Mercurial > hg > cfcfd3
changeset 2417:c2daa7b406e3
Small adjustments for the web pages, now that the repo is public.
Also, refreshed set of group members, etc.
author | Peter Jacobs <peterj@mech.uq.edu.au> |
---|---|
date | Fri, 01 Apr 2016 14:56:56 +1000 |
parents | 77e45df79ea8 |
children | a4b1e4542903 |
files | app/eilmer3/source/e3_flow.py doc/doxygen/mainpage.txt doc/sphinx/codes.rst doc/sphinx/getting-started.rst doc/sphinx/intro.rst |
diffstat | 5 files changed, 24 insertions(+), 17 deletions(-) [+] |
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--- a/app/eilmer3/source/e3_flow.py Fri Apr 01 13:43:08 2016 +1000 +++ b/app/eilmer3/source/e3_flow.py Fri Apr 01 14:56:56 2016 +1000 @@ -896,7 +896,7 @@ :param rootName: job name that will be used to build file names :param solutionWorkDir: the directory where we'll find our ExistingSolution files. :param nblock: number of blocks in the ExistingSolution data set - :param tindx: the time index to select 0..9999: + :param tindx: the time index to select 0..9999 Do not specify with leading zeros because the Python interpreter will assume that you want to count the time index in octal. @@ -912,8 +912,10 @@ :param add_velocity: is the value to be aded to the old-solution's velocity. If it is a float value, it becomes the x-component. Otherwise, a Vector value should be supplied and all components will be used. + :param tke: is the value for the initial tke for the turbulent flow. This is applied when we change our simulations from laminar to turbulent + : param omega: is the value for the initial omega for the turbulent flow. This is also applied when we change our simulations from laminar to turbulent. """
--- a/doc/doxygen/mainpage.txt Fri Apr 01 13:43:08 2016 +1000 +++ b/doc/doxygen/mainpage.txt Fri Apr 01 14:56:56 2016 +1000 @@ -3,7 +3,7 @@ \section intro Introduction This is the developer documentation for the C++ source code collection -of the CFCFD group. Refer to the home page at http://mech.uq.edu.au/cfcfd +of the CFCFD group. Refer to the home page at http://cfcfd.mechmining.uq.edu.au for documentation of python sources. */
--- a/doc/sphinx/codes.rst Fri Apr 01 13:43:08 2016 +1000 +++ b/doc/sphinx/codes.rst Fri Apr 01 14:56:56 2016 +1000 @@ -1,7 +1,7 @@ The CFCFD Code Collection ========================= -For local and external collaborators, these are available via a Mercurial repository. +For local and external collaborators, these are available via a public Mercurial repository. #. *eilmer3*: The current compresible-flow Navier-Stokes simulation code for 2D and 3D flows.
--- a/doc/sphinx/getting-started.rst Fri Apr 01 13:43:08 2016 +1000 +++ b/doc/sphinx/getting-started.rst Fri Apr 01 14:56:56 2016 +1000 @@ -3,14 +3,15 @@ The code repository ------------------- -The codes are available for download from a Mercurial repository. +The codes are available for download from a public Mercurial repository. To make a clone of the repository:: $ cd $HOME $ hg clone https://source.eait.uq.edu.au/hg/cfcfd3 cfcfd3 -and provide the username "cfcfd-user@svn.itee.uq.edu.au" for authentication. -This takes about 40 seconds on campus at UQ. +You may provide the username "cfcfd-user@svn.itee.uq.edu.au" for authentication but +no password is required for reading. +Cloning the repository takes about 40 seconds on campus at UQ. It may take much longer, depending on your internet connection. To see what's changed:: @@ -22,7 +23,7 @@ Notes -#. You will need a password for any access. Please ask. +#. You do not need a password for for read access. #. You can read but not write with the "cfcfd-user" username. #. Some usernames (cfcfd-dev@svn.itee.uq.edu.au) may push changesets back to the repository. You will need to negotiate a developer role for this access. @@ -37,9 +38,9 @@ Licence ------- CFCFD program collection is a set of flow simulation tools for compressible fluids. -Copyright (C) 1991-2012 Peter Jacobs, Rowan Gollan, Daniel Potter, -Brendan O'Flaherty, Fabian Zander, Wilson Chan, Peter Blyton and -other members of the CFCFD group. +Copyright (C) 1991-2016 Peter Jacobs, Rowan Gollan, Daniel Potter, +Ingo Jahn, Anand Veeraragavan, Vince Wheatley, Daryl Bond, Chris James +and other members of the CFCFD group. This collection is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by
--- a/doc/sphinx/intro.rst Fri Apr 01 13:43:08 2016 +1000 +++ b/doc/sphinx/intro.rst Fri Apr 01 14:56:56 2016 +1000 @@ -55,25 +55,28 @@ Current group members --------------------- Daryl Bond; +James Burgess; Wilson Chan; +Kyle Damm; Zac Denman; -Luke Doherty, University of Oxford; Elise Fahy; David Gildfind; Rowan J. Gollan; +Jonathan Ho; Peter A. Jacobs; Ingo Jahn; Chris James; Xin Kang; Matthew McGilvray, University of Oxford; +Heather Muir; Paul J. Petrie-Repar, RPM-Turbo, Brisbane; +Peter Roman, Brisbane; Daniel Potter, CSIRO, Newcastle; Jason (Kan) Qin; Anand Veeraragavan; -Carlos de Miranda Ventura; Han Wei; Vincent Wheatley; -Fabian Zander. +Lachlan Whyborn. Past members and associates --------------------------- @@ -84,13 +87,14 @@ Brian Cook; Jason Czapla; Andrew Denman; +Luke Doherty, University of Oxford; Michael Elford; James M. Faddy; Tony Gardner, DLR; Richard J. Goozee; Klaus Hannemann and Monika Hannemann, DLR, Goettingen; Haruko Ishikawa, Tokyo; -Carolyn Jacobs, Ecole Centrale, Paris; +Carolyn Jacobs, Ecole Centrale-Supelec, Paris; Ian A. Johnston, DSTO, Adelaide; Charles Lilley, Melbourne; Michael N. Macrossan; @@ -103,9 +107,9 @@ Todd Silvester; Ben Stewart; Joseph Tang, WBM Pty Ltd, Brisbane; +Carlos de Miranda Ventura, Department of Engineering, University of Cambridge; Tina Weichel, Germany; Michael Wendt, CSIRO, Brisbane; -Adriaan Window, Brisbane. +Adriaan Window, Brisbane; +Fabian Zander. - -