SaveNXSPE v1¶

SaveNXSPE dialog.

Table of Contents

Summary
- See Also
Properties
Description
- Restrictions on the Input Workspace
- Child Algorithms Used
Usage
Source

Summary ¶

Writes a MatrixWorkspace to a file in the NXSPE format.

Properties ¶

Name	Direction	Type	Default	Description
InputWorkspace	Input	MatrixWorkspace	Mandatory	The name of the workspace to save.
Filename	Input	string	Mandatory	The name of the NXSPE file to write, as a full or relative path. Allowed extensions: [‘.nxspe’]
Efixed	Input	number	Optional	Value of the fixed energy to write into NXSPE file.
Psi	Input	number	Optional	Value of PSI to write into NXSPE file.
KiOverKfScaling	Input	boolean	True	Flags in the file whether Ki/Kf scaling has been done or not.
ParFile	Input	string	not_used.par	If provided, will replace detectors parameters in resulting nxspe file with the values taken from the file. Should be used only if the parameters, calculated by the [[FindDetectorsPar]] algorithm are not suitable for some reason. See [[FindDetectorsPar]] description for the details. Allowed extensions: [‘.par’, ‘.phx’]

Description ¶

Saves the given MatrixWorkspace to a file in the NeXus-based ‘NXSPE’ format.

Restrictions on the Input Workspace ¶

The input workspace must have units of Momentum Transfer (‘DeltaE’) and contain histogram data with common binning on all spectra.

Child Algorithms Used ¶

The FindDetectorsPar v1 algorithm is used to calculate detectors parameters from the instrument description.

Usage ¶

Example - Save/Load “Roundtrip”

import os
import numpy

# Create dummy workspace.
out_ws = CreateSimulationWorkspace(Instrument="IRIS", BinParams="0,500,2000")
out_ws.setY(0, numpy.array([10.0, 50.0, 30.0, 60.0]))
AddSampleLog(out_ws, 'Ei', LogText='321', LogType='Number', NumberType='Double')
out_ws.setDistribution(True)

file_path = os.path.join(config["defaultsave.directory"], "NXSPEData.nxspe")

# Do a "roundtrip" of the data.
SaveNXSPE(out_ws, file_path,Psi=32)

# By desigghn, SaveMXSPE does not store detector's ID-s. LoadNXSPE sets detector's ID-s to defaults.
# To compare loaded and saved workspaces here, one needs to set-up default detector's ID-s to the source workspace.
nSpec = out_ws.getNumberHistograms()
for i in range(0,nSpec):
    sp=out_ws.getSpectrum(i);
    sp.setDetectorID(i+1);
in_ws = LoadNXSPE(file_path)

ws_comparison_rez = CompareWorkspaces(out_ws,in_ws,1.e-9,CheckInstrument=False)
print("Contents of the first spectrum = {}.".format(in_ws.readY(0)))
print("Initial and loaded workspaces comparison is: {}".format(str(ws_comparison_rez[0])))
run = in_ws.getRun();
print("Loaded workspace has attached incident energy Ei={0:.1f} and rotation angle Psi= {1:.1f}deg".format(run.getLogData('Ei').value,run.getLogData('psi').value))

Output:

Contents of the first spectrum = [ 10.  50.  30.  60.].
Initial and loaded workspaces comparison is: True
Loaded workspace has attached incident energy Ei=321.0 and rotation angle Psi= 32.0deg

Note that LoadNXSPE v1 automatically applies the distribution flag to the loaded workspace. This is because all examples of workspaces saved to NXSPE format by the reduction algorithms are distributions (signal is count rate and should be multiplied by bin widths to get counts). SaveNXSPE does not require its input is a distribution, however, and the NXSPE format does not have a distribution flag.

Categories: AlgorithmIndex | DataHandling\Nexus | DataHandling\SPE | Inelastic\DataHandling

Source ¶

C++ source: SaveNXSPE.cpp (last modified: 2019-07-17)

C++ header: SaveNXSPE.h (last modified: 2018-10-05)