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This is a to-do page for the next release. These are specific tasks we should do.
The GoldVersionToDo page has the general steps for creating a gold version of the code.
where do we want to store the output from the test suite? The gradj ftp site appears dead. Really should be on nublado.
~~ Merge the chianti branch onto trunk before creating c13_branch, but understand why func_test_grid.out does not repeat - checkall error says "PROBLEM: the output in func_test_grid.out did not repeat exactly func_test_grid.out: returned with FAILURE status" ~~
run programs, review commands Peter had to comment out.
~~ Merge the Romas branch onto the trunk before creating c13_branch ~~
~~ update copyright year to 2013 ~~
grain compile bug, ticket #221 #233
~~ There are the problems with BLR calculations. The most recent botches look likely to be symptomatic of this. I'm not sure we can plan to address them in any time-boxed fashion; the trunk is no worse than where c10 is in this regard, and better in a lot of other ways. ~~ These have been moved to the "radiative transfer" milestone in the tickets.
~~ the changes to the grid command will need to be accepted de facto; otherwise re-implementing the associated bug fixes and documentation updates would be too time consuming - putting them in a beta/release candidate may get some usability feedback on them from users 'outside the fence'. ~~
Maybe we should plan to make the beta in one week, on the nice round October 15th? I could get in the escape probability fixes by then. Then make the release candidate Nov. 15 or Dec. 1, and release one or two months later? I very much like the idea of actually getting it out in the month of January.
~~ silence warnings about chemistry at startup - added test on release so print will not occur ~~
~~ Merge the optnl branch - only documentation and code changes to make atom xx-like agree with documentation. ~~
~~ coronal dr bug ~~ documented in hazy, but still there ~~
~~ ortho para issue with save species - for now document that we only report ~~
hazy1 section 12.2, g-bar approximation, copy section from cooling function paper explaining what we do
section 15.46, Save Chianti, should give energy in wavenumbers
section 18.14.21 set gbar of - what do we do about forbidden transitions? should use something like 1
~~ the quick start guide has shown something indicating speed. Racehorses, fighter jets, speed skaters. Wonder if we could get an image of a 8 on the Cam? The Bumps? I tried to google up such an image but they were mostly copyrighted. Wonder if Robin might have a way to get something we could use? Or we could ask Andy or Paul Hewett.
~~ for hazy 1 and 2 we have tried to show off something that cloudy can do, that people may not appreciate. there have been x-ray and IR spectra. Any ideas?? The new thing we have now is much better Fe x-ray spectra thanks to chianti. An x-ray image showing L-shell Fe lines and H&He-like O and C might be impressive.
~~ we have not been providing compiled copies of hazy 3 so maybe it does not need an update.
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