== Background ==
This is a tutorial for Lau and Kaare in SBiNLab, and hopefully others.
To get inspiration of example scripts files and '''see''' how the protocol is performed, have a look here:
* [https://github.com/nmr-relax-code/test_suiterelax/system_testsblob/scriptsmaster/model_freeauto_analyses/dauvergne_protocol.py* nmr-relax-code/auto_analyses/dauvergne_protocol.py]
== Scripts ==For references, see [http://www.nmr-relax.com/refs.shtml relax references]:To get * [[Model-free_analysis_single_field#Protocol|See this description of the protocol by Edward]] and image [http://www.nmr-relax.com/manual/The_diffusion_seeded_paradigm.html The diffusion seeded paradigm]* [http://www.nmr-relax.com/manual/Model_free_analysis.html Link to the manual]* [http://www.nmr-relax.com/manual/The_model_free_models.html Summary of model-free models]* [http://www.nmr-relax.com/manual/molmol_macro_apply.html#SECTION081284600000000000000 Summary of parameter meaning and value to workpymol visualization]* d'Auvergne, E. J. and Gooley, P. R. (2008). [http://dx.doi.org/10.1007/s10858-007-9214-2 Optimisation of NMR dynamic models I. Minimisation algorithms and their performance within the model-free and Brownian rotational diffusion spaces. J. Biomol. NMR, 40(2), 107-119.]* d'Auvergne, E. J. and Gooley, P. R. (2008). [http://dx.doi.org/10.1007/s10858-007-9213-3 Optimisation of NMR dynamic models II. A new methodology for the dual optimisation of the model-free parameters and the Brownian rotational diffusion tensor. J. Biomol. NMR, we need to 40(2), 121-133.]
* Load a PDB structure= Script inspiration =* Assign the "data structure" in relax through spin== model-assignmentsfree : Script inspiration for setup and analysis ==* Assign necessary "information" as isotope information to each spin-assignmentThe distribution of relax includes a folder '''sample_scripts/model_free''' which contain* Read "R1, R2 and NOE" a folder with scripts for different magnet field strengths* Calculate some properties* Check the data* Run the protocolanalysis.
To work most efficiently, it is important to perform each step 1 by 1, and closely inspect the log for any errorsIt can be seen here: https://github.com/nmr-relax/relax/tree/master/sample_scripts/model_free
For similar tutorial, have Here is the current list* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/back_calculate.py back_calculate.py]. Back-calculate and save relaxation data starting from a saved model-free results file.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/bmrb_deposition.py bmrb_deposition.py] Script for creating a NMR-STAR 3.1 formatted file for BMRB deposition of model-free results.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/cv.py cv.py] Script for model-free analysis using cross-validation model selection.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/dasha.py dasha.py] Script for model-free analysis using the program Dasha.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/dauvergne_protocol.py dauvergne_protocol.py] Script for black-box model-free analysis.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/diff_min.py diff_min.py] Demonstration script for diffusion tensor optimisation in a model-free analysis.]* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/final_data_extraction.py final_data_extraction.py] Extract Data to Table* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/generate_ri.py generate_ri.py] Script for back-calculating the relaxation data.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/grace_S2_vs_te.py grace_S2_vs_te.py] Script for creating a grace plot of the simulated order parameters vs. simulated correlation times.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/ grace_ri_data_correlation.py] Script for creating correlations plots of experimental verses back calculated relaxation data.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/map.py map.py] Script for mapping the model-free space for OpenDX visualisation.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/mf_multimodel.py mf_multimodel.py] This script performs a look atmodel-free analysis for the models 'm0' to 'm9' (or 'tm0' to 'tm9').* [https: //github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/modsel.py modsel.py] Script for model-free model selection.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/molmol_plot.py molmol_plot.py] Script for generating Molmol macros for highlighting model-free motions* [Tutorial_for_modelhttps://github.com/nmr-free_analysis_sam_mahdi|Tutorial relax/relax/blob/master/sample_scripts/model_free/palmer.py palmer.py] Script for model-free analysis sam mahdiusing Art Palmer's program 'Modelfree4'. Download from http://comdnmr.nysbc.org/comd-nmr-dissem/comd-nmr-software* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/remap.py remap.py]Script for mapping the model-free space.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/single_model.py single_model.py]This script performs a model-free analysis for the single model 'm4'.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/table_csv.py table_csv.py] Script for converting the model-free results into a CSV table.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/model_free/table_latex.py table_latex.py] Script for converting the model-free results into a LaTeX table.
=== Test load of PDB =Other script inspiration for checking ==First we just want to test to read the PDB fileThe distribution of relax includes a folder '''sample_scripts/''' which contain a folder with scripts for analysis.
'''01_read_pdbIt can be seen here: https://github.py'''<source lang="python"># Python module imports.from time import asctime, localtimeimport oscom/nmr-relax/relax/tree/master/sample_scripts
# '''R1 / R2 Calculation'''* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/relax_fit.py relax_fit.py] Script for relaxation curve fitting.* [https://github.com/nmr-relax/relax module imports/blob/master/sample_scripts/relax_curve_diff.py relax_curve_diff.py] Script for creating a Grace plot of peak intensity differences.The resultant plot is useful for finding bad points or bad spectra when fitting exponential curves determine the R1 and R2 relaxation rates. If the averages deviate systematically from auto_analyseszero, bias in the spectra or fitting will be clearly revealed. To use this script, R1 or R2 exponential curve fitting must have previously have been carried out the program state saved to the file 'rx.save' (either with or without the .gz or .bz2 ). The file name of the saved state can be changed at the top of this script.dauvergne_protocol import dAuvergne_protocol
# Set up the data pipe'''NOE calculation'''* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/noe.py noe.py] Script for calculating NOEs.#######################
# '''Test data'''* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/jw_mapping.py jw_mapping.py] Script for reduced spectral density mapping.* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/consistency_tests.py consistency_tests.py] Script for consistency testing. Severe artifacts can be introduced if model-free analysis is performed from inconsistent multiple magnetic field datasets. The following sequence use of user function calls simple tests as validation tools for the consistency assessment can help avoid such problems in order to extract more reliable information from spin relaxation experiments. In particular, these tests are useful for detecting inconsistencies arising from R2 data. Since such inconsistencies can yield artifactual Rex parameters within model-free analysis, these tests should be use routinely prior to any analysis such as model-free calculations.This script will allow one to calculate values for the three consistency tests J(0), F_eta and F_R2. Once this is done, qualitative analysis can be changed performed by comparing values obtained at different magnetic fields. Correlation plots and histograms are useful tools for such comparison, such as neededpresented in Morin & Gagne (2009a) J. Biomol. NMR, 45: 361-372.
# Create '''Other representations'''* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/angles.py angles.py] Script for calculating the data pipeprotein NH bond vector angles with respect to the diffusion tensor.bundle_name = "mf (%s)" % asctime(localtime())* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/xh_vector_dist.py xh_vector_dist.py] Script for creating a PDB representation of the distribution of XH bond vectors.name = "origin"pipe* [https://github.com/nmr-relax/relax/blob/master/sample_scripts/diff_tensor_pdb.py diff_tensor_pdb.py] Script for creating a PDB representation of the Brownian rotational diffusion tensor.create(name, 'mf', bundle=bundle_name)
# Load the PDB file.= Scripts - Part 2 =structure.read_pdb('energy_1We now try to setup things a little more efficient.pdb', set_mol_name='TEMP', read_model=1)
# Set Relax is able to read previous results file, so let us divide the task up the 15N and 1H spins (both backbone and Trp indole sidechains).structure.load_spins('@N', ave_pos=True)structure.load_spins('@NE1', ave_pos=True)structure.load_spins('@H', ave_pos=True)structure.load_spins('@HE1', ave_pos=True)into:
# Assign isotopes* 1: Load the data and save as state file. Inspect in GUI before running.spin* 2: Run the Model 1: local_tm.isotope('15N', spin_id='@N* 3: Here make 4 scripts. Each of them only depends on Model 1:** Model 2: sphere** Model 3: prolate** Model 4: oblate**')Model 5: ellipsoidspin.isotope(* 4: Make an intermediate '1Hfinal', spin_idmodel script. This will automatically detect files from above. == Prepare data =='@H*')</source>We make a new folder and try.
Run with{| class="mw-collapsible mw-collapsed wikitable"! See commands|-|
<source lang="bash">
relax 01_read_pdbmkdir 20171010_model_free_2_HADDOCKcp 20171010_model_free/*.py dat 20171010_model_free_2_HADDOCKcp 20171010_model_free/*.pdb 20171010_model_free_2_HADDOCK # Get scriptscd 20171010_model_free_2_HADDOCKgit initgit remote add origin git@github.com:tlinnet/relax_modelfree_scripts.gitgit fetchgit checkout -t 01_read_pdb.logorigin/master
</source>
|}
And a new one, changing the NOE error
{| class="mw-collapsible mw-collapsed wikitable"
! Output from logfileSee commands
|-
|
<source lang="bash">
script = '01_read_pdbmkdir 20171010_model_free_3_HADDOCKcp 20171010_model_free/*.py'----------------------------------------------------------------------------------------------------dat 20171010_model_free_3_HADDOCK# Python module importscp 20171010_model_free/*.from time import asctime, localtimeimport ospdb 20171010_model_free_3_HADDOCK
# relax module importsGet scriptscd 20171010_model_free_3_HADDOCKgit initgit remote add origin git@github.com:tlinnet/relax_modelfree_scripts.gitfrom auto_analyses.dauvergne_protocol import dAuvergne_protocolgit fetchgit checkout -t origin/master
# Set up the data pipeChange NOE errorsed -i 's/0.1*$/0.05/' NOE_600MHz_new.datsed -i 's/0.1*$/0.05/' NOE_750MHz.dat</source>#######################|}
# The following sequence of user function calls can be changed as needed. # Create the data pipe.bundle_name = "mf (%s)" % asctime(localtime())name = "origin"pipe.create(nameAnd a new one, 'mf', bundle=bundle_name) # Load changing the PDB file.structure.read_pdb('energy_1.pdb'NOE error, set_mol_name='TEMP', read_model=1) # Set up the 15N and 1H spins (both backbone and Trp indole sidechains).structure.load_spins('@deselecting N', ave_pos=True)structure-terminal.load_spins('@NE1', ave_pos=True)<br>structure.load_spins('@H'Consistency test, ave_pos=True)structurefound that this stretch contained outliers.load_spins('@HE1', ave_pos=True) # Assign isotopesspin.isotope('15N', spin_id{| class='@N*')"mw-collapsible mw-collapsed wikitable"spin.isotope('1H', spin_id='@H*')! See commands ---------------------------------------------------------------------------------------------------|-|relax> pipe.create(pipe_name<source lang='origin', pipe_type='mf', bundle='mf (Fri Oct 13 17:44:18 2017)') relax"bash"> structure.read_pdb(file='energy_1.pdb', dir=None, read_mol=None, set_mol_name='TEMP', read_model=1, set_model_num=None, alt_loc=None, verbosity=1, merge=False)mkdir 20171010_model_free_4_HADDOCKInternal relax PDB parsercp 20171010_model_free/*.dat 20171010_model_free_4_HADDOCKOpening the file 'energy_1cp 20171010_model_free/*.pdb' for reading.RelaxWarning: Cannot determine the element associated with atom 'X'.RelaxWarning: Cannot determine the element associated with atom 'Z'.RelaxWarning: Cannot determine the element associated with atom 'OO'.RelaxWarning: Cannot determine the element associated with atom 'OO2'.Adding molecule 'TEMP' to model 1 (from the original molecule number 1 of model 1). relax> structure.load_spins(spin_id='@N', from_mols=None, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to the relax data store. # mol_name res_num res_name spin_num spin_name REMOVED FROM DISPLAY relax> structure.load_spins(spin_id='@NE1', from_mols=None, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to the relax data store. # mol_name res_num res_name spin_num spin_name REMOVED FROM DISPLAY relax> structure.load_spins(spin_id='@H', from_mols=None, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to the relax data store. # mol_name res_num res_name spin_num spin_name REMOVED FROM DISPLAY relax> structure.load_spins(spin_id='@HE1', from_mols=None, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to the relax data store. # mol_name res_num res_name spin_num spin_name REMOVED FROM DISPLAY20171010_model_free_4_HADDOCK
relax> spin# Get scriptscd 20171010_model_free_4_HADDOCKgit initgit remote add origin git@github.isotope(isotope='15N', spin_id='@N*', force=False)com:tlinnet/relax_modelfree_scripts.gitgit fetchgit checkout -t origin/master
relax> spin# Change NOE errorsed -i 's/0.1*$/0.isotope(isotope=05/'1HNOE_600MHz_new.datsed -i ', spin_id='@Hs/0.1*$/0.05/', force=False)NOE_750MHz.dat
# Make deselection
echo "#" > deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t151" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t152" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t153" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t154" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t155" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t156" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t157" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t158" >> deselect.txt
cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t159" >> deselect.txt
</source>
|}
And a new one, changing the NOE error, and deselecting spins found from consistency test.<br>{| class="mw-collapsible mw-collapsed wikitable"! See commands|-|<source lang== Test load of data ==="bash">mkdir 20171010_model_free_5_HADDOCKcp 20171010_model_free/*.dat 20171010_model_free_5_HADDOCKThat looked to go fine, so let us try to just load datacp 20171010_model_free/*.pdb 20171010_model_free_5_HADDOCK
Copy '''01_read_pdb.py''' to '''02_read_data.py''' and add:<source lang="python"># Load the relaxation data.Get scriptsrelax_data.read(ri_id='R1_600', ri_type='R1', frq=600.17*1e6, file='R1_600MHz_new_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)relax_data.read(ri_id='R2_600', ri_type='R2', frq=600.17*1e6, file='R2_600MHz_new_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)cd 20171010_model_free_5_HADDOCKrelax_data.read(ri_id='NOE_600', ri_type='NOE', frq=600.17*1e6, file='NOE_600MHz_new.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)git initrelax_datagit remote add origin git@github.read(ri_id='R1_750', ri_type='R1', frq=750com:tlinnet/relax_modelfree_scripts.06*1e6, file='R1_750MHz_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)gitrelax_data.read(ri_id='R2_750', ri_type='R2', frq=750.06*1e6, file='R2_750MHz_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)git fetchrelax_data.read(ri_id='NOE_750', ri_type='NOE', frq=750.06*1e6, file='NOE_750MHz.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)git checkout -t origin/master
# Define the magnetic dipoleChange NOE errorsed -dipole relaxation interactioni 's/0.interatom1*$/0.define(spin_id1=05/'@N', spin_id2='@H', direct_bond=True)NOE_600MHz_new.datinteratom.define(spin_id1='@NE1', spin_id2='@HE1sed -i ', direct_bond=True)interatoms/0.set_dist(spin_id1='@N1*$/0.05/', spin_id2='@H*', ave_dist=1.02 * 1e-10)interatomNOE_750MHz.unit_vectors()dat
# Define the chemical shift relaxation interactionMake deselectionecho "#" > deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t158" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t157" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t17" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t159" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t120" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t59" >> deselect.txtvaluecat R1_600MHz_new_model_free.set(dat | grep -172 * 1eP "ArcCALD\t98" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -6, 'csa', spin_id='@N*')P "ArcCALD\t49" >> deselect.txt</sourcecat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t76" >>deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t155" >> deselect.txtRun withcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t156" >> deselect.txt<source lang=cat R1_600MHz_new_model_free.dat | grep -P "bashArcCALD\t48">> deselect.txtrelax 02_read_datacat R1_600MHz_new_model_free.py dat | grep -t 02_read_dataP "ArcCALD\t154" >> deselect.logtxt
</source>
|}
And a new one, without changing the NOE error, and deselecting spins found from consistency test.<br>
{| class="mw-collapsible mw-collapsed wikitable"
! Output from logfileSee commands
|-
|
<source lang="bash">
script = '02_read_datamkdir 20171010_model_free_6_HADDOCKcp 20171010_model_free/*.py'----------------------------------------------------------------------------------------------------dat 20171010_model_free_6_HADDOCK# Python module importscp 20171010_model_free/*.from time import asctime, localtimeimport ospdb 20171010_model_free_6_HADDOCK
# relax module importsGet scriptscd 20171010_model_free_6_HADDOCKgit initgit remote add origin git@github.com:tlinnet/relax_modelfree_scripts.gitfrom auto_analyses.dauvergne_protocol import dAuvergne_protocolgit fetchgit checkout -t origin/master
# Set up the data pipeMake deselectionecho "#" > deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t158" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t157" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t17" >> deselect.txt#######################cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t159" >> deselect.txt
# The following sequence of user function calls can be changed as neededcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t59" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t98" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t76" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t155" >> deselect.txtcat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t156" >> deselect.txt cat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t120" >> deselect.txt
# Create the data pipecat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t49" >> deselect.txtbundle_name = cat R1_600MHz_new_model_free.dat | grep -P "mf (%s)ArcCALD\t48" % asctime(localtime())>> deselect.txtname = cat R1_600MHz_new_model_free.dat | grep -P "originArcCALD\t154"pipe>> deselect.create(name, 'mf', bundle=bundle_name)txt
# Load the PDB filecat R1_600MHz_new_model_free.dat | grep -P "ArcCALD\t33" >> deselect.txtstructurecat R1_600MHz_new_model_free.read_pdb('energy_1dat | grep -P "ArcCALD\t67" >> deselect.pdb', set_mol_name='TEMP', read_model=1)txt</source>|}
# Set up the 15N and 1H spins (both backbone and Trp indole sidechains).structure.load_spins('@N', ave_pos=True)structure= 11_read_data_GUI_inspect.load_spins('@NE1', ave_pospy - Read data GUI inspect =True)structure.load_spins('@H', ave_pos=True)structureThis will read the data and save as a state.load_spins('@HE1', ave_pos=True)
# Assign isotopesspinThe GUI can be a good place to inspect the setup and files.isotope('15N', spin_id='@N*')spin.isotope('1H', spin_id='@H*')
# Load the relaxation data.relax_data.read(ri_id='R1_600', ri_type='R1', frq=600.17*1e6, file='R1_600MHz_new_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)relax_data.read(ri_id='R2_600', ri_type='R2', frq=600.17*1e6, file='R2_600MHz_new_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)relax_data.read(ri_id='NOE_600', ri_type='NOE', frq=600.17*1e6, file='NOE_600MHz_new.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)relax_data.read(ri_id='R1_750', ri_type='R1', frq=750.06*1e6, file='R1_750MHz_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)relax_data.read(ri_id='R2_750', ri_type='R2', frq=750.06*1e6, file='R2_750MHz_model_free.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)See content of:relax_data[https://github.read(ri_id='NOE_750', ri_type='NOE', frq=750com/tlinnet/relax_modelfree_scripts/blob/master/11_read_data_GUI_inspect.06*1e6, file='NOE_750MHzpy 11_read_data_GUI_inspect.dat', mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7)py]
# Define the magnetic dipole-dipole relaxation interaction.Run withinteratom.define(spin_id1='@N', spin_id2='@H', direct_bond<source lang=True)"bash">interatomrelax 11_read_data_GUI_inspect.define(spin_id1='@NE1', spin_id2='@HE1', direct_bond=True)interatom.set_dist(spin_id1='@N*', spin_id2='@H*', ave_dist=1py -t 11_read_data_GUI_inspect.02 * 1e-10)loginteratom.unit_vectors()</source>
# Define the chemical shift relaxation interactionTo check in GUI* relax -g* File -> Open relax state* In folder "result_10" open "result_10_ini.bz2"value.set(* View -172 > Data pipe editor* 1eRight click on pipe, and select "Associate with a new auto-6, 'csa', spin_id='@N*')analysis"
=== relax 11_test_consistency.py ----------------------------------------------------------------------------------------------------Consistency test of our data ===Before running the analysis, it is wise to run a script for [[Tutorial_for_model_free_SBiNLab#Other_script_inspiration_for_checking|consistency testing]].
relax> pipeSee here:* Morin & Gagne (2009a) [http://dx.doi.org/10.1007/s10858-009-9381-4 Simple tests for the validation of multiple field spin relaxation data. J. Biomol.create(pipe_name='origin', pipe_type='mf'NMR, bundle='mf (Fri Oct 13 1745:51:28 2017)')361-372.]
relax> structureHighlights:* Comparing results obtained at different magnetic fields should, in the case of perfect consistency and assuming the absence of conformational exchange, yield equal values independently of the magnetic field.* avoid the potential extraction of erroneous information as well as the waste of time associated to dissecting inconsistent datasets using numerous long model-free minimisations with different subsets of data.read_pdb* The authors prefer the use of the spectral density at zero frequency J(file=0) alone since it 'energy_1.pdb', dir=None, read_mol=None, set_mol_name='TEMPdoes not rely''' on an estimation of the global correlation time '''tc/tm''', read_model=1neither on a measure of theta, set_model_num=Nonethe angle between the 15N–1H vector and the principal axis of the 15N chemical shift tensor. Hence, alt_loc=None, verbosity=1, merge=FalseJ(0)is less likely to be affected by incorrect parameterisation of input parameters.
Internal relax PDB parser.See content of:Opening the file 'energy_1[https://github.pdb' for readingcom/tlinnet/relax_modelfree_scripts/blob/master/11_test_consistency.RelaxWarning: Cannot determine the element associated with atom 'X'py 11_test_consistency.py]RelaxWarning: Cannot determine the element associated with atom 'Z'.<source lang="bash">RelaxWarning: Cannot determine the element associated with atom 'OO'relax 11_test_consistency.RelaxWarning: Cannot determine the element associated with atom 'OO2'py -t 11_test_consistency.Adding molecule 'TEMP' to model 1 (from the original molecule number 1 of model 1)py.log
relax> structure.load_spins(spin_id='@N', from_mols=None#Afterwards, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to go into the relax folder at plot data store.python plot_txt_files.py./grace2images.py </source>
# mol_name res_num res_name spin_num spin_name == 12_Model_1_I_local_tm.py - Only run local_tm ==REMOVED FROM DISPLAYNow we only run '''Model 1'''.
relax> structure.load_spins(spin_id* DIFF_MODEL =['@NE1local_tm', from_mols]* GRID_INC =None, mol_name_target11 # This is the standard* MC_NUM =None, ave_pos=True, spin_num0 # This has no influence in Model 1-5* MAX_ITER =True)Adding the following spins to the relax data store.20 # Stop if it has not converged in 20 rounds
# mol_name res_num res_name spin_num spin_name Normally between 8 to 15 multiple rounds of optimisation of the are required for the proper execution of this script.<br>REMOVED FROM DISPLAYThis is can also be see here in Figure 2.* d'Auvergne, E. J. and Gooley, P. R. (2008). [http://dx.doi.org/10.1007/s10858-007-9213-3 Optimisation of NMR dynamic models II. A new methodology for the dual optimisation of the model-free parameters and the Brownian rotational diffusion tensor. J. Biomol. NMR, 40(2), 121-133.]
relax> structure.load_spins(spin_id='@H'Relax should stop calculation, from_mols=None, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to the relax data storeif a model does not converge.
# mol_name res_num res_name spin_num spin_name See content of:REMOVED FROM DISPLAY[https://github.com/tlinnet/relax_modelfree_scripts/blob/master/12_Model_1_I_local_tm.py 12_Model_1_I_local_tm.py]
relax> structureWe use [http://www.load_spins(spin_id='@HE1'dayid.org/comp/tm.html tmux] to make a terminal-session, from_mols=Nonewe can get back to, mol_name_target=None, ave_pos=True, spin_num=True)Adding the following spins to the relax data storeif our own terminal connection get closed.
Run with<source lang="bash"># mol_name res_num res_name spin_num spin_name Make terminal-sessionREMOVED FROM DISPLAYtmux new -s m1
relax> spin12_Model_1_I_local_tm.isotope(isotope='15N', spin_id='@N*', force=False)py -t 12_Model_1_I_local_tm.log
# ortmux new -s m1mpirun -np 22 relax> spin.isotope(isotope--multi='1Hmpi4py', spin_id='@H*', force=False)12_Model_1_I_local_tm.py -t 12_Model_1_I_local_tm.log</source>
relaxYou can then in another terminal follow the logfile by<source lang="bash"> relax_dataless +F 12_Model_I_local_tm.read(ri_id='R1_600', ri_type='R1', frq=600170000.0, file='R1_600MHz_new_model_free.dat', dir=None, spin_id_col=None, mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7, sep=None, spin_id=None)logOpening the file 'R1_600MHz_new_model_free.dat' for reading.</source>
The following 600.17 MHz R1 relaxation data with the ID * To scroll up and down, use keyboard: '''R1_600Ctrl+c' has been loaded into the relax data store''* To return to follow mode, use keyboard:'''Shift+f'''* To exit, use keyboard: '''Ctrl+c''' and then: '''q'''
# Spin_ID Value Error == 13_Model_2-5 - Run Model 2 to 5 ==REMOVED FROM DISPLAY When Model 1 is completed, then make 4 terminal windows and run them at the same time.
relax> relax_data.read(ri_id='R2_600', ri_type='R2', frq=600170000.0, file='R2_600MHz_new_model_free.dat', dir=None, spin_id_col=None, mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7, sep=None, spin_id=None)These scripts do:Opening * Read the state file 'R2_600MHz_new_model_free.dat' for reading.from before with setup* Change DIFF_MODEL accordingly
The following 600[https://github.com/tlinnet/relax_modelfree_scripts/blob/master/13_Model_2_II_sphere.py 13_Model_2_II_sphere.py]<source lang="bash">tmux new -s m2relax 13_Model_2_II_sphere.17 MHz R2 relaxation data with the ID py -t 13_Model_2_II_sphere.log# Ormpirun -np 5 relax --multi='R2_600mpi4py' has been loaded into the relax data store:13_Model_2_II_sphere.py -t 13_Model_2_II_sphere.log
# Spin_ID Value Error When relax is running, push: Ctrl+b and then d, to disconnect without exitREMOVED FROM DISPLAY </source>
relax> relax_data.read(ri_id='NOE_600', ri_type='NOE', frq=600170000.0, file='NOE_600MHz_new.dat', dir=None, spin_id_col=None, mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7, sep=None, spin_id=None)Opening the file 'NOE_600MHz_new.dat' for reading. The following 600.17 MHz NOE relaxation data with the ID 'NOE_600' has been loaded into the relax data store: # Spin_ID Value Error REMOVED FROM DISPLAY relax> relax_data.read(ri_id='R1_750', ri_type='R1', frq=750060000.0, file='R1_750MHz_model_free.dat', dir=None, spin_id_col=None, mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7, sep=None, spin_id=None)Opening the file 'R1_750MHz_model_free.dat' for reading. The following 750.06 MHz R1 relaxation data with the ID 'R1_750' has been loaded into the relax data store[https: # Spin_ID Value Error REMOVED FROM DISPLAY relax> relax_data.read(ri_id='R2_750', ri_type='R2', frq=750060000//github.0, file='R2_750MHz_model_free.dat', dir=None, spin_id_col=None, mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7, sep=None, spin_id=None)Opening the file 'R2_750MHz_model_freecom/tlinnet/relax_modelfree_scripts/blob/master/13_Model_3_III_prolate.dat' for readingpy 13_Model_3_III_prolate.py] The following 750.06 MHz R2 relaxation data with the ID 'R2_750' has been loaded into the relax data store: # Spin_ID Value Error REMOVED FROM DISPLAY relax> relax_data.read(ri_id='NOE_750', ri_type<source lang='NOE', frq=750060000.0, file='NOE_750MHz.dat', dir=None, spin_id_col=None, mol_name_col=1, res_num_col=2, res_name_col=3, spin_num_col=4, spin_name_col=5, data_col=6, error_col=7, sep=None, spin_id=None)Opening the file 'NOE_750MHz.dat' for reading. The following 750.06 MHz NOE relaxation data with the ID 'NOE_750' has been loaded into the relax data store: # Spin_ID Value Error REMOVED FROM DISPLAY relax"bash"> interatom.define(spin_id1='@N', spin_id2='@H', direct_bond=True, spin_selection=True, pipe=None)Interatomic interactions are now defined for the following spins: # Spin_ID_1 Spin_ID_2 '#TEMP:3@N' '#TEMP:3@H' '#TEMP:4@N' '#TEMP:4@H' '#TEMP:5@N' '#TEMP:5@H' '#TEMP:6@N' '#TEMP:6@H' '#TEMP:7@N' '#TEMP:7@H' '#TEMP:8@N' '#TEMP:8@H' '#TEMP:9@N' '#TEMP:9@H' '#TEMP:10@N' '#TEMP:10@H' '#TEMP:11@N' '#TEMP:11@H' '#TEMP:13@N' '#TEMP:13@H' '#TEMP:14@N' '#TEMP:14@H' '#TEMP:15@N' '#TEMP:15@H' '#TEMP:16@N' '#TEMP:16@H' '#TEMP:17@N' '#TEMP:17@H' '#TEMP:18@N' '#TEMP:18@H' '#TEMP:19@N' '#TEMP:19@H' '#TEMP:20@N' '#TEMP:20@H' '#TEMP:21@N' '#TEMP:21@H' '#TEMP:22@N' '#TEMP:22@H' '#TEMP:23@N' '#TEMP:23@H' '#TEMP:24@N' '#TEMP:24@H' '#TEMP:25@N' '#TEMP:25@H' '#TEMP:26@N' '#TEMP:26@H' '#TEMP:27@N' '#TEMP:27@H' '#TEMP:28@N' '#TEMP:28@H' '#TEMP:29@N' '#TEMP:29@H' '#TEMP:30@N' '#TEMP:30@H' '#TEMP:31@N' '#TEMP:31@H' '#TEMP:32@N' '#TEMP:32@H' '#TEMP:33@N' '#TEMP:33@H' '#TEMP:34@N' '#TEMP:34@H' '#TEMP:35@N' '#TEMP:35@H' '#TEMP:36@N' '#TEMP:36@H' '#TEMP:37@N' '#TEMP:37@H' '#TEMP:38@N' '#TEMP:38@H' '#TEMP:39@N' '#TEMP:39@H' '#TEMP:40@N' '#TEMP:40@H' '#TEMP:41@N' '#TEMP:41@H' '#TEMP:42@N' '#TEMP:42@H' '#TEMP:43@N' '#TEMP:43@H' '#TEMP:45@N' '#TEMP:45@H' '#TEMP:46@N' '#TEMP:46@H' '#TEMP:47@N' '#TEMP:47@H' '#TEMP:48@N' '#TEMP:48@H' '#TEMP:49@N' '#TEMP:49@H' '#TEMP:50@N' '#TEMP:50@H' '#TEMP:51@N' '#TEMP:51@H' '#TEMP:52@N' '#TEMP:52@H' '#TEMP:53@N' '#TEMP:53@H' '#TEMP:54@N' '#TEMP:54@H' '#TEMP:55@N' '#TEMP:55@H' '#TEMP:56@N' '#TEMP:56@H' '#TEMP:57@N' '#TEMP:57@H' '#TEMP:58@N' '#TEMP:58@H' '#TEMP:59@N' '#TEMP:59@H' '#TEMP:60@N' '#TEMP:60@H' '#TEMP:61@N' '#TEMP:61@H' '#TEMP:62@N' '#TEMP:62@H' '#TEMP:63@N' '#TEMP:63@H' '#TEMP:64@N' '#TEMP:64@H' '#TEMP:65@N' '#TEMP:65@H' '#TEMP:66@N' '#TEMP:66@H' '#TEMP:67@N' '#TEMP:67@H' '#TEMP:68@N' '#TEMP:68@H' '#TEMP:69@N' '#TEMP:69@H' '#TEMP:70@N' '#TEMP:70@H' '#TEMP:71@N' '#TEMP:71@H' '#TEMP:72@N' '#TEMP:72@H' '#TEMP:73@N' '#TEMP:73@H' '#TEMP:74@N' '#TEMP:74@H' '#TEMP:75@N' '#TEMP:75@H' '#TEMP:76@N' '#TEMP:76@H' '#TEMP:77@N' '#TEMP:77@H' '#TEMP:78@N' '#TEMP:78@H' '#TEMP:79@N' '#TEMP:79@H' '#TEMP:80@N' '#TEMP:80@H' '#TEMP:81@N' '#TEMP:81@H' '#TEMP:82@N' '#TEMP:82@H' '#TEMP:83@N' '#TEMP:83@H' '#TEMP:84@N' '#TEMP:84@H' '#TEMP:85@N' '#TEMP:85@H' '#TEMP:87@N' '#TEMP:87@H' '#TEMP:88@N' '#TEMP:88@H' '#TEMP:89@N' '#TEMP:89@H' '#TEMP:90@N' '#TEMP:90@H' '#TEMP:91@N' '#TEMP:91@H' '#TEMP:93@N' '#TEMP:93@H' '#TEMP:94@N' '#TEMP:94@H' '#TEMP:95@N' '#TEMP:95@H' '#TEMP:96@N' '#TEMP:96@H' '#TEMP:97@N' '#TEMP:97@H' '#TEMP:98@N' '#TEMP:98@H' '#TEMP:99@N' '#TEMP:99@H' '#TEMP:100@N' '#TEMP:100@H' '#TEMP:101@N' '#TEMP:101@H' '#TEMP:102@N' '#TEMP:102@H' '#TEMP:103@N' '#TEMP:103@H' '#TEMP:104@N' '#TEMP:104@H' '#TEMP:105@N' '#TEMP:105@H' '#TEMP:106@N' '#TEMP:106@H' '#TEMP:107@N' '#TEMP:107@H' '#TEMP:108@N' '#TEMP:108@H' '#TEMP:109@N' '#TEMP:109@H' '#TEMP:110@N' '#TEMP:110@H' '#TEMP:111@N' '#TEMP:111@H' '#TEMP:112@N' '#TEMP:112@H' '#TEMP:113@N' '#TEMP:113@H' '#TEMP:114@N' '#TEMP:114@H' '#TEMP:115@N' '#TEMP:115@H' '#TEMP:116@N' '#TEMP:116@H' '#TEMP:117@N' '#TEMP:117@H' '#TEMP:118@N' '#TEMP:118@H' '#TEMP:119@N' '#TEMP:119@H' '#TEMP:120@N' '#TEMP:120@H' '#TEMP:121@N' '#TEMP:121@H' '#TEMP:122@N' '#TEMP:122@H' '#TEMP:123@N' '#TEMP:123@H' '#TEMP:124@N' '#TEMP:124@H' '#TEMP:125@N' '#TEMP:125@H' '#TEMP:127@N' '#TEMP:127@H' '#TEMP:128@N' '#TEMP:128@H' '#TEMP:129@N' '#TEMP:129@H' '#TEMP:130@N' '#TEMP:130@H' '#TEMP:131@N' '#TEMP:131@H' '#TEMP:132@N' '#TEMP:132@H' '#TEMP:133@N' '#TEMP:133@H' '#TEMP:134@N' '#TEMP:134@H' '#TEMP:136@N' '#TEMP:136@H' '#TEMP:138@N' '#TEMP:138@H' '#TEMP:139@N' '#TEMP:139@H' '#TEMP:140@N' '#TEMP:140@H' '#TEMP:141@N' '#TEMP:141@H' '#TEMP:142@N' '#TEMP:142@H' '#TEMP:143@N' '#TEMP:143@H' '#TEMP:144@N' '#TEMP:144@H' '#TEMP:145@N' '#TEMP:145@H' '#TEMP:146@N' '#TEMP:146@H' '#TEMP:147@N' '#TEMP:147@H' '#TEMP:148@N' '#TEMP:148@H' '#TEMP:149@N' '#TEMP:149@H' '#TEMP:150@N' '#TEMP:150@H' '#TEMP:151@N' '#TEMP:151@H' '#TEMP:152@N' '#TEMP:152@H' '#TEMP:153@N' '#TEMP:153@H' '#TEMP:154@N' '#TEMP:154@H' '#TEMP:155@N' '#TEMP:155@H' '#TEMP:156@N' '#TEMP:156@H' '#TEMP:157@N' '#TEMP:157@H' '#TEMP:158@N' '#TEMP:158@H' '#TEMP:159@N' '#TEMP:159@H' relax> interatom.define(spin_id1='@NE1', spin_id2='@HE1', direct_bond=True, spin_selection=True, pipe=None)Interatomic interactions are now defined for the following spins: # Spin_ID_1 Spin_ID_2 '#TEMP:33@NE1' '#TEMP:33@HE1' '#TEMP:48@NE1' '#TEMP:48@HE1' '#TEMP:49@NE1' '#TEMP:49@HE1' '#TEMP:59@NE1' '#TEMP:59@HE1' '#TEMP:98@NE1' '#TEMP:98@HE1' relax> interatom.set_dist(spin_id1='@N*', spin_id2='@H*', ave_dist=1.0200000000000001e-10, unit='meter')The following averaged distances have been set: # Spin_ID_1 Spin_ID_2 Ave_distance(meters) '#TEMP:3@N' '#TEMP:3@H' 1.0200000000000001e-10 '#TEMP:4@N' '#TEMP:4@H' 1.0200000000000001e-10 '#TEMP:5@N' '#TEMP:5@H' 1.0200000000000001e-10 '#TEMP:6@N' '#TEMP:6@H' 1.0200000000000001e-10 '#TEMP:7@N' '#TEMP:7@H' 1.0200000000000001e-10 '#TEMP:8@N' '#TEMP:8@H' 1.0200000000000001e-10 '#TEMP:9@N' '#TEMP:9@H' 1.0200000000000001e-10 '#TEMP:10@N' '#TEMP:10@H' 1.0200000000000001e-10 '#TEMP:11@N' '#TEMP:11@H' 1.0200000000000001e-10 '#TEMP:13@N' '#TEMP:13@H' 1.0200000000000001e-10 '#TEMP:14@N' '#TEMP:14@H' 1.0200000000000001e-10 '#TEMP:15@N' '#TEMP:15@H' 1.0200000000000001e-10 '#TEMP:16@N' '#TEMP:16@H' 1.0200000000000001e-10 '#TEMP:17@N' '#TEMP:17@H' 1.0200000000000001e-10 '#TEMP:18@N' '#TEMP:18@H' 1.0200000000000001e-10 '#TEMP:19@N' '#TEMP:19@H' 1.0200000000000001e-10 '#TEMP:20@N' '#TEMP:20@H' 1.0200000000000001e-10 '#TEMP:21@N' '#TEMP:21@H' 1.0200000000000001e-10 '#TEMP:22@N' '#TEMP:22@H' 1.0200000000000001e-10 '#TEMP:23@N' '#TEMP:23@H' 1.0200000000000001e-10 '#TEMP:24@N' '#TEMP:24@H' 1.0200000000000001e-10 '#TEMP:25@N' '#TEMP:25@H' 1.0200000000000001e-10 '#TEMP:26@N' '#TEMP:26@H' 1.0200000000000001e-10 '#TEMP:27@N' '#TEMP:27@H' 1.0200000000000001e-10 '#TEMP:28@N' '#TEMP:28@H' 1.0200000000000001e-10 '#TEMP:29@N' '#TEMP:29@H' 1.0200000000000001e-10 '#TEMP:30@N' '#TEMP:30@H' 1.0200000000000001e-10 '#TEMP:31@N' '#TEMP:31@H' 1.0200000000000001e-10 '#TEMP:32@N' '#TEMP:32@H' 1.0200000000000001e-10 '#TEMP:33@N' '#TEMP:33@H' 1.0200000000000001e-10 '#TEMP:34@N' '#TEMP:34@H' 1.0200000000000001e-10 '#TEMP:35@N' '#TEMP:35@H' 1.0200000000000001e-10 '#TEMP:36@N' '#TEMP:36@H' 1.0200000000000001e-10 '#TEMP:37@N' '#TEMP:37@H' 1.0200000000000001e-10 '#TEMP:38@N' '#TEMP:38@H' 1.0200000000000001e-10 '#TEMP:39@N' '#TEMP:39@H' 1.0200000000000001e-10 '#TEMP:40@N' '#TEMP:40@H' 1.0200000000000001e-10 '#TEMP:41@N' '#TEMP:41@H' 1.0200000000000001e-10 '#TEMP:42@N' '#TEMP:42@H' 1.0200000000000001e-10 '#TEMP:43@N' '#TEMP:43@H' 1.0200000000000001e-10 '#TEMP:45@N' '#TEMP:45@H' 1.0200000000000001e-10 '#TEMP:46@N' '#TEMP:46@H' 1.0200000000000001e-10 '#TEMP:47@N' '#TEMP:47@H' 1.0200000000000001e-10 '#TEMP:48@N' '#TEMP:48@H' 1.0200000000000001e-10 '#TEMP:49@N' '#TEMP:49@H' 1.0200000000000001e-10 '#TEMP:50@N' '#TEMP:50@H' 1.0200000000000001e-10 '#TEMP:51@N' '#TEMP:51@H' 1.0200000000000001e-10 '#TEMP:52@N' '#TEMP:52@H' 1.0200000000000001e-10 '#TEMP:53@N' '#TEMP:53@H' 1.0200000000000001e-10 '#TEMP:54@N' '#TEMP:54@H' 1.0200000000000001e-10 '#TEMP:55@N' '#TEMP:55@H' 1.0200000000000001e-10 '#TEMP:56@N' '#TEMP:56@H' 1.0200000000000001e-10 '#TEMP:57@N' '#TEMP:57@H' 1.0200000000000001e-10 '#TEMP:58@N' '#TEMP:58@H' 1.0200000000000001e-10 '#TEMP:59@N' '#TEMP:59@H' 1.0200000000000001e-10 '#TEMP:60@N' '#TEMP:60@H' 1.0200000000000001e-10 '#TEMP:61@N' '#TEMP:61@H' 1.0200000000000001e-10 '#TEMP:62@N' '#TEMP:62@H' 1.0200000000000001e-10 '#TEMP:63@N' '#TEMP:63@H' 1.0200000000000001e-10 '#TEMP:64@N' '#TEMP:64@H' 1.0200000000000001e-10 '#TEMP:65@N' '#TEMP:65@H' 1.0200000000000001e-10 '#TEMP:66@N' '#TEMP:66@H' 1.0200000000000001e-10 '#TEMP:67@N' '#TEMP:67@H' 1.0200000000000001e-10 '#TEMP:68@N' '#TEMP:68@H' 1.0200000000000001e-10 '#TEMP:69@N' '#TEMP:69@H' 1.0200000000000001e-10 '#TEMP:70@N' '#TEMP:70@H' 1.0200000000000001e-10 '#TEMP:71@N' '#TEMP:71@H' 1.0200000000000001e-10 '#TEMP:72@N' '#TEMP:72@H' 1.0200000000000001e-10 '#TEMP:73@N' '#TEMP:73@H' 1.0200000000000001e-10 '#TEMP:74@N' '#TEMP:74@H' 1.0200000000000001e-10 '#TEMP:75@N' '#TEMP:75@H' 1.0200000000000001e-10 '#TEMP:76@N' '#TEMP:76@H' 1.0200000000000001e-10 '#TEMP:77@N' '#TEMP:77@H' 1.0200000000000001e-10 '#TEMP:78@N' '#TEMP:78@H' 1.0200000000000001e-10 '#TEMP:79@N' '#TEMP:79@H' 1.0200000000000001e-10 '#TEMP:80@N' '#TEMP:80@H' 1.0200000000000001e-10 '#TEMP:81@N' '#TEMP:81@H' 1.0200000000000001e-10 '#TEMP:82@N' '#TEMP:82@H' 1.0200000000000001e-10 '#TEMP:83@N' '#TEMP:83@H' 1.0200000000000001e-10 '#TEMP:84@N' '#TEMP:84@H' 1.0200000000000001e-10 '#TEMP:85@N' '#TEMP:85@H' 1.0200000000000001e-10 '#TEMP:87@N' '#TEMP:87@H' 1.0200000000000001e-10 '#TEMP:88@N' '#TEMP:88@H' 1.0200000000000001e-10 '#TEMP:89@N' '#TEMP:89@H' 1.0200000000000001e-10 '#TEMP:90@N' '#TEMP:90@H' 1.0200000000000001e-10 '#TEMP:91@N' '#TEMP:91@H' 1.0200000000000001e-10 '#TEMP:93@N' '#TEMP:93@H' 1.0200000000000001e-10 '#TEMP:94@N' '#TEMP:94@H' 1.0200000000000001e-10 '#TEMP:95@N' '#TEMP:95@H' 1.0200000000000001e-10 '#TEMP:96@N' '#TEMP:96@H' 1.0200000000000001e-10 '#TEMP:97@N' '#TEMP:97@H' 1.0200000000000001e-10 '#TEMP:98@N' '#TEMP:98@H' 1.0200000000000001e-10 '#TEMP:99@N' '#TEMP:99@H' 1.0200000000000001e-10 '#TEMP:100@N' '#TEMP:100@H' 1.0200000000000001e-10 '#TEMP:101@N' '#TEMP:101@H' 1.0200000000000001e-10 '#TEMP:102@N' '#TEMP:102@H' 1.0200000000000001e-10 '#TEMP:103@N' '#TEMP:103@H' 1.0200000000000001e-10 '#TEMP:104@N' '#TEMP:104@H' 1.0200000000000001e-10 '#TEMP:105@N' '#TEMP:105@H' 1.0200000000000001e-10 '#TEMP:106@N' '#TEMP:106@H' 1.0200000000000001e-10 '#TEMP:107@N' '#TEMP:107@H' 1.0200000000000001e-10 '#TEMP:108@N' '#TEMP:108@H' 1.0200000000000001e-10 '#TEMP:109@N' '#TEMP:109@H' 1.0200000000000001e-10 '#TEMP:110@N' '#TEMP:110@H' 1.0200000000000001e-10 '#TEMP:111@N' '#TEMP:111@H' 1.0200000000000001e-10 '#TEMP:112@N' '#TEMP:112@H' 1.0200000000000001e-10 '#TEMP:113@N' '#TEMP:113@H' 1.0200000000000001e-10 '#TEMP:114@N' '#TEMP:114@H' 1.0200000000000001e-10 '#TEMP:115@N' '#TEMP:115@H' 1.0200000000000001e-10 '#TEMP:116@N' '#TEMP:116@H' 1.0200000000000001e-10 '#TEMP:117@N' '#TEMP:117@H' 1.0200000000000001e-10 '#TEMP:118@N' '#TEMP:118@H' 1.0200000000000001e-10 '#TEMP:119@N' '#TEMP:119@H' 1.0200000000000001e-10 '#TEMP:120@N' '#TEMP:120@H' 1.0200000000000001e-10 '#TEMP:121@N' '#TEMP:121@H' 1.0200000000000001e-10 '#TEMP:122@N' '#TEMP:122@H' 1.0200000000000001e-10 '#TEMP:123@N' '#TEMP:123@H' 1.0200000000000001e-10 '#TEMP:124@N' '#TEMP:124@H' 1.0200000000000001e-10 '#TEMP:125@N' '#TEMP:125@H' 1.0200000000000001e-10 '#TEMP:127@N' '#TEMP:127@H' 1.0200000000000001e-10 '#TEMP:128@N' '#TEMP:128@H' 1.0200000000000001e-10 '#TEMP:129@N' '#TEMP:129@H' 1.0200000000000001e-10 '#TEMP:130@N' '#TEMP:130@H' 1.0200000000000001e-10 '#TEMP:131@N' '#TEMP:131@H' 1.0200000000000001e-10 '#TEMP:132@N' '#TEMP:132@H' 1.0200000000000001e-10 '#TEMP:133@N' '#TEMP:133@H' 1.0200000000000001e-10 '#TEMP:134@N' '#TEMP:134@H' 1.0200000000000001e-10 '#TEMP:136@N' '#TEMP:136@H' 1.0200000000000001e-10 '#TEMP:138@N' '#TEMP:138@H' 1.0200000000000001e-10 '#TEMP:139@N' '#TEMP:139@H' 1.0200000000000001e-10 '#TEMP:140@N' '#TEMP:140@H' 1.0200000000000001e-10 '#TEMP:141@N' '#TEMP:141@H' 1.0200000000000001e-10 '#TEMP:142@N' '#TEMP:142@H' 1.0200000000000001e-10 '#TEMP:143@N' '#TEMP:143@H' 1.0200000000000001e-10 '#TEMP:144@N' '#TEMP:144@H' 1.0200000000000001etmux new -10 '#TEMP:145@N' '#TEMP:145@H' 1.0200000000000001e-10 '#TEMP:146@N' '#TEMP:146@H' 1.0200000000000001e-10 '#TEMP:147@N' '#TEMP:147@H' 1.0200000000000001e-10 '#TEMP:148@N' '#TEMP:148@H' 1.0200000000000001e-10 '#TEMP:149@N' '#TEMP:149@H' 1.0200000000000001e-10 '#TEMP:150@N' '#TEMP:150@H' 1.0200000000000001e-10 '#TEMP:151@N' '#TEMP:151@H' 1.0200000000000001e-10 '#TEMP:152@N' '#TEMP:152@H' 1.0200000000000001e-10 '#TEMP:153@N' '#TEMP:153@H' 1.0200000000000001e-10 '#TEMP:154@N' '#TEMP:154@H' 1.0200000000000001e-10 '#TEMP:155@N' '#TEMP:155@H' 1.0200000000000001e-10 '#TEMP:156@N' '#TEMP:156@H' 1.0200000000000001e-10 '#TEMP:157@N' '#TEMP:157@H' 1.0200000000000001e-10 '#TEMP:158@N' '#TEMP:158@H' 1.0200000000000001e-10 '#TEMP:159@N' '#TEMP:159@H' 1.0200000000000001e-10 '#TEMP:33@NE1' '#TEMP:33@HE1' 1.0200000000000001e-10 '#TEMP:48@NE1' '#TEMP:48@HE1' 1.0200000000000001e-10 '#TEMP:49@NE1' '#TEMP:49@HE1' 1.0200000000000001e-10 '#TEMP:59@NE1' '#TEMP:59@HE1' 1.0200000000000001e-10 '#TEMP:98@NE1' '#TEMP:98@HE1' 1.0200000000000001e-10 s m3relax> interatom13_Model_3_III_prolate.unit_vectors(ave=True)Averaging all vectors.Calculated 1 Npy -H unit vector between the spins '#TEMP:3@N' and '#TEMP:3@H't 13_Model_3_III_prolate.logCalculated 1 N-H unit vector between the spins '#TEMP:4@N' and '#TEMP:4@H'.OrCalculated 1 Nmpirun -H unit vector between the spins '#TEMP:np 5@N' and '#TEMP:5@H'.Calculated 1 Nrelax -H unit vector between the spins '#TEMP:6@N' and '#TEMP:6@H'.Calculated 1 N-H unit vector between the spins '#TEMP:7@N' and '#TEMP:7@H'.Calculated 1 N-H unit vector between the spins '#TEMP:8@N' and '#TEMP:8@H'.Calculated 1 N-H unit vector between the spins '#TEMP:9@N' and '#TEMP:9@H'.Calculated 1 N-H unit vector between the spins '#TEMP:10@Nmulti=' and '#TEMP:10@Hmpi4py'13_Model_3_III_prolate.Calculated 1 Npy -H unit vector between the spins '#TEMP:11@N' and '#TEMP:11@H't 13_Model_3_III_prolate.Calculated 1 N-H unit vector between the spins '#TEMP:13@N' and '#TEMP:13@H'.Calculated 1 N-H unit vector between the spins '#TEMP:14@N' and '#TEMP:14@H'.Calculated 1 N-H unit vector between the spins '#TEMP:15@N' and '#TEMP:15@H'.Calculated 1 N-H unit vector between the spins '#TEMP:16@N' and '#TEMP:16@H'.Calculated 1 N-H unit vector between the spins '#TEMP:17@N' and '#TEMP:17@H'.Calculated 1 N-H unit vector between the spins '#TEMP:18@N' and '#TEMP:18@H'.Calculated 1 N-H unit vector between the spins '#TEMP:19@N' and '#TEMP:19@H'.Calculated 1 N-H unit vector between the spins '#TEMP:20@N' and '#TEMP:20@H'.Calculated 1 N-H unit vector between the spins '#TEMP:21@N' and '#TEMP:21@H'.Calculated 1 N-H unit vector between the spins '#TEMP:22@N' and '#TEMP:22@H'.Calculated 1 N-H unit vector between the spins '#TEMP:23@N' and '#TEMP:23@H'.Calculated 1 N-H unit vector between the spins '#TEMP:24@N' and '#TEMP:24@H'.Calculated 1 N-H unit vector between the spins '#TEMP:25@N' and '#TEMP:25@H'.Calculated 1 N-H unit vector between the spins '#TEMP:26@N' and '#TEMP:26@H'.Calculated 1 N-H unit vector between the spins '#TEMP:27@N' and '#TEMP:27@H'.Calculated 1 N-H unit vector between the spins '#TEMP:28@N' and '#TEMP:28@H'.Calculated 1 N-H unit vector between the spins '#TEMP:29@N' and '#TEMP:29@H'.Calculated 1 N-H unit vector between the spins '#TEMP:30@N' and '#TEMP:30@H'.Calculated 1 N-H unit vector between the spins '#TEMP:31@N' and '#TEMP:31@H'.Calculated 1 N-H unit vector between the spins '#TEMP:32@N' and '#TEMP:32@H'.Calculated 1 N-H unit vector between the spins '#TEMP:33@N' and '#TEMP:33@H'.Calculated 1 N-H unit vector between the spins '#TEMP:34@N' and '#TEMP:34@H'.Calculated 1 N-H unit vector between the spins '#TEMP:35@N' and '#TEMP:35@H'.Calculated 1 N-H unit vector between the spins '#TEMP:36@N' and '#TEMP:36@H'.Calculated 1 N-H unit vector between the spins '#TEMP:37@N' and '#TEMP:37@H'.Calculated 1 N-H unit vector between the spins '#TEMP:38@N' and '#TEMP:38@H'.Calculated 1 N-H unit vector between the spins '#TEMP:39@N' and '#TEMP:39@H'.Calculated 1 N-H unit vector between the spins '#TEMP:40@N' and '#TEMP:40@H'.Calculated 1 N-H unit vector between the spins '#TEMP:41@N' and '#TEMP:41@H'.Calculated 1 N-H unit vector between the spins '#TEMP:42@N' and '#TEMP:42@H'.Calculated 1 N-H unit vector between the spins '#TEMP:43@N' and '#TEMP:43@H'.Calculated 1 N-H unit vector between the spins '#TEMP:45@N' and '#TEMP:45@H'.Calculated 1 N-H unit vector between the spins '#TEMP:46@N' and '#TEMP:46@H'.Calculated 1 N-H unit vector between the spins '#TEMP:47@N' and '#TEMP:47@H'.Calculated 1 N-H unit vector between the spins '#TEMP:48@N' and '#TEMP:48@H'.Calculated 1 N-H unit vector between the spins '#TEMP:49@N' and '#TEMP:49@H'.Calculated 1 N-H unit vector between the spins '#TEMP:50@N' and '#TEMP:50@H'.Calculated 1 N-H unit vector between the spins '#TEMP:51@N' and '#TEMP:51@H'.Calculated 1 N-H unit vector between the spins '#TEMP:52@N' and '#TEMP:52@H'.Calculated 1 N-H unit vector between the spins '#TEMP:53@N' and '#TEMP:53@H'.Calculated 1 N-H unit vector between the spins '#TEMP:54@N' and '#TEMP:54@H'.Calculated 1 N-H unit vector between the spins '#TEMP:55@N' and '#TEMP:55@H'.Calculated 1 N-H unit vector between the spins '#TEMP:56@N' and '#TEMP:56@H'.Calculated 1 N-H unit vector between the spins '#TEMP:57@N' and '#TEMP:57@H'.Calculated 1 N-H unit vector between the spins '#TEMP:58@N' and '#TEMP:58@H'.Calculated 1 N-H unit vector between the spins '#TEMP:59@N' and '#TEMP:59@H'.Calculated 1 N-H unit vector between the spins '#TEMP:60@N' and '#TEMP:60@H'.Calculated 1 N-H unit vector between the spins '#TEMP:61@N' and '#TEMP:61@H'.Calculated 1 N-H unit vector between the spins '#TEMP:62@N' and '#TEMP:62@H'.Calculated 1 N-H unit vector between the spins '#TEMP:63@N' and '#TEMP:63@H'.Calculated 1 N-H unit vector between the spins '#TEMP:64@N' and '#TEMP:64@H'.Calculated 1 N-H unit vector between the spins '#TEMP:65@N' and '#TEMP:65@H'.Calculated 1 N-H unit vector between the spins '#TEMP:66@N' and '#TEMP:66@H'.Calculated 1 N-H unit vector between the spins '#TEMP:67@N' and '#TEMP:67@H'.Calculated 1 N-H unit vector between the spins '#TEMP:68@N' and '#TEMP:68@H'.Calculated 1 N-H unit vector between the spins '#TEMP:69@N' and '#TEMP:69@H'.Calculated 1 N-H unit vector between the spins '#TEMP:70@N' and '#TEMP:70@H'.Calculated 1 N-H unit vector between the spins '#TEMP:71@N' and '#TEMP:71@H'.Calculated 1 N-H unit vector between the spins '#TEMP:72@N' and '#TEMP:72@H'.Calculated 1 N-H unit vector between the spins '#TEMP:73@N' and '#TEMP:73@H'.Calculated 1 N-H unit vector between the spins '#TEMP:74@N' and '#TEMP:74@H'.Calculated 1 N-H unit vector between the spins '#TEMP:75@N' and '#TEMP:75@H'.Calculated 1 N-H unit vector between the spins '#TEMP:76@N' and '#TEMP:76@H'.Calculated 1 N-H unit vector between the spins '#TEMP:77@N' and '#TEMP:77@H'.Calculated 1 N-H unit vector between the spins '#TEMP:78@N' and '#TEMP:78@H'.Calculated 1 N-H unit vector between the spins '#TEMP:79@N' and '#TEMP:79@H'.Calculated 1 N-H unit vector between the spins '#TEMP:80@N' and '#TEMP:80@H'.Calculated 1 N-H unit vector between the spins '#TEMP:81@N' and '#TEMP:81@H'.Calculated 1 N-H unit vector between the spins '#TEMP:82@N' and '#TEMP:82@H'.Calculated 1 N-H unit vector between the spins '#TEMP:83@N' and '#TEMP:83@H'.Calculated 1 N-H unit vector between the spins '#TEMP:84@N' and '#TEMP:84@H'.Calculated 1 N-H unit vector between the spins '#TEMP:85@N' and '#TEMP:85@H'.Calculated 1 N-H unit vector between the spins '#TEMP:87@N' and '#TEMP:87@H'.Calculated 1 N-H unit vector between the spins '#TEMP:88@N' and '#TEMP:88@H'.Calculated 1 N-H unit vector between the spins '#TEMP:89@N' and '#TEMP:89@H'.Calculated 1 N-H unit vector between the spins '#TEMP:90@N' and '#TEMP:90@H'.Calculated 1 N-H unit vector between the spins '#TEMP:91@N' and '#TEMP:91@H'.Calculated 1 N-H unit vector between the spins '#TEMP:93@N' and '#TEMP:93@H'.Calculated 1 N-H unit vector between the spins '#TEMP:94@N' and '#TEMP:94@H'.Calculated 1 N-H unit vector between the spins '#TEMP:95@N' and '#TEMP:95@H'.Calculated 1 N-H unit vector between the spins '#TEMP:96@N' and '#TEMP:96@H'.Calculated 1 N-H unit vector between the spins '#TEMP:97@N' and '#TEMP:97@H'.Calculated 1 N-H unit vector between the spins '#TEMP:98@N' and '#TEMP:98@H'.Calculated 1 N-H unit vector between the spins '#TEMP:99@N' and '#TEMP:99@H'.Calculated 1 N-H unit vector between the spins '#TEMP:100@N' and '#TEMP:100@H'.Calculated 1 N-H unit vector between the spins '#TEMP:101@N' and '#TEMP:101@H'.Calculated 1 N-H unit vector between the spins '#TEMP:102@N' and '#TEMP:102@H'.Calculated 1 N-H unit vector between the spins '#TEMP:103@N' and '#TEMP:103@H'.Calculated 1 N-H unit vector between the spins '#TEMP:104@N' and '#TEMP:104@H'.Calculated 1 N-H unit vector between the spins '#TEMP:105@N' and '#TEMP:105@H'.Calculated 1 N-H unit vector between the spins '#TEMP:106@N' and '#TEMP:106@H'.Calculated 1 N-H unit vector between the spins '#TEMP:107@N' and '#TEMP:107@H'.Calculated 1 N-H unit vector between the spins '#TEMP:108@N' and '#TEMP:108@H'.Calculated 1 N-H unit vector between the spins '#TEMP:109@N' and '#TEMP:109@H'.Calculated 1 N-H unit vector between the spins '#TEMP:110@N' and '#TEMP:110@H'.Calculated 1 N-H unit vector between the spins '#TEMP:111@N' and '#TEMP:111@H'.Calculated 1 N-H unit vector between the spins '#TEMP:112@N' and '#TEMP:112@H'.Calculated 1 N-H unit vector between the spins '#TEMP:113@N' and '#TEMP:113@H'.Calculated 1 N-H unit vector between the spins '#TEMP:114@N' and '#TEMP:114@H'.Calculated 1 N-H unit vector between the spins '#TEMP:115@N' and '#TEMP:115@H'.Calculated 1 N-H unit vector between the spins '#TEMP:116@N' and '#TEMP:116@H'.Calculated 1 N-H unit vector between the spins '#TEMP:117@N' and '#TEMP:117@H'.Calculated 1 N-H unit vector between the spins '#TEMP:118@N' and '#TEMP:118@H'.Calculated 1 N-H unit vector between the spins '#TEMP:119@N' and '#TEMP:119@H'.Calculated 1 N-H unit vector between the spins '#TEMP:120@N' and '#TEMP:120@H'.Calculated 1 N-H unit vector between the spins '#TEMP:121@N' and '#TEMP:121@H'.Calculated 1 N-H unit vector between the spins '#TEMP:122@N' and '#TEMP:122@H'.Calculated 1 N-H unit vector between the spins '#TEMP:123@N' and '#TEMP:123@H'.Calculated 1 N-H unit vector between the spins '#TEMP:124@N' and '#TEMP:124@H'.Calculated 1 N-H unit vector between the spins '#TEMP:125@N' and '#TEMP:125@H'.Calculated 1 N-H unit vector between the spins '#TEMP:127@N' and '#TEMP:127@H'.Calculated 1 N-H unit vector between the spins '#TEMP:128@N' and '#TEMP:128@H'.Calculated 1 N-H unit vector between the spins '#TEMP:129@N' and '#TEMP:129@H'.Calculated 1 N-H unit vector between the spins '#TEMP:130@N' and '#TEMP:130@H'.Calculated 1 N-H unit vector between the spins '#TEMP:131@N' and '#TEMP:131@H'.Calculated 1 N-H unit vector between the spins '#TEMP:132@N' and '#TEMP:132@H'.Calculated 1 N-H unit vector between the spins '#TEMP:133@N' and '#TEMP:133@H'.Calculated 1 N-H unit vector between the spins '#TEMP:134@N' and '#TEMP:134@H'.Calculated 1 N-H unit vector between the spins '#TEMP:136@N' and '#TEMP:136@H'.Calculated 1 N-H unit vector between the spins '#TEMP:138@N' and '#TEMP:138@H'.Calculated 1 N-H unit vector between the spins '#TEMP:139@N' and '#TEMP:139@H'.Calculated 1 N-H unit vector between the spins '#TEMP:140@N' and '#TEMP:140@H'.Calculated 1 N-H unit vector between the spins '#TEMP:141@N' and '#TEMP:141@H'.Calculated 1 N-H unit vector between the spins '#TEMP:142@N' and '#TEMP:142@H'.Calculated 1 N-H unit vector between the spins '#TEMP:143@N' and '#TEMP:143@H'.Calculated 1 N-H unit vector between the spins '#TEMP:144@N' and '#TEMP:144@H'.Calculated 1 N-H unit vector between the spins '#TEMP:145@N' and '#TEMP:145@H'.Calculated 1 N-H unit vector between the spins '#TEMP:146@N' and '#TEMP:146@H'.Calculated 1 N-H unit vector between the spins '#TEMP:147@N' and '#TEMP:147@H'.Calculated 1 N-H unit vector between the spins '#TEMP:148@N' and '#TEMP:148@H'.Calculated 1 N-H unit vector between the spins '#TEMP:149@N' and '#TEMP:149@H'.Calculated 1 N-H unit vector between the spins '#TEMP:150@N' and '#TEMP:150@H'.Calculated 1 N-H unit vector between the spins '#TEMP:151@N' and '#TEMP:151@H'.Calculated 1 N-H unit vector between the spins '#TEMP:152@N' and '#TEMP:152@H'.Calculated 1 N-H unit vector between the spins '#TEMP:153@N' and '#TEMP:153@H'.Calculated 1 N-H unit vector between the spins '#TEMP:154@N' and '#TEMP:154@H'.Calculated 1 N-H unit vector between the spins '#TEMP:155@N' and '#TEMP:155@H'.Calculated 1 N-H unit vector between the spins '#TEMP:156@N' and '#TEMP:156@H'.Calculated 1 N-H unit vector between the spins '#TEMP:157@N' and '#TEMP:157@H'.Calculated 1 N-H unit vector between the spins '#TEMP:158@N' and '#TEMP:158@H'.Calculated 1 N-H unit vector between the spins '#TEMP:159@N' and '#TEMP:159@H'.Calculated 1 NE1-HE1 unit vector between the spins '#TEMP:33@NE1' and '#TEMP:33@HE1'.Calculated 1 NE1-HE1 unit vector between the spins '#TEMP:48@NE1' and '#TEMP:48@HE1'.Calculated 1 NE1-HE1 unit vector between the spins '#TEMP:49@NE1' and '#TEMP:49@HE1'.Calculated 1 NE1-HE1 unit vector between the spins '#TEMP:59@NE1' and '#TEMP:59@HE1'.Calculated 1 NE1-HE1 unit vector between the spins '#TEMP:98@NE1' and '#TEMP:98@HE1'. relax> value.set(val=-0.00017199999999999998, param='csa', index=0, spin_id='@N*', error=False, force=True)log
</source>
|}
=== Inspect data in GUI ===The GUI can be a good place to inspect the setup and files[https://github. Copy '''02_read_datacom/tlinnet/relax_modelfree_scripts/blob/master/13_Model_4_IV_oblate.py''' to '''03_save_state_inspect_GUI13_Model_4_IV_oblate.py''' and add:]<source lang="pythonbash"># Analysis variables.###################### The modeltmux new -free models. Do not change these unless absolutely necessary, the protocol is likely to fail if these are changed.MF_MODELS = ['m0', 'm1', 'm2', 'm3', 's m4', 'm5', 'm6', 'm7', 'm8', 'm9']#MF_MODELS = ['m1', 'm2']LOCAL_TM_MODELS = ['tm0', 'tm1', 'tm2', 'tm3', 'tm4', 'tm5', 'tm6', 'tm7', 'tm8', 'tm9'] # The grid search size (the number of increments per dimension)relax 13_Model_4_IV_oblate.GRID_INC = 11 # The optimisation techniquepy -t 13_Model_4_IV_oblate. Standard is: min_algor='newton' : and cannot be changed in the GUI.MIN_ALGOR = 'newton'log# The number of Monte Carlo simulations to be used for error analysis at the end of the analysis.Or#MC_NUM = 500MC_NUM = 20 # The diffusion model. Standard is 'Fully automated', which means: DIFF_MODEL=['local_tm', 'sphere', 'prolate', 'oblate', 'ellipsoid', 'final']# 'local_tm', 'sphere', ''prolate', 'oblate', 'ellipsoid', or 'final'#DIFF_MODEL = 'local_tm'DIFF_MODEL = ['local_tm', 'sphere', 'prolate', 'oblate', 'ellipsoid', 'final'] # The maximum number of iterations for the global iteration. Set to None, then the algorithm iterates until convergence.MAX_ITER = None # Automatic looping over all rounds until convergence (must be a boolean value of True or False). Standard is: conv_loop=True : and cannot be changed in the GUI.CONV_LOOP = True # Change some minimise opt params. # This goes into: minimise.execute(self.min_algor, func_tol=self.opt_func_tol, max_iter=self.opt_max_iterations)######################dAuvergne_protocol.opt_func_tol = 1empirun -np 5 # Standard: opt_func_tol = 1e-25 #dAuvergne_protocol.opt_max_iterations = 1000 # Standard: opt_max_iterations = int(1e7)dAuvergne_protocol.opt_func_tol = 1erelax -10 # Standard: opt_func_tol = 1e-25 dAuvergne_protocol.opt_max_iterations = int(1e5) # Standard: opt_max_iterations = int(1e7) ##################################### # The results dir.var multi= 'result_03mpi4py'results_dir = os13_Model_4_IV_oblate.getcwd() + os.sep + var # Save the state before running. Open and check in GUI!state.save(state=var+'_ini.bz2', dir=results_dir, force=True) # To check in GUI# relax -g# File py -> Open relax state# In folder "result_03" open "result_03_init 13_Model_4_IV_oblate.bz2"# View -> Data pipe editor# Right click on pipe, and select "Associate with a new auto-analysis"log
</source>
Run with[https://github.com/tlinnet/relax_modelfree_scripts/blob/master/13_Model_5_V_ellipsoid.py 13_Model_5_V_ellipsoid.py]
<source lang="bash">
tmux new -s m5relax 13_Model_5_V_ellipsoid.py -t 13_Model_5_V_ellipsoid.log# Ormpirun -np 5 relax 03_save_state_inspect_GUI--multi='mpi4py' 13_Model_5_V_ellipsoid.py -t 03_save_state_inspect_GUI13_Model_5_V_ellipsoid.log
</source>
To check in GUIjoin session* relax -g* File -> Open relax state* In folder <source lang="result_03" open "result_03_ini.bz2bash">* View -> Data pipe editor# List* Right click on pipe, and select "Associate with a new autotmux list-analysis"s
=== Try fast run ===# Join eitherNow we try tmux a fast run, to see if everything is setup-t m1tmux a -t m2tmux a -t m3tmux a -t m4tmux a -t m5</source>
Copy '''03_save_state_inspect_GUI== 14_intermediate_final.py''' to '''04_run_default_with_tolerance_lim- Inspection during model optimization ==During running of model 2-5, the current results can be inspected withthis nifty scripts.py''' and modify last lines:
<source lang="python"># The results dirscript will ask for input of MC numbers.var = 'result_04'results_dir = osSo just run it.getcwd() + os.sep + var
# Save the state before running[https://github. Open and check in GUI!com/tlinnet/relax_modelfree_scripts/blob/master/14_intermediate_final.py 14_intermediate_final.py]state<source lang="bash">tmux new -s finalrelax 14_intermediate_final.save(state=var+'_inipy -t 14_intermediate_final.bz2', dir=results_dir, force=True)log</source>
# To check in GUIThis does:# relax * Option: Collect current best result from Model 2-g5, and make MC simulations, and finalize to get current results files # File ** [http://comdnmr.nysbc.org/comd-> Open relax statenmr-dissem/comd-nmr-software Make analysis script for palmer Modelfree4]# In folder "result_03" open "result_03_ini.bz2"** Get more spin information# View -> Data pipe editor* Make a pymol file, that collects all of relax pymol command files into 1 pymol session# Right click on pipe* Option: Collect all chi2 and number of params k, and select "Associate with for each iteration per model** Make a new auto-analysis"python plot file for plotting this results
dAuvergne_protocol(pipe_name=name, pipe_bundle=bundle_name, results_dir=results_dir, diff_model=DIFF_MODELPer iteration get: chi2, mf_models=MF_MODELSk, local_tm_modelstm =LOCAL_TM_MODELS, grid_inc=GRID_INC, min_algor=MIN_ALGOR, mc_sim_num=MC_NUM, max_iter=MAX_ITERAfterwards, conv_loopplot the data.<source lang=CONV_LOOP)"bash">python results_collected.py
</source>
Before running, is worth to note, which values are NOT set to default values in the GUI.* dAuvergne_protocol.opt_func_tol = 1e-10 # Standard: opt_func_tol = 1e-25 * dAuvergne_protocol.opt_max_iterations = int(1e5) # Standard: opt_max_iterations Pymol macro === int(1e7) These 2 values is used in the '''minfx''' python package, and is an instruction to the minimiser function, to continue changing parameter values,UNTIL either the difference in chi2 values between "2 steps" is less than 1e-10, OR if the number all steps is larger than 10^5.It's an instruction not to be tooooo pedantic, here in the exploration phase. When finalising for publication, these valuesshould be set to their standard valueYou also get a pymol folder.
See here for info how the macro is applied* MC_NUM = 20Number of Monte[http://www.nmr-Carlo simulationsrelax. The protocol will find optimum com/manual/molmol_macro_apply.html#SECTION081284600000000000000 Summary of parameter values in this protocol, but errorestimation will not be very reliable. Standard is 500.meaning and value to pymol visualization]
Run with
<source lang="bash">
relax 04_run_default_with_tolerance_limpymol 0_0_apply_all_pymol_commands.py -t 04_run_default_with_tolerance_lim.log</source> You can then in another terminal follow the logfile by<source lang="bash">less +F 04_run_default_with_tolerance_lim.logpml
</source>
* To scroll up and down, use keyboard: '''Ctrl+c'''* To return to follow mode, use keyboard: '''Shift+f'''* To exit, use keyboard: '''Ctrl+c''' and then: '''q''' == To run on Haddock ==
Have a look here, how to get standalone python [[Anaconda_linux_mac|Anaconda linux]].
Also have a look here [[OpenMPI]].
</source>
= Useful commands to log file =
While the analysis is running, these commands could be used to check the logfile for errors
<source lang="bash">
### Check convergence
# For chi2
cat 04_run_default_with_tolerance_lim.log | grep -A 10 "Chi-squared test:"
# For other tests
cat 04_run_default_with_tolerance_lim.log | grep -A 10 "Identical "
cat 04_run_default_with_tolerance_lim.log | grep -A 10 "Identical model-free models test:"
cat 04_run_default_with_tolerance_lim.log | grep -A 10 "Identical diffusion tensor parameter test:"
cat 04_run_default_with_tolerance_lim.log | grep -A 10 "Identical model-free parameter test:"
# To look for not converged errors
# For chi2
cat 04_run_default_with_tolerance_lim.log | grep -B 7 "The chi-squared value has not converged."
# For other tests
cat 04_run_default_with_tolerance_lim.log | grep -B 7 " have not converged."
cat 04_run_default_with_tolerance_lim.log | grep -B 7 "The model-free models have not converged."
cat 04_run_default_with_tolerance_lim.log | grep -B 7 "The diffusion parameters have not converged."
cat 04_run_default_with_tolerance_lim.log | grep -B 7 "The model-free parameters have not converged."
</source>
You can then inspect the logfile by '''less''': [http://www.thegeekstuff.com/2010/02/unix-less-command-10-tips-for-effective-navigation 10-tips for less]
<source lang="bash">
less 04_run_default_with_tolerance_lim.log
</source>
'''To find pattern:''' We have to escape with '''\''' for special character like: ()[] etc.
<source lang="bash">
# Search forward
/Value \(iter 14\)
/The chi-squared value has not converged
</source>
'''n''' or '''N''' – for next match in forward / previous match in backward
* To return to follow mode, use keyboard: '''Shift+f'''
* To exit, use keyboard: '''Ctrl+c''' and then: '''q'''
= rsync files =
== rsync files after completion to Sauron ==
When a run is completed, then sync files to Sauron file server.
Make a '''rsync_to_sbinlab.sh''' file with content
{| class="mw-collapsible mw-collapsed wikitable"! See file content|-|
<source lang="bash">
#!/bin/bash
FROM=${PWD}
TO=${RUSER}@${SAURON}:/data/sbinlab2/${RUSER}/Downloads/${PROJ}
# -a: "archive" and - archive mode; equals -rlptgoD (no -H,-A,-X). syncs recursively and preserves symbolic links, special and device files, modification times, group, owner, and permissions.# We want to remove the -o and -g options:# -o, --owner preserve owner (super-user only)# -g, --group preserve group# -rlptD : Instead or# -a --no-o --no-g
# -z: Compression over network
# -P: It combines the flags --progress and --partial. The first of these gives you a progress bar for the transfers and the second allows you to resume interrupted transfers:
if [[ $REPLY =~ ^[Yy]$ ]]; then
rsync -aPzhn rlptDPzh -n ${FROM} ${TO}
else
echo "Not doing DRY RUN"
fi
echo ""
if [[ $REPLY =~ ^[Yy]$ ]]; then
rsync -aPzh rlptDPzh ${FROM} ${TO}
else
echo "Not doing anything"
./rsync_to_sbinlab2.sh
</source>
|}
== rsync files from BIO to home mac ==
To inspect from home mac.
Make a '''rsync_from_bio_to_home.sh''' file with content
{| class="mw-collapsible mw-collapsed wikitable"
! See file content
|-
|
<source lang="bash">
#!/bin/bash
read -p "Username on bio:" -r
RUSER=$REPLY
BIO=ssh-bio.science.ku.dk
#PROJ=Desktop/kaare_relax
PROJ=Desktop/kaare_relax/20171010_model_free_HADDOCK
PROJDIR=`basename "$PROJ"`
FROM=${RUSER}@${BIO}:/home/${RUSER}/${PROJ}
TO=${PWD}/${PROJDIR}
# -a: "archive"- archive mode; equals -rlptgoD (no -H,-A,-X). syncs recursively and preserves symbolic links, special and device files, modification times, group, owner, and permissions.
# We want to remove the -o and -g options:
# -o, --owner preserve owner (super-user only)
# -g, --group preserve group
# -rlptD : Instead or
# -a --no-o --no-g
# -z: Compression over network
# -P: It combines the flags --progress and --partial. The first of these gives you a progress bar for the transfers and the second allows you to resume interrupted transfers:
# -h, Output numbers in a more human-readable format.
# Always double-check your arguments before executing an rsync command.
# -n
echo "I will now do a DRY RUN, which does not move files"
read -p "Are you sure? y/n :" -n 1 -r
echo ""
if [[ $REPLY =~ ^[Yy]$ ]]; then
rsync -rlptDPzh -n ${FROM} ${TO}
else
echo "Not doing DRY RUN"
fi
echo ""
echo "I will now do the sync of files"
read -p "Are you sure? y/n :" -n 1 -r
echo ""
if [[ $REPLY =~ ^[Yy]$ ]]; then
rsync -rlptDPzh ${FROM} ${TO}
else
echo "Not doing anything"
fi
</source>
Make it executable and run
<source lang="bash">
chmod +x rsync_from_bio_to_home.sh
#run
./rsync_from_bio_to_home.sh
</source>
|}
= About the protocol =
'''Model I - 'local_tm''''<br>
This will optimise the diffusion model whereby all spin of the molecule have a local tm value, i.e. there is no global diffusion tensor. This model needs to be optimised prior to optimising any of the other diffusion models. Each spin is fitted to the multiple model-free models separately, where the parameter tm is included in each model.
'''Model II - 'sphere''''<br>
This will optimise the isotropic diffusion model. Multiple steps are required, an initial optimisation of the diffusion tensor, followed by a repetitive optimisation until convergence of the diffusion tensor. In the relax script UI each of these steps requires this script to be rerun, unless the conv_loop flag is True. In the GUI (graphical user interface), the procedure is repeated automatically until convergence. For the initial optimisation, which will be placed in the directory './sphere/init/', the following steps are used:
* The model-free models and parameter values for each spin are set to those of diffusion model MI.
* The local tm parameter is removed from the models.
* The model-free parameters are fixed and a global spherical diffusion tensor is minimised
* For the repetitive optimisation, each minimisation is named from 'round_1' onwards. The initial 'round_1' optimisation will extract the diffusion tensor from the results file in './sphere/init/', and the results will be placed in the directory './sphere/round_1/'. Each successive round will take the diffusion tensor from the previous round. The following steps are used:
** The global diffusion tensor is fixed and the multiple model-free models are fitted to each spin.
** AIC model selection is used to select the models for each spin.
** All model-free and diffusion parameters are allowed to vary and a global optimisation of all parameters is carried out.
'''Model III - 'prolate''''<br>
The methods used are identical to those of diffusion model MII, except that an axially symmetric diffusion tensor with Da >= 0 is used. The base directory containing all the results is './prolate/'.
'''Model IV -'oblate''''<br>
The methods used are identical to those of diffusion model MII, except that an axially symmetric diffusion tensor with Da <= 0 is used. The base directory containing all the results is './oblate/'.
'''Model V - 'ellipsoid''''<br>
The methods used are identical to those of diffusion model MII, except that a fully anisotropic diffusion tensor is used (also known as rhombic or asymmetric diffusion). The base directory is './ellipsoid/'
''''final''''<br>
Once all the diffusion models have converged, the final run can be executed. This is done by setting the variable diff_model to 'final'. This consists of two steps, diffusion tensor model selection, and Monte Carlo simulations. Firstly AIC model selection is used to select between the diffusion tensor models. Monte Carlo simulations are then run solely on this selected diffusion model. Minimisation of the model is bypassed as it is assumed that the model is already fully optimised (if this is not the case the final run is not yet appropriate).
The final black-box model-free results will be placed in the file 'final/results'.
== See also ==
[[Category:Tutorials]]
[[Category:Model-free_analysis]]