CSVD
Fast and Scalable Water Removal in MR Spectroscopic Data using Casorati Lanczos Singular Value Decomposition
Example code:
import numpy as np
import matplotlib.pyplot as plt
from numpy.fft import fft, fftshift
from CSVD import CSVD
t=np.arange(0,1024)*.01
ampl = np.random.normal(1,0.2,(1000,1))
fr = np.random.normal(-15,0.1,(1000,1))
sig1 = ampl * np.exp(-2*t) *np.exp(2*np.pi*fr*t*1j)
ampl2 = np.random.normal(1,0.2,(1000,1))
fr2 = np.random.normal(0,0.1,(1000,1))
sig2 = ampl2 * np.exp(-2*t) *np.exp(2*np.pi*fr2*t*1j)
ampl3 = np.random.normal(1,0.2,(1000,1))
fr3 = np.random.normal(15,0.1,(1000,1))
sig3 = ampl3 * np.exp(-2*t) *np.exp(2*np.pi*fr3*t*1j)
sig = sig1 + sig2 +sig3
noise = np.random.normal(0,1,(sig.shape)) + 1j*np.random.normal(0,1,(sig.shape))
sig = sig + 0.1*noise
csvd = CSVD(sig.T, 0.01)
sig_ = csvd.remove('auto',([-5,-20],[5,-10]),3)
plt.plot(fftshift(fft(sig[0,:])).T)
plt.plot(fftshift(fft(sig_[:,0])).T)
plt.legend(['Orginal signal', 'Water-removed signal'])
plt.savefig('example.jpg')
plt.show()
output:
Acknowledgments
This project has received funding from the European Union's Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No 813120.
Release files for CSVD 0.1.6
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | |
|---|---|---|---|
| CSVD-0.1.6.tar.gz | 4.2 kB | Details |
Built distribution (wheel)
| File | Interpreter | ABI | Platform | Reset |
|---|---|---|---|---|
| CSVD-0.1.6-py3-none-any.whl | Python 3 | none | any | Details |
Total release size: 9.1 kB
Release files / CSVD-0.1.6.tar.gz
| Download URL | CSVD-0.1.6.tar.gz |
|---|---|
| Size | 4.2 kB |
| Tags | Source |
|
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No |
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twine/4.0.2 CPython/3.7.5
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Release files / CSVD-0.1.6-py3-none-any.whl
| Download URL | CSVD-0.1.6-py3-none-any.whl |
|---|---|
| Size | 4.8 kB |
| Tags | Python 3 |
|
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No |
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twine/4.0.2 CPython/3.7.5
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