Source code for SMBcorr.mar_interp_mean

#!/usr/bin/env python
u"""
mar_interp_mean.py
Written by Tyler Sutterley (09/2024)
Interpolates mean MAR products to times and coordinates

INPUTS:
    DIRECTORY: full path to the MAR data directory
        <path_to_mar>/MARv3.11/Greenland/ERA_1958-2019-15km/daily_15km
        <path_to_mar>/MARv3.11/Greenland/NCEP1_1948-2020_20km/daily_20km
        <path_to_mar>/MARv3.10/Greenland/NCEP1_1948-2019_20km/daily_20km
        <path_to_mar>/MARv3.9/Greenland/ERA_1958-2018_10km/daily_10km
    EPSG: projection of input spatial coordinates
    tdec: dates to interpolate in year-decimal
    X: x-coordinates to interpolate
    Y: y-coordinates to interpolate

OPTIONS:
    XNAME: x-coordinate variable name in MAR netCDF4 file
    YNAME: x-coordinate variable name in MAR netCDF4 file
    TIMENAME: time variable name in MAR netCDF4 file
    VARIABLE: MAR product to interpolate
    RANGE: start year and end year of mean file
    SIGMA: Standard deviation for Gaussian kernel
    FILL_VALUE: output fill_value for invalid points

PYTHON DEPENDENCIES:
    numpy: Scientific Computing Tools For Python
        https://numpy.org
        https://numpy.org/doc/stable/user/numpy-for-matlab-users.html
    scipy: Scientific Tools for Python
        https://docs.scipy.org/doc/
    netCDF4: Python interface to the netCDF C library
         https://unidata.github.io/netcdf4-python/netCDF4/index.html
    pyproj: Python interface to PROJ library
        https://pypi.org/project/pyproj/

UPDATE HISTORY:
    Updated 09/2024: use wrapper to importlib for optional dependencies
    Updated 08/2022: updated docstrings to numpy documentation format
    Updated 11/2021: don't attempt triangulation if large number of points
    Updated 01/2021: using conversion protocols following pyproj-2 updates
        https://pyproj4.github.io/pyproj/stable/gotchas.html
    Written 08/2020
"""
from __future__ import print_function

import sys
import os
import re
import warnings
import numpy as np
import scipy.spatial
import scipy.ndimage
import scipy.interpolate
import SMBcorr.spatial
import SMBcorr.utilities

# attempt imports
netCDF4 = SMBcorr.utilities.import_dependency('netCDF4')
pyproj = SMBcorr.utilities.import_dependency('pyproj')

# PURPOSE: read and interpolate a mean field of MAR outputs
[docs]def interpolate_mar_mean(DIRECTORY, EPSG, VERSION, tdec, X, Y, VARIABLE='SMB', XNAME=None, YNAME=None, TIMENAME='TIME', RANGE=[2000,2019], SIGMA=1.5, FILL_VALUE=None): """ Read and interpolates the temporal mean of MAR products Parameters ---------- DIRECTORY: str Working data directory EPSG: str or int input coordinate reference system VERSION: str MAR Version - ``v3.5.2`` - ``v3.9`` - ``v3.10`` - ``v3.11`` tdec: float time coordinates to interpolate in year-decimal X: float x-coordinates to interpolate Y: float y-coordinates to interpolate VARIABLE: str, default 'SMB' MAR product to interpolate - ``SMB``: Surface Mass Balance - ``PRECIP``: Precipitation - ``SNOWFALL``: Snowfall - ``RAINFALL``: Rainfall - ``RUNOFF``: Melt Water Runoff - ``SNOWMELT``: Snowmelt - ``REFREEZE``: Melt Water Refreeze - ``SUBLIM``: Sublimation XNAME: str or NoneType, default None Name of the x-coordinate variable YNAME: str or NoneType, default None Name of the y-coordinate variable TIMENAME: str or NoneType, default 'TIME' Name of the time variable RANGE: list, default [2000,2019] Start and end year of mean SIGMA: float, default 1.5 Standard deviation for Gaussian kernel FILL_VALUE: float or NoneType, default None Output fill_value for invalid points Default will use fill values from data file """ # MAR model projection: Polar Stereographic (Oblique) # Earth Radius: 6371229 m # True Latitude: 0 # Center Longitude: -40 # Center Latitude: 70.5 proj4_params = ("+proj=sterea +lat_0=+70.5 +lat_ts=0 +lon_0=-40.0 " "+a=6371229 +no_defs") # regular expression pattern for MAR dataset rx = re.compile('MAR_SMBavg(.*?){0}-{1}.nc$'.format(*RANGE)) # find mar mean file for RANGE #print(f"looking for files matching MAR_SMBavg {str(RANGE)} in {DIRECTORY}") FILE, = [f for f in os.listdir(DIRECTORY) if rx.match(f)] # Open the MAR NetCDF file for reading with netCDF4.Dataset(os.path.join(DIRECTORY,FILE), 'r') as fileID: nx = len(fileID.variables[XNAME][:]) ny = len(fileID.variables[YNAME][:]) # python dictionary with file variables fd = {} # create a masked array with all data fd[VARIABLE] = np.ma.zeros((ny,nx),fill_value=FILL_VALUE) fd[VARIABLE].mask = np.zeros((ny,nx),dtype=bool) # python dictionary with gaussian filtered variables gs = {} # use a gaussian filter to smooth each model field gs[VARIABLE] = np.ma.zeros((ny,nx), fill_value=FILL_VALUE) gs[VARIABLE].mask = np.ones((ny,nx), dtype=bool) # Open the MAR NetCDF file for reading with netCDF4.Dataset(os.path.join(DIRECTORY,FILE), 'r') as fileID: # surface type SRF=fileID.variables['SRF'][:] # indices of specified ice mask i,j=np.nonzero(SRF == 4) # Get data from netCDF variable and remove singleton dimensions tmp=np.squeeze(fileID.variables[VARIABLE][:]) # combine sectors for multi-layered data if (np.ndim(tmp) == 3): # ice fraction FRA=fileID.variables['FRA'][:]/100.0 # create mask for combining data MASK = np.zeros((ny,nx)) MASK[i,j] = FRA[i,j] # combine data fd[VARIABLE][:,:] = MASK*tmp[0,:,:] + \ (1.0-MASK)*tmp[1,:,:] else: # copy data fd[VARIABLE][:,:] = tmp.copy() # verify mask object for interpolating data fd[VARIABLE].mask[:,:] |= (SRF != 4) # combine mask object through time to create a single mask fd['MASK']=1.0 - np.array(fd[VARIABLE].mask,dtype=np.float64) # MAR coordinates fd['LON']=fileID.variables['LON'][:,:].copy() fd['LAT']=fileID.variables['LAT'][:,:].copy() # convert x and y coordinates to meters fd['x']=1000.0*fileID.variables[XNAME][:].copy() fd['y']=1000.0*fileID.variables[YNAME][:].copy() # use a gaussian filter to smooth mask gs['MASK']=scipy.ndimage.gaussian_filter(fd['MASK'],SIGMA, mode='constant',cval=0) # indices of smoothed ice mask ii,jj = np.nonzero(np.ceil(gs['MASK']) == 1.0) # replace fill values before smoothing data temp1 = np.zeros((ny,nx)) i,j = np.nonzero(~fd[VARIABLE].mask) temp1[i,j] = fd[VARIABLE][i,j].copy() # smooth spatial field temp2 = scipy.ndimage.gaussian_filter(temp1, SIGMA, mode='constant', cval=0) # scale output smoothed field gs[VARIABLE].data[ii,jj] = temp2[ii,jj]/gs['MASK'][ii,jj] # replace valid values with original gs[VARIABLE].data[i,j] = temp1[i,j] # set mask variables for time gs[VARIABLE].mask[ii,jj] = False # convert projection from input coordinates (EPSG) to model coordinates crs1 = pyproj.CRS.from_string(EPSG) crs2 = pyproj.CRS.from_string(proj4_params) transformer = pyproj.Transformer.from_crs(crs1, crs2, always_xy=True) # calculate projected coordinates of input coordinates ix,iy = transformer.transform(X, Y) # check that input points are within convex hull of valid model points gs['x'],gs['y'] = np.meshgrid(fd['x'],fd['y']) # attempt to find a valid delaunay triangulation v,triangle = SMBcorr.spatial.find_valid_triangulation( gs['x'][ii,jj], gs['y'][ii,jj] ) # check if there is a valid triangulation if v: # check where points are within the complex hull of the triangulation interp_points = np.concatenate((ix[:,None],iy[:,None]),axis=1) valid = (triangle.find_simplex(interp_points) >= 0) else: # Check ix and iy against the bounds of x and y valid = (ix >= fd['x'].min()) & (ix <= fd['x'].max()) & \ (iy >= fd['y'].min()) & (iy <= fd['y'].max()) # number of output data points npts = len(tdec) # output interpolated arrays of model variable interp = np.ma.zeros((npts),fill_value=FILL_VALUE,dtype=np.float64) interp.mask = np.ones((npts),dtype=bool) # initially set all values to fill value interp.data[:] = interp.fill_value # if there are valid points if np.any(valid): # indices of valid spatial points ind, = np.nonzero(valid) # create an interpolator for model variable RGI = scipy.interpolate.RegularGridInterpolator( (fd['y'],fd['x']), gs[VARIABLE].data) # create an interpolator for input mask MI = scipy.interpolate.RegularGridInterpolator( (fd['y'],fd['x']), gs[VARIABLE].mask) # interpolate to points interp.data[ind] = RGI.__call__(np.c_[iy[ind],ix[ind]]) interp.mask[ind] = MI.__call__(np.c_[iy[ind],ix[ind]]) # complete mask if any invalid in data invalid, = np.nonzero((interp.data == interp.fill_value) | np.isnan(interp.data)) interp.mask[invalid] = True # return the interpolated values return interp