ballast-repro / data /extract_suntans.py
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#!/usr/bin/env python3
"""
Extract a regular-grid, time-varying 2D surface velocity field from the SUNTANS
internal-tide harmonic atlas (NW Australian shelf / Timor Sea).
This reproduces the physics of `iwatlas/uvdriver.py::extract_hc_uv_spatial` +
`sshdriver.predict_scalar` without depending on the `iwatlas` / `sfoda` stack
(whose requirements.txt pins dead `git+git://` URLs).
Pipeline
--------
1. Read the unstructured cell-centre SSH harmonic amplitudes
SSH_BC_Aa (real) and SSH_BC_Ba (imaginary), shape (Ntide, Nc).
2. Restrict to a rectangular sub-region (+ margin) in the projected coords,
build a single Delaunay triangulation, and reuse it to interpolate all
Ntide x 2 amplitude fields onto a fine regular grid.
3. Take spatial gradients (eta_x, eta_y) with np.gradient on the fine grid,
in TRUE metres.
4. Apply the linear polarization relations (calc_u_complex / calc_v_complex,
copied verbatim from uvdriver.py, including the u/v `den` asymmetry) to get
complex u, v amplitudes per constituent.
5. Reconstruct the time series and subsample onto the final 21x21 grid.
Output (written next to this script):
suntans_fields.npy -- (501, 441, 2) float64, u/v in m/s,
flattened as index = ix*21 + iy
suntans_meta.json -- grid coords, lon/lat bounds, time axis, stats
Projection
----------
xv/yv are projected metres. Inverting them as Web Mercator (EPSG:3857) lands the
mesh in 107.7-142.4 E, 4.2-23.8 S, which matches the documented dataset extent
(NW Australian shelf / Timor Sea), so EPSG:3857 is confirmed.
Note on Web Mercator scale: Web Mercator metres are inflated by 1/cos(lat)
relative to true ground distance. np.gradient is therefore taken with respect to
TRUE metres (dx_true = dx_mercator * cos(lat)), otherwise the gradients -- and
hence the velocities -- would be ~4.5% too small at this latitude.
"""
import json
import os
import numpy as np
import xarray as xr
from scipy.interpolate import LinearNDInterpolator
from scipy.spatial import Delaunay
# ----------------------------------------------------------------------------
# Configuration
# ----------------------------------------------------------------------------
HERE = os.path.dirname(os.path.abspath(__file__))
ATLAS = os.path.join(HERE, "suntans_atlas.nc")
R_EARTH = 6378137.0 # Web Mercator sphere radius [m]
# Region centre, in projected (Web Mercator) metres. Selected by scanning the
# Australian NW shelf band (112-126 E, 11-20 S) for the box with the largest mean
# SSH_BC_var subject to: dense mesh coverage, full containment in the mesh hull,
# and no cell shallower than 150 m.
#
# That last constraint matters. The single most energetic box (~118.8 E, 17.2 S)
# straddles the coastline/islands, where neighbouring cell depths jump abruptly
# (e.g. 55 m -> 395 m over ~2 km, with some 10-15 m coastal cells). SSH_BC
# amplitude steps across those bathymetry discontinuities, so np.gradient there
# returns huge, largely spurious gradients -- that box produced ~10 isolated
# grid points spiking to 1-3.7 m/s against a 0.1-0.5 m/s background. Restricting
# to depths > 150 m keeps the shelf-break generation zone while excluding those
# near-land steps, and every point then lands in the physical range.
#
# Chosen: Rowley Shelf break / continental slope, ~lon 118.1 E, lat 17.3 S,
# depth range ~240-5200 m.
X_CENTRE = 13147867.0
Y_CENTRE = -1952977.0
# Half-width chosen to match the paper's *dimensionless* advection regime rather
# than an arbitrary box size. BALLAST's benefit comes from drifters being
# advected across/out of the region, so what must match is
# (typical speed x horizon) / domain width.
# The paper's stated SUNTANS hyperparameters imply velocity sd
# sqrt((20/5^2 + 0.01/4^2)*15) = 3.47 units/time over a horizon T=5 on a 21-point
# grid, i.e. a ratio of ~0.87. This field's drifters travel ~34 km in the 5 M2
# periods, so a ~40 km box reproduces that ratio (~0.85); the original 150 km box
# gave only 0.24, where drifters barely move and the look-ahead is moot.
# 40 km over 21 points is also ~2 km spacing, i.e. the SUNTANS mesh's native
# resolution -- so this box resolves the model rather than super-resolving it.
HALF_WIDTH = 21e3 # half-width of the target box, in projected metres
MARGIN = 30e3 # extra halo fed to the triangulation, projected metres
MIN_DEPTH = 150.0 # reject the region if any cell is shallower than this [m]
N_OUT = 21 # final grid is N_OUT x N_OUT
SUBSAMPLE = 4 # fine grid is (N_OUT-1)*SUBSAMPLE + 1 = 161 points/side
N_FINE = (N_OUT - 1) * SUBSAMPLE + 1
N_TIMES = 501
N_PERIODS = 5 # total span = N_PERIODS * M2 period
GRAV = 9.81
# ----------------------------------------------------------------------------
# Projection helpers (inverse Web Mercator, EPSG:3857)
# ----------------------------------------------------------------------------
def merc_to_lonlat(x, y):
"""Inverse Web Mercator: projected metres -> (lon, lat) in degrees."""
lon = np.degrees(x / R_EARTH)
lat = np.degrees(2.0 * np.arctan(np.exp(y / R_EARTH)) - np.pi / 2.0)
return lon, lat
# ----------------------------------------------------------------------------
# Physics -- copied EXACTLY from iwatlas/uvdriver.py
# ----------------------------------------------------------------------------
def calc_coriolis(latdeg):
omega = 2 * np.pi / 86400.0
degrad = np.pi / 180.0
return 2 * omega * np.sin(latdeg * degrad)
def calc_u_complex(eta_x, eta_y, omega, f, g=GRAV, tau=1e6):
omegaT = omega + 1j / tau
num = -1j * omegaT * g * eta_x + f * g * eta_y
den = omegaT ** 2.0 - f ** 2.0
return num / den
def calc_v_complex(eta_x, eta_y, omega, f, g=GRAV, tau=1e6):
omegaT = omega + 1j / tau
num = -1j * omegaT * g * eta_y - f * g * eta_x
# NOTE: `omega` here, not `omegaT` -- this u/v asymmetry is present in the
# original iwatlas source and is preserved deliberately.
den = omega ** 2.0 - f ** 2.0
return num / den
# ----------------------------------------------------------------------------
# Main
# ----------------------------------------------------------------------------
def main():
ds = xr.open_dataset(ATLAS)
xv = ds["xv"].values
yv = ds["yv"].values
omega = ds["omega"].values
ntide = omega.shape[0]
lon_all, lat_all = merc_to_lonlat(xv, yv)
print(f"Mesh extent: lon {lon_all.min():.2f} to {lon_all.max():.2f} E, "
f"lat {lat_all.min():.2f} to {lat_all.max():.2f}")
# --- Restrict to sub-region + margin so the triangulation stays small ----
half = HALF_WIDTH + MARGIN
sel = (np.abs(xv - X_CENTRE) < half) & (np.abs(yv - Y_CENTRE) < half)
n_sel = int(sel.sum())
print(f"Cells in sub-region (+{MARGIN/1e3:.0f} km margin): {n_sel}")
if n_sel < 100:
raise RuntimeError("Too few cells in sub-region for interpolation")
# Guard the depth constraint the region was chosen to satisfy (see above):
# shallow cells neighbour abrupt bathymetry steps that corrupt the gradients.
# This applies to the TARGET box only -- the margin is just triangulation
# support outside the output grid, so shallow cells there are harmless.
box = ((np.abs(xv - X_CENTRE) < HALF_WIDTH)
& (np.abs(yv - Y_CENTRE) < HALF_WIDTH))
dv_box = ds["dv"].values[box]
print(f"Depth in target box: min {dv_box.min():.0f} m, "
f"mean {dv_box.mean():.0f} m, max {dv_box.max():.0f} m")
if dv_box.min() < MIN_DEPTH:
raise RuntimeError(
f"Target box contains cells shallower than {MIN_DEPTH} m "
f"(min {dv_box.min():.0f} m); expect spurious gradient spikes."
)
pts = np.column_stack([xv[sel], yv[sel]])
# --- Build the Delaunay triangulation ONCE and reuse for all 35 x 2 fields
print("Building Delaunay triangulation ...")
tri = Delaunay(pts)
# --- Fine regular grid, in projected metres ------------------------------
gx_fine = np.linspace(X_CENTRE - HALF_WIDTH, X_CENTRE + HALF_WIDTH, N_FINE)
gy_fine = np.linspace(Y_CENTRE - HALF_WIDTH, Y_CENTRE + HALF_WIDTH, N_FINE)
GX, GY = np.meshgrid(gx_fine, gy_fine, indexing="ij") # (N_FINE, N_FINE)
# Every fine grid point must fall inside the triangulation, else NaNs.
outside = tri.find_simplex(np.column_stack([GX.ravel(), GY.ravel()])) < 0
if outside.any():
raise RuntimeError(f"{outside.sum()} fine-grid points outside mesh hull")
_, GLAT = merc_to_lonlat(GX, GY)
f_cor = calc_coriolis(GLAT) # (N_FINE, N_FINE)
# --- Grid spacing in TRUE metres ----------------------------------------
# Web Mercator metres are inflated by 1/cos(lat); undo that.
dx_merc = gx_fine[1] - gx_fine[0]
dy_merc = gy_fine[1] - gy_fine[0]
coslat = np.cos(np.radians(GLAT))
print(f"Fine grid: {N_FINE}x{N_FINE}, spacing {dx_merc:.0f} m (Mercator) "
f"~ {dx_merc*coslat.mean():.0f} m (true)")
# --- Interpolate the SSH harmonic amplitudes onto the fine grid ----------
eta_re_all = ds["SSH_BC_Aa"][...].values[:, sel] # (ntide, n_sel)
eta_im_all = ds["SSH_BC_Ba"][...].values[:, sel]
u_c = np.zeros((ntide, N_FINE, N_FINE), np.complex128)
v_c = np.zeros((ntide, N_FINE, N_FINE), np.complex128)
amp_mean = np.zeros(ntide)
print(f"Interpolating and applying polarization relations for {ntide} "
f"constituents ...")
for ii in range(ntide):
# Reuse `tri` -- LinearNDInterpolator accepts a prebuilt Delaunay.
eta_re = LinearNDInterpolator(tri, eta_re_all[ii, :])(GX, GY)
eta_im = LinearNDInterpolator(tri, eta_im_all[ii, :])(GX, GY)
amp_mean[ii] = np.mean(np.abs(eta_re + 1j * eta_im))
# np.gradient along axis 0 = x, axis 1 = y. Spacing in TRUE metres.
eta_re_dx, eta_re_dy = np.gradient(eta_re, dx_merc, dy_merc)
eta_im_dx, eta_im_dy = np.gradient(eta_im, dx_merc, dy_merc)
eta_re_dx, eta_im_dx = eta_re_dx / coslat, eta_im_dx / coslat
eta_re_dy, eta_im_dy = eta_re_dy / coslat, eta_im_dy / coslat
eta_x = eta_re_dx + 1j * eta_im_dx
eta_y = eta_re_dy + 1j * eta_im_dy
u_c[ii] = calc_u_complex(eta_x, eta_y, omega[ii], f_cor)
v_c[ii] = calc_v_complex(eta_x, eta_y, omega[ii], f_cor)
# --- Subsample to the final 21x21 grid ----------------------------------
sl = slice(None, None, SUBSAMPLE)
x_coords = gx_fine[sl]
y_coords = gy_fine[sl]
assert x_coords.size == N_OUT and y_coords.size == N_OUT
u_c = u_c[:, sl, sl] # (ntide, 21, 21)
v_c = v_c[:, sl, sl]
# --- Time axis: 5 M2 periods, 501 steps ---------------------------------
# M2 = the constituent with the largest mean SSH amplitude in this region.
i_m2 = int(np.argmax(amp_mean))
omega_m2 = float(omega[i_m2])
period_m2 = 2 * np.pi / omega_m2
print(f"Dominant constituent: index {i_m2}, omega={omega_m2:.6e} rad/s, "
f"period={period_m2/3600:.3f} h")
times = np.linspace(0.0, N_PERIODS * period_m2, N_TIMES) # seconds
# --- Reconstruct the time series ----------------------------------------
# u(t) = sum_ii [ Re(u_ii)*cos(omega_ii*t) + Im(u_ii)*sin(omega_ii*t) ]
# (matches sshdriver.predict_scalar; mean amplitude a0 = 0 for velocity)
cos_t = np.cos(omega[None, :] * times[:, None]) # (nt, ntide)
sin_t = np.sin(omega[None, :] * times[:, None])
u_t = (np.einsum("tk,kxy->txy", cos_t, u_c.real)
+ np.einsum("tk,kxy->txy", sin_t, u_c.imag))
v_t = (np.einsum("tk,kxy->txy", cos_t, v_c.real)
+ np.einsum("tk,kxy->txy", sin_t, v_c.imag))
# --- Flatten as index = ix*21 + iy (x-major, y-minor) -------------------
# u_t is (nt, ix, iy); C-order ravel of the last two axes gives ix*21+iy.
fields = np.stack([u_t.reshape(N_TIMES, N_OUT * N_OUT),
v_t.reshape(N_TIMES, N_OUT * N_OUT)], axis=-1)
fields = np.ascontiguousarray(fields, dtype=np.float64)
# --- Verify --------------------------------------------------------------
assert fields.shape == (N_TIMES, N_OUT * N_OUT, 2), fields.shape
assert np.isfinite(fields).all(), "NaN/Inf in output"
# Explicitly confirm the ix*21+iy ordering round-trips.
_chk = fields[:, :, 0].reshape(N_TIMES, N_OUT, N_OUT)
assert np.allclose(_chk, u_t)
for ix in (0, 7, 20):
for iy in (0, 13, 20):
assert fields[3, ix * N_OUT + iy, 0] == u_t[3, ix, iy]
print("Ordering check passed: index = ix*21 + iy")
speed = np.hypot(fields[..., 0], fields[..., 1])
stats = {
"mean_speed": float(speed.mean()),
"max_speed": float(speed.max()),
"std_u": float(fields[..., 0].std()),
"std_v": float(fields[..., 1].std()),
}
time_var = fields.std(axis=0).mean()
space_var = fields.std(axis=1).mean()
print(f"Shape: {fields.shape}")
print(f"mean_speed={stats['mean_speed']:.4f} m/s "
f"max_speed={stats['max_speed']:.4f} m/s")
print(f"std_u={stats['std_u']:.4f} std_v={stats['std_v']:.4f} m/s")
print(f"Variation over time (mean std over t): {time_var:.4f} m/s")
print(f"Variation over space (mean std over x): {space_var:.4f} m/s")
assert time_var > 0, "field does not vary in time"
assert space_var > 0, "field does not vary in space"
lon_c, lat_c = merc_to_lonlat(np.array([x_coords[0], x_coords[-1]]),
np.array([y_coords[0], y_coords[-1]]))
meta = {
"x_coords": [float(v) for v in x_coords],
"y_coords": [float(v) for v in y_coords],
"lon_bounds": [float(lon_c[0]), float(lon_c[1])],
"lat_bounds": [float(lat_c[0]), float(lat_c[1])],
"times_seconds": [float(t) for t in times],
"omega_M2": omega_m2,
"region_note": (
"Australian NW shelf: Rowley Shelf break / continental slope "
"internal-tide generation zone. Centre ~118.1 E, 17.3 S; box "
"150 km x 150 km in EPSG:3857 (Web Mercator) metres, ~143 km true. "
"Depth range ~240-5200 m. Selected as the highest mean SSH_BC_var "
"box within 112-126 E, 11-20 S subject to dense mesh coverage, full "
"containment in the mesh hull, and no cell shallower than 150 m "
"(shallow/coastal cells sit next to abrupt bathymetry steps that "
"make np.gradient return spurious gradients). Coordinates "
"x_coords/y_coords are projected EPSG:3857 metres. Fields are "
"flattened as index = ix*21 + iy."
),
"velocity_stats": stats,
"projection": "EPSG:3857 (Web Mercator)",
"n_constituents": int(ntide),
"dominant_constituent_index": i_m2,
"m2_period_seconds": float(period_m2),
}
np.save(os.path.join(HERE, "suntans_fields.npy"), fields)
with open(os.path.join(HERE, "suntans_meta.json"), "w") as fh:
json.dump(meta, fh, indent=2)
print(f"lon bounds: {meta['lon_bounds']}")
print(f"lat bounds: {meta['lat_bounds']}")
print("Wrote suntans_fields.npy and suntans_meta.json")
if __name__ == "__main__":
main()