Changes between Version 11 and Version 12 of ModulesOnAstroBear

Timestamp:

07/12/11 19:18:51 (14 years ago)

Author:

ehansen

Comment:

—

ModulesOnAstroBear

@@ -52 +52 @@
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+The best way to understand how a module works is by example. The following example is a module for the Rayleigh-Taylor instability.
+
+{{{
+Place sample module here
+}}}
+
 ==== Simulation Data ====
 
@@ -59 +65 @@
 }}} 
 
-There are two major data arrays in {{{InfoDef}}}: the {{{q}}} array and the {{{aux}}} array.  {{{q}}} holds the cell-centered data and is used by all AstroBEAR simulations.  The {{{q}}} array takes the form {{{q(x,y,z,variable}}} where {{{variable}}} is itself a 1D array that holds the physical quantities such as density, momentum, energy, etc. The order of the quantities in the {{{variable}}} array is {{{(rho, px, py, pz, E)}}}. The {{{aux}}} array holds face-centered data, and is only used in MHD problems.  If you are running a strictly hydrodynamic problem or a hydrodynamic + elliptic problem, then you will not need {{{aux}}}.
+There are two major data arrays in {{{InfoDef}}}: the {{{q}}} array and the {{{aux}}} array.  {{{q}}} holds the cell-centered data and is used by all AstroBEAR simulations.  The {{{q}}} array takes the form {{{q(x,y,z,variable)}}} where {{{variable}}} is itself a 1D array that holds the physical quantities such as density, momentum, energy, etc. The order of the quantities in the {{{variable}}} array is {{{(rho, px, py, pz, E)}}}. The {{{aux}}} array holds face-centered data, and is only used in MHD problems.  If you are running a strictly hydrodynamic problem or a hydrodynamic + elliptic problem, then you will not need {{{aux}}}.
 
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