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Integration v1¶
Summary¶
Integration takes a 2D workspace or an EventWorkspace as input and sums the data values. Optionally, the range summed can be restricted in either dimension.
See Also¶
Properties¶
Name 
Direction 
Type 
Default 
Description 

InputWorkspace 
Input 
Mandatory 
The input workspace to integrate. 

OutputWorkspace 
Output 
Mandatory 
The output workspace with the results of the integration. 

RangeLower 
Input 
number 
Optional 
The lower integration limit (an X value). 
RangeUpper 
Input 
number 
Optional 
The upper integration limit (an X value). 
StartWorkspaceIndex 
Input 
number 
0 
Index of the first spectrum to integrate. 
EndWorkspaceIndex 
Input 
number 
Optional 
Index of the last spectrum to integrate. 
IncludePartialBins 
Input 
boolean 
False 
If true then partial bins from the beginning and end of the input range are also included in the integration. 
RangeLowerList 
Input 
dbl list 
A list of lower integration limits (as X values). 

RangeUpperList 
Input 
dbl list 
A list of upper integration limits (as X values). 
Description¶
Integration sums up spectra in a Workspace and outputs a Workspace that contains only 1 value per spectrum (i.e. the sum). The associated errors are added in quadrature. The two X values per spectrum are set to the limits of the range over which the spectrum has been integrated. By default, the entire range is integrated and all spectra are included.
Optional properties¶
If only a portion of the workspace should be integrated then the
optional parameters may be used to restrict the range.
StartWorkspaceIndex
and EndWorkspaceIndex
may be used to select a
contiguous range of spectra in the workspace (note that these parameters
refer to the workspace index value rather than spectrum numbers as taken
from the raw file). If only a certain range of each spectrum should be
summed then the RangeLower
and RangeUpper
properties, as well as their List
versions should be used. RangeLower
and RangeUpper
are single values
limiting the summing range over all histograms. RangeLowerList
and
RangeUpperList
contain the ranges for each individual histogram. The
properties can be mixed: for instance, the histogram specific lower
integration limits can be given by RangeLowerList
while all upper limits
can be set to the same value by RangeUpper
. If both list and nonlist versions
are given, then the range is chosen which gives stricter limits for each
histogram.
No rebinning takes place as part of this algorithm. If the integration limits given
do not coincide with a bin boundary then the behaviour depends on the IncludePartialBins
parameter. If IncludePartialBins=True
then a contribution is calculated for any
bins that partially sit inside the integration limits. If IncludePartialBins=False
then the integration only includes bins that sit entirely within the integration limits.
If an integration limit is given that is beyond the X range covered by the spectrum then
the integration will proceed up to final bin boundary. The data that falls outside any
integration limits set will not contribute to the output workspace.
EventWorkspaces¶
If an EventWorkspace is used as the input, the output will be a MatrixWorkspace. Rebin v1 is recommended if you want to keep the workspace as an EventWorkspace.
Integration for event workspaces refers to internal binning, provided by Rebin v1 or load algorithm and may ignore limits, provided as algorithm input. For example, attempt to integrate loaded ISIS event workspace in the range [18000,20000] yields workspace integrated in the range [0,200000], assuming the data were collected in the time range [0,20000]. This happens because the event data would have single histogram workspace bin in range [0,20000]. To obtain integral in the desired range, user have to Rebin v1 first, and one of the binning intervals have to start from 18000 and another (or the same) end at 20000.
Distribution Data¶
Mantid workspaces store their data internally in one of two formats: as counts or as
frequencies (counts divided by binwidth). When the \(y\) values are stored as
frequencies, the workspace is called a distribution.
The algorithms ConvertToDistribution and
ConvertFromDistribution converts the internal
representation from counts to frequencies or vice versa.
The Integration
algorithm will correctly deal with the data to give the total
counts as output. That is, if you integrate a distribution workspace directly or
convert it first to counts and then call Integration
the output workspace will have
the same \(y\) values.
Note that the unintegrated axis (say the \(x\) axis) may still be binned, in which case the result of integrating distribution vs nondistribution data will not be equivalent. That is, integrating a distribution will create a new distribution where the internal \(y\) values represent the summed counts per \(x\)binwidth. Whereas, integrating a nondistribution workspace will yield the same internal \(y\) values but these now represent counts (not counts per \(x\)binwidth).
Fractional Rebinning¶
Some algorithms create a special type of Workspace2D called a RebinnedOutput
workspace,
in which each bin contains both a value and the fractional overlap area of this bin over
that of the original data. There is more discussion of this in the FractionalRebinning
concepts page.
The Integration algorithm differs for RebinnedOutput workspaces, please consult the page FractionalRebinning for more information.
Usage¶
Example  Integration over limited number of histograms:
# Create a workspace filled with a constant value = 1.0
ws=CreateSampleWorkspace('Histogram','Flat background')
# Integrate 10 spectra over all X values
intg=Integration(ws,StartWorkspaceIndex=11,EndWorkspaceIndex=20)
# Check the result
print('The result workspace has {0} spectra'.format(intg.getNumberHistograms()))
print('Integral of spectrum 11 is {0}'.format(intg.readY(0)[0]))
print('Integral of spectrum 12 is {0}'.format(intg.readY(1)[0]))
print('Integral of spectrum 13 is {0}'.format(intg.readY(2)[0]))
print('Integration range is [ {0}, {1} ]'.format(intg.readX(0)[0], intg.readX(0)[1]))
Output:
The result workspace has 10 spectra
Integral of spectrum 11 is 100.0
Integral of spectrum 12 is 100.0
Integral of spectrum 13 is 100.0
Integration range is [ 0.0, 20000.0 ]
Example  Total peak intensity:
from mantid.kernel import DeltaEModeType, UnitConversion
import numpy
ws = CreateSampleWorkspace(
Function='Flat background',
XMin=0,
XMax=12000,
BinWidth=20)
nHisto = ws.getNumberHistograms()
# Add elastic peaks to 'ws'. They will be at different TOFs
# since the detector banks will be 5 and 10 metres from the sample.
# First, a helper function for the peak shape
def peak(shift, xs):
xs = (xs[:1] + xs[1:]) / 2.0 # Convert to bin centres.
return 50 * numpy.exp(numpy.square(xs  shift) / 1200)
# Now, generate the elastic peaks.
Ei = 23.0 # Incident energy, meV
L1 = 10.0 # Sourcesample distance, m
sample = ws.getInstrument().getSample()
for i in range(nHisto):
detector = ws.getDetector(i)
L2 = sample.getDistance(detector)
tof = UnitConversion.run('Energy', 'TOF', Ei, L1, L2, 0.0, DeltaEModeType.Direct, Ei)
ys = ws.dataY(i)
ys += peak(tof, ws.readX(i))
# Fit Gaussians to the workspace.
# Fit results will be put into a table workspace 'epps'.
epps = FindEPP(ws)
# Integrate the peaks over +/ 3*sigma
lowerLimits = numpy.empty(nHisto)
upperLimits = numpy.empty(nHisto)
for i in range(nHisto):
peakCentre = epps.cell('PeakCentre', i)
sigma = epps.cell('Sigma', i)
lowerLimits[i] = peakCentre  3 * sigma
upperLimits[i] = peakCentre + 3 * sigma
totalIntensity = Integration(ws,
RangeLowerList=lowerLimits,
RangeUpperList=upperLimits)
print('Intensity of the first peak: {:.5}'.format(totalIntensity.dataY(0)[0]))
print('Intensity of the last peak: {:.5}'.format(totalIntensity.dataY(nHisto1)[0]))
Output:
Intensity of the first peak: ...
Intensity of the last peak: ...
Categories: AlgorithmIndex  Arithmetic  Transforms\Rebin
Source¶
C++ header: Integration.h
C++ source: Integration.cpp