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- | ~~NOTOC~~ | ||
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- | ===== sx3dvariability ===== | ||
- | 3D Variablity Estimation: Calculate 3D variability using a set of aligned projection images as an input. | ||
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- | ===== Usage ===== | ||
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- | Usage in command line: | ||
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- | sx3dvariability.py | ||
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- | ===== Typical usage ===== | ||
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- | sx3dvariability exists only in MPI version. | ||
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- | - For asymmetric structures: < | ||
- | mpirun -np 472 sx3dvariability.py stack --CTF --img_per_grp=100 --fl=0.25 --aa=0.1 --ave3D=vol.hdf --var3D=var_vol.hdf ''' | ||
- | </ | ||
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- | - For symmetric structures (e.g. c2):< | ||
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- | sx3dvariability.py stack --symmetrize --sym=c2 | ||
- | mpirun -np 472 sx3dvariability.py bdb:sdata --CTF --img_per_grp=100 --fl=0.25 --aaf=0.1 --ave3D=vol.hdf --var3D=var_vol.hdf --sym=c2 | ||
- | </ | ||
- | |||
- | ===== Input ===== | ||
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- | === Main Parameters === | ||
- | ; prj_stack : Input image stack: The images must containt the 3D orientation parameters in the header and optionally CTF information. (default required string) | ||
- | ; fl : Low-pass filter frequency [1/Pixel]: Filter to be applied to the images prior to variability calculation. By default, no filtering. (default 0.0) | ||
- | ; aa : Low-pass filter fall-off: Filter to be applied to the images prior to variability calculation. By default, no filtering. (default 0.0) | ||
- | ; CTF : Use CTF: If set to true, the a CTF correction will be applied using the parameters found in the image headers. (default False) | ||
- | ; img_per_grp : Number of projections: | ||
- | ; symmetrize : Symmetrise input stack: Please skip this preparation step if the structure is asymmetrical (i.e. c1), since it is required only when the structure has internal symmetry. (default False) | ||
- | ; sym : Point-group symmetry: Only required if the structure has symmetry higher than c1. Notice this step can be run with only one CPU and there is no MPI version for it. (default c1) | ||
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- | === Advanced Parameters === | ||
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- | ; no_norm : Skip normalization: | ||
- | ; radius : Radius for 3D variability [Pixels]: Normally, use the particle radius. (default -1) | ||
- | ; npad : Image padding factor: The images are padded to achieve the original size times this option. (default 2) | ||
- | ; VAR : Stack on input consists of 2D variances: (default False) | ||
- | ; SND : Squared normalized differences: | ||
- | ; VERBOSE : Verbose: Useful for debugging. (default False) | ||
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- | ===== Output ===== | ||
- | ; ave2D : Output 2D averages: (default none) | ||
- | ; var2D : Output 2D variances: (default none) | ||
- | ; ave3D : Output 3D average: 3D reconstruction computed from projections averaged within respective angular neighbourhood. It should be used to assess the resolvability and possible artifacts of the variability map. (default none) | ||
- | ; var3D : Output 3D variability: | ||
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- | ===== Description ===== | ||
- | The program calculates the variability observed in a collection of image projections. Structures with symmetry require preparing data before calculating the variability. The data preparation step would symmetrise the data and output a bdb:sdata for variability calculation. sx3dvariability.py can be slow. | ||
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- | ==== Author / Maintainer ==== | ||
- | Pawel Penczek | ||
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- | ==== Keywords ==== | ||
- | Category 1:: APPLICATIONS | ||
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- | ==== Files ==== | ||
- | sx3dvariability.py | ||
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- | ==== Maturity ==== | ||
- | alpha:: it works. | ||
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- | ==== Known Bugs ==== | ||
- | None. | ||