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fileformat:gve [2019/09/04 13:34]
smerkel
fileformat:gve [2019/09/04 13:51] (current)
smerkel
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 The can be used for indexing grains, as described in the sections on [[processing:​indexing_with_grainspotter|Grain indexing with GrainSpotter]] and [[processing:​indexing_with_imaged11|Grain indexing with ImageD11]]. Typically, ''​gve''​ files are generated while [[processing:​compute_gvectors|Computing G-vectors]]. The can be used for indexing grains, as described in the sections on [[processing:​indexing_with_grainspotter|Grain indexing with GrainSpotter]] and [[processing:​indexing_with_imaged11|Grain indexing with ImageD11]]. Typically, ''​gve''​ files are generated while [[processing:​compute_gvectors|Computing G-vectors]].
  
-Attached ​is a [[fileformat:​gveexample| full example ​for aluminum]] ​extracted from the [[software:grainspotter|GrainSpotter]] source code. +Below is an exampleextracted from the [[software:imaged11|ImageD11]] manual at [[https://​pythonhosted.org/​ImageD11/​fileformats.html]].
- +
-Below is a short extract and explanations+
  
 <​code>​ <​code>​
-4.049750 4.049750 4.049750 ​90.000000 90.000000 90.000000 ​ +78.712000 78.712000 78.712000 ​90.000000 90.000000 90.000000 ​I 
-# wavelength = 0.153636 +# wavelength = 0.939500 
-# wedge = 0.000000+# wedge = -0.051189 
 +# axis 0.000000 ​0.000000 1.000000 
 +[... the remaining part of the parameter information is snipped ...]
 # ds h k l # ds h k l
-0.427693 ​-1 1  + 0.0179669 ​  -1   -   0 
-0.427693 ​-1 -1  + 0.0179669 ​  -1    ​0 ​  -1 
-0.427693 1 -1 1  + 0.0179669 ​  -1    ​0 ​   ​
-0.427693 1 -1 -1  + 0.0179669 ​  -1       0 
-0.427693 ​-1 -1 -1  + 0.0179669 ​   0   -1   ​-1 
-0.427693 1 1 1  + ​0.0179669 ​   0   -1    ​
-0.427693 ​1 1 -1  + 0.0179669 ​   0    ​  -
-0.427693 -1 -1 1  + 0.0179669 ​   0    ​   1 
-0.493858 ​0 0 -2  + ​0.0179669 ​   ​  ​-1    0 
-0.493858 0 0 2  + 0.0179669 ​   ​   ​0 ​  -1 
-  + ​0.0179669 ​   1    0    ​
-  . + 0.0179669 ​   1    1    ​0 
-  . + 0.0254091 ​  -2    ​0 ​   0 
-xr yr zr xc yc ds eta omega + 0.0254091 ​   ​  -   0 
--1.064488 ​0.487933 ​-0.303576 393.350339 967.555462 1.209699 255.401608 ​-59.865730 0 + 0.0254091 ​   0    0   -2 
--0.647861 ​0.323941 ​0.382165 659.957013 791.719538 ​0.818970 297.876500 ​-59.355276 1 + [ lots of hkl's snipped ] 
--0.694335 ​0.422749 ​-0.099470 473.489709 826.087974 ​0.818970 263.009860 ​-55.030765 2 + ​gx ​ gy  gz  ​xc  yc  ds  eta  omega  ​spot3d_id ​ xl  yl  zl 
-0.277708 -0.258757 -0.586271 285.515284 366.081243 ​0.698420 147.207272 ​-52.688612 3 +-0.006049 -0.006821 ​-0.011411 1553.000000 1506.534500 0.014605 141.377789 41.000000 35325 211440.500505 ​-1811.094736 -2266.916293 
-0.601890 ​-0.616322 ​-0.690907 242.754491 178.278465 1.104299 128.896483 ​-50.564083 4 +-0.012846 ​0.008203 -0.009504 1564.869800 1510.194700 ​0.017962 121.948198 122.022400 105544 211439.925254 ​-3027.977786 -1888.286052 
-  ​+0.013156 0.009757 0.007648 1503.726500 1543.564400 0.018077 ​-64.969351 54.000300 46271 211436.535556 3254.006490 1519.487824 
-  . +0.000474 ​0.018005 ​-0.001647 1500.521000 1525.574600 ​0.018086 -95.223069 1.993700 3308 211438.759075 3578.198430 ​-327.094270 
-  ​.+-0.003736 ​0.010752 ​0.014069 1557.512700 1555.861300 ​0.018097 38.972120 160.000000 155486 211434.450605 ​-2261.233048 2795.170225 
 +-0.013099 ​-0.009687 ​-0.007903 1566.912500 1513.290200 0.018108 115.878145 53.000000 44665 211439.526323 ​-3236.750899 -1570.156341 
 +0.017023 -0.001041 -0.006196 1502.350000 1516.761000 0.018145 -109.965181 93.999200 78237 211439.811196 338
 </​code>​ </​code>​
  
-Explanations +Explanations ​(directly inspired from the ImageD11 manual) 
-  * The first line are information on the sample crystal structure+  * The first line of the file contains the unit cell parameters and lattice centering (one of P,​A,​B,​C,​I,​F)
-  * Wavelength is on the second line +  * The wavelength and wedge angle are expected ​on the next lines (needed to compute ideal two theta, omega and azimuth angles for computed orientations). 
-  * Wedge is on the third line +  * A list of computed theoretical g-vectors for the unit cell with 
-  Lines below are a list of hkl'swhich will be used during indexingNot that [[software:​grainspotter|GrainSpotter]] can override this list of the genhkl option is set in the input file. For each, you have ds (||**G**|| = 1/d), h, k, and l+      ds = d*= ||**G**|| = 1/d (expressed in Angstrom) 
 +      * hk, l values for the unit cell. 
 +  * Note that [[software:​grainspotter|GrainSpotter]] can override this list of the ''​genhkl'' ​option is set in the input file.  
 +  * The actual scattering vectors ​(g-vectors) extracted from the experimental data follow and 
 +    ​gx = x-component of scattering vector (along the beam) with all angles at zero (units 1/Angstrom)  
 +    ​gy = y-component of scattering vector (toward the door) with all angles at zero (units 1/Angstrom)  
 +    ​gz = z-component of scattering vector (roughly up) with all angles at zero (units 1/Angstrom)  
 +    ​xc spatially corrected peak x-position on detector (units: pixels) 
 +    * yc = spatially corrected peak y-position on detector (units: pixels)  
 +    * ds 1/d-spacing - modulus of scattering vector - <​math>​ ds = λ / (2 sin θ) 
 +    * eta = azimuthal angle 
 +    * omega = rotation angle of scan  
 +    * spotid is an spot identifier to follow the individual spot at any process step  
 +    * xl = x-component of scattering vector in the laboratory coordinate system (along the beam) with all angles at zero (units microns)  
 +    * yl = y-component of scattering vector in the laboratory coordinate system (toward the door) with all angles at zero (units microns)  
 +    * zl = z-component of scattering vector in the laboratory coordinate system (roughly up) with all angles at zero (units microns)  
 + 
 +These files are written by ImageD11/​guitransformer.py ​and read by ImageD11/​indexing.py and GrainSpotter and possibly other programs. 
fileformat/gve.1567604099.txt.gz · Last modified: 2019/09/04 13:34 by smerkel