\(\renewcommand\AA{\unicode{x212B}}\)
SpecularReflectionPositionCorrect v2¶
Summary¶
Corrects a reflectometer’s detector component’s position.
See Also¶
Properties¶
Name |
Direction |
Type |
Default |
Description |
---|---|---|---|---|
InputWorkspace |
Input |
Mandatory |
An input workspace to correct. |
|
TwoTheta |
Input |
number |
Optional |
Angle used to correct the detector component [degrees]. |
DetectorCorrectionType |
Input |
string |
VerticalShift |
Whether detectors should be shifted vertically or rotated around the sample position. Allowed values: [‘VerticalShift’, ‘RotateAroundSample’] |
DetectorComponentName |
Input |
string |
Name of the detector component to correct, for example point-detector |
|
DetectorID |
Input |
number |
Optional |
The ID of the detector to correct; if both the component name and the detector ID are set the latter will be used. |
SampleComponentName |
Input |
string |
some-surface-holder |
Name of the sample component; if the given name is not found in the instrument, the default sample is used. |
OutputWorkspace |
Output |
Mandatory |
A workspace with corrected detector position. |
|
DetectorFacesSample |
Input |
boolean |
False |
If true, a normal vector at the centre of the detector always points towards the sample. |
LinePosition |
Input |
number |
Optional |
A fractional workspace index for the specular line centre. |
PixelSize |
Input |
number |
Optional |
Size of a detector pixel, in metres. |
Description¶
Moves the specified detector component to a given angle between the beam and the sample-to-detector vector. The detector component is moved as a block. The rest of the instrument components remain in original positions. The component can be shifted vertically (default), or rotated around the sample position. When rotating around the sample, an optional rotation can be applied so that the detector always faces the sample.
In the most basic operation, the detector is moved to the angle specified by TwoTheta
.
This case is schematically shown below for rotation around the sample position and
DetectorFacesSample
set to True
.
If LinePosition
and PixelSize
are also given, the detector will be moved such
that the angle will be TwoTheta
for the pixel at workspace index LinePosition
.
Note that LinePosition
can be a fractional index making it possible to adjust the
detector angle to a fitted line position. The figure below illustrates this option.
Note
The line positions can be acquired by using, for instance, FindReflectometryLines.
Previous Versions¶
For version 1 of the algorithm, please see SpecularReflectionPositionCorrect-v1.
Usage¶
Note
To run these usage examples please first download the usage data, and add these to your path. In Mantid this is done using Manage User Directories.
Example - Correct ‘point-detector’
print('point-detector')
polref = Load(Filename=r'POLREF00004699.raw', PeriodList=1)
polref = polref[0]
instr = polref.getInstrument()
print('Original position: ' + str(instr.getComponentByName('point-detector').getPos()))
polref_vert = SpecularReflectionPositionCorrect(polref, TwoTheta = 2*0.49, DetectorComponentName='point-detector', DetectorCorrectionType='VerticalShift')
instr = polref_vert.getInstrument()
print('Vertical shift: ' + str(instr.getComponentByName('point-detector').getPos()))
polref_rot = SpecularReflectionPositionCorrect(polref, TwoTheta = 2*0.49, DetectorComponentName='point-detector', DetectorCorrectionType='RotateAroundSample')
instr = polref_rot.getInstrument()
print('Rotated: ' + str(instr.getComponentByName('point-detector').getPos()))
Output:
Note that in this case the difference between shifting the detectors vertically or rotating them is negligible.
point-detector
Original position: [25.6,0,0.0444961]
Vertical shift: [25.6,0,0.0444753]
Rotated: [25.6,0,0.0444753]
Example - Correct ‘lineardetector’
print('lineardetector')
polref = Load(Filename=r'POLREF00004699.raw', PeriodList=1)
polref = polref[0]
instr = polref.getInstrument()
print('Original position: ' + str(instr.getComponentByName('lineardetector').getPos()))
polref_vert = SpecularReflectionPositionCorrect(polref, TwoTheta = 2*0.49, DetectorComponentName='lineardetector')
instr = polref_vert.getInstrument()
print('Vertical shift: ' + str(instr.getComponentByName('lineardetector').getPos()))
polref_rot = SpecularReflectionPositionCorrect(polref, TwoTheta = 2*0.49, DetectorComponentName='lineardetector', DetectorCorrectionType='RotateAroundSample')
instr = polref_rot.getInstrument()
print('Rotated: ' + str(instr.getComponentByName('lineardetector').getPos()))
Output:
lineardetector
Original position: [26,0,0]
Vertical shift: [26,0,0.0513177]
Rotated: [25.9996,0,0.0513102]
Example - Correct ‘OSMOND’
print('OSMOND')
polref = Load(Filename=r'POLREF00004699.raw', PeriodList=1)
polref = polref[0]
instr = polref.getInstrument()
print('Original position: ' + str(instr.getComponentByName('OSMOND').getPos()))
polref_vert = SpecularReflectionPositionCorrect(polref, TwoTheta = 2*0.49, DetectorComponentName='OSMOND')
instr = polref_vert.getInstrument()
print('Vertical shift: ' + str(instr.getComponentByName('OSMOND').getPos()))
polref_rot = SpecularReflectionPositionCorrect(polref, TwoTheta = 2*0.49, DetectorComponentName='OSMOND', DetectorCorrectionType='RotateAroundSample')
instr = polref_rot.getInstrument()
print('Rotated: ' + str(instr.getComponentByName('OSMOND').getPos()))
Output:
OSMOND
Original position: [26,0,0]
Vertical shift: [26,0,0.0513177]
Rotated: [25.9996,0,0.0513102]
Example - Rotate given pixel
import numpy
# We'll just use an empty workspace here.
ws = LoadEmptyInstrument(InstrumentName='D17')
# Get rid of monitors
ExtractMonitors(ws, DetectorWorkspace='ws')
ws = mtd['ws']
line_position = 22.
spectrum_info = ws.spectrumInfo()
two_theta = numpy.rad2deg(spectrum_info.twoTheta(int(line_position)))
print('Pixel {} 2theta'.format(int(line_position)))
print('before angle correction: {:.3}'.format(two_theta))
ws = SpecularReflectionPositionCorrect(
ws,
TwoTheta=1.5,
DetectorCorrectionType='RotateAroundSample',
DetectorComponentName='detector',
DetectorFacesSample=True,
LinePosition=line_position,
PixelSize=0.001195)
spectrum_info = ws.spectrumInfo()
two_theta = numpy.rad2deg(spectrum_info.twoTheta(int(line_position)))
print('after angle correction: {:.3}'.format(two_theta))
Output:
Pixel 22 2theta
before angle correction: 2.33
after angle correction: 1.5
Categories: AlgorithmIndex | Reflectometry
Source¶
C++ header: SpecularReflectionPositionCorrect2.h
C++ source: SpecularReflectionPositionCorrect2.cpp