mrcImageFourierNeighborCorrelation
From EosPedia
mrcImageFourierNeighborCorrelation is Eos's Command to check a resolution by utilizing the redundancy of Fourier Space.
Contents
List of option
Main option
Option | Essential/Optional | Description | Default |
---|---|---|---|
-i | Essential | Input: mrcImage(3D) | NULL |
-o | Optional | Output: ASCII(FNC) | stdout |
-d | Optional | delta on Fourier Space | 0.0 |
-C | Optional | CentreMode | 0 |
-M | Optional | Interpolation Mode | 0 |
-FSC | Optional | Output flag of predicted FSC | |
-mask | Optional | Input: mrcImage(3D)(Mask for FSC) | NULL |
-maskBack | Optional | Input: mrcImage(3D)(Mask for FSC Back) | NULL |
-c | Optional | ConfigurationFile | NULL |
-m | Optional | Mode | 0 |
-h | Optional | Help |
-C details
Value | Description |
---|---|
0 | Centre is ImageCentre Shift: (Nx/2.0, Ny/2.0, Nz/2.0 ) |
1 | Centre is BottomLeft Shift: (0, 0, 0 ) |
2 | Use StartN Shift: (StartNx,StartNy,StartNz) |
-mask details
Use the binary file as same shape as -i file.
(Example)
First, Get Low-frequency component of -i file by using mrcImageLowPassFilter.
Next, binarize it by using mrcImageBinalization(m=32).
-maskBack details
Use the file. (The size is same as -i file, and the all value is 1)
In addition, In addition, multiply the same windowing as -i file.
(Example)
First, get size of -i file by using mrcInfo.
Next, create the image whose value of all is 1, by using mrcImageNullImageCreate(v=1).
Finally, multiply the same windowing by using mrcImageWindowing.
-M details
c.f. Interpolation Mode
-m details
Value | Description |
---|---|
0 |