pypeline.impl.oct package¶
Submodules¶
pypeline.impl.oct.basedata module¶
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class
pypeline.impl.oct.basedata.BaseData(shape, dtype)[source]¶ Bases:
objectBase class for all common data types: spectrum, interferogram, complex and real array, image. etc.
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data¶ the array that contains the actual data
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shape¶ list of int that is the shape of the data array
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dtype¶ the data type for each element in the data array
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dsize¶ total number of elements in data array
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pypeline.impl.oct.conf module¶
This file specifies all the general impl inis
TODO: define what is need to be configured here
pypeline.impl.oct.image module¶
pypeline.image¶
this module contains misc to manipulate general images, 8bit, 16bit, 24bit, etc.
set_dimension: set_voxsize:
- display:
- display image, default to adjust the image size based on the vox_size
- merge: merge2d: merge3d
- merge different color/measurement channels
- project:
- min/max intensity projection, mean projection
segmentation:
pypeline.impl.oct.mock module¶
pypeline.impl.oct.proc module¶
preprocess¶
this module contains all the common processing of OCT rawdata before reconstruct it into images
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pypeline.impl.oct.proc.corr_dispersion(data, disp_coeff)[source]¶ compensate dispersion using 3rd and 2nd order dispersionc oeff
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pypeline.impl.oct.proc.gen_calib(data, win=[], order=4, conf_file_path=[])[source]¶ function gen_calib_coeff(data, win = [], file_path = []) generate the calibration coeff data as non-linear array from 0 to 1 data: input data win: window to filter the data for calcuation file_path: file to save the calib_coeff
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pypeline.impl.oct.proc.gen_disp(data, win=[], conf_file_path=[])[source]¶ function gen_disp_coeff(data, win = [], file_path = []) generate the disp coeff (3rd and 2nd order) by mirror signal data: input data win: the window to filter data update_cfg: update pypeline.ini
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pypeline.impl.oct.proc.gen_disp2(data, win=[0, 1], conf_file_path=[])[source]¶ function gen_disp_coeff2(data, win = [], file_path = []) generate the disp coeff (3rd and 2nd order) iteratively data: input data win: the window to filter data update_cfg: update pypeline.ini
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pypeline.impl.oct.proc.gen_fr_data(data, r2i_ratio, bandwidth=0.4)[source]¶ function gen_fr_data(data, r2i_ratio, bandwidth = 0.4) generate the complex data for full range OCT reconstruction data: input data r2i_ratio: the real to imaginary ratio, tan(phi) where phi is phase modulation depth bandwidth: the bandwidth to separate the real and imaginary part.
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pypeline.impl.oct.proc.recon_magnitude_img(data, full_range=0, fft_num=2048, scale='log')[source]¶ function recon_magnitude_img(data, real_input = True, depth_dim = 1024, scale = ‘log’, disp_range = [0.5, 0]) reconstruct the amplitude image: data: input data full_range: if ture, use full range depth_dim: pixel num in depth scale: log or linear disp_range: display range for contrast/dynamic range, relative value if within [0,1],
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pypeline.impl.oct.proc.recon_phase_img(data, thresh=0, full_range=0, fft_num=2048, filter_size=3)[source]¶ function recon_magnitude_img(data, real_input = True, depth_dim = 1024, scale = ‘log’, disp_range = [0.5, 0]) reconstruct the amplitude image: data: input data full_range: if ture, use full range depth_dim: pixel num in depth scale: log or linear disp_range: display range for contrast/dynamic range, relative value if within [0,1],
pypeline.impl.oct.remove_dc module¶
pypeline.impl.oct.spectrum module¶
pypeline.spectrum¶
this module defines the spectrum or interferogram in OCT it should be the subclass of BaseData
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class
pypeline.impl.oct.spectrum.Spectrum(shape, dtype)[source]¶ Bases:
pypeline.impl.oct.basedata.BaseDataspectrum data based off the BaseData class with additional attributes and memeber functions Only supports Gaussian shape in k-space spectrum at this moment
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wc¶ center wavelength in unit nm
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range¶ wavelength range from end to end
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set_profile(fwhm)[source]¶ set the envelope shapre of the spectrum in wavenumber domain
Parameters: fwhm (float) – the full width half maxium of the spectrum Returns: None
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wavelengths¶ return the wavelengths at begein, center and end for the spectrum
Returns: the 3 wavelength at begin, center and end respectively Return type: [w0, wc, we]
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wavenumbers¶ return the wavelengths at begein, center and end for the spectrum
Returns: the 3 wavenumber at begin, center and end respectively Return type: [k0, kc, ke]
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