Difference: IVOATheorySimDBDM_Flash (1 vs. 4)

Revision 42012-06-26 - root

 
META TOPICPARENT name="IVOATheorySimDBDMDiscussion"
TBD describe Flash simulator.

Revision 32009-06-18 - GerardLemson

 
META TOPICPARENT name="IVOATheorySimDBDMDiscussion"
Changed:
<
<		[ back ]
>
>		TBD describe Flash simulator.
Deleted:
<
<		 (notes made during conversation with Marcus Brueggen on use of a simulation database)

Would like to be able to get information/query on:

  • size of box
  • time scales
  • physics used:
    • star formation
    • cosmology
    • hydro
    • particles
    • chemical reactions
    • nuclear reactions
    • gravity
    • radiation
    • MHD
    • cosmic rays
    • feedback
    • ...
  • algorithms used:
    • mesh resolution
    • amr
  • how many particles/cells
  • what is simulated
  • initial conditions (linked to target)
    • glassy
    • cosmological (initial redshift)
    • galaxy disk in equilibrium
    • galaxy merger configuration
    • galaxy cluster in hydrostatic equilibrium
  • resolution (not trivial to define)
    • size smallest grid cell
    • smallest smoothing radius SPH particles
    • gravitational (plumber) smoothing length
  • what is in results, mainly:
    • point particles
    • SPH particles
    • (adaptive) mesh cells
  • log files (for Flash in particular) very useful

 
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Revision 22009-06-18 - GerardLemson

 
META TOPICPARENT name="IVOATheorySimDBDMDiscussion"
Added:
>
>		[ back ]
 
Changed:
<
<		Thanks to Marcus Brueggen...
>
>		(notes made during conversation with Marcus Brueggen on use of a
Added:
>
>		simulation database)
 
Changed:
<
<

>
>		Would like to be able to get information/query on:
  • size of box
  • time scales
  • physics used:
Added:
>
>
    • star formation
    • cosmology
    • hydro
    • particles
    • chemical reactions
    • nuclear reactions
    • gravity
    • radiation
    • MHD
    • cosmic rays
    • feedback
    • ...
  • algorithms used:
    • mesh resolution
    • amr
  • how many particles/cells
  • what is simulated
  • initial conditions (linked to target)
    • glassy
    • cosmological (initial redshift)
    • galaxy disk in equilibrium
    • galaxy merger configuration
    • galaxy cluster in hydrostatic equilibrium
  • resolution (not trivial to define)
    • size smallest grid cell
    • smallest smoothing radius SPH particles
    • gravitational (plumber) smoothing length
  • what is in results, mainly:
    • point particles
    • SPH particles
    • (adaptive) mesh cells
  • log files (for Flash in particular) very useful
  


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Revision 12009-06-18 - GerardLemson

 
META TOPICPARENT name="IVOATheorySimDBDMDiscussion"

Thanks to Marcus Brueggen... 


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