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July 15, 2015 22:47
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analysis_name: RUBY_SWEEP_0 # defaults to analysis | |
## working directory defaults to current working directory | |
## all relative paths specified herein are assumed to be in the working_dir | |
## any files not in working_dir should be specified with an absolute path | |
#working_dir: | |
multiprocessing: 1 # "all", or "half", or -1 means all but one, defaults to -1 | |
material: | |
definitions: materials.cpl | |
active: ruby | |
image_series: | |
file: | |
stem: raw_data/RUBY_%04d # can include relative or absolute path | |
ids: [4537, 4538] # or can use globs: ["*2[4-9]"] | |
images: | |
start: 2 | |
omega: | |
start: -60.0 | |
step: 0.25 | |
stop: 60.0 | |
dark: RUBY_4537_medianDark | |
flip: v # ~, v, h, hv, vh, cw, ccw | |
instrument: | |
parameters: example_calibration.yml | |
detector: # this section is only needed to convert old files to the new spec | |
parameters_old: ge_ceo2.par # the old detector spec, produced by the GUI | |
pixels: # this section required to convert from old detector spec | |
rows: 2048 | |
columns: 2048 | |
size: [0.200, 0.200] # [row height, col width] mm | |
find_orientations: | |
orientation_maps: | |
# A file name must be specified. If it doesn't exist, one will be created | |
file: RUBY_4537-4538_t15_eta-omega.cpl | |
threshold: 15 | |
bin_frames: 1 # defaults to 1 | |
## "all", or a list of hkl orders used to find orientations | |
## defaults to all orders listed in the material definition | |
active_hkls: [0,1,2,3,4,5] | |
## either search full quaternion grid, or seed search based on sparse | |
## orientation maps | |
#use_quaternion_grid: some/file/name # defaults to seeded search | |
seed_search: # this section is ignored if use_quaternion_grid is defined | |
hkl_seeds: [0,1,2] # hkls ids to use, must be defined for seeded search | |
fiber_step: 1.0 # degrees, defaults to ome tolerance | |
threshold: 1 # defaults to 1 | |
omega: | |
tolerance: 1.0 # in degrees, defaults to 2x ome step | |
## specify the branch cut, in degrees. The range must be 360 degrees. | |
## defaults to ["image_series:omega:start", "image_series:omega:start"+-360] | |
## depending on sign of "image_series:omega:step" | |
#period: [-180, 180] # in degrees, defaults to full 360 starting at "ome start" | |
eta: | |
tolerance: 1.0 # in degrees, defaults to 2x ome step | |
mask: 5 # degrees, mask angles close to ome rotation axis, defaults to 5 | |
clustering: | |
radius: 1.0 | |
completeness: 0.51 # completeness threshold | |
#algorithm: fclusterdata # defaults to dbscan | |
fit_grains: | |
do_fit: true # if false, extracts grains but doesn't fit. defaults to true | |
estimate: RUBY_SWEEP_0/grains.out # defaults to None | |
npdiv: 2 # number of polar pixel grid subdivisions, defaults to 2 | |
panel_buffer: 10 # don't fit spots within this many pixels from edge | |
threshold: 25 | |
tolerance: | |
tth: [0.25, 0.086] # tolerance lists must be identical length | |
eta: [2.0, 0.75] | |
omega: [1.0, 0.25] | |
tth_max: 14.75 # true, false, or a non-negative value, defaults to true | |
--- | |
analysis_name: RUBY_SWEEP_1 # defaults to analysis | |
image_series: | |
file: | |
ids: [4539, 4540] # or can use globs: ["*2[4-9]"] | |
--- | |
analysis_name: RUBY_SWEEP_2 # defaults to analysis | |
image_series: | |
file: | |
ids: [4541, 4542] # or can use globs: ["*2[4-9]"] |
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