| commit | 10c707747293586a92e12e3bc89bd4cddf022b0d | |
| author | Mark Abraham <mark.j.abraham@gmail.com> | |
| Mon, 26 Sep 2011 14:37:44 +0000 (27 00:37 +1000) | ||
| committer | Mark Abraham <mark.j.abraham@gmail.com> | |
| Mon, 26 Sep 2011 14:37:44 +0000 (27 00:37 +1000) | ||
| tree | 1c98c8388fffbc2639ada650f6785af5062184b7 | treesnapshot (tar.gz zip) |
| parent | c9635cec6fd784301000b4330022a227c3a6da2a | commitdiff |
Dropped some hints in the documentation
Users should collect data more often than the time scale of the
autocorrelation, actually save velocities for computing velocity
ACF, and trjconv -ur compact is useful for rhombic dodecahedra.
Change-Id: I9c59b3798dbb8d86b862859bf8f217b12d33906a
Users should collect data more often than the time scale of the
autocorrelation, actually save velocities for computing velocity
ACF, and trjconv -ur compact is useful for rhombic dodecahedra.
Change-Id: I9c59b3798dbb8d86b862859bf8f217b12d33906a
| src/tools/gmx_analyze.c | diffblobblamehistory | |
| src/tools/gmx_trjconv.c | diffblobblamehistory | |
| src/tools/gmx_velacc.c | diffblobblamehistory |