https://github.com/GeoscienceAustralia/PyRate
Tip revision: 870e8de119e875c47d19bc97f4c8518cc5bf8f20 authored by Sudipta Basak on 18 August 2021, 23:54:39 UTC
ported build.yml from develop
ported build.yml from develop
Tip revision: 870e8de
input_parameters.conf
# PyRate configuration file for GAMMA-format interferograms
#
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# Optional ON/OFF switches - ON = 1; OFF = 0
# Coherence masking (PREPIFG)
cohmask: 0
# Orbital error correction (CORRECT)
orbfit: 1
# APS correction using spatio-temporal filter (CORRECT)
apsest: 0
# Optional save of numpy array files for output products (MERGE)
savenpy: 0
# Optional save of incremental time series products (TIMESERIES/MERGE)
savetsincr: 0
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# Multi-threading parameters used by correct/stacking/timeseries
# gamma prepifg runs in parallel on a single machine if parallel = 1
# parallel: 1 = parallel, 0 = serial
parallel: 0
# number of processes
processes: 8
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# Input/Output file locations
#
# File containing the list of interferograms to use.
ifgfilelist: tests/test_data/small_test/gamma_obs/ifms_17
# The DEM file used in the InSAR processing
demfile: tests/test_data/small_test/gamma_obs/20060619_utm.dem
# The DEM header file from GAMMA (*.par) or ROI_PAC (*.rsc).
demHeaderFile: tests/test_data/small_test/gamma_obs/20060619_utm_dem.par
# File listing the pool of available header files (GAMMA: *slc.par, ROI_PAC: *.rsc)
hdrfilelist: tests/test_data/small_test/gamma_obs/headers
# File listing the pool of available coherence files.
cohfilelist: tests/test_data/small_test/coherence/coherence_17
# Directory to write the outputs to
outdir: out/
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# PREPIFG parameters
#------------------------------------
# Input data format: ROI_PAC = 0, GAMMA = 1
processor: 1
# Coherence threshold value for masking, between 0 and 1
cohthresh: 0.3
# Multi-look/subsampling factor in east (x) and north (y) dimension
ifglksx: 1
ifglksy: 1
# Cropping options
# ifgcropopt: 1 = minimum extent 2 = maximum extent 3 = crop 4 = no cropping
# ifgxfirst,ifgyfirst: longitude (x) and latitude (y) of north-west corner
# ifgxlast,ifgylast: longitude (x) and latitude (y) of south-east corner
ifgcropopt: 4
ifgxfirst: 150.92
ifgyfirst: -34.18
ifgxlast: 150.94
ifgylast: -34.22
# No-data averaging threshold (0 = 0%; 1 = 100%)
noDataAveragingThreshold: 0.5
# The No-data value used in the interferogram files
noDataValue: 0.0
# Nan conversion flag. Set to 1 if missing No-data values are to be converted to NaN
nan_conversion: 1
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# CORRECT parameters
#------------------------------------
# Reference pixel search options
# refx/y: Lon/Lat coordinate of reference pixel. If left blank then search for best pixel will be performed
# refnx/y: number of search grid points in x/y image dimensions
# refchipsize: size of the data window at each search grid point
# refminfrac: minimum fraction of valid (non-NaN) pixels in the data window
refx: 150.941666654
refy: -34.218333314
refnx: 5
refny: 5
refchipsize: 5
refminfrac: 0.01
#------------------------------------
# Reference phase correction method
# refest: 1 = median of the whole interferogram
# refest: 2 = median within the window surrounding the chosen reference pixel
refest: 2
#------------------------------------
# Orbital error correction
# orbfitmethod = 1: interferograms corrected independently; 2: network method
# orbfitdegrees: Degree of polynomial surface to fit (1 = planar; 2 = quadratic; 3 = part-cubic)
# orbfitlksx/y: additional multi-look factor for network orbital correction
orbfitmethod: 2
orbfitdegrees: 1
orbfitlksx: 1
orbfitlksy: 1
#------------------------------------
# APS spatial low-pass filter parameters
# slpfmethod: Spatial low-pass filter method (1: butterworth; 2: gaussian)
# slpfcutoff: cutoff d0 (greater than zero) in km for both butterworth and gaussian filters
# slpforder: order n for butterworth filter (default 1)
# slpnanfill: 1 for interpolation, 0 for zero fill
# slpnanfill_method: linear, nearest, cubic; only used when slpnanfill=1
slpfmethod: 2
slpfcutoff: 0.001
slpforder: 1
slpnanfill: 1
slpnanfill_method: cubic
#------------------------------------
# APS temporal low-pass filter parameters
# tlpfmethod: 1 = Gaussian, 2 = Triangular, 3 = Mean filter
# tlpfcutoff: cutoff t0 for gaussian filter in year;
# tlpfpthr: valid pixel threshold;
tlpfmethod: 3
tlpfcutoff: 0.25
tlpfpthr: 1
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# TIMESERIES parameters
#------------------------------------
# tsmethod: Method for time series inversion (1 = Laplacian Smoothing; 2 = SVD)
# smorder: order of Laplacian smoothing operator (1 = first-order difference; 2 = second-order difference)
# smfactor: smoothing factor for Laplacian smoothing (value provided is converted as 10**smfactor)
# ts_pthr: valid observations threshold for time series inversion
tsmethod: 2
smorder: 2
smfactor: -0.25
ts_pthr: 10
#%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
# STACK parameters
#------------------------------------
# pthr: threshold for minimum number of ifg observations for each pixel
# nsig: threshold for iterative removal of observations
# maxsig: maximum sigma (std dev) used as an output masking threshold applied in Merge step. 0 = OFF.
pthr: 5
nsig: 3
maxsig: 1000