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Generate XDS.INP (view source)

Revision as of 09:41, 16 October 2021

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→‎The script: improve wording
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== The script ==
== The script ==
<pre>
<pre>


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# revision 1.01 . KD 07/12/2020 ROTATION_AXIS=0 -1 0 for Pilatus3 2M, S/N 24-0118 at ID23-2 (http://www.globalphasing.com/autoproc/wiki/index.cgi?BeamlineSettings)
# revision 1.01 . KD 07/12/2020 ROTATION_AXIS=0 -1 0 for Pilatus3 2M, S/N 24-0118 at ID23-2 (http://www.globalphasing.com/autoproc/wiki/index.cgi?BeamlineSettings)
# revision 1.02 . KD 11/01/2021 recognize mar555 detector as mar345 (thanks to Thomas Hauß, HZB)  
# revision 1.02 . KD 11/01/2021 recognize mar555 detector as mar345 (thanks to Thomas Hauß, HZB)  
REVISION="1.02 (11-Jan-2021)"
# revision 1.03 . Feng YU 18/7/2021 fix/expand information about Shanghai Synchrotron Radiation Facility (SSRF)
# revision 1.04 . Zhipu Luo 13/08/2021 extract ORGX,ORGY for electron diffraction from SMV header if the wavelength value starts with 0.0
# revision 1.05 . KD specialcase extraction of number of images for BNL detectors E-32-0101 and E-18-0104
# revision 1.06 . KD fix URLs in output. Availability of Apple M1 processor dectris-neggia-Apple-arm64.so . LC_ALL=C .
REVISION="1.06 (15-OCT-2021)"


#                                                                                                             
#                                                                                                             
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   exit                                                                                                           
   exit                                                                                                           
fi                                                                                                               
fi                                                                                                               
# make sure the locale does not interfere with e.g. awk calculations:
LC_ALL="C";export LC_ALL
#                                                                                                                 
#                                                                                                                 
# defaults:                                                                                                       
# defaults:                                                                                                       
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SEPMIN=7.0
SEPMIN=7.0
CLUSTER_RADIUS=3.5
CLUSTER_RADIUS=3.5
REFINE_CORRECT="CELL BEAM ORIENTATION AXIS POSITION ! Default is: refine everything"


dname=`echo "$1" | xargs dirname`
dname=`echo "$1" | xargs dirname`
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  data_last=`cut -b $pos1-$pos2 tmp1 | tail -n1 | bc`
  data_last=`cut -b $pos1-$pos2 tmp1 | tail -n1 | bc`
  DATA_RANGE="$data_first $data_last"
  DATA_RANGE="$data_first $data_last"
echo DATA_RANGE=$DATA_RANGE
   
   
  # set SPOT_RANGE to first half of DATA_RANGE
  # set SPOT_RANGE to first half of DATA_RANGE
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FIRSTFRAME=`head -1 tmp1`
FIRSTFRAME=`head -1 tmp1`
echo $FIRSTFRAME | grep "\.h5$" && is_h5=1 || is_h5=0
echo $FIRSTFRAME | grep "\.h5$" && is_h5=1 || is_h5=0
if [ "$is_h5" == 1 ]; then
# nframes=`h5dump -A -g "/entry/data" $FIRSTFRAME | grep "DATASPACE  SIMPLE" | sed -e "s/,.*//" | awk '{a+=$5}END{print a}'`
nframes=`h5dump -d "/entry/instrument/detector/detectorSpecific/nimages" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
DATA_RANGE="1 $nframes"
SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`"
fi
echo DATA_RANGE=$DATA_RANGE


# find out detector type
# find out detector type
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  grep -q BRUKER tmp2 && grep -q CBF tmp2  && DET=Bruker-cbf   
  grep -q BRUKER tmp2 && grep -q CBF tmp2  && DET=Bruker-cbf   
  grep -q CMOS1 tmp2 && DET=adsc-CMOS1   
  grep -q CMOS1 tmp2 && DET=adsc-CMOS1   
  grep -q MARCONTROL tmp2 && DET=OLDMAR                  
  grep -q MARCONTROL tmp2 && DET=OLDMAR
grep -q "WAVELENGTH=0.0" tmp2 && DET=experimental-ED                                   
else
else
  h5dump -d "/entry/instrument/detector/description" $FIRSTFRAME | grep -i Eiger > /dev/null && DET=eiger
  h5dump -d "/entry/instrument/detector/description" $FIRSTFRAME | grep -i Eiger > /dev/null && DET=eiger
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   DETECTOR_DISTANCE=`grep ^DISTANCE tmp2 | sed s/DISTANCE=/-/`                                                                     
   DETECTOR_DISTANCE=`grep ^DISTANCE tmp2 | sed s/DISTANCE=/-/`                                                                     
   OSCILLATION_RANGE=`grep OMEGA_DELTA tmp2 | sed s/OMEGA_DELTA=//`   
   OSCILLATION_RANGE=`grep OMEGA_DELTA tmp2 | sed s/OMEGA_DELTA=//`   
   DIRECTION_OF_DETECTOR_X_AXIS="-1 0 0"                                                                 
   DIRECTION_OF_DETECTOR_X_AXIS="-1 0 0"  
                                                                  
elif [ "$DET" == "experimental-ED" ]; then
  DETECTOR="ADSC MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65000  ! OVERLOAD is really unknown "
  echo --- Electron diffraction data in SMV format!
  SENSOR_THICKNESS=0.01                                                       
  sed s/\;// tmp2 > tmp1                                                     
  mv tmp1 tmp2                                                               
  X_RAY_WAVELENGTH=`grep WAVELENGTH tmp2 | head -1 | sed s/WAVELENGTH=//`
  NX=`grep SIZE1 tmp2 | tail -1 | sed s/SIZE1=//`
  QX=`grep PIXEL_SIZE tmp2 | sed s/PIXEL_SIZE=//`
  NY=`grep SIZE2 tmp2 | tail -1 | sed s/SIZE2=//`                                           
  QY=$QX 
  BEAM_CENTER_X=`grep BEAM_CENTER_X tmp2 | sed s/BEAM_CENTER_X=//`
  BEAM_CENTER_Y=`grep BEAM_CENTER_Y tmp2 | sed s/BEAM_CENTER_Y=//`
  QXY=`echo "scale=1; $QX*($BEAM_CENTER_X+$BEAM_CENTER_Y)" | bc -l`
      if [ "$QXY" "<" "$BEAM_CENTER_X" ] ; then
      ORGX=`echo "scale=2; $BEAM_CENTER_Y/$QX" | bc -l`
      ORGY=`echo "scale=2; $BEAM_CENTER_X/$QX" | bc -l`
      else
      ORGX=`echo "scale=2; $BEAM_CENTER_X/1" | bc -l`
      ORGY=`echo "scale=2; $BEAM_CENTER_Y/1" | bc -l`
      fi
  DETECTOR_DISTANCE=`grep ^DISTANCE tmp2 | sed s/DISTANCE=//`                                                                   
  OSCILLATION_RANGE=`grep OSC_RANGE tmp2 | sed s/OSC_RANGE=//`
  STARTING_ANGLE=`grep OSC_START tmp2 | sed s/OSC_START=//`
  echo --- For TIMEPIX detector, please fix ROTATION_AXIS yourself!
  DIRECTION_OF_DETECTOR_X_AXIS="1 0 0"
  REFINE_CORRECT="ORIENTATION CELL AXIS BEAM ! for ED, no POSITION when CELL is refined"


elif [ "$DET" == "pilatus" ]; then
elif [ "$DET" == "pilatus" ]; then
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elif [ "$DET" == "eiger" ]; then
elif [ "$DET" == "eiger" ]; then
nframes=`h5dump -d "/entry/instrument/detector/detectorSpecific/nimages" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
DATA_RANGE="1 $nframes"
SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`"
# find out if HDF5 from Diamond (DLS=1) or Dectris (DLS=0)
# find out if HDF5 from Diamond (DLS=1) or Dectris (DLS=0)
   DLS=0
   DLS=0
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   # STARTING_ANGLE:  the \- was introduced in version 0.91 to allow negative values :
   # STARTING_ANGLE:  the \- was introduced in version 0.91 to allow negative values :
     STARTING_ANGLE=`h5dump -d "/entry/sample/goniometer/omega_start" $FIRSTFRAME | awk '/\(0\): [\-0-9]/{print $2}'`
     STARTING_ANGLE=`h5dump -d "/entry/sample/goniometer/omega_start" $FIRSTFRAME | awk '/\(0\): [\-0-9]/{print $2}'`
  # /entry/sample/goniometer/omega_start is missing in some eiger2 detectors (e.g. Eiger2 9M with fw version release-2020.2.1 and SIMPLON API 1.8) (Feng YU 2021-07-18)
    if [ "$STARTING_ANGLE" == "" ]; then
  echo "/entry/sample/goniometer/omega_start not found, try /entry/sample/goniometer/omega"
  STARTING_ANGLE=`h5dump -d /entry/sample/goniometer/omega $FIRSTFRAME | grep "(0):" | head -n 1 | awk '{print $2}' | sed -e "s/,//g"`
    fi
    echo "STARTING_ANGLE=$STARTING_ANGLE"
   # If rotation vector set (NeXus)
   # If rotation vector set (NeXus)
     rotation_axis=`h5dump -a "/entry/sample/transformations/omega/vector" $FIRSTFRAME 2>/dev/null | grep "(0):" | sed -e "s/^.*://; s/,//g"`
     rotation_axis=`h5dump -a "/entry/sample/transformations/omega/vector" $FIRSTFRAME 2>/dev/null | grep "(0):" | sed -e "s/^.*://; s/,//g"`
   # Eiger 16M SSRF BL17U1 has S/N E-32-0111;  EIGER2 16M CHESS ID7B2 has S/N E-32-0123 (A. Finke 2020-11-07) v0.99
   # EIGER2 16M CHESS ID7B2 has S/N E-32-0123 (A. Finke 2020-11-07) v0.99
     SN=`h5dump -d "/entry/instrument/detector/detector_number" $FIRSTFRAME | awk '/\(0\): /{print $2}' | sed s/\"//g`
     SN=`h5dump -d "/entry/instrument/detector/detector_number" $FIRSTFRAME | awk '/\(0\): /{print $2}' | sed s/\"//g`
     if [ "$SN" == "E-32-0111" ] || [ "$SN" == "E-32-0123" ]; then
     if [ "$SN" == "E-32-0123" ]; then
       rotation_axis="-1 0 0"
       rotation_axis="-1 0 0"
       echo SSRF BL17U1 or CHESS ID7B2 with inverted rotation axis
       echo CHESS ID7B2 with inverted rotation axis
     fi  
    fi
  # SSRF BL17U1 and SSRF BL10U2 (Feng YU 2021-07-18)
  # Eiger X 16M (S/N E-32-0111) was installed at SSRF BL17U1 from Oct 2017 to Feb 2021. After Feb 2021, it was moved back to SSRF BL10U2.
# 2021-02-01 00:00:00 CST time stamp is 1612108800
    if [ "$SN" == "E-32-0111" ]; then
      collection_time=`h5dump -d "/entry/instrument/detector/detectorSpecific/data_collection_date" $FIRSTFRAME | grep "(0):" | awk '{print $2}' | sed -e "s/\.\(.*\)/CST/g; s/\"//g"`
      if [ `uname -s` == "Darwin" ]; then
        collection_timestamp=`date -j -f "%Y-%m-%dT%H:%M:%S%Z" $collection_time +%s`
      elif [ `uname -s` == "Linux" ]; then
        collection_timestamp=`date -d $collection_time +%s`
      else
        collection_timestamp=0
      fi
      if [ $collection_timestamp -eq 0 ]; then
        is_rotation_axis_set=1
        rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME 2>/dev/null || is_rotation_axis_set=0`
        if [ "$is_rotation_axis_set" == "1" ]; then
          rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME | grep "(0):" | sed -e "s/^.*://; s/,//g"`
          echo "The rotation axis of SSRF BL10U2 (Eiger X 16M) is $rotation_axis"
        else
          rotation_axis="-1 0 0    ! Cannot determine rotation axis. SSRF BL17U1: -1 0 0; SSRF BL02U1: 0 -1 0"
        fi
      elif [ $collection_timestamp -ge 0 ] && [ $collection_timestamp -le 1612108800 ]; then
        # SSRF BL17U1
        rotation_axis="-1 0 0"
        echo "SSRF BL17U1 (Eiger X 16M) with inverted rotation axis"
      else
        # SSRF BL10U2
        is_rotation_axis_set=1
        rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME 2>/dev/null || is_rotation_axis_set=0`
        if [ "$is_rotation_axis_set" == "1" ]; then
          rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME | grep "(0):" | sed -e "s/^.*://; s/,//g"`
          echo "The rotation axis of SSRF BL10U2 (Eiger X 16M) is $rotation_axis"
        else
          rotation_axis="0 -1 0"
          echo "SSRF BL10U2 (Eiger X 16M) with vertical rotation axis"
        fi
      fi
    fi
  # SSRF BL02U1 (Feng YU 2021-07-18)
  # EIGER2 S 9M SSRF BL02U1 has S/N E-18-0121
    if [ "$SN" == "E-18-0121" ]; then
      is_rotation_axis_set=1
      rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME 2>/dev/null || is_rotation_axis_set=0`
      if [ "$is_rotation_axis_set" == "1" ]; then
        rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME | grep "(0):" | sed -e "s/^.*://; s/,//g"`
        echo "The rotation axis of SSRF BL02U1 (Eiger2 S 9M) is $rotation_axis"
      else
        rotation_axis="1 0 0"
        echo "SSRF BL02U1 (Eiger2 S 9M) with horizontal rotation axis"
      fi
    fi
# revision 1.05 specialcase nframes for Eiger detectors at BNL
    if [ "$SN" == "E-18-0121" -o "$SN" == "E-32-0101" ]; then
      echo specialcase nframes for Eiger detectors at BNL:
      nframes=`h5dump -A -g "/entry/data" $FIRSTFRAME | grep "DATASPACE  SIMPLE" | sed -e "s/,.*//" | awk '{a+=$5}END{print a}'`
      DATA_RANGE="1 $nframes"
      SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`"
     fi
   fi
   fi
  echo DATA_RANGE=$DATA_RANGE
   DETECTOR="EIGER MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD= $OVERLOAD"
   DETECTOR="EIGER MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD= $OVERLOAD"
   QX=`h5dump -d "/entry/instrument/detector/x_pixel_size" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
   QX=`h5dump -d "/entry/instrument/detector/x_pixel_size" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
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! however, if the spots from COLSPOT extend to 2A then POSITION could, and if 1.5A POSITION should be refined
! however, if the spots from COLSPOT extend to 2A then POSITION could, and if 1.5A POSITION should be refined
REFINE(IDXREF)=CELL BEAM ORIENTATION AXIS  ! add POSITION if high resolution, or DETECTOR_DISTANCE inaccurate
REFINE(IDXREF)=CELL BEAM ORIENTATION AXIS  ! add POSITION if high resolution, or DETECTOR_DISTANCE inaccurate
REFINE(INTEGRATE)= POSITION BEAM ORIENTATION ! AXIS CELL . If 1.5A or higher it is ok to refine CELL
REFINE(INTEGRATE)= POSITION BEAM ORIENTATION ! AXIS CELL . If 1.5A or higher it is ok to refine CELL (unless electron diffraction)
! REFINE(CORRECT)=CELL BEAM ORIENTATION AXIS POSITION ! Default is: refine everything
REFINE(CORRECT)= $REFINE_CORRECT
 
! parameters specifically for this detector and beamline:
! parameters specifically for this detector and beamline:
DETECTOR= $DETECTOR
DETECTOR= $DETECTOR
Line 891: Line 988:
     if [ -e /usr/local/lib64/dectris-neggia.so ]; then
     if [ -e /usr/local/lib64/dectris-neggia.so ]; then
       echo LIB=/usr/local/lib64/dectris-neggia.so >> XDS.INP
       echo LIB=/usr/local/lib64/dectris-neggia.so >> XDS.INP
       echo LIB= line was written to XDS.INP
       echo LIB= line was written to XDS.INP . For Apple ARM64 processors, you must modify the name.
     else
     else
       echo !LIB=/usr/local/lib64/dectris-neggia.so >> XDS.INP
       echo !LIB=/usr/local/lib64/dectris-neggia.so >> XDS.INP
Line 1,097: Line 1,194:
fi
fi
echo XDS.INP is ready for use. The file has only the most important keywords.
echo XDS.INP is ready for use. The file has only the most important keywords.
echo Full documentation, including complete detector templates, is at
echo Full documentation, including complete detector templates, at xds.mr.mpg.de .
echo http://www.mpimf-heidelberg.mpg.de/~kabsch/xds . More documentation in XDSwiki
echo More documentation in strucbio.biologie.uni-konstanz.de/xdswiki/index.php .
echo After running xds, inspect, using XDS-Viewer, at least the beamstop mask in
echo After running xds, inspect at least the agreement of predicted and observed  
echo BKGPIX.cbf, and the agreement of predicted and observed spots in FRAME.cbf!
echo spots in FRAME.cbf!
rm -f tmp1 tmp2
rm -f tmp1 tmp2
</pre>
</pre>


Kay
Bureaucrats
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