Scripts

As this page is getting crowded, we created another page to explain all the scripts we wrote. The current page has some kind of step by step tutorials, but if you want fast informations, you better go to the script page.

Examples

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

Maxwell-Boltzmann Energy Distribution

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Here we will confirm that the kinetic energy distribution of the atoms in a system corresponds to the Maxwell distribution for a given temperature.

1. In VMD, load the .psf file. Browse for the restart velocity file (in our case, it was 2v0w_hydr_wb_i_eq.restart.vel), the type of file need this time to be selected. In the Determine file type: pull-down menu, choose NAMD Binary Coordinates, and load again.
The molecule looks terrible! That is because VMD is reading the velocities as if they were coordinates, but how it looks doesn't matter: we just need VMD to make a file containing the masses and velocities for every atom.

2. We create a selection with all the atoms in the system, by typing in the TkCon window:
      set all [atomselect top all]
Open a file energy.dat for writing:
      set fil [open energy.dat w]

3. For each atom in the system, calculate the kinetic energy, and write it to a file :
      foreach m [$all get mass] v [$all get {x y z}] {
      puts $fil [expr 0.5 * $m * [vecdot $v $v] ]
      }
Close the file:
      close $fil

All these steps can be avoided by typing in the Terminal Window:
      vmd -dispdev text -e get energy.tcl

We now have a file of raw data that can be used to fit the obtained energy distribution to the Maxwell-Boltzmann distribution. The temperature of the distribution can be obtained from that fit.

1. In a Terminal window, type xmgrace. In the xmgrace window, choose the Data → Import → ASCI I menu item. In the Files box, select the file energy.dat. Click on the OK button. You should see a black trace which correspond to the raw data.

2. To look at the distribution of points, we will make a histogram of this data. Choose the Data → Transformations → Histograms menu item. In the Source → Set window, click on the first line, in order to make a histogram of the data just loaded.
Click on the Normalize option.
Fill in Start: 0, Stop at: 10, and # of bins: 100, and Apply.

3. The plot has been created, but cannot be seen yet. Use the right button of the mouse to click on the first set (in the Source → Set window).
Click on Hide. Now, go to the main Grace window and click on the button labeled AS: it will resize the plot to fit the existing values. This is the distribution of energies.
Now, we will fit a Maxwell-Boltzmann distribution to this plot and find out the temperature that the distribution corresponds to.

4. Choose the Data → Transformations → Non-linear curve fitting menu item. In the Source → Set window, click on the last line, which corresponds to the histogram you created.

In the Main tab, type in the Formula window:
      y = (2/ sqrt(Pi * a0 ∧3 )) * sqrt(x) * exp (-x / a0)
This will fit the curve and get a fit for the parameter a0, which corresponds to kB T in units of kcal/mol.

5. In the Parameters drop-down menu, choose 1. You can give an initial value to A0, so that the iterations will look for a value in the vicinity of your initial guess. In the A0 window, type 0.6, which in kcal/mol corresponds to a temperature of ∼ 300K.

Click on the Apply button. This will open a window with the new value for a0, as well as some statistical measures, including the Correlation Coefficient, which is a measure of the fit.

The value of a0 obtained corresponds to kB T . Obtain the temperature T for this distribution with kB = 0.00198657 kcal /mol /K.
We obtain the following histogramm!

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

Energies

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Temperature distribution

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Objective: Simulate our protein in an NVE ensemble, and analyze the temperature distribution.

In order to obtain the data for the temperature from the log file we will again use the script namdstats.tcl, which was already sourced. Type in a terminal window:
      data_time TEMP namd_log
It will store each timestep and its corresponding temperature in the file TEMP.dat.

Using EXCEL, we obtain the following graph, which represents the evolution of the temperature in function of time:

The first part corresponds the the heating, then we let the system reach an equilibrium (NPT state), a NVT portion, and finally a NPT portion again.

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

Density

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In order to obtain the data for the volume from the log file we will again use the script ''namdstats.tcl'', which was already sourced. Type in a terminal window:
      data_time VOLUME namd_log
It will store each timestep and its corresponding temperature in the file TEMP.dat.

Using EXCEL, we obtain the following graph, which represents the evolution of the density in function of time:

The first part corresponds the the heating, then we let the system reach an equilibrium (NPT state), a NVT portion, and finally a NPT portion again.

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

Pressure as a function of simulation time

In order to obtain the data for the pressure from the log file we will again use the script namdstats.tcl, which has been updated for the occasion. The file can be found here. Please rename to namdstats.tcl after download.

Here are the steps to use this script:

source namdstats.tcl

data_time DATA_NAME LOG_FILE

It will extract data from LOG_FILE, creating a DATA_NAME.dat containing values and time informations.

Available DATA_NAME can be: BOND, ANGLE, DIHED, IMPRP, ELECT, VDW, BOUNDARY, MISC, KINETIC, TOTAL, TEMP, TOTAL2, TOTAL3, TEMPAVG, PRESSURE, GPRESSURE, VOLUME, PRESSAVG, GPRESSAVG.

So, to extract pressure from our first simulation, the command is: data_time PRESSURE namd_log

Here is a small plot of pressure and temperature in function of time

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

RMSD for individual residues

We aim at finding the average RMSD over time for each residue in the protein using VMD.

1. We load the .psf and .dcd files obtained after the first round of simulation.

2. In the TkCon window type:

source residue_rmsd.tcl

set sel_resid [[atomselect top "protein and alpha"] get resid]

This will get all the residues number of all alpha-carbons in the protein. Since there is just one and only one α-carbon per residue, it is a good option.

3. Now we will calculate the RMSD values of all atoms in the newly created selection:

rmsd_residue_over_time top $sel resid

At the end of the calculation, we have a list of the avergae RMSD per residue (in the file residue_rmsd.dat)

Remark: we updated the script residue_rmsd.tcl to be able to specify on which frames the rsmd has to be computed. Please have a look on this wiki for a more up-to-date version of the file... Command is:

rmsd_residue_over_time top $sel resid FIRST_FRAME LAST_FRAME

4. In VMD, in Graphics → Representations, do the following actions:

• create two replicates: protein and resname FMN in selected atoms
• for the FMN, choose CPK as a drawing method
• for the protein, choose tube as drawing method, and user as coloring method. Now click on the Trajectory tab, and in the Color Scale Data Range, type 0.40 and 1.00.

The protein is colored according to its average RMSD values. The residues displayed in blue are more mobile while the ones in red move less.

Here is a movie with the protein colored according to average RMSD values.

RMSD moving residues

5. Now we can plot the RMSD value per residue by typing in a Terminal window :

xmgrace residue rmsd.dat

We obtain the following picture:

RMSD of residue within 3 angström of the FMN

We can see that the residues that move the most are the residue number: 425, 451, 453

RMSD of residue within 6 angström of the FMN

We can see that the residues that move the most are the residue number: 424, 425, 464, 468

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

RMSD of selected atoms compared to initial position along time

This script was highly updated, please go to the script page if you encounter a problem!!!

Selections are not precise here!

We made a small TCL script to calculate RMSD from selected atoms compared to their initial position along timestep. The file can be found here. Please rename to Residue_rmsd_igem09.tcl after download.

Example to run the script:

load .dcd + .psf on VMD

source residue_rmsd_igem09.tcl

set sel_resid [[atomselect top "protein and alpha"] get resid]

rmsd_residue_over_time top $sel_resid 0 0

We tried to select only backbone from protein + FMN → change

set sel_resid [[atomselect top "backbone"] get resid]

The script was updated to be able to define reference frame and first frame were RMSD will be calculated. We usually don't need to compute RMSD during heating, for instance. RMSD takes a lot of time. In our first run 1 frame = 100 timesteps * 2 fs*timesteps^-1 = 200 fs

complete form for run is:

rmsd_residue_over_time top $sel_resid FIRST_FRAME REFERENCE_FRAME

For our first run, if we want to select only the 295°K NPT plateau, and set its first frame as reference, we have to launch:

rmsd_residue_over_time top $sel_resid 1115 1115

Here is how the script processes:

• calculate how many frames are in .dcd
• for each timestep, the script aligns (best fit) the backbone of the protein to the eference position to minimize RMDS. (Test: "and not mass 1,008000" == and noh was added in selection to remove hydrogen)
• for each residue (selected by sel_resid), RMSD is computed and the sum of all RMSD (one for each residue) is stored for current timestep
• script's output is data_rmsd.dat

Here is a fast graph of the output of the average RMSD of the atoms in function of time. It seems normal.

Here is what we got with FIRST_FRAME=1115 REFERENCE_FRAME=1115. Average=921.477, standard deviation=202.1708

FIRST_FRAME=0 REFERENCE_FRAME=0. The difference of the sum probably comes from the new selection of atoms from the backbone. We should compute an average value to normalize amplitude. (fluctuation is conserved, anyway) Average=781.3913, standard deviation=118.1393

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

Salt bridges

As we wanted to redo the analysis from Schulten's article, we looked for salt bridges. VMD can easily compute this, it even propose an easy GUI. Standard configuration is just fine for now. You'll have a log file containing the list of nitrogen-oxygen susceptible of forming a salt bridge. You'll also get a file for each bridge containing the distance between both atoms along the simulation.

In the light state, we have 9 salt bridges witin the protein and 12 if we consider the protein and the flavin (use "protein or resname FMN" as selection).

ASP471-ARG467

GLU409-ARG442

FMN450-FMN450

ASP540-LYS544

ASP432-ARG442

FMN450-ARG451

GLU457-LYS489

GLU444-LYS485

ASP522-ARG521

ASP424-ARG451

GLU475-LYS533

FMN450-ARG467

Here is a plot for one of the bridges. We have to look for the max distance for a salt bridge.

Go to: Maxwell-Boltzmann Energy Distribution EnergiesTemperature distributionDensity PressureRMSD for individual residuesRMSD of selected atomsSalt bridgesRMSF

RMSF

After changing the script [see here], we perform an interesting analysis from these 2 files. First, we have to correct the RMSF, that can be linked to beta factor using this equation:

If you plot beta factor and RMSF, you get such a thing.

This is a 1 nanosecond NPT run at 300°K. We hope to see a RMSF curve identical to the beta factor. It should only be shifted higher because of the increased temperature. But having a similar tendency would mean our simulation show oscillations similar to what was observed during crystallography. This is really a quite nice validation of our run!