g_rmsdist(1) [debian man page]
g_rmsdist(1) GROMACS suite, VERSION 4.5.4-dev-20110404-bc5695c g_rmsdist(1) NAME
g_rmsdist - calculates atom pair distances averaged with power -2, -3 or -6 VERSION 4.5.4-dev-20110404-bc5695c SYNOPSIS
g_rmsdist -f traj.xtc -s topol.tpr -n index.ndx -equiv equiv.dat -o distrmsd.xvg -rms rmsdist.xpm -scl rmsscale.xpm -mean rmsmean.xpm -nmr3 nmr3.xpm -nmr6 nmr6.xpm -noe noe.dat -[no]h -[no]version -nice int -b time -e time -dt time -[no]w -xvg enum -nlevels int -max real -[no]sumh -[no]pbc DESCRIPTION
g_rmsdist computes the root mean square deviation of atom distances, which has the advantage that no fit is needed like in standard RMS deviation as computed by g_rms. The reference structure is taken from the structure file. The RMSD at time t is calculated as the RMS of the differences in distance between atom-pairs in the reference structure and the structure at time t. g_rmsdist can also produce matrices of the rms distances, rms distances scaled with the mean distance and the mean distances and matrices with NMR averaged distances (1/r3 and 1/r6 averaging). Finally, lists of atom pairs with 1/r3 and 1/r6 averaged distance below the maximum distance ( -max, which will default to 0.6 in this case) can be generated, by default averaging over equivalent hydrogens (all triplets of hydrogens named *[123]). Additionally a list of equivalent atoms can be supplied ( -equiv), each line containing a set of equivalent atoms specified as residue number and name and atom name; e.g.: 3 SER HB1 3 SER HB2 Residue and atom names must exactly match those in the structure file, including case. Specifying non-sequential atoms is undefined. FILES
-f traj.xtc Input Trajectory: xtc trr trj gro g96 pdb cpt -s topol.tpr Input Structure+mass(db): tpr tpb tpa gro g96 pdb -n index.ndx Input, Opt. Index file -equiv equiv.dat Input, Opt. Generic data file -o distrmsd.xvg Output xvgr/xmgr file -rms rmsdist.xpm Output, Opt. X PixMap compatible matrix file -scl rmsscale.xpm Output, Opt. X PixMap compatible matrix file -mean rmsmean.xpm Output, Opt. X PixMap compatible matrix file -nmr3 nmr3.xpm Output, Opt. X PixMap compatible matrix file -nmr6 nmr6.xpm Output, Opt. X PixMap compatible matrix file -noe noe.dat Output, Opt. Generic data file OTHER OPTIONS
-[no]hno Print help info and quit -[no]versionno Print version info and quit -nice int 19 Set the nicelevel -b time 0 First frame (ps) to read from trajectory -e time 0 Last frame (ps) to read from trajectory -dt time 0 Only use frame when t MOD dt = first time (ps) -[no]wno View output .xvg, .xpm, .eps and .pdb files -xvg enum xmgrace xvg plot formatting: xmgrace, xmgr or none -nlevels int 40 Discretize rms in levels -max real -1 Maximum level in matrices -[no]sumhyes average distance over equivalent hydrogens -[no]pbcyes Use periodic boundary conditions when computing distances SEE ALSO
gromacs(7) More information about GROMACS is available at <http://www.gromacs.org/>. Mon 4 Apr 2011 g_rmsdist(1)
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do_dssp(1) GROMACS suite, VERSION 4.5.4-dev-20110404-bc5695c do_dssp(1) NAME
do_dssp - assigns secondary structure and calculates solvent accessible surface area VERSION 4.5.4-dev-20110404-bc5695c SYNOPSIS
do_dssp -f traj.xtc -s topol.tpr -n index.ndx -ssdump ssdump.dat -map ss.map -o ss.xpm -sc scount.xvg -a area.xpm -ta totarea.xvg -aa aver- area.xvg -[no]h -[no]version -nice int -b time -e time -dt time -tu enum -[no]w -xvg enum -sss string DESCRIPTION
do_dssp reads a trajectory file and computes the secondary structure for each time frame calling the dssp program. If you do not have the dssp program, get it from http://swift.cmbi.ru.nl/gv/dssp. do_dssp assumes that the dssp executable is located in /usr/local/bin/dssp. If this is not the case, then you should set an environment variable DSSP pointing to the dssp executable, e.g.: setenv DSSP /opt/dssp/bin/dssp The structure assignment for each residue and time is written to an .xpm matrix file. This file can be visualized with for instance xv and can be converted to postscript with xpm2ps. Individual chains are separated by light grey lines in the .xpm and postscript files. The number of residues with each secondary structure type and the total secondary structure ( -sss) count as a function of time are also written to file ( -sc). Solvent accessible surface (SAS) per residue can be calculated, both in absolute values (A2) and in fractions of the maximal accessible surface of a residue. The maximal accessible surface is defined as the accessible surface of a residue in a chain of glycines. Note that the program g_sas can also compute SAS and that is more efficient. Finally, this program can dump the secondary structure in a special file ssdump.dat for usage in the program g_chi. Together these two programs can be used to analyze dihedral properties as a function of secondary structure type. FILES
-f traj.xtc Input Trajectory: xtc trr trj gro g96 pdb cpt -s topol.tpr Input Structure+mass(db): tpr tpb tpa gro g96 pdb -n index.ndx Input, Opt. Index file -ssdump ssdump.dat Output, Opt. Generic data file -map ss.map Input, Lib. File that maps matrix data to colors -o ss.xpm Output X PixMap compatible matrix file -sc scount.xvg Output xvgr/xmgr file -a area.xpm Output, Opt. X PixMap compatible matrix file -ta totarea.xvg Output, Opt. xvgr/xmgr file -aa averarea.xvg Output, Opt. xvgr/xmgr file OTHER OPTIONS
-[no]hno Print help info and quit -[no]versionno Print version info and quit -nice int 19 Set the nicelevel -b time 0 First frame (ps) to read from trajectory -e time 0 Last frame (ps) to read from trajectory -dt time 0 Only use frame when t MOD dt = first time (ps) -tu enum ps Time unit: fs, ps, ns, us, ms or s -[no]wno View output .xvg, .xpm, .eps and .pdb files -xvg enum xmgrace xvg plot formatting: xmgrace, xmgr or none -sss string HEBT Secondary structures for structure count SEE ALSO
gromacs(7) More information about GROMACS is available at <http://www.gromacs.org/>. Mon 4 Apr 2011 do_dssp(1)