ramses_users

Oh ok... so it'll find 'clumps' going forward! Good to know. Thanks Romain.... Cheers,

Hey all, Since I mostly use ear...@gmail.com with SLACK, can someone invite me to the RAMSES channel

We are excited to announce that we are organising a conference on “Building Galaxies from Scratch:

Hi Arturo, Thanks for your reply. Yes it seems like the problem is with AGN runs, also I gave energy

Hi Fichtner, I have had this happen in a zoom simulation, and the run crashed. In the end I just used

Hi Romain, Thank you for the reply. I already included the sink_refine option in the simulation.

Hi Yvonne, Not sure if this ever got sorted out, but I think it is: https://ui.adsabs.harvard.edu/abs

Hi all, I was wondering whether there is any documentation or a paper that explains the turbulence

Hi Romain, Thanks for your reply, that helps! Cheers Thor ___________________________ Dr. Thor Tepper

Hello everyone, I have a question about the following geometrical criterion in the star_formation

Dear Graeme, With Benoît Commerçon, we have developed an implicit solver for (anisotropic) thermal

Hi Thor, You can achieve this with yt: import yt # Load a sample dataset. You can load whatever

Hi guys, Whatever happened to the Boolean parameter 'star' in the most recent Ramses version?

Hi Thor, This has now been fixed as of yt 3.6.1 (and later). You can install yt 3.6.1 using pip

The simulation I use usually for that is sedov3d.nml in directory namelist. It is quite a simple test

To make sure we are on the same page: output_00001 contains the initial conditions from MUSIC. There

Hi Thor, I've experienced this problem before on multiple machines. My workaround is to set

Hi Romain, Thanks for spotting this point. The preliminary test seems to work. Best e On Thursday,

Dear RAMSES User/Developers, I have a high level question about RAMSES's predictor-corrector

Thank you, that is reassuring! Is there some way to recover the gravitational potential energy from

Oh right. Well reducing nremap works anyway, and I assumed it is because it does not have such a

I encourage you to come in the separata now to listen to what Davide have to say !

Hi Asiyeh, 1) No it is not possible to do it, unless you choose a very low value for the gas density,

If this is it, there's a feature written by Valentin Perret, where you can use nrestart_quad in

What kind of simulations are you performing here ? What are your magnetic field initial conditions ?

B^2/2 is the magnetic energy density. It is in units of erg/cm^3 if you need to convert it from code

Hi all, There is something really weird happening with the automatic test page since a couple of

Hi, Two other solutions I could suggest: 1) Read in the output via pynbody and dump the arrays as

Hi Romain, Many thanks for your prompt and enlightening reply. So, would you say that convergence of

Hi Mark, I have started some prototyping some years ago. It is relatively straightforward, based on