Working with ECOSTRESS Evapotranspiration Data

Details:

Published: March 14, 2019

Working with ECOSTRESS Evapotranspiration Data

This tutorial demonstrates how to work with the ECOSTRESS Evapotranspiration PT-JPL Daily L3 Global 70m Version 1 (ECO3ETPTJPL.001) data product in Python.

The Land Processes Distributed Active Archive Center (LP DAAC) distributes the Ecosystem Spaceborne Thermal Radiometer Experiment on Space Station (ECOSTRESS) data products. The ECOSTRESS mission is tasked with measuring the temperature of plants to better understand how much water plants need and how they respond to stress. ECOSTRESS products are archived and distributed in the HDF5 file format as swath-based products.

In this tutorial, you will use Python to perform a swath to grid conversion to project the swath data on to a grid with a defined coordinate reference system (CRS), compare ECOSTRESS data with ground-based AmeriFlux flux tower observations, and export science dataset (SDS) layers as GeoTIFF files that can be loaded into a GIS and/or Remote Sensing software program.


Example: Converting a swath ECO3ETPTJPL.001 HDF5 file into a GeoTIFF with a defined CRS and comparing ECOSTRESS Evapotranspiration (ET) with ground-based ET observations from an AmeriFlux flux tower location in California.

Data Used in the Example:

  • Data Product: ECOSTRESS Evapotranspiration PT-JPL Daily L3 Global 70m Version 1 (ECO3ETPTJPL.001)
    • Science Dataset (SDS) layers:
      • ETinst
      • ETinstUncertainty
  • Data Product: ECOSTRESS Geolocation Daily L1B Global 70m Version 1 (ECO1BGEO.001)
    • Science Dataset (SDS) layers:
      • Latitude
      • Longitude
  • Data Product: AmeriFlux Ground Observations for Flux Tower US-CZ3: Sierra Critical Zone, Sierra Transect, Sierran Mixed Conifer, P301
    • Variables:
      • Latent Heat (W/m2)

Topics Covered:

  1. Getting Started
    1a. Import Packages
    1b. Set Up the Working Environment
    1c. Retrieve Files
  2. Importing and Interpreting Data
    2a. Open an ECOSTRESS HDF5 File and Read File Metadata
    2b. Subset SDS Layers
  3. Performing Swath2grid Conversion
    3a. Import Geolocation File
    3b. Define Projection and Output Grid
    3c. Read SDS Metadata
    3d. Perform K-D Tree Resampling
    3e. Basic Image Processing
  4. Exporting Results
    4a. Set Up a Dictionary
    4b. Define CRS and Export as GeoTIFFs
  5. Combining ECOSTRESS and AmeriFlux Tower Data
    5a. Loading Tables with Pandas
    5b. Locate ECOSTRESS Pixel from Lat/Lon Coordinates
  6. Visualizing Data
    6a. Create Colormap
    6b. Plot ET Data
    6c. Exporting an Image
  7. Comparing Observations
    7a. Calculate Distribution of ECOSTRESS Data
    7b. Visualize Ground Observations
    7c. Combine ECOSTRESS and Ground Observations

Before Starting this Tutorial:

Dependencies:

  • This tutorial was tested using Python 3.6.7.
  • A NASA Earthdata Login account is required to download the data used in this tutorial. You can create an account at the link provided.
  • Libraries: h5py, numpy, pandas, matplotlib, datetime, pyproj, pyresample, gdal
  • The Geospatial Data Abstraction Library (GDAL) is required.

For a complete list of packages and a yml file that can be used to create your own environment, check out windows-py.yml or mac-py.yml.

  • Need help setting up an environment? check out the Python Environment Setup section in the README.

Example Data:

This tutorial uses an ECO3ETPTJPL.001 (and accompanying ECO1BGEO.001) observation from August 05, 2018. Until the data are released publicly, you can download the files directly via NASA Earthdata Search using the query in the link provided. Note that NASA Earthdata Search will only work for Early Adopters. You can alternatively download the granules below from the following location (follow the Workshop Training Material link).
- ECOSTRESS_L1B_GEO_00468_007_20180805T220314_0502_02.h5
- ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02.h5

The AmeriFlux Latent Heat data used in Section 4 can be downloaded via a csv file

Source Code used to Generate this Tutorial:

If you are simply looking to batch process/perform the swath2grid conversion for ECOSTRESS files, be sure to check out the ECOSTRESS Swath to Grid Conversion Script.

NOTE: This tutorial was developed specifically for the ECOSTRESS Evapotranspiration PT-JPL Level 3, Version 1 HDF5 files and will need to be adapted to work with other ECOSTRESS products.


1. Getting Started


1a. Import Packages

Import the python packages required to complete this tutorial.

# Import packages
import h5py
import os
from os.path import join
import pyproj
import numpy as np
import pandas as pd
import datetime
from dateutil import parser
import matplotlib.pyplot as plt
from matplotlib.colors import LinearSegmentedColormap
from pyresample import geometry as geom
from pyresample import kd_tree as kdt
from osgeo import gdal, gdal_array, gdalconst, osr

# Set plots inside of the Jupyter Notebook
%matplotlib inline

1b. Set Up the Working Environment

The input directory is defined as the current working directory. Note that you will need to have the jupyter notebook and example data (.h5 and .csv) stored in this directory in order to execute the tutorial successfully.

# Current working directory will be set as the input directory
inDir = os.getcwd() + os.sep                                                     
print("input directory:\n{}".format(inDir))

# Set output directory
outDir = os.path.normpath(os.path.split(inDir)[0] + os.sep + 'output') + os.sep  
print("output directory:\n{}".format(outDir))

# Create output directory
if not os.path.exists(outDir): 
    os.makedirs(outDir)
input directory:
C:\ECOSTRESS\
output directory:
C:\ECOSTRESS\output\

Make sure that the ECOSTRESS .h5 data files, and Ameriflux ET data file (.csv) are located in the input directory printed above.


1c. Retrieve Files

Make sure that the ECO1BGEO and ECO3ETPTJPL .h5 files listed in the directions have been downloaded to the inDir defined above to follow along in the tutorial.

# List directory contents and create lists of ECOSTRESS HDF5 files (GEO, ET)
geoList = [file for file in os.listdir() if file.endswith('.h5') and 'GEO' in file]
print("geolocation:\n{}".format("\n".join(geoList)))
ecoList = [file for file in os.listdir() if file.endswith('.h5') and 'GEO' not in file]
print("products:\n{}".format("\n".join(ecoList)))
geolocation:
ECOSTRESS_L1B_GEO_00468_007_20180805T220314_0502_02.h5
products:
ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02.h5

The standard format for ECOSTRESS filenames is as follows:

ECOSTRESS_L3_ET_PT-JPL: Product Type
00468: Orbit number; starting at start of mission, ascending equatorial crossing
007: Scene ID; starting at first scene of first orbit
20180805T220314: Date and time of data start: YYYYMMDDThhmmss
0502: Build ID of software that generated product, Major+Minor (2+2 digits)
02: Product version number (2 digits)


2. Importing and Interpreting Data


2a. Open an ECOSTRESS HDF5 File

Read in an ECOSTRESS HDF5 file using the h5py package.

f = h5py.File(ecoList[0])             # Read in ECOSTRESS HDF5 file
ecoName = ecoList[0].split('.h5')[0]  # Keep original filename
print(ecoName)
ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02

2b. Subset SDS Layers and read SDS Metadata

Identify and generate a list of all the SDS layers in the HDF5 file.

# Create a list of all SDS inside of the .h5 file
eco_objs = []
f.visit(eco_objs.append)
ecoSDS = [str(obj) for obj in eco_objs if isinstance(f[obj], h5py.Dataset)] 
for dataset in ecoSDS[0:10]: 
    print(dataset)
EVAPOTRANSPIRATION PT-JPL/ETcanopy
EVAPOTRANSPIRATION PT-JPL/ETdaily
EVAPOTRANSPIRATION PT-JPL/ETinst
EVAPOTRANSPIRATION PT-JPL/ETinstUncertainty
EVAPOTRANSPIRATION PT-JPL/ETinterception
EVAPOTRANSPIRATION PT-JPL/ETsoil
L3_ET_PT-JPL Metadata/AncillaryFileAerosolOpticalDepth
L3_ET_PT-JPL Metadata/AncillaryFileAirTemperatureNWP
L3_ET_PT-JPL Metadata/AncillaryFileAirTemperatureRS
L3_ET_PT-JPL Metadata/AncillaryFileAlbedo

Below, subset the SDS list to the two layers needed for comparison with the ground-based AmeriFlux data, ETinst and ETinstUncertainty.

# Subset list to ETinst and ETinstUncertainty
sds = ['ETinst', 'ETinstUncertainty']
ecoSDS = [dataset for dataset in ecoSDS if dataset.endswith(tuple(sds))]
for dataset in ecoSDS:
    print(dataset.split('/')[-1])
ETinst
ETinstUncertainty

3. Performing Swath2grid Conversion

Resample the native ECOSTRESS swath data to a grid with defined coordinate reference system (CRS).


3a. Import Geolocation File

The latitude and longitude arrays from the ECO1BGEO product for the same ECOSTRESS orbit/scene ID are needed to perform the swath2grid conversion on the ECO3ETPT-JPL file.

# Find the matching ECO1BGEO file from the file list
geo = [geoFile for geoFile in geoList if ecoList[0][-37:] in geoFile]
print(geo[0])
print(ecoList[0])
ECOSTRESS_L1B_GEO_00468_007_20180805T220314_0502_02.h5
ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02.h5

Read in the ECO1BGEO file, search for the latitude and longitude SDS, and import into Python as arrays.

# Open Geo File
g = h5py.File(geo[0])
geo_objs = []
g.visit(geo_objs.append)

# Search for lat/lon SDS inside data file
latSD = [str(obj) for obj in geo_objs if isinstance(g[obj], h5py.Dataset) and '/latitude' in obj]
lonSD = [str(obj) for obj in geo_objs if isinstance(g[obj], h5py.Dataset) and '/longitude' in obj]

# Open SDS as arrays
lat = g[latSD[0]].value.astype(np.float)
lon = g[lonSD[0]].value.astype(np.float)

# Read the array dimensions
dims = lat.shape
print(dims)
(5632, 5400)

3b. Define Projection and Output Grid

The latitude and longitude arrays from the ECO1BGEO product for the same ECOSTRESS orbit/scene ID are needed to perform the swath2grid conversion on the ECO3ETPT-JPL file.

The following sections use the pyresample package to resample the ECOSTRESS swath dataset to a grid using nearest neighbor method. This process begins by defining the swath dimensions using the lat/lon arrays below.

# Set swath definition from lat/lon arrays
swathDef = geom.SwathDefinition(lons=lon, lats=lat)
swathDef.corners
[(-118.72374893600771, 34.220901494817554),
 (-121.8667573806392, 36.84466762740315),
 (-118.81986958831025, 39.05335446928084),
 (-115.71680093109661, 36.355977323511624)]

Define the coordinates in the middle of the swath, which are used to calculate an estimate of the output rows/columns for the gridded output.

# Define the lat/lon for the middle of the swath
mid = [int(lat.shape[1] / 2) - 1, int(lat.shape[0] / 2) - 1]
midLat, midLon = lat[mid[0]][mid[1]], lon[mid[0]][mid[1]]
midLat, midLon
(36.63135938975165, -118.8874589751626)

Below, pyproj.Proj is used to perform a cartographic transformation by defining an Azimuthal Equidistant projection centered on the midpoint of the swath. Once the projection is defined, convert the lower left and upper right corners of the lat/lon arrays to a location (in meters) in the new projection. Lastly, measure the distance between the corners and divide by 70 (meters), the nominal pixel size that we are aiming for. Azimuthal Equidistant projection was chosen here based on the following characteristics of this projection:

  • Units in meters (necessary for defining 70 m pixels)
  • Distances between all points are proportionally correct from center point
  • Azimuth (direction) are correct from the center point
# Define AEQD projection centered at swath center
epsgConvert = pyproj.Proj("+proj=aeqd +lat_0={} +lon_0={}".format(midLat, midLon))

# Use info from AEQD projection bbox to calculate output cols/rows/pixel size
llLon, llLat = epsgConvert(np.min(lon), np.min(lat), inverse=False)
urLon, urLat = epsgConvert(np.max(lon), np.max(lat), inverse=False)
areaExtent = (llLon, llLat, urLon, urLat)
cols = int(round((areaExtent[2] - areaExtent[0]) / 70))  # 70 m pixel size
rows = int(round((areaExtent[3] - areaExtent[1]) / 70))

Use number of rows and columns generated above from the AEQD projection to set a representative number of rows and columns in the Geographic area definition, which will then be translated to degrees below, then take the smaller of the two pixel dims to determine output size and ensure square pixels.

# Define Geographic projection
epsg, proj, pName = '4326', 'longlat', 'Geographic'

# Define bounding box of swath
llLon, llLat, urLon, urLat = np.min(lon), np.min(lat), np.max(lon), np.max(lat)
areaExtent = (llLon, llLat, urLon, urLat)

# Create area definition with estimated number of columns and rows
projDict = {'proj': proj, 'datum': 'WGS84', 'units': 'degree'}
areaDef = geom.AreaDefinition(epsg, pName, proj, projDict, cols, rows, areaExtent)
areaDef
Area ID: 4326
Description: Geographic
Projection ID: longlat
Projection: {'datum': 'WGS84', 'proj': 'longlat', 'units': 'degree'}
Number of columns: 7844
Number of rows: 7667
Area extent: (-121.8667573806392, 34.220901494817554, -115.71680093109661, 39.05335446928083)

Below, square the pixels by setting the pixel size to the smaller of the x any y values output by the AreaDefinition, then use the pixel size to recalculate the number of output cols/rows.

# Square pixels and calculate output cols/rows
ps = np.min([areaDef.pixel_size_x, areaDef.pixel_size_y])
cols = int(round((areaExtent[2] - areaExtent[0]) / ps))
rows = int(round((areaExtent[3] - areaExtent[1]) / ps))

# Set up a new Geographic area definition with the refined cols/rows
areaDef = geom.AreaDefinition(epsg, pName, proj, projDict, cols, rows, areaExtent)

Below, use pyresample kd_tree's get_neighbour_info to create arrays with information on the nearest neighbor to each grid point.

This is the most computationally heavy task in the swath2grid conversion and using get_neighbour_info speeds up the process if you plan to resample multiple SDS within an ECOSTRESS product (compute once instead of for every SDS).

# Get arrays with information about the nearest neighbor to each grid point 
index, outdex, indexArr, distArr = kdt.get_neighbour_info(swathDef, areaDef, 210, neighbours=1)

Above, the function is comparing the swath and area definitions to locate the nearest neighbor (neighbours=1). 210 is the radius_of_influence, or the radius used to search for the nearest neighboring pixel in the swath (in meters).


3c. Read SDS Metadata

List the attributes for the ETinst layer, which can then be used to define the fill value and scale factor.

# Read in ETinst and print out SDS attributes
s = ecoSDS[0]
ecoSD = f[s].value 
for attr in f[s].attrs:
    if type(f[s].attrs[attr]) == np.ndarray:
        print(f'{attr} = {f[s].attrs[attr][0]}')
    else:
        print(f'{attr} = {f[s].attrs[attr].decode("utf-8")}')
_FillValue = nan
units = W/m^2
long_name = Instantaneous Latent Heat Flux
valid_max = 2000.0
valid_min = 0.0

Extract the scale factor, add offset and fill value from the SDS metadata.

# Read SDS attributes and define fill value, add offset, and scale factor if available
try:
    fv = int(f[s].attrs['_FillValue'])
except KeyError:
    fv = None
except ValueError:
    fv = f[s].attrs['_FillValue'][0]
try:
    sf = f[s].attrs['_Scale'][0]
except:
    sf = 1
try:
    add_off = f[s].attrs['_Offset'][0]
except:
    add_off = 0
try:
    units = f[s].attrs['units'].decode("utf-8")
except:
    units = 'none'

3d. Perform K-D Tree Resampling

Remember that the resampling has been split into two steps. In section 3b. arrays containing the nearest neighbor to each grid point were created. The second step is to use those arrays to retrieve a resampled result.

# Perform K-D Tree nearest neighbor resampling (swath 2 grid conversion)
ETgeo = kdt.get_sample_from_neighbour_info('nn', areaDef.shape, ecoSD, index, outdex, indexArr, fill_value=fv)

Above, resample the swath ecoSD array using nearest neighbor (already calculated in section 3b. and defined above as the index, outdex, and indexArr), and also set the fill value that was defined in section 3c.

Below, define the geotransform for the output (upper left x, horizontal pixel size, rotation, upper left y, rotation, vertical pixel size).

# Define the geotransform 
gt = [areaDef.area_extent[0], ps, 0, areaDef.area_extent[3], 0, -ps]
gt
[-121.8667573806392,
 0.0006302925491669857,
 0,
 39.05335446928083,
 0,
 -0.0006302925491669857]

3e. Basic Image Processing

Apply the scale factor and add offset and set the fill value defined in the previous section on the resampled data.

ETgeo = ETgeo * sf + add_off            # Apply Scale Factor and Add Offset
ETgeo[ETgeo == fv * sf + add_off] = fv  # Set Fill Value

Rerun steps 3c - 3e for ETinstUncertainty.

s = ecoSDS[1]
ecoSD = f[s].value
try:
    fv = int(f[s].attrs['_FillValue'])
except KeyError:
    fv = None
except ValueError:
    fv = f[s].attrs['_FillValue'][0]
try:
    sf = f[s].attrs['_Scale'][0]
except:
    sf = 1
try:
    add_off = f[s].attrs['_Offset'][0]
except:
    add_off = 0
UNgeo = kdt.get_sample_from_neighbour_info('nn', areaDef.shape, ecoSD, index, outdex, indexArr, fill_value=fv)
UNgeo = UNgeo * sf + add_off
UNgeo[UNgeo == fv * sf + add_off] = fv

4. Exporting Results


4a. Set Up a Dictionary

In this section, create a dictionary containing each of the arrays that will be exported as GeoTIFFs.

# Set up dictionary of arrays to export
outFiles = {'ETinst': ETgeo, 'ETinstUncertainty': UNgeo}

4b. Define CRS and Export as GeoTIFFs

Now that the data have been imported and resampled into a gridded raster array, export the results as GeoTIFFs using a for loop in this section.

# Loop through each item in dictionary created above
for file in outFiles:

    # Set up output name
    outName = join(outDir, '{}_{}.tif'.format(ecoName, file))
    print("output file:\n{}\n".format(outName))

    # Get driver, specify dimensions, define and set output geotransform
    height, width = outFiles[file].shape
    driv = gdal.GetDriverByName('GTiff')
    dataType = gdal_array.NumericTypeCodeToGDALTypeCode(outFiles[file].dtype)
    d = driv.Create(outName, width, height, 1, dataType)
    d.SetGeoTransform(gt)

    # Create and set output projection, write output array data
    # Define target SRS
    srs = osr.SpatialReference()
    srs.ImportFromEPSG(int(epsg))
    d.SetProjection(srs.ExportToWkt())
    srs.ExportToWkt()

    # Write array to band
    band = d.GetRasterBand(1)
    band.WriteArray(outFiles[file])

    # Define fill value if it exists, if not, set to mask fill value
    if fv is not None and fv != 'NaN':
        band.SetNoDataValue(fv)
    else:
        try:
            band.SetNoDataValue(outFiles[file].fill_value)
        except AttributeError:
            pass
    band.FlushCache()
    d, band = None, None    
output file:
C:\ECOSTRESS\output\ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02_ETinst.tif

output file:
C:\ECOSTRESS\output\ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02_ETinstUncertainty.tif

5. Combining ECOSTRESS and AmeriFlux Tower Data


5a. Loading Tables with Pandas

In this section, begin by highlighting how to open a csv file using the pandas package.

The AmeriFlux tower data was provided by Mike Goulden for the AmeriFlux US-CZ3 tower. The csv includes half-hourly observations of Latent Heat (W/m2) for the same day as the ECOSTRESS observation.

# Import csv file with AmeriFlux data and drop NaNs
towerData = pd.read_csv('tower_data.csv')
towerData = towerData.dropna()

Next, use the parser package and a lambda function to go through each time stamp and reformat to date and time objects.

# Define a lambda function to use the parser packgage to convert each time stamp to a datetime object
towerData["Date/Time"] = towerData["Time"].apply(lambda x: parser.parse(x))
towerData["Time"] = towerData["Date/Time"].apply(lambda x: datetime.time(x.hour, x.minute))
towerData = towerData[["Date/Time", "Time", "LE"]]
towerData
.dataframe tbody tr th:only-of-type { vertical-align: middle; } .dataframe tbody tr th { vertical-align: top; } .dataframe thead th { text-align: right; }
Date/Time Time LE
1 2018-08-05 09:30:00 09:30:00 18.027752
3 2018-08-05 10:00:00 10:00:00 68.495970
5 2018-08-05 10:30:00 10:30:00 89.050031
7 2018-08-05 11:00:00 11:00:00 154.564199
9 2018-08-05 11:30:00 11:30:00 118.685090
11 2018-08-05 12:00:00 12:00:00 107.071870
13 2018-08-05 12:30:00 12:30:00 189.551249
15 2018-08-05 13:00:00 13:00:00 129.985112
19 2018-08-05 14:00:00 14:00:00 139.651745
21 2018-08-05 14:30:00 14:30:00 155.416112
23 2018-08-05 15:00:00 15:00:00 124.511936
25 2018-08-05 15:30:00 15:30:00 106.666146
27 2018-08-05 16:00:00 16:00:00 176.321112
29 2018-08-05 16:30:00 16:30:00 203.363058
31 2018-08-05 17:00:00 17:00:00 166.714904
33 2018-08-05 17:30:00 17:30:00 124.236027
35 2018-08-05 18:00:00 18:00:00 96.232450
37 2018-08-05 18:30:00 18:30:00 133.121365
39 2018-08-05 19:00:00 19:00:00 44.660266
41 2018-08-05 19:30:00 19:30:00 11.618052
43 2018-08-05 20:00:00 20:00:00 44.201492

5b. Locate ECOSTRESS Pixel from Lat/Lon Coordinates

Calculate the gridded pixel nearest to the tower location.

towerLat, towerLon = 37.0674, -119.1951  # AmeriFlux US-CZ3 tower location

# Calculate tower lat/lon distance from upper left corner, then divide by pixel size to find x,y pixel location
Tcol = int(round((towerLon - gt[0]) / gt[1]))
Trow = int(round((towerLat - gt[3]) / gt[5]))

# Print ET at the tower location
ETgeo[Trow, Tcol]                               
162.27896

6. Visualizing Data


6a. Create a Colormap

Before plotting the ET data, set up an Evapotranspiration color map using LinearSegmentedColormap from the matplotlib package.

# Create a colormap for the ET data
ETcolors = ["#f6e8c3", "#d8b365", "#99974a", "#53792d", "#6bdfd2", "#1839c5"]
ETcmap = LinearSegmentedColormap.from_list("ET", ETcolors)

6b. Calculate Local Overpass Time

ECOSTRESS observation times are reported in Universal Time Coordinated (UTC). Below, grab the observation time from the filename and convert to local time using the longitude location of the tower.

# Grab UTC time of observation from file name
ecoTime = ecoName.split('_')[-3]
ecoTime
'20180805T220314'

Next, convert UTC observation time to local overpass time.

observationTime = parser.parse(ecoTime)
solarOverpass = observationTime + datetime.timedelta(hours=(np.radians(towerLon) / np.pi * 12))
overpass = datetime.time(solarOverpass.hour, solarOverpass.minute)
date = observationTime.strftime('%Y-%m-%d')

6c. Plot ET Data

In this section, begin by highlighting the functionality of the matplotlib plotting package. First, make a plot of the entire gridded ET output. Next, zoom in on the tower location and add some additional parameters to the plot. Finally, export the completed plot to an image file.

title = 'ECO3ETPTJPL Evapotranspiration'
SDSname = ecoSDS[0].split("/")[-1]
fig = plt.figure(figsize=(9.7,7.6))                                                       # Set the figure size (x,y)
fig.suptitle(f'{title} ({ecoSDS[0].split("/")[-1]})\n{date} at {overpass}', fontsize=22)  # Add title for the plots
plt.axis('off')                                                                           # Remove axes from plot
im = plt.imshow(ETgeo, cmap=ETcmap);                                                        # Plot array using colormap
plt.scatter(Tcol, Trow, color="black", marker='x')                                        # Plot tower location

# Add a colormap legend
plt.colorbar(im, orientation='horizontal', fraction=0.05, pad=0.004, label=f'ET ({units})', shrink=0.6).outline.set_visible(True)

png


6d. Exporting an Image

Zoom in to get a closer look at the region surrounding the AmeriFlux tower by creating a subset.

# Set a Radius and calculate subset region from flux tower location (row, col)
radius = 1700
ETsubset = ETgeo[(Trow - radius):(Trow + radius + 1), (Tcol - radius):(Tcol + radius + 1)]

Make another plot, this time zoomed in to the tower location. Export the plot as a .png file.

fig = plt.figure(figsize=(14,12))                                                 # Set the figure size (x,y)
fig.suptitle(f'{title} ({SDSname})\n{date} at {overpass}', fontsize=26)           # Add title for the plots
plt.axis('off')                                                                   # Remove axes from plot
im = plt.imshow(ETsubset, cmap=ETcmap);                                             # Plot array using colormap
plt.scatter(ETsubset.shape[0]/2, ETsubset.shape[1]/2, color="black", marker='x')  # Tower is in middle of subset

# Add a colormap legend
plt.colorbar(im, orientation='horizontal', fraction=0.05, pad=0.004, label=f'ET ({units})', shrink=0.6).outline.set_visible(True)

# Set up file name and export to png file
figure_filename = join(outDir, "{}_{}.png".format(ecoName, SDSname))
print("figure filename: {}".format(figure_filename))
fig.savefig(figure_filename, dpi=300)
plt.show()
figure filename: C:\ECOSTRESS\output\ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02_ETinst.png

png


7. Comparing Observations


7a. Calculate Distribution of ECOSTRESS Data

First, collect a 3x3 grid centered on the flux tower pixel as a subset to calculate statistics on.

# Subset data to 3x3 grid surrounding flux tower for both layers
ETfootprint = ETgeo[(Trow - 1):(Trow + 2), (Tcol - 1):(Tcol + 2)] 
UNfootprint = UNgeo[(Trow - 1):(Trow + 2), (Tcol - 1):(Tcol + 2)] 
print(ETfootprint)
[[155.45839 132.1322  132.1322 ]
 [162.27896 162.27896 181.59097]
 [170.64388 170.89914 175.31497]]

In case the 3x3 grid contains missing values, use np.nanmedian to ignoring missing values and calculate the measure of central tendency.

ETmedian = np.nanmedian(ETfootprint)
UNmedian = np.nanmedian(UNfootprint)
print(f"Median ET: {ETmedian:0.3f} \nUncertainty: {UNmedian:0.3f}")
Median ET: 162.279 
Uncertainty: 161.677

Next, generate a probability density function for the 3x3 grid of ET values.

pd.DataFrame({title: ETfootprint.flatten()}).plot.kde()                                   # Pandas Kernel Density Estimate
plt.title(f'Probability Density of {SDSname} Surrounding US-CZ3\n{date} at {overpass}');  # Title
plt.xlabel(f'{SDSname} ({units})');                                                       # X-axis label

png


7b. Visualize Ground Observations

Next, examine the series of eddy covariance observations from the AmeriFlux US-CZ3 dataset.

fig = plt.figure(figsize=(12,7))                                                                      # Set fig size (x,y)
ax = fig.add_subplot(111)                                                                             # Create a subplot
ax.plot(towerData.Time, towerData.LE, 'k', lw=2.5, color='black')                                     # Plot as a black line
ax.set_title(f'Time Series of Eddy Covariance Data at Site US-CZ3', fontsize=20, fontweight='bold');  # Set Title
ax.set_ylabel('Latent Heat (W/m^2)', fontsize=18);                                                    # Y-axis label
ax.set_xlabel(f'Time of Day ({date})', fontsize=18);                                                  # X-axis label
ax.set_xticks(np.array(towerData.Time));                                                              # Set the x ticks
ax.set_xticklabels(towerData.Time, rotation=45,fontsize=12);                                          # Set x tick labels

png

Above, we can see the daily range in Latent Heat as captured by the eddy covariance observations on the flux tower.


7c. Combine ECOSTRESS and Ground Observations

Finally, compare the ECOSTRESS Evapotranspiration and uncertainty with the time series of observations from the flux tower.

# Set the figure size, create a subplot
fig = plt.figure(1, figsize=(12, 7))
ax = fig.add_subplot(111)

# Plot the flux tower observatisons followed by the ecostress median ET and median uncertainty
ax.plot(towerData.Time, towerData.LE, 'k', lw=2.5, color='black')
ax.plot(overpass, ETmedian, 'bo', ms=10, color='darkgreen')
ax.errorbar(overpass, ETmedian, yerr=UNmedian, lw=2.0, c='lightgreen', fmt='o', capsize=3, capthick=2)

# Set x/y axes and labels
ax.set_xlabel(f'Time of Day ({date})', fontsize=18);
ax.set_xticks(np.array(towerData.Time));
ax.set_xticklabels(towerData.Time, rotation=45,fontsize=12);
ax.set_ylabel("Latent Heat Flux (Wm2)", fontsize=16, fontweight='bold')

# Add a title and export figure as png file
ax.set_title(f"Time Series of Eddy Covariance Data at Site US-CZ3\n vs. {title} ({SDSname})", fontsize=22)
figure_filename = join(outDir, "{}_{}_vs_fluxtower.png".format(ecoName, SDSname))
print("figure filename: {}".format(figure_filename))
fig.savefig(figure_filename, bbox_inches='tight')
figure filename: C:\ECOSTRESS\output\ECOSTRESS_L3_ET_PT-JPL_00468_007_20180805T220314_0502_02_ETinst_vs_fluxtower.png

png


Citations

  • Fisher, J.B., Halverson, G.H., Jewell, L., Freepartner, R., Cawse-Nicholson, K., Freeborn, D., (2018). ECOSTRESS Evapotranspiration PT-JPL Daily L3 Global 70m Version 1 [Data set]. NASA EOSDIS Land Processes DAAC. doi: 10.5067/ECOSTRESS/ECO3ETPTJPL.001

  • Goulden, M., (2018). AmeriFlux US-CZ3 Sierra Critical Zone, Sierra Transect, Sierran Mixed Conifer, P301, doi:10.17190/AMF/1419512.

  • Krehbiel, C., and Halverson, G.H., (2019). Working with ECOSTRESS Evapotranspiration Data [Jupyter Notebook]. Retrieved from https://git.earthdata.nasa.gov/projects/LPDUR/repos/tutorial-ecostress/browse


Contact Information

Material written by Cole Krehbiel1 and Gregory Halverson2

Contact: LPDAAC@usgs.gov

Voice: +1-866-573-3222

Organization: Land Processes Distributed Active Archive Center (LP DAAC)

Website: https://lpdaac.usgs.gov/

Date last modified: 03-13-2019

1Innovate! Inc., contractor to the U.S. Geological Survey, Earth Resources Observation and Science (EROS) Center, Sioux Falls, South Dakota, 57198-001, USA. Work performed under USGS contract G15PD00467 for LP DAAC3.

3LP DAAC Work performed under NASA contract NNG14HH33I.

2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA

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