Table of Contents
Name | Direction | Type | Default | Description |
---|---|---|---|---|
NormalizationTable | Input | TableWorkspace | Mandatory | Name of the table containing the normalizations for the asymmetries. |
UnNormalizedWorkspaceList | Input | str list | Mandatory | An ordered list of workspaces (to get the initial values for the normalizations). |
ReNormalizedWorkspaceList | Input | str list | Mandatory | An ordered list of workspaces (to get the initial values for the normalizations). |
OutputFitWorkspace | Input | string | fit | The name of the output fit workspace. |
StartX | Input | number | 0.1 | The lower limit for calculating the asymmetry (an X value). |
EndX | Input | number | 15 | The upper limit for calculating the asymmetry (an X value). |
InputFunction | Input | Function | Mandatory | The fitting function to be converted. |
Minimizer | Input | string | Levenberg-MarquardtMD | Minimizer to use for fitting. Allowed values: [‘BFGS’, ‘Conjugate gradient (Fletcher-Reeves imp.)’, ‘Conjugate gradient (Polak-Ribiere imp.)’, ‘Damped GaussNewton’, ‘FABADA’, ‘Levenberg-Marquardt’, ‘Levenberg-MarquardtMD’, ‘Simplex’, ‘SteepestDescent’, ‘Trust Region’] |
MaxIterations | Input | number | 500 | Stop after this number of iterations if a good fit is not found |
OutputStatus | Output | string | ||
ChiSquared | Output | number | ||
OutputFunction | Output | Function | The fitting function after fit. |
This algorithm calculates the asymmetry from the first muon spectra in a workspace. in a workspace will be corrected.
The formula for calculating the asymmetry (from counts) is given by:
where is the muon lifetime (2.1969811e-6 seconds),
is the number of good frames and
is a
fitted normalisation constant. The normalisation is calculated by fitting to the normalised counts which is given by
and the fitting function is given by
and the renormalized data is transformed via the equation:
Example - Calculating Asymmetry: This example is for calculating the Asymmetry for a single data set.
import math
import numpy as np
def makeData(name,norm):
xData=np.linspace(start=0,stop=10,num=200)
yData=np.sin(5.2*xData)
result = (1-yData )*norm
ws= CreateWorkspace(DataX=xData, DataY=result,OutputWorkspace=name)
return ws
#create a normalisation table
tab = CreateEmptyTableWorkspace()
tab.addColumn('double', 'norm')
tab.addColumn('str', 'name')
tab.addColumn('str', 'method')
tab.addRow([11.,"a","Estimate"])
tab.addRow([22.,"b","Estimate"])
ws= makeData("a",2.30)
ws2= makeData("b",1.10)
myFunc='name=GausOsc,$domains=i,Frequency=5.;'
TFFunc = ConvertFitFunctionForMuonTFAsymmetry(myFunc,tab,["a"],"Construct")
CalculateMuonAsymmetry(tab,["a"],["b"],str(TFFunc),OutputFitWorkspace="fit_result",StartX=0.1,EndX=9.9)
print("Normalization constant for b: {0:.2f}".format(tab.column(0)[1]))
Output:
Normalization constant for b: 2.30
Example - Calculating Asymmetry For multiple data sets: This example is for calculating the Asymmetry for multuiple data sets.
import math
import numpy as np
def makeData(name,norm):
xData=np.linspace(start=0,stop=10,num=200)
yData=np.sin(5.2*xData)
result = (1-yData )*norm
ws= CreateWorkspace(DataX=xData, DataY=result,OutputWorkspace=name)
return ws
#create a normalisation table
tab = CreateEmptyTableWorkspace()
tab.addColumn('double', 'norm')
tab.addColumn('str', 'name')
tab.addColumn('str', 'method')
tab.addRow([11.,"a","Estimate"])
tab.addRow([22.,"b","Estimate"])
tab.addRow([22.,"c","Estimate"])
tab.addRow([22.,"d","Estimate"])
#create original function and workspace
myFunc='name=GausOsc,$domains=i,Frequency=5.;'
myFunc2='name=GausOsc,$domains=i,Frequency=5.;'
multiFunc='composite=MultiDomainFunction,NumDeriv=1;'+myFunc+myFunc2+'ties=(f0.Frequency=f1.Frequency)'
ws= makeData("a",2.30)
ws2= makeData("b",1.10)
ws3= makeData("c",4.1)
ws4= makeData("d",2.0)
TFFunc = ConvertFitFunctionForMuonTFAsymmetry(multiFunc,tab,["a","c"],"Construct")
CalculateMuonAsymmetry(tab,["a","c"],["b","d"],str(TFFunc),OutputFitWorkspace="fit_result",StartX=0.1,EndX=9.9)
print("Normalization constant for b: {0:.2f}".format(tab.column(0)[1]))
print("Normalization constant for d: {0:.2f}".format(tab.column(0)[3]))
Output:
Normalization constant for b: 2.30
Normalization constant for d: 4.10
Categories: Algorithm Index | Muon
C++ source: CalculateMuonAsymmetry.cpp (last modified: 2018-10-05)
C++ header: CalculateMuonAsymmetry.h (last modified: 2018-10-05)