AMBER: CPPTRAJ Tutorial C0

An Introduction to CPPTRAJ

By Daniel R. Roe, July 2014. Updated by tec3 July 2015.

Note: This tutorial was designed for use with CPPTRAJ from AmberTools 14.X or more recent versions. Note: In general, the newer versions have fewer bugs, better support and more features. Current release is in AmberTools 15 with bleeding edge CPPTRAJ on GitHub at: https://github.com/mojyt/cpptraj.

trpzip2

TABLE OF CONTENTS

Introduction
Loading a Topology and Trajectory
Specifying an Action
Processing the Trajectory
Working With Data Sets
Running in Batch Mode
Associated Files

Introduction

This tutorial will give a brief overview of analyzing simulation data with CPPTRAJ. CPPTRAJ is the successor to PTRAJ, with many additional features. Some basic and common types of analysis will be covered, as well as the basics of data set handling in CPPTRAJ. This assumes that AmberTools has been successfully installed and has been tested. This also assumes some familiarity with Amber atom mask selection syntax. For more details on atom mask selection syntax see the Amber manual (section 28.2.3. Atom Mask Selection Syntax in the Amber 14 manual). In addition, xmgrace will be required to view some of the output data.

Throughout this tutorial a short example trajectory of the beta-hairpin trpzip2 will be used. The trajectory is in NetCDF format, which is faster to process, more compact, higher precision, and more robust than the ASCII format. NetCDF is enabled by default in Amber, but if you find that your CPPTRAJ cannot read this trajectory please contact the Amber mailing list for help. The trajectory and associated topology can be downloaded here:

For more detailed information on CPPTRAJ, see here:

Daniel R. Roe and Thomas E. Cheatham, III,
"PTRAJ and CPPTRAJ: Software for Processing and Analysis of Molecular Dynamics Trajectory Data".
J. Chem. Theory Comput., 2013, 9 (7), pp 3084-3095.

This tutorial features interactive use of CPPTRAJ; while useful, for better provenance, to keep track of the workflow, and in production use it is often better to use a script file with CPPTRAJ commands.

Loading a Topology and Trajectory

To start CPPTRAJ, type 'cpptraj' from the command line. Note: Commands typed by the user will be displayed in red with output text from CPPTRAJ in black.

[user@computer ~]$ cpptraj

CPPTRAJ: Trajectory Analysis. V14.05
    ___  ___  ___  ___
     | \/ | \/ | \/ | 
    _|_/\_|_/\_|_/\_|_
>

Running CPPTRAJ with no arguments brings up the interactive command line. The command line is useful for running simple or short analyses. The command line allows tab completion of file names and commands. Also, in interactive mode all commands used are written to the file 'cpptraj.log' (this name can be changed with the '--log ' command line switch). There is also extensive help available.

Before reading in a trajectory, CPPTRAJ needs to know what the system looks like. This information is contained with topology files. The first step is to load the topology file with the 'parm' command:

> parm trpzip2.ff10.mbondi.parm7
	Reading 'trpzip2.ff10.mbondi.parm7' as Amber Topology

The topology has now been loaded. You can see what topologies are loaded with the 'list' command:

> list parm

PARAMETER FILES:
 0: 'trpzip2.ff10.mbondi.parm7', 220 atoms, 13 res, box: None, 1 mol

The output shows the topology index (which starts from 0) followed by some brief information on the topology. More detailed information can be obtained using the 'parminfo <#>' command, where <#> is the index of the desired topology.

> parminfo 0
	Topology trpzip2.ff10.mbondi.parm7 contains 220 atoms.
		13 residues.
		1 molecules.
		227 bonds (104 to H, 123 other).
		402 angles (233 with H, 169 other).
		853 dihedrals (481 with H, 372 other).
		Box: None
		GB radii set: modified Bondi radii (mbondi)

Now that the topology file is loaded, we can tell CPPTRAJ which trajectory we are going to process:

> trajin trpzip2.gb.nc
	Reading 'trpzip2.gb.nc' as Amber NetCDF

Note that this does not immediately read the trajectory, rather it places the trajectory in the input trajectory list for processing later. To see what trajectories are currently in the input trajectory list we can again use the 'list' command:

> list trajin

INPUT TRAJECTORIES:
 0: 'trpzip2.gb.nc' is a NetCDF AMBER trajectory, Parm trpzip2.ff10.mbondi.parm7 (reading 1201 of 1201)
  Coordinate processing will occur on 1201 frames.

Specifying an Action

Actions are defined functions or data processing that is applied to each frame loaded from the trajectory, such as RMS fitting, stripping atoms, calculation of various properties, etc.

Now that a topology and trajectory have been loaded, we can specify actions to generate data from the trajectory. Say for example we would like to know the end-to-end distance for the hairpin over the course of the trajectory. We can use the 'distance' command to get this information. First, we can use the 'help' command to remind us of the syntax for 'distance':

> help distance
	[<name>] <mask1> <mask2> [out <filename>] [geom] [noimage] [type noe]
	Options for 'type noe':
	  [bound <lower> bound <upper>] [rexp <expected>] [noe_strong] [noe_medium] [noe_weak]

  Calculate distance between atoms in <mask1> and <mask2>

The 'help' command can be used with no arguments to bring up a list of all commands.

In order to figure out which atoms correspond with the end residues of trpzip2, we can use the 'resinfo' command:

> resinfo
#Res  Name First  Last Natom #Orig
    1 SER      1    13    13     1
    2 TRP     14    37    24     2
    3 THR     38    51    14     3
    4 TRP     52    75    24     4
    5 GLU     76    90    15     5
    6 ASN     91   104    14     6
    7 GLY    105   111     7     7
    8 LYS    112   133    22     8
    9 TRP    134   157    24     9
   10 THR    158   171    14    10
   11 TRP    172   195    24    11
   12 LYS    196   217    22    12
   13 NHE    218   220     3    13

From this output we can see that our end residues are 1 and 13. In general, the 'resinfo', 'atominfo', and 'molinfo' commands are useful for examining your system layout and/or testing the result of an atom mask expression. For example, to see what atoms will be selected by the atom mask ':13' (residue 13):

> atominfo :13
#Atom Name  #Res Name  #Mol Type   Charge     Mass GBradius El
  218 N       13 NHE      1 N     -0.4630  14.0100   1.5500  N
  219 HN1     13 NHE      1 H      0.2315   1.0080   1.3000  H
  220 HN2     13 NHE      1 H      0.2315   1.0080   1.3000  H

We can now enter our 'distance' command:

> distance end-to-end :1 :13 out dist-end-to-end.agr
    DISTANCE: :1 to :13, center of mass.

This says to calculate a distance named end-to-end from the center of mass of residue 1 to residue 13, writing the results to a file named 'dist-end-to-end.agr'. The file format will be xmgrace-readable because the filename extension '.agr' is recognized by CPPTRAJ as xmgrace. We could change the format to gnuplot-readable by specifying a '.gnu' extension instead. If the extension is '.dat' or not recognized, CPPTRAJ will default to a standard column format. For a complete list of supported formats and their associated extensions see the Amber 14 manual.

Note that similar to 'trajin', entering an action does not execute it right away. Instead, it has gone into the action list. To see what actions are currently present in the action list we can use the 'list' command:

> list actions

ACTIONS:
  0: [distance end-to-end :1 :13 out dist-end-to-end.agr]

Processing the Trajectory

We have now loaded a topology, a trajectory, and have specified an action. The command can now be executed by specifying 'run' or 'go'. This tells CPPTRAJ to process each loaded trajectory, executing any specified actions on each frame. During trajectory processing some information will be printed that describes what CPPTRAJ is doing. First, information on the currently loaded topologies and trajectories are printed:

> run
---------- RUN BEGIN -------------------------------------------------

PARAMETER FILES:
 0: 'trpzip2.ff10.mbondi.parm7', 220 atoms, 13 res, box: None, 1 mol, 1201 frames

INPUT TRAJECTORIES:
 0: 'trpzip2.gb.nc' is a NetCDF AMBER trajectory, Parm trpzip2.ff10.mbondi.parm7 (reading 1201 of 1201)
  Coordinate processing will occur on 1201 frames.
TIME: Run Initialization took 0.0000 seconds.

Note that if any reference coordinates or output trajectories are specified they will appear here as well.

Next, the first trajectory will be loaded and any actions will be set up for that trajectory/topology:

BEGIN TRAJECTORY PROCESSING:
.....................................................
ACTION SETUP FOR PARM 'trpzip2.ff10.mbondi.parm7' (1 actions):
  0: [distance end-to-end :1 :13 out dist-end-to-end.agr]
	:1 (13 atoms) to :13 (3 atoms), imaging off.

Here our 'distance' action has been set up.

Next, each frame in the trajectory will be read and processed:

----- trpzip2.gb.nc (1-1201, 1) -----
 0% 10% 20% 30% 40% 50% 60% 70% 80% 90% 100% Complete.
 

When all trajectories have been processed, a summary of the total run will be written, including number of frames processed, any action-specific output, data sets generated, and data files written.

Read 1201 frames and processed 1201 frames.
TIME: Trajectory processing: 0.0094 s
TIME: Avg. throughput= 127372.9982 frames / second.

ACTION OUTPUT:

DATASETS:
  1 data set:
	end-to-end "end-to-end" (double, distance), size is 1201

DATAFILES:
  dist-end-to-end.agr (Grace File):  end-to-end
---------- RUN END ---------------------------------------------------

If xmgrace is installed and you are running and X-server, you can view the output right from the CPPTRAJ command line:

> xmgrace dist-end-to-end.agr
dist-end-to-end

Working With Data Sets

From the 'DATASETS' section of the output:

DATASETS:
  1 data set:
	end-to-end "end-to-end" (double, distance), size is 1201

we see that we have generated one data set named 'end-to-end', with the legend "end-to-end", that is a double-precision distance data set with 1201 elements. We can now continue to manipulate this data set if desired. Say for example you also want to write this data in the standard (column) data format. You can use the 'writedata' command like so:

> writedata end-to-end.dat end-to-end
 end-to-end

The linux 'head' command can be used directly from the CPPTRAJ command line to view the first few lines of 'end-to-end.dat'

> head end-to-end.dat 
#Frame     end-to-end
       1       6.4251
       2       5.9250
       3       6.7926
       4       6.3125
       5       5.7580
       6       5.4389
       7       6.1086
       8       6.5588
       9       5.6949

Now that we are finished, type 'quit' or 'exit' to exit CPPTRAJ.

> quit
TIME: Total execution time: 131.2112 seconds.
--------------------------------------------------------------------------------
To cite CPPTRAJ use:
Daniel R. Roe and Thomas E. Cheatham, III, "PTRAJ and CPPTRAJ: Software for
  Processing and Analysis of Molecular Dynamics Trajectory Data". J. Chem.
  Theory Comput., 2013, 9 (7), pp 3084-3095.

Running in Batch Mode

Instead of running interactively, CPPTRAJ can also be run using one or more input files. Since the log file 'cpptraj.log' has recorded every command used, you can use the log file as the basis for a cpptraj "script". For example to generate everything we have done so far the following input could be used:

parm trpzip2.ff10.mbondi.parm7
trajin trpzip2.gb.nc
distance end-to-end :1 :13 out dist-end-to-end.agr
run
writedata end-to-end.dat end-to-end

Paste the above commands into a file called 'cpptraj.in'. The commands can then be executed like so:

[user@computer ~]$ cpptraj -i cpptraj.in 

CPPTRAJ: Trajectory Analysis. V14.05
    ___  ___  ___  ___
     | \/ | \/ | \/ | 
    _|_/\_|_/\_|_/\_|_
INPUT: Reading Input from file cpptraj.in
  [parm trpzip2.ff10.mbondi.parm7]
	Reading 'trpzip2.ff10.mbondi.parm7' as Amber Topology
  [trajin trpzip2.gb.nc]
	Reading 'trpzip2.gb.nc' as Amber NetCDF
  [distance end-to-end :1 :13 out dist-end-to-end.agr]
    DISTANCE: :1 to :13, center of mass.
  [run]
---------- RUN BEGIN -------------------------------------------------

The rest of the output will be similar to what was seen previously.

Note that it is VERY IMPORTANT to check your output for lines containing 'Warning:' or 'Error:' as these messages indicate there may be a problem with your input.

Associated Files

These files can be used to check your output.

dist-end-to-end.agr
end-to-end.dat
cpptraj.in

Copyright Daniel R. Roe, 2014