atdotde
Contributor
Any idea when this will make it into the repositories? Fedora in particular?
Also, it's been forever since I looked at any of the deep stops threads. Anyone have a quick guide to reading the heat maps?
It is unlikely that any future version of Subsurface will make it to the repositories since we decided this model does not work for end user applications (or at least for us): As I understand, Fedora currently ships version 4.4.2 which is now over 18 months old. A lot has happened since (for example VPM-B integration) and the distributions just don't catch up. In addition, Subsurface relies on very specific (and recent) versions of certain libraries which makes packaging non-trivial and ends up in frustrated users (and Subsurface getting complains about the program not running properly when actually the packaging is to blame).
The way out is the AppImage, a binary package that should work out of the box for any linux distribution (and yes, for some the current daily build has problems, we are working on that). This way of distributing software is very close to what is done on Windows and Mac and allows us to ship everything we need and make it just work. The program will inform you once there is a new version out and installing it is really not much more than a single mouse click. If you want to learn more about this decision, a good starting point is the Wikipedia article about Subsurface.
What the heat map shows you is the loadings of the tissues over time normalised to Bühlmann m-values (or gradient factors if you like). The main advantage is that you get an impression of the gas loadings (and thus supposed bubble feeding rate) of all tissues and not just the leading one. The main point in that thread was that the slow tissues are still on-gassing during the deeper stops (while they are not the leading tissue) and and that this way you get much more gas released than with shallower stops (which you cannot see if you only look at the leading tissue).