Daniel Price
Daniel Price
from @jameswurster: for the particle splitting, we will need to introduce ghost particles for each of the two types of gas particles, where the ghosts will be similar but not...
either by using their age and mass to give a luminosity and colour (as in real stars) or just to give them a twinkling effect (just for show)
with multigrain dust output, we need to be able to define particle "sub-types" as child types of a single generic type. Otherwise we end up with potentially hundreds of particle...
for phantom simulations with multiple dust species, splash currently shows something like the following in the menu: ``` 1) x [au] 43) deltavz 2) y [au] 44) deltavx 3) z...
this is needed, some work sitting in pull request
Issue raised by Geoff Bryan:  something is wrong with 3D interpolation to cylindrical grid, particles do not seem to interpolate correctly near -ve z boundary. Problem always occurs near...
can do this in separate panels, current workaround is to create a bunch of ascii files that have to be read in separately
Would be nice if particle tracking could automatically find the particle with maximum or minimum of a particular column (e.g. maximum density)
Type of PR: same as #521 Description: porosity evolution Testing: compiles with no warnings or errors Did you run the bots? no Did you update relevant documentation in the docs...
See comment on #523 , we need to adapt the scripts/kernels.py kernel module generator to also generate the relevant routine needed for the forward symplectic integrator...