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SaveGSASInstrumentFile v1¶
Summary¶
Generate a GSAS instrument file from either a table workspace containing profile parameters or a Fullprof’s instrument resolution file (.irf file).
See Also¶
Properties¶
Name |
Direction |
Type |
Default |
Description |
---|---|---|---|---|
InputWorkspace |
Input |
Name of the table workspace containing the parameters. |
||
InputFileName |
Input |
string |
Name of the input Fullprof resolution file (.irf). Allowed extensions: [‘.irf’] |
|
OutputFileName |
Input |
string |
Mandatory |
Name of the output GSAS instrument file. Allowed extensions: [‘.iparam’, ‘.prm’] |
BankIDs |
Input |
class std::vector<unsigned int,class std::allocator<unsigned int> > |
Bank IDs of the banks to be written to GSAS instrument file. |
|
Instrument |
Input |
string |
powgen |
Name of the instrument that parameters are belonged to. So far, only PG3 and NOM are supported. Allowed values: [‘powgen’, ‘nomad’] |
ChopperFrequency |
Input |
string |
60 |
Frequency of the chopper. Allowed values: [‘10’, ‘30’, ‘60’] |
IDLine |
Input |
string |
ID line to be written in GSAS instrument file |
|
Sample |
Input |
string |
Sample information written to header (title) |
|
L1 |
Input |
number |
Optional |
L1 (primary flight path) of the instrument. |
L2 |
Input |
number |
Optional |
L2 (secondary flight path) of the instrument. It must be given if 2Theta is not given. |
TwoTheta |
Input |
number |
Optional |
Angle of the detector bank. It must be given if L2 is not given. |
Description¶
Convert Fullprof’s instrument resolution file (.irf) to GSAS’s instrument file (.iparm/.prm).
Supported peak profiles¶
Time-of-flight back-to-back exponential convoluted with pseudo-voigt (in future)
Fullprof: Profile 9;
GSAS: Type 3 TOF profile.
Thermal neutron time-of-flight back-to-back exponential convoluted with pseudo-voigt (implemented)
Fullprof: Profile 10;
GSAS: tabulated peak profile.
Supported input Fullprof file¶
There can be several types of Fullprof files as the input file
resolution file .irf (implemented)
configuration file .pcr (in future)
Set up \(2\theta\)¶
There are several places in this algorithm that can set the value of \(2\theta\). From the highest priority, here is the list how \(2\theta\) is set up.
Algorithms’ input property
TwoTheta
;Either input TableWorkspace or input Fullprof resolution (.irf) file;
Hard coded default “TwoTheta” of a certain instrument.
Set up \(L_1\)¶
There are 2 places in this algorithm that can set the value of \(L_1\). From the highest priority, here is the list how \(2\theta\) is set up.
Algorithms’ input property
L1
;Hard coded default “TwoTheta” of a certain instrument.
Calculation of \(L_2\)¶
If “TwoTheta” (\(2\theta\)) is given, L2 will be calculated from given 2Theta and L1 by \(DIFC = 252.816\cdot2sin(\theta)\sqrt{L1+L2}\). Notice that \(2\theta\) given in input .irf file may have subtle difference to “2Theta”, which is input by user in order to calculate L2.
If “2Theta” (\(2\theta\)) is not given, L2 will be read from user input.
Usage¶
Example - save GSAS instrument file from a Fullprof .irf file:
# Run the algorithm to save for GSAS instrument file
SaveGSASInstrumentFile(InputFileName = "PG3_Bank1.irf", OutputFileName = "/tmp/PG3_Bank1.iparam",
BankIDs = 1, Instrument = "powgen", ChopperFrequency = "60",
IDLine = "60Hz 2011 Bank 1", Sample = "LaB6", L1 = 60.0, TwoTheta = 90.0)
# Load GSAS parameter files
gfile = open("/tmp/PG3_Bank1.iparam", "r")
lines = gfile.readlines()
gfile.close()
# Print out some result
print("Number of lines in GSAS instrument file: {}".format(len(lines)))
print("Line 0: {}".format(lines[0].strip()))
print("Line 1: {}".format(lines[1].strip()))
print("Line 2: {}".format(lines[2].strip()))
print("Line 3: {}".format(lines[3].strip()))
print("Line 305: {}".format(lines[305].strip()))
Output:
Number of lines in GSAS instrument file: 306
Line 0: 12345678901234567890123456789012345678901234567890123456789012345678
Line 1: ID 60Hz 2011 Bank 1
Line 2: INS BANK 1
Line 3: INS FPATH1 60.000000
Line 305: INS 1PAB590 0.00213 0.46016 1.99061 -3.12296
Categories: AlgorithmIndex | Diffraction\DataHandling
Source¶
C++ header: SaveGSASInstrumentFile.h
C++ source: SaveGSASInstrumentFile.cpp