rdparm reads in AMBER prmtop files and allows users to inspect the stored information (see rdparm.html).
ptraj is a program for processing AMBER, CHARMM, and PDB trajectory files. It can convert trajectories, calculate bond, angles, dihedrals, RMSd value, mean-squared displacements, atomic positional fluctuations, order parameters/correlation functions, imaging of trajectories to various unit cells, etc.. A limited snapshot of the documentation is in ptraj.html.
Although ptraj is distributed within AMBER as part of the free set of "Amber Tools" (see ambermd.org, it can be obtained as a standalone version from the author (Cheatham).
Please let us know if you find bugs or add features of general use...
This is a snapshot of what is available in Amber Tools within AMBER 10. This includes updates to the atom selection parser to be compatible with AMBER, addition of the ability to cluster MD trajectories, and other significant changes. The standalone version now includes support for all of the matrix functionality. The documentation is not complete; please refer to the comments in the code and previous documentation. Additional preliminary information on the clustering is here in this PDF file; see also our clustering paper:
J. Shao, S. W. Tanner, N. Thompson, T.E. Cheatham, III. "Clustering
molecular dynamics trajectories: I. Characterizing the performance of
different clustering algorithms." J. Chem. Theory Comp. 3,
2312-2334 (2007).
     [
local PDF:
ACS Link
+ Supporting info
]
Files are also available individually in this directory...
Note: new source code update as of 25 June 2003 fixes more bugs. See the file README.UPDATES for more information. This version properly handles DOS formatted prmtop files and more correctly handles X-PLOR PSF files. Imaging can be done to other unit cells with the xoffset, yoffset and zoffset commands (which may be useful for building up PDB files to show packing of unit cells)... More changes should come in time.
In the previous version, a long-standing (and ADDITIONAL) bug with the B-factors is fixed. B-factors are the positional fluctuations SQUARED multiplied by 8pi**2 (not the sqrt() as I mistakening posted on the AMBER e-mail reflector; whoops?). Other than this, the most useful addition is a new command to randomly swap solvent and ion positions to randomize initial ion placement and fixes in supporting AMBER7 prmtop files.