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loop branch for mutable timestepper added parameters to EKSStabilityTimestepper added DMC timestepper timestepper interface bugfixes format externalize dim-check error, bugfix stableEKS timestep Unscented consistent, and tests pass update Delt =... to timestepper = ... in unit tests` update example unit test for constructors format consistency wiith 1,9 (not-yet-refined) timestepper example with various plots Timestepper termination condition upheld docstrings unit tests loosen tol typo improved output example loosen tolerance cleaned up plots and experiment repeated for many runs format removed nothing # hide, and added more strings rename timestepper to scheduler added continue options for DMC run test longer preliminary docs for scheduler comparison example improve plot legend and docs typos etc examples/LearningRateSchedulers/compare_schedulers.jl move docs page out of examples subfolder move docs in contents modify conclusions API docstrings docs and example improvements added SEKI and UKI tests for schedulers (UKI fails), fixed dangerous pattern where G applied to untransformed coordinates format uki example and docs consistency with seeding for plots separate posterior vs optimize, add uki descriptions format typo easier tests for UKI, but it still fails
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# [Learning Rate Schedulers (a.k.a) Timestepping](@id learning-rate-schedulers) | ||
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## Overview | ||
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We demonstrate the behaviour of different learning rate schedulers through solution of a nonlinear inverse problem. | ||
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In this example we have a model that produces the exponential of a sinusoid ``f(A, v) = \exp(A \sin(t) + v), \forall t \in [0,2\pi]``. Given an initial guess of the parameters as ``A^* \sim \mathcal{N}(2,1)`` and ``v^* \sim \mathcal{N}(0,5)``, the inverse problem is to estimate the parameters from a noisy observation of only the maximum and mean value of the true model output. | ||
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We shall compare the following configurations of implemented schedulers. | ||
1. Fixed, long timestep `DefaultScheduler(0.5)` - orange | ||
2. Fixed, short timestep `DefaultScheduler(0.02)` - green | ||
3. Adaptive timestep (designed originally to ensure EKS remains stable) `EKSStableScheduler()` [Kovachki & Stuart 2018](https://doi.org/10.1088/1361-6420/ab1c3a) - red | ||
4. Misfit controlling timestep (Terminating) `DataMisfitController()` [Iglesias & Yang 2021](https://doi.org/10.1088/1361-6420/abd29b) - purple | ||
5. Misfit controlling timestep (Continuing beyond Terminate condition) `DataMisfitController(on_terminate="continue")` - brown | ||
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## Timestep and termination time | ||
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Recall, for example for EKI, we perform updates of our ensemble of parameters ``j=1,\dots,J`` at step ``n = 1,\dots,N_\mathrm{it}`` using | ||
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`` \theta_{n+1}^{(j)} = \theta_{n}^{(j)} - \dfrac{\Delta t_n}{J}\sum_{k=1}^J \left \langle \mathcal{G}(\theta_n^{(k)}) - \bar{\mathcal{G}}_n \, , \, \Gamma_y^{-1} \left ( \mathcal{G}(\theta_n^{(j)}) - y \right ) \right \rangle \theta_{n}^{(k)},`` | ||
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where ``\bar{\mathcal{G}}_n`` is the mean value of ``\mathcal{G}(\theta_n)`` | ||
across ensemble members. We denote the current time ``t_n = \sum_{i=1}^n\Delta t_i``, and the termination time as ``T = t_{N_\mathrm{it}}``. | ||
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!!! note | ||
Adaptive Schedulers typically try to make the biggest update that controls some measure of this update. For example, `EKSStableScheduler()` controls the frobenius norm of the update, while `DataMisfitController()` controls the Jeffrey divergence between the two steps. Largely they follow a pattern of scheduling very small initial timesteps, leading to much larger steps at later times. | ||
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There are two termination times that the theory indicates are useful | ||
- ``T=1``: In the linear Gaussian case, the ``\{\theta_{N_\mathrm{it}}\}`` will represent the posterior distribution. In nonlinear case it should still provide an approximation to the posterior distribution. Note that as the posterior does not necessarily optimize the data-misfit we find ``\bar{\theta}_{N_\mathrm{it}}`` (the ensemble mean) provides a conservative estimate of the true parameters, while retaining spread. It is noted in [Iglesias & Yang 2021](https://doi.org/10.1088/1361-6420/abd29b) that with small enough (or well chosen) step-sizes this estimate at ``T=1`` satisfies a discrepancy principle with respect to the observational noise. | ||
- ``T\to \infty``: Though theoretical concerns have been made with respect to continuation beyond ``T=1`` for inversion methods such as EKI, in practice we commonly see better optimization of the data-misfit, and thus better representation ``\bar{\theta}_{N_\mathrm{it}}`` to the true parameters. As expected this procedure leads to ensemble collapse, and so no meaningful information can be taken from the posterior spread, and the optimizer is not likely to be the posterior mode. | ||
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## The experiment with EKI & UKI | ||
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We assess the schedulers by solving the inverse problem with EKI and UKI (we average results over 100 initial ensembles in the case of EKI). We will not draw comparisons between EKI and UKI here, rather we use them to observe consistent behavior in the schedulers. Shown below are the solution plots of one solve with each timestepper, for both methods. | ||
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![Solution EKI](assets/ensemble_compare_scheduler.png) ![Solution UKI](assets/ensemble_uki_compare_scheduler.png) | ||
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*Top: EKI, Bottom: UKI. Left: The true model over ``[0,2\pi]`` (black), and solution schedulers (colors). | ||
Right: The noisy observation (black) of mean and max of the model; the distribution it was sampled from (gray-ribbon), and the corresponding ensemble-mean approximation given from each scheduler (colors).* | ||
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To assess the timestepping we show the convergence plot against the algorithm iteration we measure two quantities. | ||
- error (solid) is defined by ``\frac{1}{N_{ens}}\sum^{N_{ens}}_{i=1} \| \theta_i - \theta^* \|^2`` where ``\theta_i`` are ensemble members and ``\theta^*`` is the true value used to create the observed data. | ||
- spread (dashed) is defined by ``\frac{1}{N_{ens}}\sum^{N_{ens}}_{i=1} \| \theta_i - \bar{\theta} \|^2`` where ``\theta_i`` are ensemble members and ``\bar{\theta}`` is the mean over these members. | ||
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![Error vs spread EKI](assets/error_vs_spread_over_iteration_compare_scheduler.png) ![Error vs spread UKI](assets/error_vs_spread_over_iteration_uki_compare_scheduler.png) | ||
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*Top: EKI. Bottom: UKI. Left: the error and spread of the different timesteppers at over iterations of the algorithm for a single run. | ||
Right: the error and spread of the different timesteppers at their final iterations, (for EKI, averaged from 100 initial conditions).* | ||
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Finding the Posterior (terminating at ``T=1``): | ||
- DMC with termination (purple), closely mimics a small-fixed timestep (green) that finishes stepping at ``T=1``. Both retain more spread than other approaches, and DMC is far more efficient, typically terminating after around 10-20 steps, where fixed-stepping takes 50. We see that (for this experiment) this is a conservative estimate, as continuing to solve (e.g. brown) until later times often leads to a better error while still retaining similar "error vs spread" curves (before inevitable collapse). This is consistent with the concept of approximating the posterior, over seeking an optimizer. | ||
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Optimizing the objective function (continuing ``T \to \infty``): | ||
- Large fixed step (orange). This is very efficient, but can get stuck when drawn too large, (perhaps unintuitive from a gradient-descent perspective). It typically also collapses the ensemble. On average it gives lower error to the true parameters than DMC. | ||
- Both EKSStable and DMC with continuation schedulers, perform very similarly. Both retain good ensemble spread during convergence, and collapse after finding a local optimum. This optimum on average has the best error to the true parameters in this experiment. They appear to consistently find the same optimum as ``T\to\infty`` but DMC finds this in fewer iterations. | ||
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### DMC as a default in future? | ||
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This experiment motivates the possibility of making DMC (with/without) continuation a default timestepper in future releases, for EKI/SEKI/UKI. | ||
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Currently we will retain constant timestepping while we investigate further, though the DMC is available for use. | ||
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Please let us know how you get on by setting the keyword argument in EKP | ||
```julia | ||
scheduler = DataMisfitController() # terminating | ||
scheduler = DataMisfitController(on_terminate = "continue") #non-terminating | ||
``` | ||
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!!! warning "Ensemble Kalman Sampler" | ||
We observe blow-up in EKS, when not using the `EKSStableScheduler`. | ||
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[deps] | ||
ColorSchemes = "35d6a980-a343-548e-a6ea-1d62b119f2f4" | ||
Distributions = "31c24e10-a181-5473-b8eb-7969acd0382f" | ||
EnsembleKalmanProcesses = "aa8a2aa5-91d8-4396-bcef-d4f2ec43552d" | ||
Plots = "91a5bcdd-55d7-5caf-9e0b-520d859cae80" |
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# # Comparison of different Learning rate schedulers | ||
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# In this example we have a model that produces the exponential of a sinusoid | ||
# ``f(A, v) = exp(A \sin(t) + v), \forall t \in [0,2\pi]``. Given an initial guess of the parameters as | ||
# ``A^* \sim \mathcal{N}(2,1)`` and ``v^* \sim \mathcal{N}(0,5)``, our goal is | ||
# to estimate the parameters from a noisy observation of the maximum, minimum, | ||
# and mean of the true model output. | ||
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# We repeat the experiment using several timestepping methods with EKI, | ||
# we also repeat the experiment over many seeds | ||
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# We produce 3 plots: | ||
# (1) Final model ensembles of a single run, and reproduction of the observed data (max & mean of model) | ||
# (2) Convergence of a single run over iterations, and the average performance over many runs. | ||
# (3) Convergence of a single run over algorithm time, and the average performance ovver many runs. | ||
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# First, we load the packages we need: | ||
using LinearAlgebra, Random | ||
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using Distributions, Plots, ColorSchemes | ||
using Plots.PlotMeasures | ||
using EnsembleKalmanProcesses | ||
using EnsembleKalmanProcesses.ParameterDistributions | ||
const EKP = EnsembleKalmanProcesses | ||
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## We set up the file syste, | ||
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homedir = pwd() | ||
println(homedir) | ||
figure_save_directory = homedir * "/output/" | ||
data_save_directory = homedir * "/output/" | ||
if ~isdir(figure_save_directory) | ||
mkdir(figure_save_directory) | ||
end | ||
if ~isdir(data_save_directory) | ||
mkdir(data_save_directory) | ||
end | ||
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# Seed for pseudo-random number generator. | ||
repeats = 100 | ||
rng_seeds = [199 + 135 * i for i in 1:repeats] | ||
rngs = [Random.MersenneTwister(rs) for rs in rng_seeds] | ||
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# Now, we define a model which generates a sinusoid given parameters ``\theta``: an | ||
# amplitude and a vertical shift. It then is exponentiated, We will estimate these parameters from data. | ||
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# The model adds a random phase shift upon evaluation. | ||
dt = 0.01 | ||
trange = 0:dt:(2 * pi + dt) | ||
function model(amplitude, vert_shift) | ||
return exp.(amplitude * sin.(trange) .+ vert_shift) | ||
end | ||
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# We then define ``G(\theta)``, which returns the observables of the sinusoid | ||
# given a parameter vector. These observables should be defined such that they | ||
# are informative about the parameters we wish to estimate. | ||
function G(u) | ||
theta, vert_shift = u | ||
sincurve = model(theta, vert_shift) | ||
return [maximum(sincurve), mean(sincurve)] | ||
end | ||
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# Suppose we have a noisy observation of the true system. Here, we create a | ||
# pseudo-observation ``y`` by running our model with the correct parameters | ||
# and adding Gaussian noise to the output. | ||
dim_output = 2 | ||
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Γ = 0.1 * I | ||
noise_dist = MvNormal(zeros(dim_output), Γ) | ||
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u_true = [1.0, 0.8] | ||
y_nonoise = G(u_true) | ||
y = y_nonoise .+ rand(rngs[1], noise_dist) | ||
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gr() | ||
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## Solving the inverse problem | ||
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# We now define prior distributions on the two parameters. For the amplitude, | ||
# we define a prior with mean 2 and standard deviation 1. It is | ||
# additionally constrained to be nonnegative. For the vertical shift we define | ||
# a Gaussian prior with mean 0 and standard deviation 5. | ||
prior_u1 = constrained_gaussian("amplitude", 2, 1, 0, Inf) | ||
prior_u2 = constrained_gaussian("vert_shift", 0, 5, -Inf, Inf) | ||
prior = combine_distributions([prior_u1, prior_u2]) | ||
unconstrained_u_true = transform_constrained_to_unconstrained(prior, u_true) | ||
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# We now generate the initial ensemble and set up the ensemble Kalman inversion. | ||
N_ensemble = 50 | ||
N_iterations = 50 | ||
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# Set up some initial plot information | ||
clrs = palette(:tab10) | ||
plt = plot( | ||
trange, | ||
model(u_true...), | ||
c = :black, | ||
label = "Truth", | ||
legend = :topright, | ||
linewidth = 2, | ||
title = "Solution evaluation", | ||
) | ||
xlabel!(plt, "Time") | ||
plt_thin = plot(grid = false, xticks = false, title = "(max, mean)") | ||
for i in 1:2 | ||
plot!( | ||
plt_thin, | ||
trange, | ||
repeat([y_nonoise[i]], length(trange)), | ||
ribbon = [2 * sqrt(Γ[i, i]); 2 * sqrt(Γ[i, i])], | ||
linestyle = :dash, | ||
c = :grey, | ||
label = "", | ||
) | ||
plot!(plt_thin, trange, repeat([y[i]], length(trange)), c = :black, label = "") | ||
end | ||
plt2 = | ||
plot(xlabel = "iterations", yscale = :log10, ylim = [1e-4, 1e2], ylabel = "L2 norm", title = "Example convergence") | ||
plt3 = plot( | ||
xlabel = "algorithm time", | ||
yscale = :log10, | ||
ylim = [1e-4, 1e2], | ||
ylabel = "L2 norm", | ||
title = "Example convergence", | ||
) | ||
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final_misfit = zeros(5, repeats) | ||
final_u_err = zeros(5, repeats) | ||
final_u_spread = zeros(5, repeats) | ||
ts_tmp = [] | ||
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# We run two loops, over `repeats` number of random initial samples | ||
# and over the collection of schedulers `timestepppers` | ||
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for (rng_idx, rng) in enumerate(rngs) | ||
initial_ensemble = EKP.construct_initial_ensemble(rng, prior, N_ensemble) | ||
N_iters = repeat([N_iterations], 5) | ||
schedulers = [ | ||
DefaultScheduler(0.5), | ||
DefaultScheduler(0.02), | ||
EKSStableScheduler(), | ||
DataMisfitController(), | ||
DataMisfitController(on_terminate = "continue"), | ||
] | ||
push!(ts_tmp, schedulers) | ||
for (idx, scheduler, N_iter) in zip(1:length(schedulers), schedulers, N_iters) | ||
ensemble_kalman_process = | ||
EKP.EnsembleKalmanProcess(initial_ensemble, y, Γ, Inversion(); scheduler = scheduler, rng = rng) | ||
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# We are now ready to carry out the inversion. At each iteration, we get the | ||
# ensemble from the last iteration, apply ``G(\theta)`` to each ensemble member, | ||
# and apply the Kalman update to the ensemble. | ||
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u_err = zeros(N_iter + 1) | ||
u_spread = zeros(N_iter + 1) | ||
for i in 1:N_iter | ||
params_i = get_ϕ_final(prior, ensemble_kalman_process) | ||
u_i = get_u_final(ensemble_kalman_process) | ||
u_err[i] = 1 / size(u_i, 2) * sum((u_i .- unconstrained_u_true) .^ 2) | ||
u_spread[i] = 1 / size(u_i, 2) * sum((u_i .- mean(u_i, dims = 2)) .^ 2) | ||
G_ens = hcat([G(params_i[:, i]) for i in 1:N_ensemble]...) | ||
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terminated = EKP.update_ensemble!(ensemble_kalman_process, G_ens) | ||
if !isnothing(terminated) | ||
N_iters[idx] = i - 1 | ||
break # if the timestep was terminated due to timestepping condition | ||
end | ||
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end | ||
# this will change in on failure condition | ||
N_iter = N_iters[idx] | ||
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# required for plots | ||
u_err = u_err[1:(N_iter + 1)] | ||
u_spread = u_spread[1:(N_iter + 1)] | ||
u_i = get_u_final(ensemble_kalman_process) | ||
u_err[N_iter + 1] = 1 / size(u_i, 2) * sum((u_i .- unconstrained_u_true) .^ 2) | ||
u_spread[N_iter + 1] = 1 / size(u_i, 2) * sum((u_i .- mean(u_i, dims = 2)) .^ 2) | ||
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final_u_err[idx, rng_idx] = u_err[end] | ||
final_u_spread[idx, rng_idx] = u_spread[end] | ||
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Δt = ensemble_kalman_process.Δt | ||
alg_time = [sum(Δt[1:i]) for i in 1:length(Δt)] | ||
pushfirst!(alg_time, 0.0) | ||
misfit = get_error(ensemble_kalman_process) | ||
final_misfit[idx, rng_idx] = misfit[end] | ||
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if rng_idx == 1 | ||
plot!(plt2, 0:N_iter, u_err, c = clrs[idx + 1], label = "$(nameof(typeof(scheduler)))") | ||
plot!(plt2, 0:N_iter, u_spread, c = clrs[idx + 1], ls = :dash, label = "") | ||
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plot!(plt3, alg_time, u_err, c = clrs[idx + 1], label = "$(nameof(typeof(scheduler)))") | ||
plot!(plt3, alg_time, u_spread, c = clrs[idx + 1], ls = :dash, label = "") | ||
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# Finally, we get the ensemble after the last iteration. This provides our estimate of the parameters. | ||
final_ensemble = get_ϕ_final(prior, ensemble_kalman_process) | ||
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# To visualize the success of the inversion, we plot model with the true | ||
# parameters, the initial ensemble, and the final ensemble. | ||
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plot!( | ||
plt, | ||
trange, | ||
model(mean(final_ensemble, dims = 2)...), | ||
alpha = 1.0, | ||
c = clrs[idx + 1], | ||
label = "$(nameof(typeof(scheduler)))", | ||
) | ||
G_final_mean = G(mean(final_ensemble, dims = 2)[:]) | ||
for k in 1:2 | ||
plot!( | ||
plt_thin, | ||
trange, | ||
repeat([G_final_mean[k]], length(trange)), | ||
linestyle = :dot, | ||
c = clrs[idx + 1], | ||
label = "", | ||
) | ||
end | ||
end | ||
end | ||
end | ||
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#some final plot tweaking / combining | ||
ylims!(plt_thin, ylims(plt)) | ||
ll = @layout [a{0.8w} b{0.2w}] | ||
plt = plot(plt, plt_thin, layout = ll, right_margin = 10mm) | ||
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mean_final_misfit = mean(final_misfit, dims = 2) | ||
mean_final_u_err = mean(final_u_err, dims = 2) | ||
mean_final_u_spread = mean(final_u_spread, dims = 2) | ||
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plot!(plt2, [1], [ylims(plt2)[2] + 1], c = :gray, label = "error") | ||
plot!(plt2, [1], [ylims(plt2)[2] + 1], c = :gray, ls = :dash, label = "spread") | ||
plot!(plt3, [1], [ylims(plt3)[2] + 1], c = :gray, label = "error") | ||
plot!(plt3, [1], [ylims(plt3)[2] + 1], c = :gray, ls = :dash, label = "spread") | ||
plt2_thin = plot(yscale = :log10, grid = false, xticks = false, title = "Final ($(repeats) runs)") | ||
for i in 1:5 | ||
plot!( | ||
plt2_thin, | ||
trange, | ||
repeat([mean_final_u_err[i]], length(trange)), | ||
yscale = :log10, | ||
c = clrs[i + 1], #idx + 1 for colours | ||
label = "", | ||
) | ||
plot!( | ||
plt2_thin, | ||
trange, | ||
repeat([mean_final_u_spread[i]], length(trange)), | ||
c = clrs[i + 1], #idx + 1 for colours | ||
ls = :dash, | ||
label = "", | ||
) | ||
end | ||
plt3_thin = plt2_thin | ||
ylims!(plt2_thin, ylims(plt2)) | ||
plt2 = plot(plt2, plt2_thin, layout = ll, right_margin = 10mm) | ||
ylims!(plt3_thin, ylims(plt3)) | ||
plt3 = plot(plt3, plt3_thin, layout = ll, right_margin = 10mm) | ||
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for (i, t) in enumerate(ts_tmp[1]) | ||
println(" ") | ||
println("Method : ", t) | ||
println("Final misfit: ", mean_final_misfit[i]) | ||
println("Final error : ", mean_final_u_err[i]) | ||
println("Final spread: ", mean_final_u_spread[i]) | ||
end | ||
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savefig(plt, joinpath(figure_save_directory, "ensembles.png")) | ||
savefig(plt2, joinpath(figure_save_directory, "error_vs_spread_over_iteration.png")) | ||
savefig(plt3, joinpath(figure_save_directory, "error_vs_spread_over_time.png")) | ||
savefig(plt, joinpath(figure_save_directory, "ensembles.pdf")) | ||
savefig(plt2, joinpath(figure_save_directory, "error_vs_spread_over_iteration.pdf")) | ||
savefig(plt3, joinpath(figure_save_directory, "error_vs_spread_over_time.pdf")) |
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