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geetools_VH/SDS_preprocess.py

667 lines
27 KiB
Python

"""This module contains all the functions needed to preprocess the satellite images: creating a
cloud mask and pansharpening/downsampling the images.
Author: Kilian Vos, Water Research Laboratory, University of New South Wales
"""
# Initial settings
import os
import numpy as np
import matplotlib.pyplot as plt
from osgeo import gdal, ogr, osr
import skimage.transform as transform
import skimage.morphology as morphology
import sklearn.decomposition as decomposition
import skimage.exposure as exposure
from pylab import ginput
import pickle
import pdb
import SDS_tools
# Functions
def create_cloud_mask(im_qa, satname):
"""
Creates a cloud mask from the image containing the QA band information.
KV WRL 2018
Arguments:
-----------
im_qa: np.array
Image containing the QA band
satname: string
short name for the satellite (L8, L7, S2)
Returns:
-----------
cloud_mask : np.ndarray of booleans
A boolean array with True where the cloud are present
"""
# convert QA bits depending on the satellite mission
if satname == 'L8':
cloud_values = [2800, 2804, 2808, 2812, 6896, 6900, 6904, 6908]
elif satname == 'L7' or satname == 'L5' or satname == 'L4':
cloud_values = [752, 756, 760, 764]
elif satname == 'S2':
cloud_values = [1024, 2048] # 1024 = dense cloud, 2048 = cirrus clouds
# find which pixels have bits corresponding to cloud values
cloud_mask = np.isin(im_qa, cloud_values)
# remove isolated cloud pixels (there are some in the swash zone and they can cause problems)
if sum(sum(cloud_mask)) > 0 and sum(sum(~cloud_mask)) > 0:
morphology.remove_small_objects(cloud_mask, min_size=10, connectivity=1, in_place=True)
return cloud_mask
def hist_match(source, template):
"""
Adjust the pixel values of a grayscale image such that its histogram matches that of a
target image.
Arguments:
-----------
source: np.array
Image to transform; the histogram is computed over the flattened
array
template: np.array
Template image; can have different dimensions to source
Returns:
-----------
matched: np.array
The transformed output image
"""
oldshape = source.shape
source = source.ravel()
template = template.ravel()
# get the set of unique pixel values and their corresponding indices and
# counts
s_values, bin_idx, s_counts = np.unique(source, return_inverse=True,
return_counts=True)
t_values, t_counts = np.unique(template, return_counts=True)
# take the cumsum of the counts and normalize by the number of pixels to
# get the empirical cumulative distribution functions for the source and
# template images (maps pixel value --> quantile)
s_quantiles = np.cumsum(s_counts).astype(np.float64)
s_quantiles /= s_quantiles[-1]
t_quantiles = np.cumsum(t_counts).astype(np.float64)
t_quantiles /= t_quantiles[-1]
# interpolate linearly to find the pixel values in the template image
# that correspond most closely to the quantiles in the source image
interp_t_values = np.interp(s_quantiles, t_quantiles, t_values)
return interp_t_values[bin_idx].reshape(oldshape)
def pansharpen(im_ms, im_pan, cloud_mask):
"""
Pansharpens a multispectral image (3D), using the panchromatic band (2D) and a cloud mask.
A PCA is applied to the image, then the 1st PC is replaced with the panchromatic band.
KV WRL 2018
Arguments:
-----------
im_ms: np.array
Multispectral image to pansharpen (3D)
im_pan: np.array
Panchromatic band (2D)
cloud_mask: np.array
2D cloud mask with True where cloud pixels are
Returns:
-----------
im_ms_ps: np.ndarray
Pansharpened multisoectral image (3D)
"""
# reshape image into vector and apply cloud mask
vec = im_ms.reshape(im_ms.shape[0] * im_ms.shape[1], im_ms.shape[2])
vec_mask = cloud_mask.reshape(im_ms.shape[0] * im_ms.shape[1])
vec = vec[~vec_mask, :]
# apply PCA to RGB bands
pca = decomposition.PCA()
vec_pcs = pca.fit_transform(vec)
# replace 1st PC with pan band (after matching histograms)
vec_pan = im_pan.reshape(im_pan.shape[0] * im_pan.shape[1])
vec_pan = vec_pan[~vec_mask]
vec_pcs[:,0] = hist_match(vec_pan, vec_pcs[:,0])
vec_ms_ps = pca.inverse_transform(vec_pcs)
# reshape vector into image
vec_ms_ps_full = np.ones((len(vec_mask), im_ms.shape[2])) * np.nan
vec_ms_ps_full[~vec_mask,:] = vec_ms_ps
im_ms_ps = vec_ms_ps_full.reshape(im_ms.shape[0], im_ms.shape[1], im_ms.shape[2])
return im_ms_ps
def rescale_image_intensity(im, cloud_mask, prob_high):
"""
Rescales the intensity of an image (multispectral or single band) by applying
a cloud mask and clipping the prob_high upper percentile. This functions allows
to stretch the contrast of an image for visualisation purposes.
KV WRL 2018
Arguments:
-----------
im: np.array
Image to rescale, can be 3D (multispectral) or 2D (single band)
cloud_mask: np.array
2D cloud mask with True where cloud pixels are
prob_high: float
probability of exceedence used to calculate the upper percentile
Returns:
-----------
im_adj: np.array
The rescaled image
"""
# lower percentile is set to 0
prc_low = 0
# reshape the 2D cloud mask into a 1D vector
vec_mask = cloud_mask.reshape(im.shape[0] * im.shape[1])
# if image contains several bands, stretch the contrast for each band
if len(im.shape) > 2:
# reshape into a vector
vec = im.reshape(im.shape[0] * im.shape[1], im.shape[2])
# initiliase with NaN values
vec_adj = np.ones((len(vec_mask), im.shape[2])) * np.nan
# loop through the bands
for i in range(im.shape[2]):
# find the higher percentile (based on prob)
prc_high = np.percentile(vec[~vec_mask, i], prob_high)
# clip the image around the 2 percentiles and rescale the contrast
vec_rescaled = exposure.rescale_intensity(vec[~vec_mask, i],
in_range=(prc_low, prc_high))
vec_adj[~vec_mask,i] = vec_rescaled
# reshape into image
im_adj = vec_adj.reshape(im.shape[0], im.shape[1], im.shape[2])
# if image only has 1 bands (grayscale image)
else:
vec = im.reshape(im.shape[0] * im.shape[1])
vec_adj = np.ones(len(vec_mask)) * np.nan
prc_high = np.percentile(vec[~vec_mask], prob_high)
vec_rescaled = exposure.rescale_intensity(vec[~vec_mask], in_range=(prc_low, prc_high))
vec_adj[~vec_mask] = vec_rescaled
im_adj = vec_adj.reshape(im.shape[0], im.shape[1])
return im_adj
def preprocess_single(fn, satname):
"""
Creates a cloud mask using the QA band and performs pansharpening/down-sampling of the image.
KV WRL 2018
Arguments:
-----------
fn: str or list of str
filename of the .TIF file containing the image
for L7, L8 and S2 there is a filename for the bands at different resolutions
satname: str
name of the satellite mission (e.g., 'L5')
Returns:
-----------
im_ms: np.array
3D array containing the pansharpened/down-sampled bands (B,G,R,NIR,SWIR1)
georef: np.array
vector of 6 elements [Xtr, Xscale, Xshear, Ytr, Yshear, Yscale] defining the
coordinates of the top-left pixel of the image
cloud_mask: np.array
2D cloud mask with True where cloud pixels are
"""
#=============================================================================================#
# L5 images
#=============================================================================================#
if satname == 'L5':
# read all bands
data = gdal.Open(fn, gdal.GA_ReadOnly)
georef = np.array(data.GetGeoTransform())
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im_ms = np.stack(bands, 2)
# down-sample to 15 m (half of the original pixel size)
nrows = im_ms.shape[0]*2
ncols = im_ms.shape[1]*2
# create cloud mask
im_qa = im_ms[:,:,5]
im_ms = im_ms[:,:,:-1]
cloud_mask = create_cloud_mask(im_qa, satname)
# resize the image using bilinear interpolation (order 1)
im_ms = transform.resize(im_ms,(nrows, ncols), order=1, preserve_range=True,
mode='constant')
# resize the image using nearest neighbour interpolation (order 0)
cloud_mask = transform.resize(cloud_mask, (nrows, ncols), order=0, preserve_range=True,
mode='constant').astype('bool_')
# adjust georeferencing vector to the new image size
# scale becomes 15m and the origin is adjusted to the center of new top left pixel
georef[1] = 15
georef[5] = -15
georef[0] = georef[0] + 7.5
georef[3] = georef[3] - 7.5
# check if -inf or nan values on any band and add to cloud mask
for k in range(im_ms.shape[2]):
im_inf = np.isin(im_ms[:,:,k], -np.inf)
im_nan = np.isnan(im_ms[:,:,k])
cloud_mask = np.logical_or(np.logical_or(cloud_mask, im_inf), im_nan)
# calculate cloud cover
cloud_cover = sum(sum(cloud_mask.astype(int)))/(cloud_mask.shape[0]*cloud_mask.shape[1])
#=============================================================================================#
# L7 images
#=============================================================================================#
elif satname == 'L7':
# read pan image
fn_pan = fn[0]
data = gdal.Open(fn_pan, gdal.GA_ReadOnly)
georef = np.array(data.GetGeoTransform())
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im_pan = np.stack(bands, 2)[:,:,0]
# size of pan image
nrows = im_pan.shape[0]
ncols = im_pan.shape[1]
# read ms image
fn_ms = fn[1]
data = gdal.Open(fn_ms, gdal.GA_ReadOnly)
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im_ms = np.stack(bands, 2)
# create cloud mask
im_qa = im_ms[:,:,5]
cloud_mask = create_cloud_mask(im_qa, satname)
# resize the image using bilinear interpolation (order 1)
im_ms = im_ms[:,:,:5]
im_ms = transform.resize(im_ms,(nrows, ncols), order=1, preserve_range=True,
mode='constant')
# resize the image using nearest neighbour interpolation (order 0)
cloud_mask = transform.resize(cloud_mask, (nrows, ncols), order=0, preserve_range=True,
mode='constant').astype('bool_')
# check if -inf or nan values on any band and eventually add those pixels to cloud mask
for k in range(im_ms.shape[2]+1):
if k == 5:
im_inf = np.isin(im_pan, -np.inf)
im_nan = np.isnan(im_pan)
else:
im_inf = np.isin(im_ms[:,:,k], -np.inf)
im_nan = np.isnan(im_ms[:,:,k])
cloud_mask = np.logical_or(np.logical_or(cloud_mask, im_inf), im_nan)
# calculate cloud cover
cloud_cover = sum(sum(cloud_mask.astype(int)))/(cloud_mask.shape[0]*cloud_mask.shape[1])
# pansharpen Green, Red, NIR (where there is overlapping with pan band in L7)
try:
im_ms_ps = pansharpen(im_ms[:,:,[1,2,3]], im_pan, cloud_mask)
except: # if pansharpening fails, keep downsampled bands (for long runs)
im_ms_ps = im_ms[:,:,[1,2,3]]
# add downsampled Blue and SWIR1 bands
im_ms_ps = np.append(im_ms[:,:,[0]], im_ms_ps, axis=2)
im_ms_ps = np.append(im_ms_ps, im_ms[:,:,[4]], axis=2)
im_ms = im_ms_ps.copy()
#=============================================================================================#
# L8 images
#=============================================================================================#
elif satname == 'L8':
# read pan image
fn_pan = fn[0]
data = gdal.Open(fn_pan, gdal.GA_ReadOnly)
georef = np.array(data.GetGeoTransform())
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im_pan = np.stack(bands, 2)[:,:,0]
# size of pan image
nrows = im_pan.shape[0]
ncols = im_pan.shape[1]
# read ms image
fn_ms = fn[1]
data = gdal.Open(fn_ms, gdal.GA_ReadOnly)
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im_ms = np.stack(bands, 2)
# create cloud mask
im_qa = im_ms[:,:,5]
cloud_mask = create_cloud_mask(im_qa, satname)
# resize the image using bilinear interpolation (order 1)
im_ms = im_ms[:,:,:5]
im_ms = transform.resize(im_ms,(nrows, ncols), order=1, preserve_range=True,
mode='constant')
# resize the image using nearest neighbour interpolation (order 0)
cloud_mask = transform.resize(cloud_mask, (nrows, ncols), order=0, preserve_range=True,
mode='constant').astype('bool_')
# check if -inf or nan values on any band and eventually add those pixels to cloud mask
for k in range(im_ms.shape[2]+1):
if k == 5:
im_inf = np.isin(im_pan, -np.inf)
im_nan = np.isnan(im_pan)
else:
im_inf = np.isin(im_ms[:,:,k], -np.inf)
im_nan = np.isnan(im_ms[:,:,k])
cloud_mask = np.logical_or(np.logical_or(cloud_mask, im_inf), im_nan)
# calculate cloud cover
cloud_cover = sum(sum(cloud_mask.astype(int)))/(cloud_mask.shape[0]*cloud_mask.shape[1])
# pansharpen Blue, Green, Red (where there is overlapping with pan band in L8)
try:
im_ms_ps = pansharpen(im_ms[:,:,[0,1,2]], im_pan, cloud_mask)
except: # if pansharpening fails, keep downsampled bands (for long runs)
im_ms_ps = im_ms[:,:,[0,1,2]]
# add downsampled NIR and SWIR1 bands
im_ms_ps = np.append(im_ms_ps, im_ms[:,:,[3,4]], axis=2)
im_ms = im_ms_ps.copy()
#=============================================================================================#
# S2 images
#=============================================================================================#
if satname == 'S2':
# read 10m bands (R,G,B,NIR)
fn10 = fn[0]
data = gdal.Open(fn10, gdal.GA_ReadOnly)
georef = np.array(data.GetGeoTransform())
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im10 = np.stack(bands, 2)
im10 = im10/10000 # TOA scaled to 10000
# if image contains only zeros (can happen with S2), skip the image
if sum(sum(sum(im10))) < 1:
im_ms = []
georef = []
# skip the image by giving it a full cloud_mask
cloud_mask = np.ones((im10.shape[0],im10.shape[1])).astype('bool')
return im_ms, georef, cloud_mask
# size of 10m bands
nrows = im10.shape[0]
ncols = im10.shape[1]
# read 20m band (SWIR1)
fn20 = fn[1]
data = gdal.Open(fn20, gdal.GA_ReadOnly)
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im20 = np.stack(bands, 2)
im20 = im20[:,:,0]
im20 = im20/10000 # TOA scaled to 10000
# resize the image using bilinear interpolation (order 1)
im_swir = transform.resize(im20, (nrows, ncols), order=1, preserve_range=True,
mode='constant')
im_swir = np.expand_dims(im_swir, axis=2)
# append down-sampled SWIR1 band to the other 10m bands
im_ms = np.append(im10, im_swir, axis=2)
# create cloud mask using 60m QA band (not as good as Landsat cloud cover)
fn60 = fn[2]
data = gdal.Open(fn60, gdal.GA_ReadOnly)
bands = [data.GetRasterBand(k + 1).ReadAsArray() for k in range(data.RasterCount)]
im60 = np.stack(bands, 2)
im_qa = im60[:,:,0]
cloud_mask = create_cloud_mask(im_qa, satname)
# resize the cloud mask using nearest neighbour interpolation (order 0)
cloud_mask = transform.resize(cloud_mask,(nrows, ncols), order=0, preserve_range=True,
mode='constant')
# check if -inf or nan values on any band and add to cloud mask
for k in range(im_ms.shape[2]):
im_inf = np.isin(im_ms[:,:,k], -np.inf)
im_nan = np.isnan(im_ms[:,:,k])
cloud_mask = np.logical_or(np.logical_or(cloud_mask, im_inf), im_nan)
# calculate cloud cover
cloud_cover = sum(sum(cloud_mask.astype(int)))/(cloud_mask.shape[0]*cloud_mask.shape[1])
return im_ms, georef, cloud_mask
def create_jpg(im_ms, cloud_mask, date, satname, filepath):
"""
Saves a .jpg file with the RGB image as well as the NIR and SWIR1 grayscale images.
KV WRL 2018
Arguments:
-----------
im_ms: np.array
3D array containing the pansharpened/down-sampled bands (B,G,R,NIR,SWIR1)
cloud_mask: np.array
2D cloud mask with True where cloud pixels are
date: str
String containing the date at which the image was acquired
satname: str
name of the satellite mission (e.g., 'L5')
Returns:
-----------
Saves a .jpg image corresponding to the preprocessed satellite image
"""
# rescale image intensity for display purposes
im_RGB = rescale_image_intensity(im_ms[:,:,[2,1,0]], cloud_mask, 99.9)
im_NIR = rescale_image_intensity(im_ms[:,:,3], cloud_mask, 99.9)
im_SWIR = rescale_image_intensity(im_ms[:,:,4], cloud_mask, 99.9)
# make figure
fig = plt.figure()
fig.set_size_inches([18,9])
fig.set_tight_layout(True)
# RGB
plt.subplot(131)
plt.axis('off')
plt.imshow(im_RGB)
plt.title(date + ' ' + satname, fontsize=16)
# NIR
plt.subplot(132)
plt.axis('off')
plt.imshow(im_NIR, cmap='seismic')
plt.title('Near Infrared', fontsize=16)
# SWIR
plt.subplot(133)
plt.axis('off')
plt.imshow(im_SWIR, cmap='seismic')
plt.title('Short-wave Infrared', fontsize=16)
# save figure
plt.rcParams['savefig.jpeg_quality'] = 100
fig.savefig(os.path.join(filepath,
date + '_' + satname + '.jpg'), dpi=150)
plt.close()
def preprocess_all_images(metadata, settings):
"""
Saves a .jpg image for all the file contained in metadata.
KV WRL 2018
Arguments:
-----------
sitename: str
name of the site (and corresponding folder)
metadata: dict
contains all the information about the satellite images that were downloaded
cloud_thresh: float
maximum fraction of cloud cover allowed in the images
Returns:
-----------
Generates .jpg files for all the satellite images avaialble
"""
sitename = settings['sitename']
cloud_thresh = settings['cloud_thresh']
# create subfolder to store the jpg files
filepath_jpg = os.path.join(os.getcwd(), 'data', sitename, 'jpg_files', 'preprocessed')
try:
os.makedirs(filepath_jpg)
except:
print('')
# loop through satellite list
for satname in metadata.keys():
# access the images
if satname == 'L5':
# access downloaded Landsat 5 images
filepath = os.path.join(os.getcwd(), 'data', sitename, satname, '30m')
filenames = os.listdir(filepath)
elif satname == 'L7':
# access downloaded Landsat 7 images
filepath_pan = os.path.join(os.getcwd(), 'data', sitename, 'L7', 'pan')
filepath_ms = os.path.join(os.getcwd(), 'data', sitename, 'L7', 'ms')
filenames_pan = os.listdir(filepath_pan)
filenames_ms = os.listdir(filepath_ms)
if (not len(filenames_pan) == len(filenames_ms)):
raise 'error: not the same amount of files for pan and ms'
filepath = [filepath_pan, filepath_ms]
filenames = filenames_pan
elif satname == 'L8':
# access downloaded Landsat 7 images
filepath_pan = os.path.join(os.getcwd(), 'data', sitename, 'L8', 'pan')
filepath_ms = os.path.join(os.getcwd(), 'data', sitename, 'L8', 'ms')
filenames_pan = os.listdir(filepath_pan)
filenames_ms = os.listdir(filepath_ms)
if (not len(filenames_pan) == len(filenames_ms)):
raise 'error: not the same amount of files for pan and ms'
filepath = [filepath_pan, filepath_ms]
filenames = filenames_pan
elif satname == 'S2':
# access downloaded Sentinel 2 images
filepath10 = os.path.join(os.getcwd(), 'data', sitename, satname, '10m')
filenames10 = os.listdir(filepath10)
filepath20 = os.path.join(os.getcwd(), 'data', sitename, satname, '20m')
filenames20 = os.listdir(filepath20)
filepath60 = os.path.join(os.getcwd(), 'data', sitename, satname, '60m')
filenames60 = os.listdir(filepath60)
if (not len(filenames10) == len(filenames20)) or (not len(filenames20) == len(filenames60)):
raise 'error: not the same amount of files for 10, 20 and 60 m'
filepath = [filepath10, filepath20, filepath60]
filenames = filenames10
# loop through images
for i in range(len(filenames)):
# image filename
fn = SDS_tools.get_filenames(filenames[i],filepath, satname)
# preprocess image (cloud mask + pansharpening/downsampling)
im_ms, georef, cloud_mask = preprocess_single(fn, satname)
# calculate cloud cover
cloud_cover = np.divide(sum(sum(cloud_mask.astype(int))),
(cloud_mask.shape[0]*cloud_mask.shape[1]))
# skip image if cloud cover is above threshold
if cloud_cover > cloud_thresh:
continue
# save .jpg with date and satellite in the title
date = filenames[i][:10]
create_jpg(im_ms, cloud_mask, date, satname, filepath_jpg)
def get_reference_sl(metadata, settings):
sitename = settings['sitename']
# check if reference shoreline already exists
filepath = os.path.join(os.getcwd(), 'data', sitename)
filename = sitename + '_ref_sl.pkl'
if filename in os.listdir(filepath):
print('Reference shoreline already exists and was loaded')
with open(os.path.join(filepath, sitename + '_ref_sl.pkl'), 'rb') as f:
refsl = pickle.load(f)
return refsl
else:
satname = 'S2'
# access downloaded Sentinel 2 images
filepath10 = os.path.join(os.getcwd(), 'data', sitename, satname, '10m')
filenames10 = os.listdir(filepath10)
filepath20 = os.path.join(os.getcwd(), 'data', sitename, satname, '20m')
filenames20 = os.listdir(filepath20)
filepath60 = os.path.join(os.getcwd(), 'data', sitename, satname, '60m')
filenames60 = os.listdir(filepath60)
if (not len(filenames10) == len(filenames20)) or (not len(filenames20) == len(filenames60)):
raise 'error: not the same amount of files for 10, 20 and 60 m'
for i in range(len(filenames10)):
# image filename
fn = [os.path.join(filepath10, filenames10[i]),
os.path.join(filepath20, filenames20[i]),
os.path.join(filepath60, filenames60[i])]
# preprocess image (cloud mask + pansharpening/downsampling)
im_ms, georef, cloud_mask = preprocess_single(fn, satname)
# calculate cloud cover
cloud_cover = np.divide(sum(sum(cloud_mask.astype(int))),
(cloud_mask.shape[0]*cloud_mask.shape[1]))
# skip image if cloud cover is above threshold
if cloud_cover > settings['cloud_thresh']:
continue
# rescale image intensity for display purposes
im_RGB = rescale_image_intensity(im_ms[:,:,[2,1,0]], cloud_mask, 99.9)
# make figure
fig = plt.figure()
fig.set_size_inches([18,9])
fig.set_tight_layout(True)
# RGB
plt.axis('off')
plt.imshow(im_RGB)
plt.title('click <skip> if image is not clear enough to digitize the shoreline.\n' +
'Otherwise click on <keep> and start digitizing the shoreline.\n' +
'When finished digitizing the shoreline click on the scroll wheel ' +
'(middle click).', fontsize=14)
plt.text(0, 0.9, 'keep', size=16, ha="left", va="top",
transform=plt.gca().transAxes,
bbox=dict(boxstyle="square", ec='k',fc='w'))
plt.text(1, 0.9, 'skip', size=16, ha="right", va="top",
transform=plt.gca().transAxes,
bbox=dict(boxstyle="square", ec='k',fc='w'))
mng = plt.get_current_fig_manager()
mng.window.showMaximized()
# let user click on the image once
pt_keep = ginput(n=1, timeout=100, show_clicks=True)
pt_keep = np.array(pt_keep)
# if clicks next to <skip>, show another image
if pt_keep[0][0] > im_ms.shape[1]/2:
plt.close()
continue
else:
# let user click on the shoreline
pts = ginput(n=5000, timeout=100000, show_clicks=True)
pts_pix = np.array(pts)
plt.close()
# convert image coordinates to world coordinates
pts_world = SDS_tools.convert_pix2world(pts_pix[:,[1,0]], georef)
image_epsg = metadata[satname]['epsg'][i]
pts_coords = SDS_tools.convert_epsg(pts_world, image_epsg, settings['output_epsg'])
with open(os.path.join(filepath, sitename + '_ref_sl.pkl'), 'wb') as f:
pickle.dump(pts_coords, f)
print('Reference shoreline has been saved')
break
return pts_coords