Review statement

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Review statement.

This paper was edited by Christopher Paciorek and reviewed by two anonymous referees.

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Short summary

This paper presents the analysis of data from small-scale laboratory experimental smouldering fires that were digitally video-recorded. The video images of these fires bear a resemblance to remotely sensed images of wildfires and provide an opportunity to fit and assess a spatial model for fire spread that attempts to account for uncertainty in fire growth. We found that the fitting method is feasible, and the spatial model provides a suitable mathematical for the fire spread process.

This paper presents the analysis of data from small-scale laboratory experimental smouldering...

Advances in Statistical Climatology, Meteorology and Oceanography

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