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"""Wave-filtering pipeline: mask (k, f) spectrum, inverse-FFT to space-time.
Reproduces the filter used in Rios-Berrios et al. (2022, JAMES 14, e2021MS002902,
§2.2.2): meridional average → zero-pad in time → 2D FFT → zero outside a box in
(wavenumber, period) → inverse 2D FFT → trim padding. Rios-Berrios use simple
boxes in k-f space (no dispersion-curve bounds); a separate ``build_dispersion_mask``
helper wraps the existing Wheeler-Kiladis dispersion masks for users who want
tighter regions.
Sign convention (with numpy.fft.fft2 on axes (time, lon) of a real field):
eastward wave exp(i(k*x - omega*t)) lives at (f<0, k>0) and its conjugate (f>0, k<0)
westward wave exp(i(k*x + omega*t)) lives at (f>0, k>0) and its conjugate (f<0, k<0)
i.e. sign(k) * sign(f) < 0 → eastward, sign(k) * sign(f) > 0 → westward.
"""
from __future__ import annotations
from typing import Mapping, Sequence
import numpy as np
import xarray as xr
from scipy.signal import detrend as _detrend
# Rios-Berrios et al. 2022 §2.2.2 — exact filter boxes
RIOS_BERRIOS_FILTERS: Mapping[str, Mapping] = {
"kelvin": dict(k_range=(1, 14), period_range=(2.5, 20.0), direction="eastward"),
"advective": dict(k_range=(4, 28), period_range=(2.5, 20.0), direction="westward"),
"wig_n1": dict(k_range=(1, 14), period_range=(1.8, 4.5), direction="westward"),
# MRG (Yanai) n=0 box: Wheeler & Kiladis (1999), Kiladis et al. (2009) he=8-90 m westward branch.
# Overlaps advective (k=4-10, T=3-9.6 d) intentionally — consistent with existing filter design.
"mrg": dict(k_range=(1, 10), period_range=(3.0, 9.6), direction="westward"),
}
def _axis_index(da: xr.DataArray, name: str) -> int:
return da.dims.index(name)
def prepare_for_filter(
data: xr.DataArray,
pad_zeros: int = 700,
detrend: bool = False,
remove_mean: bool = True,
) -> tuple[xr.DataArray, int]:
"""Remove mean, optionally detrend, and zero-pad the time axis.
Returns (padded_array, original_time_length). The padding is appended at the
end of the time axis, matching Wheeler & Weickmann (2001) / Rios-Berrios (2022).
"""
if "time" not in data.dims:
raise ValueError(f"input must have a 'time' dim; got {data.dims}")
time_axis = _axis_index(data, "time")
n_time = data.sizes["time"]
arr = data.values.astype(np.float64, copy=True)
if detrend:
arr = _detrend(arr, axis=time_axis, type="linear")
if remove_mean:
arr = arr - arr.mean(axis=time_axis, keepdims=True)
if pad_zeros > 0:
pad_shape = list(arr.shape)
pad_shape[time_axis] = pad_zeros
pad = np.zeros(pad_shape, dtype=arr.dtype)
arr = np.concatenate([arr, pad], axis=time_axis)
# Rebuild an xarray with a synthetic padded time coord (monotonic, keeps dt).
if n_time >= 2:
dt = float(data.time.values[1] - data.time.values[0])
else:
dt = 1.0
new_time = np.arange(n_time + pad_zeros, dtype=np.float64) * dt + float(data.time.values[0])
coords = {d: data.coords[d] for d in data.dims if d != "time"}
coords["time"] = new_time
padded = xr.DataArray(arr, dims=data.dims, coords=coords, name=data.name)
padded.attrs.update(data.attrs)
return padded, n_time
def fft_spacetime(data_padded: xr.DataArray, spd: float) -> xr.DataArray:
"""2D complex FFT over (time, lon); return complex DataArray with k, f coords.
Wavenumber is integer zonal wavenumber (fftfreq * nlon).
Frequency is cycles-per-day (fftfreq with d = 1/spd).
"""
for d in ("time", "lon"):
if d not in data_padded.dims:
raise ValueError(f"input must have '{d}' dim; got {data_padded.dims}")
t_ax = _axis_index(data_padded, "time")
x_ax = _axis_index(data_padded, "lon")
nt = data_padded.sizes["time"]
nx = data_padded.sizes["lon"]
z = np.fft.fft2(data_padded.values, axes=(t_ax, x_ax))
freq = np.fft.fftfreq(nt, d=1.0 / spd) # cycles per day
wavenumber = np.fft.fftfreq(nx, d=1.0 / nx) # integer wavenumbers
wavenumber = np.rint(wavenumber).astype(np.int64)
# Replace time/lon coords with frequency/wavenumber
new_dims = tuple(("frequency" if d == "time" else "wavenumber" if d == "lon" else d)
for d in data_padded.dims)
new_coords = {}
for d, nd in zip(data_padded.dims, new_dims):
if d == "time":
new_coords["frequency"] = freq
elif d == "lon":
new_coords["wavenumber"] = wavenumber
else:
new_coords[d] = data_padded.coords[d]
return xr.DataArray(z, dims=new_dims, coords=new_coords)
def build_box_mask(
wavenumber: np.ndarray | xr.DataArray,
frequency: np.ndarray | xr.DataArray,
k_range: tuple[float, float],
period_range: tuple[float, float],
direction: str,
) -> xr.DataArray:
"""Binary mask over (frequency, wavenumber) for a simple k-T box.
k_range (k_min, k_max) magnitudes of integer zonal wavenumber.
period_range (T_min, T_max) days; frequency bounds are 1/T_max and 1/T_min.
direction 'eastward' → sign(k)*sign(f) < 0
'westward' → sign(k)*sign(f) > 0
'both' → symmetric (useful as a sanity switch)
The f=0 row and k=0 column are excluded (no stationary modes).
"""
k = np.asarray(wavenumber)
f = np.asarray(frequency)
K, F = np.meshgrid(k, f) # K,F have shape (nfreq, nwave)
k_min, k_max = k_range
T_min, T_max = period_range
f_lo, f_hi = 1.0 / T_max, 1.0 / T_min
abs_k = np.abs(K)
abs_f = np.abs(F)
in_k = (abs_k >= k_min) & (abs_k <= k_max)
in_f = (abs_f >= f_lo) & (abs_f <= f_hi)
nonzero = (K != 0) & (F != 0)
if direction == "eastward":
dir_mask = (K * F) < 0
elif direction == "westward":
dir_mask = (K * F) > 0
elif direction == "both":
dir_mask = np.ones_like(K, dtype=bool)
else:
raise ValueError(f"direction must be eastward/westward/both; got {direction!r}")
mask = (in_k & in_f & nonzero & dir_mask).astype(np.float64)
return xr.DataArray(
mask,
dims=("frequency", "wavenumber"),
coords={"frequency": f, "wavenumber": k},
attrs=dict(k_range=k_range, period_range=period_range, direction=direction),
)
def apply_mask_ifft(
fft_data: xr.DataArray,
mask: xr.DataArray,
imag_tol: float = 1e-8,
) -> xr.DataArray:
"""Multiply by mask, inverse-FFT to (time, lon), return the real part.
Raises if the recovered imaginary part is larger than ``imag_tol`` relative to
the real-part range — that signals a non-Hermitian mask and a buggy filter.
"""
t_ax = _axis_index(fft_data, "frequency")
x_ax = _axis_index(fft_data, "wavenumber")
# Broadcast mask onto fft_data (adds any extra dims like 'lat' automatically).
masked = fft_data * mask
y = np.fft.ifft2(masked.values, axes=(t_ax, x_ax))
real_range = np.ptp(y.real)
imag_amp = float(np.max(np.abs(y.imag)))
if real_range > 0 and imag_amp > imag_tol * real_range:
raise AssertionError(
f"inverse FFT imaginary residual too large: {imag_amp:.3e} "
f"(real range {real_range:.3e}) — mask likely not Hermitian symmetric"
)
new_dims = tuple(("time" if d == "frequency" else "lon" if d == "wavenumber" else d)
for d in fft_data.dims)
# Caller restores the time coord via trim_padding; here we use integer indices.
coords = {}
for d, nd in zip(fft_data.dims, new_dims):
if d == "frequency":
coords["time"] = np.arange(fft_data.sizes["frequency"])
elif d == "wavenumber":
coords["lon"] = np.arange(fft_data.sizes["wavenumber"])
else:
coords[d] = fft_data.coords[d]
return xr.DataArray(y.real, dims=new_dims, coords=coords)
def trim_padding(
filtered: xr.DataArray,
original_len: int,
reference_time: xr.DataArray,
reference_lon: xr.DataArray,
) -> xr.DataArray:
"""Drop trailing padding and restore the original time/lon coordinates."""
out = filtered.isel(time=slice(0, original_len))
out = out.assign_coords(time=reference_time.values, lon=reference_lon.values)
return out
def filter_wave(
data: xr.DataArray,
wave_type: str,
spd: float = 4.0,
pad_zeros: int = 700,
detrend: bool = False,
remove_mean: bool = True,
lat_bounds: tuple[float, float] | None = None,
filter_spec: Mapping | None = None,
) -> xr.DataArray:
"""Filter a (time, lon) or (time, lat, lon) field to a single wave band.
``wave_type`` selects an entry from ``RIOS_BERRIOS_FILTERS`` unless
``filter_spec`` is given explicitly (dict with k_range, period_range, direction).
If the input is 3D with a 'lat' dim, the field is meridionally averaged over
``lat_bounds`` (inclusive) before filtering; use ``lat_bounds=None`` to average
over all available latitudes.
"""
spec = filter_spec or RIOS_BERRIOS_FILTERS[wave_type]
if "lat" in data.dims:
if lat_bounds is not None:
lo, hi = lat_bounds
data = data.sel(lat=slice(lo, hi))
data = data.mean(dim="lat")
padded, n_time_orig = prepare_for_filter(
data, pad_zeros=pad_zeros, detrend=detrend, remove_mean=remove_mean,
)
z = fft_spacetime(padded, spd=spd)
mask = build_box_mask(z.wavenumber, z.frequency, **spec)
filtered_padded = apply_mask_ifft(z, mask)
out = trim_padding(
filtered_padded,
original_len=n_time_orig,
reference_time=data.time,
reference_lon=data.lon,
)
out.name = f"{data.name or 'field'}_{wave_type}"
out.attrs.update(
wave_type=wave_type,
k_range=tuple(spec["k_range"]),
period_range=tuple(spec["period_range"]),
direction=spec["direction"],
pad_zeros=pad_zeros,
spd=spd,
)
return out
def wave_variance(
data: xr.DataArray,
wave_types: Sequence[str] = tuple(RIOS_BERRIOS_FILTERS.keys()),
spd: float = 4.0,
pad_zeros: int = 700,
lat_bounds: tuple[float, float] | None = (-10, 10),
detrend: bool = False,
) -> xr.Dataset:
"""Variance of raw and wave-filtered fields after meridional average.
Returns a Dataset with:
total_variance scalar, var of the (mean-removed) meridionally-averaged field
filtered_variance (wave_type,), var of each filtered field
"""
if "lat" in data.dims:
if lat_bounds is not None:
data = data.sel(lat=slice(*lat_bounds))
merid = data.mean(dim="lat")
else:
merid = data
total_var = float(((merid - merid.mean(dim="time")) ** 2).mean().values)
var_by_type = []
for wt in wave_types:
f = filter_wave(
merid, wt, spd=spd, pad_zeros=pad_zeros, detrend=detrend, remove_mean=True,
)
var_by_type.append(float((f ** 2).mean().values)) # filtered field has zero mean
out = xr.Dataset(
data_vars=dict(
total_variance=xr.DataArray(total_var),
filtered_variance=xr.DataArray(
np.asarray(var_by_type), dims=("wave_type",),
coords={"wave_type": list(wave_types)},
),
),
attrs=dict(
spd=spd, pad_zeros=pad_zeros,
lat_bounds=str(lat_bounds), detrend=int(bool(detrend)),
),
)
return out
# ─── Future-proof: Wheeler-Kiladis dispersion-curve masks ──────────────────────
def build_dispersion_mask(
wavenumber: np.ndarray | xr.DataArray,
frequency: np.ndarray | xr.DataArray,
wave_type: str,
) -> xr.DataArray:
"""Wrapper over existing dispersion-curve masks in wavenumber_frequency_functions.
Not used for the Rios-Berrios 2022 reproduction; provided so callers can swap
in a Wheeler-Kiladis filter (bounded by equivalent-depth dispersion curves) if
they want tighter regions than the simple k-T box.
"""
from wavenumber_frequency_functions import (
kelvin_wave_mask,
equatorial_rossby_wave_mask,
mrg_wave_mask,
)
wn_da = wavenumber if isinstance(wavenumber, xr.DataArray) else xr.DataArray(
wavenumber, dims=("wavenumber",), coords={"wavenumber": wavenumber},
)
freq_da = frequency if isinstance(frequency, xr.DataArray) else xr.DataArray(
frequency, dims=("frequency",), coords={"frequency": frequency},
)
builders = {
"kelvin": kelvin_wave_mask,
"er": equatorial_rossby_wave_mask,
"mrg": mrg_wave_mask,
}
try:
builder = builders[wave_type]
except KeyError as e:
raise ValueError(
f"dispersion mask only supported for {list(builders)}; got {wave_type!r}"
) from e
m = builder(wn_da, freq_da).astype(np.float64)
return m.transpose("frequency", "wavenumber")