Changes for page 05. Data processing
Last modified by tabermah on 2024-12-11 11:17
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... ... @@ -1,22 +1,27 @@ 1 1 \\ 2 2 3 -**1 1.1. Automatic data processing**3 +**10.1. Automatic data processing** 4 4 5 5 Unless you un-check the option for the specific acquisition run, autoprocessing will be executed. For standard rotational data autoprocessing is via XDSAPP (Sparta et al. (2016) //J. Apple. Cryst.// **49**, 1085-1092) for strategy calculation we use Mosflm (Leslie //Acta D//**62** (2006) 48-57) and Spotfinder ((% style="color: rgb(0,0,0);text-decoration: none;" %)Zhang et al. (2006). (% style="text-decoration: none;text-align: left;" %)//J. Appl. Cryst.//(% style="color: rgb(0,0,0);text-decoration: none;" %) (% style="text-decoration: none;text-align: left;" %)**39**(% style="color: rgb(0,0,0);text-decoration: none;" %), 112–119)(%%) for producing the heatmap for the grid scans. The results are compiled into HTML-files to give you a convenient way of checking them. The output files are in the processed folders of the corresponding datasets. A self refreshing index of all results is created in the beamtimes processed folder. During the beamtime you can open it from file::~/~//gpfs/current/processed/index.html in a browser. The HTML-file is also contained in your data backup. 6 6 7 7 \\ 8 8 9 -**1 1.2. Manual data processing onsite**9 +**10.3. Manual data processing onsite** 10 10 11 -Please do not use the control computers of the beamline (haspp11user01-04) nor the haspp11eval01for data processing(latter is now fully dedicated to autoprocessing.11 +Open a terminal (see session 3.2) and type ssh haspp11eval01. Please do not use the control computers of the beamline (haspp11user01-04) for data processing. 12 12 13 - UseMaxwell-clusterfor data processingas described in the next chapter; on-site,you candirectly ssh tousername@desy-ps-cpuoruse Max-display by connectingto [[https:~~/~~/max-display.desy.de:3443>>url:https://max-display.desy.de:3443||shape="rect"]] viaweb browser. Accessto Maxwell requires a ScientificAccount.13 +Here you can launch crystallographic programs directly //e.g.//: 14 14 15 +* for XDSAPP type in the terminal (% style="color: rgb(0,128,0);" %)xdsapp 16 +* for imosflm type in the terminal (% style="color: rgb(0,128,0);" %)imosflm 17 +* for CCP4 type in the terminal (% style="color: rgb(0,128,0);" %)ccp4i 18 +* for phenix type in the terminal (% style="color: rgb(0,128,0);" %)phenix 19 + 15 15 \\ 16 16 17 -**1 1.3. Manual data processing after your beamtime or during remote session**22 +**10.4. Manual data processing after your beamtime or during remote session** 18 18 19 -Manual data processing after the beamtime or during a remote session is only available for registered [[DESY Scien tific Accounts>>doc:FSEC.Science Accounts.WebHome||shape="rect"]].24 +Manual data processing after the beamtime or during a remote session is only available for registered [[DESY Science Accounts>>doc:FSEC.Science Accounts.WebHome||shape="rect"]]. 20 20 21 21 //Accessing data from outside the DESY network~:// 22 22 In a terminal window: ... ... @@ -27,21 +27,7 @@ 27 27 cd /asap3/petra3/gpfs/p11/2020/data/beamtimeID 28 28 29 29 Data is accessible to users who were registered participants to the experiment in Door prior to the beamtime ID being opened at the beamline. If you cannot access the data, please contact your LC or the beamline manager. 30 - 31 -(% style="color: rgb(51,51,51);text-decoration: none;" %)Our processing folders now contain two folders, 'full' and 'manual'. 'Manual' contains a template that has all the correct parameters and processing will run just by typing xds_par there. However, to shorten the processing time and make use of the computational structure, you should use a script to queue the jobs in slurm. A template script (xds.sh) can be found at /asap3/petra3/gpfs/common/p11/xds.sh 32 - 33 -The partition in the script is defined psx for external users (ps should be used for internal users of Photon Science). 34 -(% style="color: rgb(51,51,51);text-decoration: none;" %)Copy the script to the folder where you run the processing and launch by (%%) 35 -(% style="color: rgb(51,51,51);text-decoration: none;" %)sbatch xds.sh(%%) 36 -(% style="color: rgb(51,51,51);text-decoration: none;" %)It will find a free node for your job and run faster than just typing xds_par(%%) 37 -(% style="color: rgb(51,51,51);text-decoration: none;" %)The xds-log you get in a file xds-job-~#~##.out 38 - 39 -(% style="color: rgb(51,51,51);text-decoration: none;" %)nxds can be used for processing Serial Crystallography data in a similar way than xds. As the computing time is long, nxds should should be used via a script to queue the jobs in slurm. The template script (nxds.sh) as well as an example of input file (nXDS.INP) can be found in /asap3/gpfs/common/p11/. 40 - 41 -(% style="color: rgb(51,51,51);text-decoration: none;" %)Copy the script and the nXDS.INP to the folder where you run the processing. The nXDS.INP file needs some editing to fit your data path and data collection parameters (wavelength, detector distance, oscillation...). The processing is launch by 42 -sbatch nxds.sh 43 - 44 -//List of software you can use is at~:// 35 +\\//List of software you can use is at~:// 45 45 (% class="Object" %)[[https:~~/~~/confluence.desy.de/display/IS/Photon+Science>>doc:IS.Photon Science.WebHome||shape="rect"]](%%) 46 46 \\//You can store analysis results in scratch_cc (temporary/testing results) or processed (final results).// 47 47 \\//To use crystallographic programs~:// ... ... @@ -49,7 +49,3 @@ 49 49 module load xray # sets the environment for xds and helper GUIs such as XDSAPP 50 50 module load ccp4/6.4 51 51 module load phenix 52 - 53 -\\ 54 - 55 -\\
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... ... @@ -1,1 +1,1 @@ 1 -https://confluence.desy.de/spaces/11/pages/ 252809700/11. Data processing1 +https://confluence.desy.de/spaces/11/pages/188798288/11. Data processing