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ReflectometryReductionOneLiveData dialog.
Table of Contents
| Name | Direction | Type | Default | Description |
|---|---|---|---|---|
| InputWorkspace | Input | MatrixWorkspace | Mandatory | |
| Instrument | Input | string | CRISP | Instrument to find live value for. Allowed values: [‘CRISP’, ‘INTER’, ‘OFFSPEC’, ‘POLREF’, ‘SURF’] |
| GetLiveValueAlgorithm | Input | string | GetLiveInstrumentValue | The algorithm to use to get live values from the instrument |
| FirstTransmissionRunList | Input | str list | A list of run numbers or workspace names for the first transmission run. Multiple runs will be summed before reduction. | |
| SecondTransmissionRunList | Input | str list | A list of run numbers or workspace names for the second transmission run. Multiple runs will be summed before reduction. | |
| SliceWorkspace | Input | boolean | False | If true, slice the input workspace |
| NumberOfSlices | Input | number | Optional | The number of uniform-length slices to slice the input workspace into |
| SummationType | Input | string | SumInLambda | The type of summation to perform. Allowed values: [‘SumInLambda’, ‘SumInQ’] |
| ReductionType | Input | string | Normal | The type of reduction to perform when summing in Q. Allowed values: [‘Normal’, ‘DivergentBeam’, ‘NonFlatSample’] |
| IncludePartialBins | Input | boolean | False | If true then partial bins at the beginning and end of the output range are included |
| AnalysisMode | Input | string | PointDetectorAnalysis | Analysis mode. This property is only used when ProcessingInstructions is not set. Allowed values: [‘PointDetectorAnalysis’, ‘MultiDetectorAnalysis’] |
| ProcessingInstructions | Input | string | Grouping pattern of spectrum numbers to yield only the detectors of interest. See GroupDetectors for syntax. | |
| CorrectDetectors | Input | boolean | True | Moves detectors to twoTheta if ThetaIn or ThetaLogName is given |
| DetectorCorrectionType | Input | string | VerticalShift | When correcting detector positions, this determines whether detectorsshould be shifted vertically or rotated around the sample position. Allowed values: [‘RotateAroundSample’, ‘VerticalShift’] |
| WavelengthMin | Input | number | Optional | Wavelength Min in angstroms |
| WavelengthMax | Input | number | Optional | Wavelength Max in angstroms |
| I0MonitorIndex | Input | number | Optional | I0 monitor workspace index |
| MonitorBackgroundWavelengthMin | Input | number | Optional | Wavelength minimum for monitor background subtraction in angstroms. |
| MonitorBackgroundWavelengthMax | Input | number | Optional | Wavelength maximum for monitor background subtraction in angstroms. |
| MonitorIntegrationWavelengthMin | Input | number | Optional | Wavelength minimum for integration in angstroms. |
| MonitorIntegrationWavelengthMax | Input | number | Optional | Wavelength maximum for integration in angstroms. |
| NormalizeByIntegratedMonitors | Input | boolean | True | Normalize by dividing by the integrated monitors. |
| SubtractBackground | Input | boolean | False | If true then perform background subtraction |
| BackgroundProcessingInstructions | Input | string | These processing instructions will be passed to the background subtraction algorithm | |
| BackgroundCalculationMethod | Input | string | PerDetectorAverage | The type of background reduction to perform. Allowed values: [‘PerDetectorAverage’, ‘Polynomial’, ‘AveragePixelFit’] |
| DegreeOfPolynomial | Input | number | 0 | Degree of the fitted polynomial. |
| CostFunction | Input | string | Least squares | The cost function to be passed to the Fit algorithm. Allowed values: [‘Least squares’, ‘Unweighted least squares’] |
| Params | Input | dbl list | A comma separated list of first bin boundary, width, last bin boundary. These parameters are used for stitching together transmission runs. Values are in wavelength (angstroms). This input is only needed if a SecondTransmission run is provided. | |
| StartOverlap | Input | number | Optional | Start wavelength for stitching transmission runs together. Only used if a second transmission run is provided. |
| EndOverlap | Input | number | Optional | End wavelength (angstroms) for stitching transmission runs together. Only used if a second transmission run is provided. |
| ScaleRHSWorkspace | Input | boolean | True | Scale the right-hand-side or left-hand-side workspace. Only used if a second transmission run is provided. |
| TransmissionProcessingInstructions | Input | string | These processing instructions will be passed to the transmission workspace algorithm | |
| CorrectionAlgorithm | Input | string | AutoDetect | The type of correction to perform. Allowed values: [‘None’, ‘AutoDetect’, ‘PolynomialCorrection’, ‘ExponentialCorrection’] |
| Polynomial | Input | dbl list | Coefficients to be passed to the PolynomialCorrection algorithm. | |
| C0 | Input | number | 0 | C0 value to be passed to the ExponentialCorrection algorithm. |
| C1 | Input | number | 0 | C1 value to be passed to the ExponentialCorrection algorithm. |
| MomentumTransferMin | Input | number | Optional | Minimum Q value in IvsQ Workspace. Used for Rebinning the IvsQ Workspace |
| MomentumTransferStep | Input | number | Optional | Resolution value in IvsQ Workspace. Used for Rebinning the IvsQ Workspace. This value will be made minus to apply logarithmic rebinning. If you wish to have linear bin-widths then please provide a negative value. |
| MomentumTransferMax | Input | number | Optional | Maximum Q value in IvsQ Workspace. Used for Rebinning the IvsQ Workspace |
| ScaleFactor | Input | number | Optional | Factor you wish to scale Q workspace by. |
| PolarizationAnalysis | Input | boolean | False | Apply polarization corrections |
| FloodCorrection | Input | string | Workspace | The way to apply flood correction: Workspace - use FloodWorkspace property to get the flood workspace, ParameterFile - use parameters in the parameter file to construct and apply flood correction workspace. Allowed values: [‘Workspace’, ‘ParameterFile’] |
| FloodWorkspace | Input | MatrixWorkspace | A flood workspace to apply; if empty and FloodCorrection is ‘Workspace’ then no correction is applied. | |
| Debug | Input | boolean | False | Whether to enable the output of extra workspaces. |
| TimeInterval | Input | dbl list | Array for lengths of time intervals for splitters: if the array is empty, then there will be one splitter created from StartTime and StopTime; if the array has one value, then if this value is positive, all splitters will have same time intervals, else the time intervals will be exponentially increasing; if the size of the array is larger than one, then the splitters can have various time interval values. | |
| LogValueInterval | Input | number | Optional | Delta of log value to be sliced into from min log value and max log value; if not given, then only value |
| LogName | Input | string | Name of the sample log to use to filter - for example, the pulse charge is recorded in ‘ProtonCharge’. | |
| UseNewFilterAlgorithm | Input | boolean | True | If true, use the new FilterEvents algorithm instead of FilterByTime. |
| ReloadInvalidWorkspaces | Input | boolean | True | If true, reload input workspaces if they are of the incorrect type |
| GroupTOFWorkspaces | Input | boolean | True | If true, group the TOF workspaces |
| OutputWorkspace | Output | MatrixWorkspace | Output workspace in Q (native binning) |
This algorithm performs a reduction with ReflectometryReductionOneAuto v3 on a live data workspace. It is intended to be run as a post-processing algorithm for StartLiveData v1, although it can also be called directly on a workspace output from live data monitoring. It is not intended to be run on a workspace for a completed run.
This algorithm does some setting up of the instrument and sample logs, which are not normally present for a live data workspace, so that the reduction can be run. This uses live values for theta and the slit gaps, which are found from the instrument using GetLiveInstrumentValue v1. Once the workspace is set up, ReflectometryReductionOneAuto v3 is run, with ThetaLogName set to the appropriate value to use the value of theta that was set in the logs.
GetLiveInstrumentValue v1 requires Mantid to have EPICS support installed, and appropriate processes must be running on the instrument to supply the EPICS values. A different algorithm for fetching live values could be specified by overriding the GetLiveValueAlgorithm property.
- StartLiveData(Instrument=’INTER’,
- PostProcessingAlgorithm=’ReflectometryReductionOneLiveData’, PostProcessingProperties=’Instrument=INTER’, AccumulationMethod=’Replace’,AccumulationWorkspace=’TOF_live’,OutputWorkspace=’IvsQ_binned_live’,)
See also
Algorithm GetLiveInstrumentValue v1, ReflectometryReductionOneAuto v3, StartLiveData v1 and the ISIS Reflectometry interface.
Categories: AlgorithmIndex | Reflectometry