Re: Phantom + Photoionization
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Daniel Price
Jul 4, 2017, 10:27:42 AM7/4/17
to Maya Petkova, phantoms...@googlegroups.com
Hi Maya,
We’re at a preliminary stage in our radiation hydro studies. The approach we are using at the moment has been to write an analysis module (analysis_mcfost.f90). This allows you to do post-simulation analysis on phantom dump files.
The trick is that you can then make this “live” by setting the flag LIVE_ANALYSIS=yes, which calls the analysis module once every dtmax. This is what we’ve been doing for the MCFOST-Phantom coupling.
The other thing you might want to take a look at are some preliminary routines for photoevaporation written by Mark Hutchison (look for #ifdef PHOTO). They have not been used much but you might be able to see how it was done.
Best wishes,
Daniel
> On 21 Jun 2017, at 1:11 am, Maya Petkova <ma...@st-andrews.ac.uk> wrote:
>
> Dear Daniel,
>
> After submitting the density mapping paper, Ian and I have discussed how to continue for the remaining one year of my PhD. We are interested in using Phantom together with a Photoionization code developed by Bert Vandenbroucke who is here in St Andrews. The aim would be to run live radiation hydrodynamics and apply it to large scale star formation and/or molecular cloud formation.
>
> We were wondering if you had any tips or suggestions for us, since you have already run live radiation hydrodynamics with Phantom?
>
> Any advice would be very much appreciated!
>
> Best wishes,
> Maya
We’re at a preliminary stage in our radiation hydro studies. The approach we are using at the moment has been to write an analysis module (analysis_mcfost.f90). This allows you to do post-simulation analysis on phantom dump files.
The trick is that you can then make this “live” by setting the flag LIVE_ANALYSIS=yes, which calls the analysis module once every dtmax. This is what we’ve been doing for the MCFOST-Phantom coupling.
The other thing you might want to take a look at are some preliminary routines for photoevaporation written by Mark Hutchison (look for #ifdef PHOTO). They have not been used much but you might be able to see how it was done.
Best wishes,
Daniel
> On 21 Jun 2017, at 1:11 am, Maya Petkova <ma...@st-andrews.ac.uk> wrote:
>
> Dear Daniel,
>
> After submitting the density mapping paper, Ian and I have discussed how to continue for the remaining one year of my PhD. We are interested in using Phantom together with a Photoionization code developed by Bert Vandenbroucke who is here in St Andrews. The aim would be to run live radiation hydrodynamics and apply it to large scale star formation and/or molecular cloud formation.
>
> We were wondering if you had any tips or suggestions for us, since you have already run live radiation hydrodynamics with Phantom?
>
> Any advice would be very much appreciated!
>
> Best wishes,
> Maya
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