positional arguments:¶

IMAGE

File with input images

options:¶

-h, --help

show this help message and exit

-V, --version

output version and exit

-v, --verbose

show information for each conversions

--debug

show debug information

main arguments:¶

-o OUTPUT, --output OUTPUT

output directory and filename template: eiger2cbf/frame_{index:04d}.cbf

-m MASK, --mask MASK

Read masked pixel from this file

-O OFFSET, --offset OFFSET

index offset, CrysalisPro likes indexes to start at 1, Python starts at 0

-D DUMMY, --dummy DUMMY

Set masked values to this dummy value

--pilatus

Select an image shape similar to Pilatus detectors for compatibiliy with Crysalis

optional behaviour arguments:¶

--dry-run

do everything except modifying the file system

Experimental setup options:¶

-e ENERGY, --energy ENERGY

Energy of the incident beam in keV

-w WAVELENGTH, --wavelength WAVELENGTH

Wavelength of the incident beam in ??

-d DISTANCE, --distance DISTANCE

Detector distance in meters

-b BEAM BEAM, --beam BEAM BEAM

Direct beam in pixels x, y

Goniometer setup:¶

--alpha ALPHA

Goniometer angle alpha value in deg.

--kappa KAPPA

Goniometer angle kappa value in deg.

--chi CHI

Goniometer angle chi value in deg. or formula f(index)

--phi PHI

Goniometer angle phi value in deg. or formula f(index)

--omega OMEGA

Goniometer angle omega value in deg. or formula f(index) like '-180+index*0.1

Image preprocessing (Important: applied in this order!):¶

--rotation ROTATION

Rotate the initial image by this value in degrees. Must be a multiple of 90??.

--transpose

Flip the x/y axis

--flip-ud

Flip the image upside-down

--flip-lr

Flip the image left-right

return codes: 0 means a success. 1 means the conversion contains a failure, 2 means there was an error in the arguments