Mercurial > hg > cfcfd3
changeset 153:5a0f5fa2a252
Small changes to eilmer3 documentation.
author | Peter Blyton <p.blyton@uq.edu.au> |
---|---|
date | Sun, 01 Apr 2012 13:54:57 +1000 |
parents | d074db9de9b4 |
children | 24529a8ac9a8 |
files | doc/sphinx/getting-started.rst examples/eilmer3/turbulence-models-user-guide/chap1-introduction/introduction.tex examples/eilmer3/user-guide/eilmer3-user-guide.tex |
diffstat | 3 files changed, 4 insertions(+), 1 deletions(-) [+] |
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--- a/doc/sphinx/getting-started.rst Sat Mar 31 15:01:34 2012 +1000 +++ b/doc/sphinx/getting-started.rst Sun Apr 01 13:54:57 2012 +1000 @@ -81,6 +81,7 @@ #. gcc #. gcc-c++ #. m4 +#. openmpi-devel #. gcc-gfortran #. swig #. python-devel
--- a/examples/eilmer3/turbulence-models-user-guide/chap1-introduction/introduction.tex Sat Mar 31 15:01:34 2012 +1000 +++ b/examples/eilmer3/turbulence-models-user-guide/chap1-introduction/introduction.tex Sun Apr 01 13:54:57 2012 +1000 @@ -307,7 +307,7 @@ of 0.1 is representative of that in wind tunnels downstream of turbulence-generating screens. Unlike the turbulence intensity, values for turbulent-to-laminar viscosity ratio cannot be measured easily. Commonly recommended values range from 0.00001 to 100 \cite{Roy2003,Fluent2006, -ESI2004,Tu2008}. Freestream values of $/omega$ computed from turbulence intensity and +ESI2004,Tu2008}. Freestream values of $\omega$ computed from turbulence intensity and turbulent-to-laminar viscosity ratio should also be checked that they are not larger than 1\% of the peak value in turbulent regions, since using these values is considered to be unrealistic \cite{Wilcox2006}.
--- a/examples/eilmer3/user-guide/eilmer3-user-guide.tex Sat Mar 31 15:01:34 2012 +1000 +++ b/examples/eilmer3/user-guide/eilmer3-user-guide.tex Sun Apr 01 13:54:57 2012 +1000 @@ -2369,5 +2369,7 @@ \input{paraview} \cleardoublepage +\phantomsection % re-set the hyperref anchor so that TOC page number link is correct. +\addcontentsline{toc}{part}{\indexname} \printindex \end{document}