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ballast/__init__.py ADDED
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ballast/experiment.py ADDED
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1
+ """Active-learning campaign driver (paper Sec. 5.2 / 5.3).
2
+
3
+ A campaign deploys M Lagrangian observers, one every `deploy_every` units of
4
+ time, the first uniformly at random and the rest by the policy under test. Each
5
+ observer is advected by the *ground-truth* field from its release until the
6
+ terminal time T (or until it leaves the region) and measures every delta_obs.
7
+
8
+ Performance after m deployments is the average L2 error of the GP posterior
9
+ predictive mean field over the spatial grid and the full set of deployment
10
+ times, using all data those m observers collect over the whole campaign -- i.e.
11
+ "what would this campaign have bought me if I had stopped at m drifters".
12
+ """
13
+
14
+ from __future__ import annotations
15
+
16
+ from dataclasses import dataclass, field
17
+ from typing import Callable
18
+
19
+ import jax
20
+ import jax.numpy as jnp
21
+ import numpy as np
22
+ from scipy.optimize import minimize
23
+
24
+ from .gp import log_marginal_likelihood, posterior_ext_state, posterior_mean_field
25
+ from .kernels import HelmParams
26
+ from .policies import (
27
+ ballast_sample_utilities,
28
+ dist_sep_scores,
29
+ eig_utilities,
30
+ sobol_indices,
31
+ )
32
+ from .spde import make_ops, prior_sample
33
+ from .trajectory import Grid, advect, observe
34
+
35
+
36
+ @dataclass
37
+ class Config:
38
+ T: float = 10.0
39
+ dt: float = 0.01
40
+ obs_every: int = 5 # delta_obs = 0.05
41
+ deploy_every: float = 0.5
42
+ n_deploy: int = 20 # 1 initial + 19 policy-chosen
43
+ sigma_obs: float = 0.1
44
+ n_samples: int = 20 # BALLAST J
45
+ grid_nx: int = 25
46
+ grid_ny: int = 25
47
+ x_lo: float = -2.0
48
+ x_hi: float = 2.0
49
+ y_lo: float = -2.0
50
+ y_hi: float = 2.0
51
+ chunk: int = 64
52
+
53
+ @property
54
+ def n_obs_total(self) -> int:
55
+ return int(round(self.T / self.dt)) // self.obs_every
56
+
57
+ @property
58
+ def obs_dt(self) -> float:
59
+ return self.dt * self.obs_every
60
+
61
+ def grid(self) -> Grid:
62
+ return Grid(
63
+ jnp.linspace(self.x_lo, self.x_hi, self.grid_nx),
64
+ jnp.linspace(self.y_lo, self.y_hi, self.grid_ny),
65
+ )
66
+
67
+
68
+ SYNTH_PARAMS = HelmParams(
69
+ phi_ls=0.8, phi_var=0.5, psi_ls=0.5, psi_var=0.5, time_ls=2.5, time_var=1.0
70
+ )
71
+
72
+ # Sec. H.3 optimisation bounds ("uniform priors with finite support")
73
+ SYNTH_BOUNDS = [(0.1, 1.0), (0.1, 1.0), (0.1, 1.0), (0.1, 1.0), (0.1, 3.0), (0.1, 3.0)]
74
+ SUNTANS_BOUNDS = [(0.1, 5.0), (10.0, 20.0), (0.1, 1.0), (0.1, 5.0), (0.1, 3.0), (10.0, 20.0)]
75
+
76
+
77
+ def make_ground_truth(key, cfg: Config, p: HelmParams) -> jnp.ndarray:
78
+ """Draw a synthetic ground-truth field from the temporal Helmholtz GP.
79
+
80
+ Exact draw via the SPDE prior (dense sampling of 25*25*1001 space-time points
81
+ would be a ~1.25M-dimensional Gaussian).
82
+ """
83
+ grid = cfg.grid()
84
+ ops = make_ops(grid.R, p, cfg.dt)
85
+ n_steps = int(round(cfg.T / cfg.dt))
86
+ return prior_sample(key, grid.R, ops, n_steps)
87
+
88
+
89
+ def optimise_hypers(
90
+ S, t, y, cfg: Config, bounds, init: HelmParams, opt_noise: bool = True
91
+ ):
92
+ """L-BFGS-B fit of the GP hyperparameters (Algorithm 2 step 5, Sec. H.3).
93
+
94
+ Optimises in the natural parameterisation with box bounds, as the paper
95
+ describes ("manually-set bounds ... to mimic uniform priors with finite
96
+ support"). Falls back to the initial values if the optimiser fails.
97
+ """
98
+ b = list(bounds) + ([(0.01, 1.0)] if opt_noise else [])
99
+ x0 = np.array(list(np.asarray(init.as_array())) + ([cfg.sigma_obs] if opt_noise else []))
100
+ x0 = np.clip(x0, [lo for lo, _ in b], [hi for _, hi in b])
101
+
102
+ def obj(x):
103
+ x = jnp.asarray(x)
104
+ p = HelmParams.from_array(x[:6])
105
+ sig = x[6] if opt_noise else cfg.sigma_obs
106
+ return -log_marginal_likelihood(p, S, t, y, sig)
107
+
108
+ vg = jax.jit(jax.value_and_grad(obj))
109
+
110
+ def f(x):
111
+ v, g = vg(jnp.asarray(x))
112
+ return float(v), np.asarray(g, dtype=np.float64)
113
+
114
+ try:
115
+ res = minimize(f, x0, jac=True, method="L-BFGS-B", bounds=b,
116
+ options={"maxiter": 60})
117
+ xs = np.clip(res.x, [lo for lo, _ in b], [hi for _, hi in b])
118
+ except Exception:
119
+ xs = x0
120
+ p = HelmParams.from_array(jnp.asarray(xs[:6]))
121
+ sig = float(xs[6]) if opt_noise else cfg.sigma_obs
122
+ return p, sig
123
+
124
+
125
+ def run_campaign(
126
+ key,
127
+ cfg: Config,
128
+ gt_fields: jnp.ndarray,
129
+ policy: str,
130
+ true_params: HelmParams,
131
+ bounds=None,
132
+ eval_params: HelmParams | None = None,
133
+ seed_offset: int = 0,
134
+ ):
135
+ """Run one campaign. Returns dict with the per-deployment error curve.
136
+
137
+ `eval_params` (default: true_params) are the hyperparameters used for the
138
+ *evaluation* GP. Held fixed across policies so the comparison measures the
139
+ quality of the data collected, not of the fitted model.
140
+ """
141
+ grid = cfg.grid()
142
+ eval_params = eval_params or true_params
143
+ n_obs_tot = cfg.n_obs_total
144
+ ops_true = make_ops(grid.R, true_params, cfg.dt)
145
+
146
+ # global observation times: 0.05, 0.10, ..., T
147
+ tg = cfg.obs_dt * (1 + jnp.arange(n_obs_tot))
148
+
149
+ pos_all = np.zeros((cfg.n_deploy, n_obs_tot, 2)) # reported (cell-centre) locations
150
+ raw_all = np.zeros((cfg.n_deploy, n_obs_tot, 2)) # true physical positions
151
+ val_all = np.zeros((cfg.n_deploy, n_obs_tot), dtype=bool)
152
+ y_all = np.zeros((cfg.n_deploy, n_obs_tot, 2))
153
+ placements = []
154
+ errors = []
155
+
156
+ t_eval = cfg.deploy_every * jnp.arange(cfg.n_deploy)
157
+
158
+ for m in range(cfg.n_deploy):
159
+ t_m = m * cfg.deploy_every
160
+ k_m = int(round(t_m / cfg.dt))
161
+ key, kp, ks, ko = jax.random.split(key, 4)
162
+
163
+ # ---- data available at decision time (strictly before/at t_m)
164
+ past = val_all & (np.asarray(tg)[None, :] <= t_m + 1e-9)
165
+ S_obs = jnp.asarray(pos_all[past])
166
+ t_obs = jnp.asarray(np.broadcast_to(np.asarray(tg)[None, :], past.shape)[past])
167
+ y_obs = jnp.asarray(y_all[past])
168
+
169
+ # ---- choose the placement
170
+ if m == 0:
171
+ idx = int(jax.random.randint(kp, (), 0, grid.n))
172
+ elif policy == "unif":
173
+ idx = int(jax.random.randint(kp, (), 0, grid.n))
174
+ elif policy == "sobol":
175
+ idx = int(sobol_indices(grid, cfg.n_deploy, seed_offset)[m])
176
+ else:
177
+ exist_idx = np.arange(m)
178
+ j_at = int(round(t_m / cfg.obs_dt)) - 1 # obs index whose time is t_m
179
+ # project from the drifters' true positions, not their reported cells
180
+ exist_pos = jnp.asarray(raw_all[exist_idx, j_at])
181
+ exist_live = jnp.asarray(val_all[exist_idx, j_at])
182
+ # drifters that already left contribute nothing: park them outside
183
+ exist_pos = jnp.where(
184
+ exist_live[:, None], exist_pos, jnp.array([1e6, 1e6])
185
+ )
186
+
187
+ p_pol, sig_pol = true_params, cfg.sigma_obs
188
+ if policy == "ballast_opt":
189
+ p_pol, sig_pol = optimise_hypers(
190
+ S_obs, t_obs, y_obs, cfg, bounds, true_params
191
+ )
192
+
193
+ if policy == "eig":
194
+ sc = eig_utilities(grid, S_obs, t_obs, t_m, p_pol, sig_pol, cfg.chunk)
195
+ else:
196
+ ops_pol = ops_true if policy != "ballast_opt" else make_ops(
197
+ grid.R, p_pol, cfg.dt
198
+ )
199
+ mean, chol = posterior_ext_state(
200
+ S_obs, t_obs, y_obs, grid.R, t_m, p_pol, sig_pol
201
+ )
202
+ if policy == "dist_sep":
203
+ sc = dist_sep_scores(
204
+ ks, grid, ops_pol, mean, chol, exist_pos, S_obs, t_m,
205
+ cfg.T, cfg.dt, cfg.obs_every, cfg.n_samples,
206
+ )
207
+ else: # ballast_true / ballast_opt
208
+ u = ballast_sample_utilities(
209
+ ks, grid, ops_pol, S_obs, t_obs, mean, chol, exist_pos,
210
+ t_m, cfg.T, cfg.dt, cfg.obs_every, p_pol, sig_pol,
211
+ cfg.n_samples, cfg.chunk,
212
+ )
213
+ sc = jnp.mean(u, axis=0)
214
+ idx = int(jnp.argmax(sc))
215
+
216
+ s_new = grid.R[idx]
217
+ placements.append((float(s_new[0]), float(s_new[1]), t_m))
218
+
219
+ # ---- advect the new drifter through the TRUE field until T
220
+ pos, valid, tidx = advect(
221
+ grid, gt_fields[k_m:], s_new[None, :],
222
+ jnp.ones(1, dtype=bool), cfg.dt, cfg.obs_every,
223
+ )
224
+ yv = observe(ko, grid, gt_fields[k_m:], pos, valid, tidx, cfg.sigma_obs)
225
+ j0 = int(round(t_m / cfg.obs_dt))
226
+ n_here = pos.shape[0]
227
+ # a drifter reports its cell's velocity, i.e. f(cell centre, t) + noise
228
+ pos_all[m, j0 : j0 + n_here] = np.asarray(grid.snap(pos)[:, 0, :])
229
+ raw_all[m, j0 : j0 + n_here] = np.asarray(pos[:, 0, :])
230
+ val_all[m, j0 : j0 + n_here] = np.asarray(valid[:, 0])
231
+ y_all[m, j0 : j0 + n_here] = np.asarray(yv[:, 0, :])
232
+
233
+ # ---- evaluate: all data from the m+1 drifters over the whole campaign
234
+ sel = val_all[: m + 1]
235
+ S_e = jnp.asarray(pos_all[: m + 1][sel])
236
+ t_e = jnp.asarray(np.broadcast_to(np.asarray(tg)[None, :], sel.shape)[sel])
237
+ y_e = jnp.asarray(y_all[: m + 1][sel])
238
+ mu = posterior_mean_field(
239
+ S_e, t_e, y_e, grid.R, t_eval, eval_params, cfg.sigma_obs
240
+ )
241
+ gt_at_eval = gt_fields[(jnp.round(t_eval / cfg.dt)).astype(int)]
242
+ err = float(jnp.mean(jnp.linalg.norm(mu - gt_at_eval, axis=-1)))
243
+ errors.append(err)
244
+
245
+ return {
246
+ "policy": policy,
247
+ "errors": errors,
248
+ "placements": placements,
249
+ "n_obs": int(val_all.sum()),
250
+ }
251
+
252
+
253
+ # --------------------------------------------------------------------------
254
+ # Iso-performance (Sec. 5.2): how many drifters a policy saves vs UNIF
255
+ # --------------------------------------------------------------------------
256
+
257
+
258
+ def iso_performance(err_policy: np.ndarray, err_unif: np.ndarray) -> np.ndarray:
259
+ """Drifters saved at each iteration, relative to the uniform benchmark.
260
+
261
+ At iteration m the uniform benchmark reaches error e = err_unif[m]. We find
262
+ the (interpolated, fractional) number of drifters n the policy needs to reach
263
+ the same error and report m - n: positive means the policy needed fewer.
264
+
265
+ Both curves are made monotone non-increasing first (running minimum): the
266
+ error curve of a single run is noisy, and "the number of drifters needed to
267
+ reach accuracy e" is only well defined for a best-so-far curve.
268
+ """
269
+ a = np.minimum.accumulate(np.asarray(err_policy, dtype=float))
270
+ b = np.minimum.accumulate(np.asarray(err_unif, dtype=float))
271
+ n = len(a)
272
+ idx = np.arange(1, n + 1, dtype=float) # number of drifters deployed
273
+ out = np.full(n, np.nan)
274
+ for m in range(n):
275
+ target = b[m]
276
+ hit = np.where(a <= target)[0]
277
+ if len(hit) == 0:
278
+ # policy never reaches it: cap at the full budget (conservative)
279
+ out[m] = idx[m] - (n + 1)
280
+ continue
281
+ k = hit[0]
282
+ if k == 0:
283
+ out[m] = idx[m] - 1.0
284
+ else:
285
+ # linear interpolation in drifter count between k-1 and k
286
+ e0, e1 = a[k - 1], a[k]
287
+ frac = 0.0 if e0 == e1 else (e0 - target) / (e0 - e1)
288
+ out[m] = idx[m] - (idx[k - 1] + frac)
289
+ return out
ballast/gp.py ADDED
@@ -0,0 +1,197 @@
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
1
+ """GP regression, posterior sampling and information-gain utilities.
2
+
3
+ Implements paper Sec. B.1 (regression), C.1 (the cheap EIG reformulation
4
+ logdet(I + sigma^-2 K(X)), which is what eq. (3)/(5) actually mean -- see note
5
+ below), and E.2 (rank-q Gram determinant updates, which the paper states is
6
+ "the default for the computation in this work").
7
+
8
+ Note on eq. (5). The main text writes the utility as
9
+ logdet(I + sigma_obs^2 K(X))
10
+ but App. C.1 derives
11
+ IG = 1/2 logdet(I + sigma_obs^{-2} K(X)),
12
+ i.e. the noise variance enters *inversely* (more noise -> less information). The
13
+ main-text form is a sign-of-exponent typo; we implement the App. C.1 form. With
14
+ sigma_obs = 0.1 the two differ by a factor 1e4 inside the logdet and would order
15
+ candidates differently, so this matters. Constant factors of 1/2 do not affect
16
+ the argmax and are dropped, but we keep them consistent across policies.
17
+ """
18
+
19
+ from __future__ import annotations
20
+
21
+ import jax
22
+ import jax.numpy as jnp
23
+ from jax.scipy.linalg import cho_factor, cho_solve, solve_triangular
24
+
25
+ from .kernels import HelmParams, k_ext_cross, k_ext_full, k_thelm_mat
26
+
27
+
28
+ def _expand_mask(mask: jnp.ndarray) -> jnp.ndarray:
29
+ """(..., n) point mask -> (..., 2n) row mask (2 velocity components/point)."""
30
+ return jnp.repeat(mask, 2, axis=-1)
31
+
32
+
33
+ def noise_gram(
34
+ S: jnp.ndarray, t: jnp.ndarray, p: HelmParams, sigma: float, mask=None
35
+ ) -> jnp.ndarray:
36
+ """M = I + sigma^-2 K(X), with invalid points replaced by identity rows.
37
+
38
+ Masking out point i (row/col -> e_i) leaves logdet(M) equal to the logdet of
39
+ the submatrix over valid points, so variable-length trajectories can be
40
+ batched at fixed shape.
41
+ """
42
+ K = k_thelm_mat(S, t, S, t, p)
43
+ n = K.shape[0]
44
+ M = jnp.eye(n) + K / sigma**2
45
+ if mask is not None:
46
+ m = _expand_mask(mask).astype(M.dtype)
47
+ M = M * m[:, None] * m[None, :]
48
+ M = M + jnp.diag(1.0 - m)
49
+ return M
50
+
51
+
52
+ def logdet_chol(M: jnp.ndarray) -> jnp.ndarray:
53
+ L = jnp.linalg.cholesky(M)
54
+ return 2.0 * jnp.sum(jnp.log(jnp.diagonal(L, axis1=-2, axis2=-1)), axis=-1)
55
+
56
+
57
+ # --------------------------------------------------------------------------
58
+ # Regression
59
+ # --------------------------------------------------------------------------
60
+
61
+
62
+ def log_marginal_likelihood(
63
+ p: HelmParams, S: jnp.ndarray, t: jnp.ndarray, y: jnp.ndarray, sigma: float
64
+ ) -> jnp.ndarray:
65
+ """Log marginal likelihood of the plain (non-extended) temporal Helmholtz GP.
66
+
67
+ y is (n, 2) velocity observations; flattened point-major/component-minor.
68
+ """
69
+ K = k_thelm_mat(S, t, S, t, p)
70
+ n = K.shape[0]
71
+ A = K + (sigma**2) * jnp.eye(n)
72
+ c, low = cho_factor(A)
73
+ yy = y.reshape(-1)
74
+ alpha = cho_solve((c, low), yy)
75
+ ld = 2.0 * jnp.sum(jnp.log(jnp.diag(c)))
76
+ return -0.5 * yy @ alpha - 0.5 * ld - 0.5 * n * jnp.log(2 * jnp.pi)
77
+
78
+
79
+ def posterior_mean_field(
80
+ S: jnp.ndarray,
81
+ t: jnp.ndarray,
82
+ y: jnp.ndarray,
83
+ R: jnp.ndarray,
84
+ t_eval: jnp.ndarray,
85
+ p: HelmParams,
86
+ sigma: float,
87
+ ) -> jnp.ndarray:
88
+ """Posterior predictive mean of the velocity field on R x t_eval.
89
+
90
+ Returns (n_teval, N_space, 2). Used for the performance metric of Sec. 5.2:
91
+ average L2 error of the posterior mean field over the spatial grid and the
92
+ full set of deployment times.
93
+ """
94
+ K = k_thelm_mat(S, t, S, t, p)
95
+ A = K + (sigma**2) * jnp.eye(K.shape[0])
96
+ c, low = cho_factor(A)
97
+ alpha = cho_solve((c, low), y.reshape(-1))
98
+
99
+ N = R.shape[0]
100
+ Rr = jnp.tile(R, (t_eval.shape[0], 1)) # (nt*N, 2)
101
+ tr = jnp.repeat(t_eval, N)
102
+ Kx = k_thelm_mat(S, t, Rr, tr, p) # (2n, 2*nt*N)
103
+ mu = Kx.T @ alpha
104
+ return mu.reshape(t_eval.shape[0], N, 2)
105
+
106
+
107
+ def posterior_ext_state(
108
+ S: jnp.ndarray,
109
+ t: jnp.ndarray,
110
+ y: jnp.ndarray,
111
+ R: jnp.ndarray,
112
+ t_m: float,
113
+ p: HelmParams,
114
+ sigma: float,
115
+ jitter: float = 1e-8,
116
+ ):
117
+ """Posterior of the extended state f(R, t_m) = [f, d_t f]^T given D_m.
118
+
119
+ This is step 6/8 of Algorithm 2: regress with the *extended* GP using a
120
+ standard dense GP, then hand the draw to the SPDE propagator. Observations
121
+ only ever touch the f-block; the d_t f block is reached through the
122
+ cross-covariance d_{t'} k_tHelm.
123
+
124
+ Returns (mean (4N,), chol of covariance (4N, 4N)).
125
+ """
126
+ K = k_thelm_mat(S, t, S, t, p)
127
+ A = K + (sigma**2) * jnp.eye(K.shape[0])
128
+ c, low = cho_factor(A)
129
+
130
+ N = R.shape[0]
131
+ tvec = jnp.full((N,), t_m)
132
+ K_ot = k_ext_cross(S, t, R, tvec, p) # (2n, 4N)
133
+ K_tt = k_ext_full(R, tvec, p) # (4N, 4N)
134
+
135
+ mean = K_ot.T @ cho_solve((c, low), y.reshape(-1))
136
+ cov = K_tt - K_ot.T @ cho_solve((c, low), K_ot)
137
+ cov = 0.5 * (cov + cov.T) + jitter * jnp.eye(cov.shape[0])
138
+ return mean, jnp.linalg.cholesky(cov)
139
+
140
+
141
+ def sample_ext_state(key, mean, cov_chol, n_space: int) -> jnp.ndarray:
142
+ """Draw an extended state and reshape to the SPDE layout (2N_space, 2)."""
143
+ z = jax.random.normal(key, mean.shape, dtype=mean.dtype)
144
+ x = mean + cov_chol @ z
145
+ return x.reshape(2 * n_space, 2)
146
+
147
+
148
+ # --------------------------------------------------------------------------
149
+ # Utilities (information gain)
150
+ # --------------------------------------------------------------------------
151
+
152
+
153
+ def base_factor(
154
+ S: jnp.ndarray, t: jnp.ndarray, p: HelmParams, sigma: float, mask=None
155
+ ):
156
+ """Cholesky factor and logdet of A = I + sigma^-2 K(Z) for the fixed base set Z."""
157
+ A = noise_gram(S, t, p, sigma, mask)
158
+ L = jnp.linalg.cholesky(A)
159
+ return L, 2.0 * jnp.sum(jnp.log(jnp.diag(L)))
160
+
161
+
162
+ def rank_q_logdet(
163
+ L_base: jnp.ndarray,
164
+ logdet_base: jnp.ndarray,
165
+ S_base: jnp.ndarray,
166
+ t_base: jnp.ndarray,
167
+ base_mask: jnp.ndarray | None,
168
+ S_new: jnp.ndarray,
169
+ t_new: jnp.ndarray,
170
+ new_mask: jnp.ndarray,
171
+ p: HelmParams,
172
+ sigma: float,
173
+ ) -> jnp.ndarray:
174
+ """logdet(I + sigma^-2 K(Z u P)) via the App. E.2 block-determinant update.
175
+
176
+ det [[A, B], [B^T, D]] = det(A) det(D - B^T A^{-1} B)
177
+
178
+ with A = I + sigma^-2 K(Z) already factorised (independent of the candidate),
179
+ B = sigma^-2 K(Z, P), D = I + sigma^-2 K(P). Cost is O(n^2 q + q^3) per
180
+ candidate instead of O((n+q)^3), which is what makes the 625-candidate x
181
+ 20-sample inner loop of Algorithm 2 affordable.
182
+
183
+ Masked-out new points contribute e_i rows to the Schur complement and hence
184
+ nothing to the logdet.
185
+ """
186
+ B = k_thelm_mat(S_base, t_base, S_new, t_new, p) / sigma**2 # (2n, 2q)
187
+ D = noise_gram(S_new, t_new, p, sigma, new_mask) # (2q, 2q)
188
+
189
+ mnew = _expand_mask(new_mask).astype(B.dtype)
190
+ B = B * mnew[None, :]
191
+ if base_mask is not None:
192
+ B = B * _expand_mask(base_mask).astype(B.dtype)[:, None]
193
+
194
+ V = solve_triangular(L_base, B, lower=True) # (2n, 2q)
195
+ Sc = D - V.T @ V
196
+ # keep the masked rows/cols exactly e_i (V columns there are already zero)
197
+ return logdet_base + logdet_chol(Sc)
ballast/kernels.py ADDED
@@ -0,0 +1,187 @@
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
1
+ """Kernels for the temporal Helmholtz GP of BALLAST (arXiv 2509.26005).
2
+
3
+ The surrogate is a separable, vector-output, spatio-temporal GP
4
+
5
+ k_tHelm((s,t),(s',t')) = k_Helm(s,s') * k_time(t,t')
6
+
7
+ with k_Helm the Helmholtz kernel of Berlinghieri et al. (2023) (paper Sec. B.2)
8
+ built from two independent RBF kernels (potential Phi, stream Psi), and k_time a
9
+ Matern-3/2 kernel (paper Sec. 2.2).
10
+
11
+ Section 4.1 of the paper additionally needs the *extended* GP f = [f, d_t f]^T,
12
+ whose kernel is the 2x2 block matrix of temporal derivatives of k_tHelm. Because
13
+ k_tHelm is separable, all t-derivatives act on the Matern-3/2 factor only.
14
+
15
+ Everything is implemented **analytically**. The paper (Sec. H.2) warns that
16
+ autodiff through a Matern kernel written with a clipped distance
17
+ (`sqrt(max(sum((x-y)**2), 1e-36))`, as in GPJax) gives d^2_{tt'}k = 0 at t=t'
18
+ instead of the correct 3*sigma^2/l^2; the analytic form has no such problem.
19
+ `tests/test_kernels.py` checks these derivatives against finite differences.
20
+
21
+ Index layout
22
+ ------------
23
+ Spatial-velocity blocks are flattened point-major / component-minor:
24
+ row index of a velocity vector at point i, component c -> i*2 + c
25
+ The extended state adds the [f, d_t f] axis last:
26
+ (i, c, a) -> i*4 + c*2 + a with a=0 -> f, a=1 -> d_t f
27
+ """
28
+
29
+ from __future__ import annotations
30
+
31
+ from typing import NamedTuple
32
+
33
+ import jax
34
+ import jax.numpy as jnp
35
+
36
+ SQRT3 = jnp.sqrt(3.0)
37
+
38
+
39
+ class HelmParams(NamedTuple):
40
+ """Hyperparameters of the temporal Helmholtz GP."""
41
+
42
+ phi_ls: jnp.ndarray # potential kernel lengthscale
43
+ phi_var: jnp.ndarray # potential kernel variance
44
+ psi_ls: jnp.ndarray # stream kernel lengthscale
45
+ psi_var: jnp.ndarray # stream kernel variance
46
+ time_ls: jnp.ndarray # Matern-3/2 temporal lengthscale
47
+ time_var: jnp.ndarray # Matern-3/2 temporal variance
48
+
49
+ def as_array(self) -> jnp.ndarray:
50
+ return jnp.stack(
51
+ [
52
+ jnp.asarray(self.phi_ls),
53
+ jnp.asarray(self.phi_var),
54
+ jnp.asarray(self.psi_ls),
55
+ jnp.asarray(self.psi_var),
56
+ jnp.asarray(self.time_ls),
57
+ jnp.asarray(self.time_var),
58
+ ]
59
+ )
60
+
61
+ @staticmethod
62
+ def from_array(a: jnp.ndarray) -> "HelmParams":
63
+ return HelmParams(a[0], a[1], a[2], a[3], a[4], a[5])
64
+
65
+
66
+ # --------------------------------------------------------------------------
67
+ # Spatial: Helmholtz kernel
68
+ # --------------------------------------------------------------------------
69
+
70
+
71
+ def _rbf_hess(S: jnp.ndarray, S2: jnp.ndarray, ls, var) -> jnp.ndarray:
72
+ """Mixed second derivatives of an RBF kernel.
73
+
74
+ Returns H with H[i, j, a, b] = d^2 / (d x_a d x'_b) k(S_i, S2_j), which for
75
+ k = var * exp(-|d|^2 / (2 l^2)), d = x - x', equals
76
+
77
+ k * (delta_ab / l^2 - d_a d_b / l^4).
78
+ """
79
+ d = S[:, None, :] - S2[None, :, :] # (N, M, 2)
80
+ sq = jnp.sum(d**2, axis=-1) # (N, M)
81
+ k = var * jnp.exp(-0.5 * sq / ls**2) # (N, M)
82
+ eye = jnp.eye(2)
83
+ outer = d[..., :, None] * d[..., None, :] # (N, M, 2, 2)
84
+ return k[..., None, None] * (eye / ls**2 - outer / ls**4)
85
+
86
+
87
+ def k_helm(S: jnp.ndarray, S2: jnp.ndarray, p: HelmParams) -> jnp.ndarray:
88
+ """Helmholtz kernel (paper Sec. B.2), returned as (N, M, 2, 2).
89
+
90
+ F = grad(Phi) + rot(Psi) with rot(Psi) = (d_2 Psi, -d_1 Psi), so
91
+
92
+ K[0,0] = d^2_{x1 x1'} k_Phi + d^2_{x2 x2'} k_Psi
93
+ K[0,1] = d^2_{x1 x2'} k_Phi - d^2_{x2 x1'} k_Psi
94
+ K[1,0] = d^2_{x2 x1'} k_Phi - d^2_{x1 x2'} k_Psi
95
+ K[1,1] = d^2_{x2 x2'} k_Phi + d^2_{x1 x1'} k_Psi
96
+ """
97
+ A = _rbf_hess(S, S2, p.phi_ls, p.phi_var) # potential
98
+ B = _rbf_hess(S, S2, p.psi_ls, p.psi_var) # stream
99
+ k00 = A[..., 0, 0] + B[..., 1, 1]
100
+ k01 = A[..., 0, 1] - B[..., 1, 0]
101
+ k10 = A[..., 1, 0] - B[..., 0, 1]
102
+ k11 = A[..., 1, 1] + B[..., 0, 0]
103
+ return jnp.stack(
104
+ [jnp.stack([k00, k01], -1), jnp.stack([k10, k11], -1)], axis=-2
105
+ ) # (N, M, 2, 2)
106
+
107
+
108
+ def k_helm_mat(S: jnp.ndarray, S2: jnp.ndarray, p: HelmParams) -> jnp.ndarray:
109
+ """Helmholtz Gram matrix flattened to (2N, 2M), point-major/component-minor."""
110
+ K = k_helm(S, S2, p) # (N, M, 2, 2)
111
+ N, M = K.shape[0], K.shape[1]
112
+ return jnp.transpose(K, (0, 2, 1, 3)).reshape(2 * N, 2 * M)
113
+
114
+
115
+ # --------------------------------------------------------------------------
116
+ # Temporal: Matern-3/2 and its derivative blocks
117
+ # --------------------------------------------------------------------------
118
+
119
+
120
+ def matern32_blocks(t: jnp.ndarray, t2: jnp.ndarray, ls, var) -> jnp.ndarray:
121
+ """Matern-3/2 kernel and its t/t' derivatives, as (N, M, 2, 2).
122
+
123
+ With lam = sqrt(3)/l, tau = t - t':
124
+
125
+ M[0,0] = k = var (1 + lam|tau|) exp(-lam|tau|)
126
+ M[0,1] = d_{t'} k = var lam^2 tau exp(-lam|tau|)
127
+ M[1,0] = d_{t} k = -var lam^2 tau exp(-lam|tau|)
128
+ M[1,1] = d^2_{t t'} k = var lam^2 (1 - lam|tau|) exp(-lam|tau|)
129
+
130
+ Note M[1,1] at tau=0 is var*lam^2 = 3 var / l^2 (= 3 for var=l=1), the value
131
+ the paper's Sec. H.2 flags as being silently zeroed by clipped-distance
132
+ autodiff implementations. It also equals P_inf[1,1] in the SPDE formulation
133
+ (spde.py), i.e. Var(d_t f) -- an internal consistency check of the two views.
134
+ """
135
+ lam = SQRT3 / ls
136
+ tau = t[:, None] - t2[None, :]
137
+ a = jnp.abs(tau)
138
+ e = jnp.exp(-lam * a)
139
+ k = var * (1.0 + lam * a) * e
140
+ dk = var * lam**2 * tau * e # d_{t'} k
141
+ d2k = var * lam**2 * (1.0 - lam * a) * e
142
+ return jnp.stack(
143
+ [jnp.stack([k, dk], -1), jnp.stack([-dk, d2k], -1)], axis=-2
144
+ ) # (N, M, 2, 2)
145
+
146
+
147
+ # --------------------------------------------------------------------------
148
+ # Full temporal-Helmholtz kernel (plain and extended)
149
+ # --------------------------------------------------------------------------
150
+
151
+
152
+ def k_thelm_mat(
153
+ S: jnp.ndarray, t: jnp.ndarray, S2: jnp.ndarray, t2: jnp.ndarray, p: HelmParams
154
+ ) -> jnp.ndarray:
155
+ """Plain k_tHelm Gram matrix between (S,t) and (S2,t2). Shape (2N, 2M)."""
156
+ KS = k_helm(S, S2, p) # (N, M, 2, 2)
157
+ kt = matern32_blocks(t, t2, p.time_ls, p.time_var)[..., 0, 0] # (N, M)
158
+ K = KS * kt[..., None, None]
159
+ N, M = K.shape[0], K.shape[1]
160
+ return jnp.transpose(K, (0, 2, 1, 3)).reshape(2 * N, 2 * M)
161
+
162
+
163
+ def k_ext_cross(
164
+ S: jnp.ndarray, t: jnp.ndarray, S2: jnp.ndarray, t2: jnp.ndarray, p: HelmParams
165
+ ) -> jnp.ndarray:
166
+ """Cov between plain observations at (S,t) and the *extended* state at (S2,t2).
167
+
168
+ Returns (2N, 4M): rows index (obs point, velocity component), columns index
169
+ (test point, velocity component, [f, d_t f]).
170
+ """
171
+ KS = k_helm(S, S2, p) # (N, M, 2, 2)
172
+ Mt = matern32_blocks(t, t2, p.time_ls, p.time_var) # (N, M, 2, 2)
173
+ # observation is the f-component (a=0); test keeps both b in {f, d_t f}
174
+ K = KS[..., :, :, None] * Mt[:, :, None, None, 0, :] # (N, M, 2, 2, 2)
175
+ N, M = K.shape[0], K.shape[1]
176
+ # (N, c, M, c', b) -> (2N, 4M)
177
+ return jnp.transpose(K, (0, 2, 1, 3, 4)).reshape(2 * N, 4 * M)
178
+
179
+
180
+ def k_ext_full(S: jnp.ndarray, t: jnp.ndarray, p: HelmParams) -> jnp.ndarray:
181
+ """Covariance of the extended state f = [f, d_t f]^T at (S,t). Shape (4N, 4N)."""
182
+ KS = k_helm(S, S, p) # (N, N, 2, 2)
183
+ Mt = matern32_blocks(t, t, p.time_ls, p.time_var) # (N, N, 2, 2)
184
+ K = KS[..., :, :, None, None] * Mt[:, :, None, None, :, :] # (N,N,2,2,2,2)
185
+ N = K.shape[0]
186
+ # (i, c, a, j, c', b) -> (4N, 4N)
187
+ return jnp.transpose(K, (0, 2, 4, 1, 3, 5)).reshape(4 * N, 4 * N)
ballast/policies.py ADDED
@@ -0,0 +1,257 @@
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
1
+ """The six placement policies of paper Sec. H.3, and the BALLAST utility.
2
+
3
+ UNIF, SOBOL, DIST-SEP, EIG, BALLAST-true, BALLAST-opt.
4
+ """
5
+
6
+ from __future__ import annotations
7
+
8
+ import functools
9
+
10
+ import jax
11
+ import jax.numpy as jnp
12
+ import numpy as np
13
+ from scipy.stats import qmc
14
+
15
+ from .gp import base_factor, rank_q_logdet, posterior_ext_state, sample_ext_state
16
+ from .kernels import HelmParams
17
+ from .spde import SpdeOps, propagate
18
+ from .trajectory import Grid, advect
19
+
20
+
21
+ # --------------------------------------------------------------------------
22
+ # Sampling posterior fields + projecting trajectories (Algorithm 2, steps 7-13)
23
+ # --------------------------------------------------------------------------
24
+
25
+
26
+ def sample_and_project(
27
+ key,
28
+ grid: Grid,
29
+ ops: SpdeOps,
30
+ ext_mean,
31
+ ext_chol,
32
+ exist_pos: jnp.ndarray,
33
+ t_m: float,
34
+ n_steps: int,
35
+ dt: float,
36
+ obs_every: int,
37
+ ):
38
+ """One BALLAST sample: draw f(R,t_m)|D_m, propagate to T, advect everything.
39
+
40
+ Particles are [all N_space candidate placements] ++ [existing drifters at
41
+ their current positions]. Returns positions/validity of both groups plus the
42
+ observation times.
43
+ """
44
+ ka, kb = jax.random.split(key)
45
+ X0 = sample_ext_state(ka, ext_mean, ext_chol, grid.n)
46
+ fields = propagate(X0, kb, ops, n_steps) # (n_steps+1, N, 2)
47
+
48
+ s0 = jnp.concatenate([grid.R, exist_pos], axis=0)
49
+ active0 = jnp.ones(s0.shape[0], dtype=bool)
50
+ pos, valid, tidx = advect(grid, fields, s0, active0, dt, obs_every)
51
+ t_traj = t_m + tidx * dt
52
+ n_cand = grid.n
53
+ # Future observations land at cell centres (see Grid.snap): the utility must
54
+ # score the locations the drifter will actually report, not its exact path.
55
+ spos = grid.snap(pos)
56
+ return (
57
+ spos[:, :n_cand, :],
58
+ valid[:, :n_cand],
59
+ spos[:, n_cand:, :],
60
+ valid[:, n_cand:],
61
+ t_traj,
62
+ pos,
63
+ )
64
+
65
+
66
+ def ballast_sample_utilities(
67
+ key,
68
+ grid: Grid,
69
+ ops: SpdeOps,
70
+ S_obs,
71
+ t_obs,
72
+ ext_mean,
73
+ ext_chol,
74
+ exist_pos,
75
+ t_m: float,
76
+ T: float,
77
+ dt: float,
78
+ obs_every: int,
79
+ p: HelmParams,
80
+ sigma: float,
81
+ n_samples: int,
82
+ chunk: int = 64,
83
+ ):
84
+ """Per-sample BALLAST utilities: returns (n_samples, N_space).
85
+
86
+ utils[j, i] = logdet(I + sigma^-2 K(X_m u P_j(s_exist) u P_j(R_i)))
87
+
88
+ Structured for the App. E.2 rank-q update: the base set X_m u P_j(s_exist)
89
+ does not depend on the candidate, so its Cholesky is computed once per
90
+ sample and reused across all N_space candidates. Averaging over j gives
91
+ eq. (5); keeping the per-sample axis is what makes the J-ablation of Sec. 5.1
92
+ computable from a single J=200 run.
93
+ """
94
+ n_steps = int(round((T - t_m) / dt))
95
+ keys = jax.random.split(key, n_samples)
96
+ out = []
97
+ for j in range(n_samples):
98
+ cpos, cval, epos, eval_, t_traj, _ = sample_and_project(
99
+ keys[j], grid, ops, ext_mean, ext_chol, exist_pos, t_m, n_steps, dt, obs_every
100
+ )
101
+ # base = past observations ++ projected trajectories of existing drifters
102
+ n_e = epos.shape[1]
103
+ S_base = jnp.concatenate([S_obs, epos.reshape(-1, 2)], axis=0)
104
+ t_base = jnp.concatenate(
105
+ [t_obs, jnp.repeat(t_traj[:, None], n_e, axis=1).reshape(-1)], axis=0
106
+ )
107
+ m_base = jnp.concatenate(
108
+ [jnp.ones(S_obs.shape[0], dtype=bool), eval_.reshape(-1)], axis=0
109
+ )
110
+ L, ld = base_factor(S_base, t_base, p, sigma, m_base)
111
+
112
+ def one(i):
113
+ return rank_q_logdet(
114
+ L, ld, S_base, t_base, m_base,
115
+ cpos[:, i, :], t_traj, cval[:, i], p, sigma,
116
+ )
117
+
118
+ vals = jnp.concatenate(
119
+ [jax.vmap(one)(jnp.arange(a, min(a + chunk, grid.n)))
120
+ for a in range(0, grid.n, chunk)]
121
+ )
122
+ out.append(vals)
123
+ return jnp.stack(out)
124
+
125
+
126
+ def true_field_utilities(
127
+ grid: Grid,
128
+ true_fields: jnp.ndarray,
129
+ S_obs,
130
+ t_obs,
131
+ exist_pos,
132
+ t_m: float,
133
+ dt: float,
134
+ obs_every: int,
135
+ p: HelmParams,
136
+ sigma: float,
137
+ chunk: int = 64,
138
+ ):
139
+ """B(s; true): utilities with trajectories simulated in the ground-truth field.
140
+
141
+ Used only for the Gap_Full diagnostic of the Sec. G.1 ablation (and never by
142
+ any policy -- it is not implementable without knowing the true field).
143
+ `true_fields` must already be sliced to [t_m, T].
144
+ """
145
+ s0 = jnp.concatenate([grid.R, exist_pos], axis=0)
146
+ pos, valid, tidx = advect(
147
+ grid, true_fields, s0, jnp.ones(s0.shape[0], dtype=bool), dt, obs_every
148
+ )
149
+ t_traj = t_m + tidx * dt
150
+ n_cand = grid.n
151
+ pos = grid.snap(pos) # observations are reported at cell centres
152
+ cpos, cval = pos[:, :n_cand, :], valid[:, :n_cand]
153
+ epos, eval_ = pos[:, n_cand:, :], valid[:, n_cand:]
154
+
155
+ n_e = epos.shape[1]
156
+ S_base = jnp.concatenate([S_obs, epos.reshape(-1, 2)], axis=0)
157
+ t_base = jnp.concatenate(
158
+ [t_obs, jnp.repeat(t_traj[:, None], n_e, axis=1).reshape(-1)], axis=0
159
+ )
160
+ m_base = jnp.concatenate(
161
+ [jnp.ones(S_obs.shape[0], dtype=bool), eval_.reshape(-1)], axis=0
162
+ )
163
+ L, ld = base_factor(S_base, t_base, p, sigma, m_base)
164
+
165
+ def one(i):
166
+ return rank_q_logdet(
167
+ L, ld, S_base, t_base, m_base, cpos[:, i, :], t_traj, cval[:, i], p, sigma
168
+ )
169
+
170
+ return jnp.concatenate(
171
+ [jax.vmap(one)(jnp.arange(a, min(a + chunk, grid.n)))
172
+ for a in range(0, grid.n, chunk)]
173
+ )
174
+
175
+
176
+ # --------------------------------------------------------------------------
177
+ # EIG (paper eq. 3): no look-ahead, only the initial placement location
178
+ # --------------------------------------------------------------------------
179
+
180
+
181
+ def eig_utilities(
182
+ grid: Grid, S_obs, t_obs, t_m: float, p: HelmParams, sigma: float, chunk: int = 128
183
+ ):
184
+ """logdet(I + sigma^-2 K(X_n u {(s, t_n)})) for every candidate s."""
185
+ L, ld = base_factor(S_obs, t_obs, p, sigma, None)
186
+ tv = jnp.array([t_m])
187
+
188
+ def one(i):
189
+ return rank_q_logdet(
190
+ L, ld, S_obs, t_obs, None,
191
+ grid.R[i][None, :], tv, jnp.ones(1, dtype=bool), p, sigma,
192
+ )
193
+
194
+ return jnp.concatenate(
195
+ [jax.vmap(one)(jnp.arange(a, min(a + chunk, grid.n)))
196
+ for a in range(0, grid.n, chunk)]
197
+ )
198
+
199
+
200
+ # --------------------------------------------------------------------------
201
+ # DIST-SEP (paper Sec. H.3, adapted from Chen et al. 2024b)
202
+ # --------------------------------------------------------------------------
203
+
204
+
205
+ def dist_sep_scores(
206
+ key,
207
+ grid: Grid,
208
+ ops: SpdeOps,
209
+ ext_mean,
210
+ ext_chol,
211
+ exist_pos,
212
+ S_obs,
213
+ t_m: float,
214
+ T: float,
215
+ dt: float,
216
+ obs_every: int,
217
+ n_samples: int,
218
+ ):
219
+ """Rank-average of (i) expected drifter path length and (ii) separation.
220
+
221
+ (i) total distance travelled, averaged over BALLAST posterior samples;
222
+ (ii) negative Euclidean distance to the closest existing observation
223
+ location. Both are converted to ranks and averaged, then maximised.
224
+ """
225
+ n_steps = int(round((T - t_m) / dt))
226
+ keys = jax.random.split(key, n_samples)
227
+ lengths = []
228
+ for j in range(n_samples):
229
+ _, cval, _, _, _, raw = sample_and_project(
230
+ keys[j], grid, ops, ext_mean, ext_chol, exist_pos, t_m, n_steps, dt, obs_every
231
+ )
232
+ # distance travelled uses the true (unsnapped) path
233
+ cpos = raw[:, : grid.n, :]
234
+ step = jnp.linalg.norm(cpos[1:] - cpos[:-1], axis=-1) # (n_obs-1, N)
235
+ ok = cval[1:] & cval[:-1]
236
+ lengths.append(jnp.sum(jnp.where(ok, step, 0.0), axis=0))
237
+ length = jnp.mean(jnp.stack(lengths), axis=0) # (N,)
238
+
239
+ d = jnp.linalg.norm(grid.R[:, None, :] - S_obs[None, :, :], axis=-1)
240
+ separation = -jnp.min(d, axis=1) # negative distance to closest observation
241
+
242
+ r1 = jnp.argsort(jnp.argsort(length))
243
+ r2 = jnp.argsort(jnp.argsort(separation))
244
+ return 0.5 * (r1 + r2)
245
+
246
+
247
+ # --------------------------------------------------------------------------
248
+ # Space-filling designs
249
+ # --------------------------------------------------------------------------
250
+
251
+
252
+ def sobol_indices(grid: Grid, n: int, seed: int) -> np.ndarray:
253
+ """Scrambled Sobol points on [0,1)^2 mapped to grid cell indices (Sec. H.3)."""
254
+ pts = qmc.Sobol(d=2, scramble=True, seed=seed).random(n)
255
+ ix = np.clip((pts[:, 0] * grid.nx).astype(int), 0, grid.nx - 1)
256
+ iy = np.clip((pts[:, 1] * grid.ny).astype(int), 0, grid.ny - 1)
257
+ return ix * grid.ny + iy
ballast/spde.py ADDED
@@ -0,0 +1,119 @@
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
1
+ """SPDE / state-space formulation of the separable spatio-temporal GP (paper Sec. 4.1, App. F).
2
+
3
+ For a separable kernel k = k_space(s,s') * k_time(t,t') with k_time Matern-3/2,
4
+ the extended field f(R,t) = [f(R,t), d_t f(R,t)]^T solves the linear SPDE
5
+
6
+ d/dt f(R,t) = (I_space (x) F) f(R,t) + (I_space (x) L) w(t)
7
+
8
+ driven by white noise with spectral density K_space (x) Q_c (paper F.2), giving
9
+ the *exact* discrete-time transition
10
+
11
+ f_{k+1} = (I (x) Phi) f_k + e_k, e_k ~ N(0, K_space (x) Q).
12
+
13
+ Why the paper's sampling scheme is exact (this is the crux of Claim 2)
14
+ ---------------------------------------------------------------------
15
+ The dynamics are *pointwise in space*: the SDE at location s is driven only by
16
+ w(s, .) and never by the field at another location. Hence f(R, t > t_m) is a
17
+ deterministic function of the extended state f(R, t_m) and the future noise
18
+ {w(R, u) : u > t_m}, and that future noise is independent of everything at times
19
+ <= t_m. So for observations D_m taken at times <= t_m -- even at *non-gridded*
20
+ Lagrangian locations --
21
+
22
+ f(R, t > t_m) _||_ D_m | f(R, t_m).
23
+
24
+ Therefore drawing the initial condition f(R,t_m) | D_m from the extended dense GP
25
+ posterior and propagating it with the SPDE gives exact posterior samples, while
26
+ never filtering over the observation locations. `tests/test_spde.py` verifies
27
+ this against a dense GP built over the full space-time test set.
28
+
29
+ State layout: X has shape (2*N_space, 2). Rows are (location, velocity
30
+ component) point-major/component-minor; columns are [f, d_t f].
31
+ """
32
+
33
+ from __future__ import annotations
34
+
35
+ from typing import NamedTuple
36
+
37
+ import jax
38
+ import jax.numpy as jnp
39
+
40
+ from .kernels import SQRT3, HelmParams, k_helm_mat
41
+
42
+
43
+ class SpdeOps(NamedTuple):
44
+ phi: jnp.ndarray # (2, 2) one-step transition e^{F dt}
45
+ L_Q: jnp.ndarray # (2, 2) chol of process noise Q
46
+ L_Pinf: jnp.ndarray # (2, 2) chol of stationary covariance P_inf
47
+ L_space: jnp.ndarray # (2N, 2N) chol of the spatial Helmholtz Gram
48
+
49
+
50
+ def temporal_matrices(time_ls, time_var, dt: float):
51
+ """Phi = exp(F dt), Q = P_inf - Phi P_inf Phi^T, P_inf (paper F.1).
52
+
53
+ F = [[0, 1], [-lam^2, -2 lam]] with lam = sqrt(3)/l is -lam*I + N with N
54
+ nilpotent (N^2 = 0), so exp(F dt) = e^{-lam dt} (I + N dt) in closed form.
55
+ """
56
+ lam = SQRT3 / time_ls
57
+ e = jnp.exp(-lam * dt)
58
+ phi = e * jnp.array(
59
+ [[1.0 + lam * dt, dt], [-(lam**2) * dt, 1.0 - lam * dt]]
60
+ )
61
+ pinf = jnp.array([[time_var, 0.0], [0.0, lam**2 * time_var]])
62
+ q = pinf - phi @ pinf @ phi.T
63
+ return phi, q, pinf
64
+
65
+
66
+ def make_ops(R: jnp.ndarray, p: HelmParams, dt: float, jitter: float = 1e-8) -> SpdeOps:
67
+ """Build the SPDE operators for spatial grid R (N, 2)."""
68
+ phi, q, pinf = temporal_matrices(p.time_ls, p.time_var, dt)
69
+ Ks = k_helm_mat(R, R, p)
70
+ Ks = Ks + jitter * jnp.eye(Ks.shape[0])
71
+ return SpdeOps(
72
+ phi=phi,
73
+ L_Q=jnp.linalg.cholesky(q + jitter * jnp.eye(2)),
74
+ L_Pinf=jnp.linalg.cholesky(pinf),
75
+ L_space=jnp.linalg.cholesky(Ks),
76
+ )
77
+
78
+
79
+ def _step(X, key, ops):
80
+ """One exact transition: X <- X Phi^T + L_space Z L_Q^T.
81
+
82
+ Cov(E_ia, E_jb) = (L_space L_space^T)_ij (L_Q L_Q^T)_ab = K_space_ij Q_ab,
83
+ i.e. vec(E) ~ N(0, K_space (x) Q) as required (App. E.1 Kronecker Cholesky).
84
+ """
85
+ Z = jax.random.normal(key, X.shape, dtype=X.dtype)
86
+ return X @ ops.phi.T + ops.L_space @ Z @ ops.L_Q.T
87
+
88
+
89
+ def propagate(X0: jnp.ndarray, key, ops: SpdeOps, n_steps: int) -> jnp.ndarray:
90
+ """Propagate an extended state n_steps times.
91
+
92
+ Returns the *velocity* field history of shape (n_steps + 1, N, 2), i.e. only
93
+ the f-component of the extended state at each step (including the initial).
94
+ """
95
+ keys = jax.random.split(key, n_steps)
96
+
97
+ def body(X, k):
98
+ Xn = _step(X, k, ops)
99
+ return Xn, Xn[:, 0]
100
+
101
+ _, hist = jax.lax.scan(body, X0, keys)
102
+ out = jnp.concatenate([X0[None, :, 0], hist], axis=0) # (n_steps+1, 2N)
103
+ return out.reshape(n_steps + 1, -1, 2)
104
+
105
+
106
+ def prior_sample(key, R: jnp.ndarray, ops: SpdeOps, n_steps: int) -> jnp.ndarray:
107
+ """Exact prior sample of the temporal Helmholtz GP on R over a time grid.
108
+
109
+ Starts from the stationary distribution f(R,0) ~ N(0, K_space (x) P_inf) and
110
+ propagates. Cost is O((2 N_space)^2 N_t) (paper F.4) versus O((2 N_space
111
+ N_t)^3) for a dense draw -- this is what makes generating the 25x25x1001
112
+ synthetic ground-truth fields of Sec. 5.2 tractable at all.
113
+
114
+ Returns velocity fields (n_steps + 1, N, 2).
115
+ """
116
+ k0, k1 = jax.random.split(key)
117
+ Z = jax.random.normal(k0, (ops.L_space.shape[0], 2), dtype=R.dtype)
118
+ X0 = ops.L_space @ Z @ ops.L_Pinf.T
119
+ return propagate(X0, k1, ops, n_steps)
ballast/trajectory.py ADDED
@@ -0,0 +1,138 @@
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
1
+ """Lagrangian observer advection and observation model (paper Sec. H.1).
2
+
3
+ An observer released at (s, t) is advected by Euler discretisation
4
+
5
+ s_{n+1} = s_n + delta_t V(s_n, t_n), t_{n+1} = t_n + delta_t
6
+
7
+ with delta_t = 0.01. The field is only known on the spatial grid, so V(s, t) is
8
+ piecewise constant over grid cells ("the velocity at a spatial location will be
9
+ that of the grid cell containing the location"). The observer is terminated as
10
+ soon as it leaves the region. Observations are taken every delta_obs = 0.05 with
11
+ i.i.d. N(0, 0.1^2) noise.
12
+
13
+ Everything is batched over particles and written for fixed shapes: a particle
14
+ that has left the region is frozen and flagged invalid, and downstream Gram
15
+ matrices mask it out (see gp.noise_gram).
16
+ """
17
+
18
+ from __future__ import annotations
19
+
20
+ import jax
21
+ import jax.numpy as jnp
22
+
23
+
24
+ class Grid:
25
+ """Regular (or mildly uneven) rectangular grid with piecewise-constant lookup.
26
+
27
+ Cell centres are R = outer product of `xs` and `ys` in row-major order
28
+ (index = ix * ny + iy), matching the spatial layout used everywhere else.
29
+ """
30
+
31
+ def __init__(self, xs: jnp.ndarray, ys: jnp.ndarray):
32
+ self.xs = jnp.asarray(xs)
33
+ self.ys = jnp.asarray(ys)
34
+ self.nx = self.xs.shape[0]
35
+ self.ny = self.ys.shape[0]
36
+ self.n = self.nx * self.ny
37
+ # cell edges: midpoints between centres, extended to the outer half-cells
38
+ self.x_edges = self._edges(self.xs)
39
+ self.y_edges = self._edges(self.ys)
40
+ X, Y = jnp.meshgrid(self.xs, self.ys, indexing="ij")
41
+ self.R = jnp.stack([X.reshape(-1), Y.reshape(-1)], axis=-1) # (n, 2)
42
+
43
+ @staticmethod
44
+ def _edges(c: jnp.ndarray) -> jnp.ndarray:
45
+ mid = 0.5 * (c[1:] + c[:-1])
46
+ lo = c[0] - (mid[0] - c[0])
47
+ hi = c[-1] + (c[-1] - mid[-1])
48
+ return jnp.concatenate([jnp.array([lo]), mid, jnp.array([hi])])
49
+
50
+ def inside(self, s: jnp.ndarray) -> jnp.ndarray:
51
+ """(..., 2) -> (...) bool: is the point within the region's outer edges?"""
52
+ return (
53
+ (s[..., 0] >= self.x_edges[0])
54
+ & (s[..., 0] <= self.x_edges[-1])
55
+ & (s[..., 1] >= self.y_edges[0])
56
+ & (s[..., 1] <= self.y_edges[-1])
57
+ )
58
+
59
+ def cell_index(self, s: jnp.ndarray) -> jnp.ndarray:
60
+ """(..., 2) -> (...) flat index of the containing cell (clipped at borders)."""
61
+ ix = jnp.clip(jnp.searchsorted(self.x_edges, s[..., 0]) - 1, 0, self.nx - 1)
62
+ iy = jnp.clip(jnp.searchsorted(self.y_edges, s[..., 1]) - 1, 0, self.ny - 1)
63
+ return ix * self.ny + iy
64
+
65
+ def lookup(self, field: jnp.ndarray, s: jnp.ndarray) -> jnp.ndarray:
66
+ """field (n, 2) at points s (..., 2) -> (..., 2), piecewise constant."""
67
+ return field[self.cell_index(s)]
68
+
69
+ def snap(self, s: jnp.ndarray) -> jnp.ndarray:
70
+ """Snap points to the centre of their containing cell.
71
+
72
+ The ground-truth field exists only on the grid, and a drifter measures
73
+ "the velocity of the grid cell containing the location" (paper Sec. H.1).
74
+ That measurement is therefore a noisy observation of f at the *cell
75
+ centre*, and is what the GP must be conditioned on.
76
+
77
+ Regressing it at the drifter's exact position instead is misspecified:
78
+ for the Sec. 5.2 setup the within-cell field variation has sd ~0.29
79
+ (cell 0.167 wide vs stream lengthscale 0.5), i.e. ~3x the assumed
80
+ sigma_obs = 0.1. Feeding that mismatch to a GP that believes the noise is
81
+ 0.1 makes it interpolate discretisation error: the posterior mean
82
+ overshoots to ~3x the true field range and the field error rises above
83
+ the prior as drifters are added. Snapping removes the misspecification
84
+ exactly and restores the expected monotone error decay.
85
+ """
86
+ return self.R[self.cell_index(s)]
87
+
88
+
89
+ def advect(
90
+ grid: Grid,
91
+ fields: jnp.ndarray,
92
+ s0: jnp.ndarray,
93
+ active0: jnp.ndarray,
94
+ dt: float,
95
+ obs_every: int,
96
+ ):
97
+ """Advect particles through a time-varying field and record observations.
98
+
99
+ Parameters
100
+ ----------
101
+ fields : (n_steps + 1, n_cells, 2) velocity field history, fields[k] is the
102
+ field at time t_start + k*dt.
103
+ s0 : (P, 2) initial positions.
104
+ active0 : (P,) bool, whether each particle exists at all.
105
+
106
+ Returns
107
+ -------
108
+ pos : (n_obs, P, 2) observation positions, n_obs = n_steps // obs_every
109
+ valid : (n_obs, P) bool, observation is inside the region and the particle
110
+ had not yet left
111
+ tidx : (n_obs,) int, step index of each observation
112
+
113
+ Observations are recorded at steps obs_every, 2*obs_every, ... The release
114
+ instant itself is not an observation; the first measurement is one
115
+ observation interval after deployment.
116
+ """
117
+ n_steps = fields.shape[0] - 1
118
+
119
+ def body(carry, k):
120
+ s, alive = carry
121
+ v = grid.lookup(fields[k], s)
122
+ s_new = jnp.where(alive[:, None], s + dt * v, s)
123
+ alive_new = alive & grid.inside(s_new)
124
+ return (s_new, alive_new), (s_new, alive_new)
125
+
126
+ (_, _), (traj, alive_hist) = jax.lax.scan(
127
+ body, (s0, active0 & grid.inside(s0)), jnp.arange(n_steps)
128
+ )
129
+ # traj[k] is the position after step k+1, i.e. at time t_start + (k+1)*dt
130
+ sel = jnp.arange(obs_every - 1, n_steps, obs_every)
131
+ return traj[sel], alive_hist[sel], sel + 1
132
+
133
+
134
+ def observe(key, grid: Grid, fields: jnp.ndarray, pos, valid, tidx, noise_sd: float):
135
+ """Sample noisy velocity measurements at the recorded observation points."""
136
+ v = jax.vmap(lambda f, s: grid.lookup(f, s))(fields[tidx], pos)
137
+ eps = noise_sd * jax.random.normal(key, v.shape, dtype=v.dtype)
138
+ return jnp.where(valid[..., None], v + eps, 0.0)