[FLASH-USERS] FLASH 4.3 Release

Fri Jul 17 21:24:52 EDT 2015

Dear Users,

 The Flash Code Group announces the release of an updated version of 
the FLASH code, version 4.3.

This update has a moderate amount of changes from FLASH 4.2.2, and a 
number of new features.

The release is available as a tarball FLASH4.3.tar.gz, in the usual 
location on the Flash Center Web site at http://flash.uchicago.edu/.
The updated RELEASE-NOTES file is attached.

Best,
-- the Flash Center Code Group
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!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!  New in FLASH 4.3 (since FLASH 4.2.2) - July 2015  !!!!! 
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!

* Flux-limited-diffusion for radiation (implemented in
  RadTransMain/MGD) is now available for astrophysical
  problem setups:

  + MatRad3 (matter+rad [2T] stored in three components)
    implementations for several Eos types: Gamma, Multigamma,
    and (experimentally) Helmholts/SpeciesBased.
  + Implemented additional terms in FLD Rad-Hydro equations
    to handle streaming and transition-to-streaming regimes
    better - including radiation pressure.
    This is currently available as a variant of the unsplit Hydro
    solver code, under HydroMain/unsplit_rad .
    We call this RADFLAH - Radiation Flux-Limiter Aware Hydro.
    Setup with shortcut +uhd3tR instead of +uhd3t .
    This has had limited testing, mostly in 1D spherical geometry.
  + New test setups under Simulation/SimulationMain/radflaHD:
    BondiAccretion, RadBlastWave
  + Various fixes in Eos implementations.
  + New "outstream" diffusion solver boundary condition for
    streaming limit. (currently 1D spherical only)
  + Added Levermore-Pomraning flux limiter.
  + More flexible setup combinations are now easily possible -
    can combine, e.g., species declared on setup command line
    with SPECIES in Config files and initialized with
    Simulation_initSpecies, by setup with ManualSpeciesDirectives=True .
  + Created an "Immediate" HeatExchange implementation.
  + EXPERIMENTAL: More accurate implementation of flux limiting
    (and evaluation of diffusion coeffs): apply limiter to
    face values, not cell centered values.
  + EXPERIMENTAL: ExpRelax variant of RadTrans diffusion solver,
    implements the algorithm described in Gittings et al (2008)
    for the RAGE code, good for handling strong matter-radiation
    coupling; for one group (grey) only.
  + EXPERIMENTAL: Unified variant of RadTrans diffusion solver,
    for handling several coupled scalar equations with HYPRE.
  + EXPERIMENTAL: More accurate implementation of flux limiting
    (and evaluation of diffusion coeffs): apply limiter to
    face values, not cell centered values.

* New unit ProtonImaging: The new unit is a simulated 
  diagnostic of the Proton Radiography used in HEDP experiments.

* Gravity can now be used in 3T simulations.

* Laser Energy Deposition:
  New ray tracing options added based on cubic interpolation techniques.
  Two variants: 1) Piecewise Parabolic Ray Tracing (PPRT) and 2) Runge
  Kutta (RK) ray tracing.

* Introduction of new numerical tool units: 1) Interpolate: currently
  contains the routines to set up and perform cubic interpolations
  on rectangular 1D,2D,3D grids, 2) Roots: (will) contain all routines
  that solve f(x)=0 (currently contains quadratic, cubic and quartic
  polynomial root solvers, 3) Runge Kutta: sets up and performs Runge
  Kutta integration of arbitrary functions (passed as arguments).

* Unsplit Hydro/MHD: Local CFL factor using CFL_VAR.
  (Declare a "VARIABLE cfl" and initialize it appropriately.)

* Unsplit Hydro/MHD: Significant reorganization.
  + reorganized definition and use of scratch data. Memory savings.
  + use hy_memAllocScratch and friends.
  + hy_fullRiemannStateArrays (~ instead of FLASH_UHD_NEED_SCRATCHVARS)
  + New runtime parameter hy_fullSpecMsFluxHandling, default TRUE.
    resulting in flux-corrected handling for species and
    mass scalars, including USM.
  + Use shockLowerCFL instead of shockDetect runtime parameter.
  + Revived EOSforRiemann option.
  + More accurate handling of geometric effects close to the origin
    in 1D spherical geometry.

From External Contributors:

* Sink particle update by Christoph Federrath.
  Major changes: removed call to fill guardcell
  in Particles_sinkCreateAccrete.F90. Merged
  Particles_sinkAccelGasOnSinks.F90 and
  Particles_sinkAccelSinksOnGas.F90 into a new routine called
  Particles_sinkAccelGasOnSinksAndSinksOnGas.F90, which computes sinks
  -> gas and gas -> sinks gravitational interactions in one go/loop
  for performance enhancement. Added support for off-domain sink
  particles, i.e., if the user switches on the runtime parameter
  sink_offDomainSupport, then sink particles remain active when they
  cross a domain boundary in case of outflow boundary conditions,
  i.e., they are not deleted. This can be useful for some special
  applications. The gravity between sinks and between gas and sinks
  remains active and I/O of sink particles outside the domain also
  remains active.

* Updates to Barnes-Hut-Tree and related code from Richard Wunsch.
  TreeCol dummy unit has been replace by TreeRay, which includes
  an implementation.

* Placeholders fo UserDefined Gravity and Simulation_freeUserArrays stub
  (John ZuHone)

* Updates for using spherical with split (PPM) hydro solver.
  (Rodrigo Fernandez - not tested by us)

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!  New in FLASH 4.2.2 (since the FLASH 4.2.1 patch)  !!!!! 
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!

* Eliminated unnecessary reconstruction calls for some guard cells
  in unsplit Hydro and staggered mesh MHD. This affects all unsplit
  Hydro and MHD calls and can result in a significant speedup,
  most noticeable for 3D PPM Hydro with small block sizes.

* New implementations for Lee & More (Phys. Fluids 1984, 27, 1273)
  electron conductivity and heat exchange, contributed by Chris Orban.
  These implementations can be used instead of their equivalent
  SpitzerHighZ and Spitzer options and should return more accurate
  results at low temperatures in 3T simulations.

* Changes in MagneticResistivity unit: uses calls that pass the
  full state. Resistive fluxes are now calculated by central
  differencing. The resistive coefficient is no longer upwinded.
  Support for cylindrical geometry added to unsplit Hydro
  implementation.

* Fixed bug where abundances could become negative for 3T setups.

* Updates to sink particle code contributed by C. Federrath.

* Improved time stepping for unsplit Hydro (or MHD) in connection
  with self-gravity and massive (including sink) particles.
  In this as in previous releases, the unsplit Hydro invocation
  calls the gravity solver at the end to apply gravitational
  accelerations in a time-centered manner; now, the code
  avoids updating the state of the global "gpot" variable
  in the course of this gravity solve, if such updating
  might interfere with the assumptions of Particles_advance.
  Also, the unsplit Driver_evolveFlash routine now avoids
  calling the gravity solver again at the end of each time
  step if the global "gpot" has already been updated earlier
  in the time step.
  New optional arguments have been added to the
  Gravity_potentialListOfBlocks and Gravity_accelOneRow
  API to support the improved behavior.

* Fixed allocated size of yCenter(:) in unsplit Hydro code for
  non-Cartesian coordinates.
  Fixed allocated size of xcent(:) in Noh_unitTest.

* Avoid access to invalid cells when BDRY_VAR is defined.
  Use stencil large enough for computing velocity divergence
  if use_hybridOrder is set and for computing flattening
  coefficients is use_flattening is set. All these changes
  can affect unsplit Hydro and staggered mesh MHD.

* Improvements to WENO reconstruction in unsplit Hydro and staggered
  mesh MHD. Introduced new runtime parameter, wenoMethod, that takes
  wenoMethod = "weno5" (default) or "wenoz".  The WENOZ method is a new
  reconstruction algorithm based on R. Borges et al., JCP, 227 (2008)
  3101-3211 and Don & Borges, JCP, 250 (2013) 347-372. Moreover, WENO
  now works with the usual 4 layers of guard cells and does not require
  increasing NGUARD to 6.

* Fixed beavior of staggered mesh MHD with the E_upwind flag enabled.
  Upwinding for the electric field is now always based on the previous
  time cell-centered state and simulation restarts work
  transparently.

* Globally reduce CFL factors from different MPI tasks before
  computing the time step for unsplit Hydro and staggered mesh MHD.
  This may affect simulations where one of the following applies:
  (a) RiemannSolver = "HYBRID", (b) use_hybridOrder = .TRUE.;
  time steps will now be independent of the number of tasks.

* Some array size optimizations for saved fluxes in unsplit Hydro
  (reduced memory footprint).

* Avoid problems with large (double precision) constants in
  Config files. Now the forms 1.d99 and 1.e99 can both be used
  for runtime parameter default values with large exponents.

* Eliminated some unnecessary "include" calls to speed up recompilations.
  Tweaks to speed up recompilation on MacOS-like file systems.

* Documentation fixes and updates in various source files.
  Eliminated unused variables in some files and similar cleanup.

* Protect against obscure failure when zmin = zmax in 2.5D simulations.

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!  New in FLASH 4.2.1 (since the FLASH 4.2 release)  !!!!! 
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!

* Fix of Gravity problem in unsplit Hydro / MHD:
  Do not call Eos in auxiliary invocation of guard cell filling.

* Fix of problems in WENO reconstruction in unsplit Hydro / MHD.

* Minor changes to prevent compilation failures in some
  environments.

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!  New in FLASH 4.2  (since the FLASH 4.0.1 patch)   !!!!! 
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!

Added CCSN physics from Sean Couch:
* Complete nuclear EOS routines (physics/Eos/EosMain/Nuclear)
* Local neutrino heating/cooling (physics/sourceTerms/Heat/HeatMain/Neutrino)
* Multispecies neutrino leakage (physics/RadTrans/RadTransMain/NeutrinoLeakage)
* Multidimensional Core-Collapse supernova test problem
  (Simulation/SimulationMain/CCSN)

Contributed by Dean Townsley, with code developed by Aaron Jackson and 
Alan Calder:
* physics/sourceTerms/Flame unit
* physics/sourceTerms/Turb unit

* Updates to Barnes Hut tree gravity solver contributed by Richard Wunsch,
  developed in collaboration with Frantisek Dinnbier (responsible for periodic
  and mixed boundary conditions) and Stefanie Walch.

Contributed by Christoph Federrath:
* Significant updates for Sink Particles
* New 'FromFile' implementation of Stir unit, now sitting beside the older
  'Generate' implementation

Two new optimizations of the unsplit solvers, Hydro_Unsplit and MHD_StaggeredMesh,
in source/physics/Hydro/HydroMain/unsplit. These new optimized unsplit solvers
are the default implementations of the unsplit hydrodynamics and MHD solvers
in FLASH 4.2. The old version of the unsplit solvers are now found in 
source/phycis/Hydro/HydroMain/unsplit_old.

Capabilities for 3T magnetohydrodynamics, for the first time.

New magnetic resistivity implementation, Spitzer HighZ, for HEDP problems.
Extended support for resistivity in cylindrical geometry in the unsplit solver.  

Laser - Async communication (experimental), some reorganization.
New feature - can run EnergyDeposition once every n time steps.

Updates to HYPRE solver coupling - avoid communicator leak with 2.0.9b.
Some changes in MGD code for increased correctness.

Threading for unsplit MHD is now available. Both strategies are supported by the new code. 

New, improved multipole Poisson solver, implementing the algorithmic 
refinements described in Couch, S.M., Graziani, C., and Flocke, N., ApJ 778, 
181 (2013), http://dx.doi.org/10.1088/0004-637X/778/2/181, 
http://arxiv.org/abs/1307.3135.  Specifically:
* Potential calculated at cell faces and averaged to produce cell-centered
  values, rather than directly at cell centers, so as to eliminate a convergence
  failure due to cell self-gravity
* Expansion center located at "square-density-weighted center-of-mass", to 
  minimize angular power at high multipoles

(smaller changes:)
* The code includes stubs for several additional code units for which
  we do not include implementations in this release (TreeCol, NSE,
  SolidMechanics, IncompNS, ImBound). Implementations may be available
  separately from their authors, and / or may be included in a future
  FLASH release.
* Hydro codes avoid unnecessary Eos calls on guard cells, this uses skipSrl
  flag to Eos_guardCells routine.
* Improved HLLD solver on MHD degeneracy.
* PARAMESH's facevariable handling for divergence-free magnetic field
  enforcement now uses gr_pmrpForceConsistency=.true. and
  gr_pmrpDivergenceFree=.true. by default.
* New Grid_bcApplyToRegionMixedGds API allows users to implement boundary
  conditions that take several types of solution variables (CENTER, FACE)
  into account.

Caveats, Limitations
--------------------

Simulations results obtained with this version of FLASH should not be
expected to match exactly with results from previous versions.
Differences can be due to algorithmic changes in solvers, in particular
the unsplit Hydro and MHD implementations. Results from simulations that
use the HYPRE library for Diffusion and/or RadTrans operators may be
slightly different because we invoke HYPRE with slightly different
parameters (based on suggestions from HYPRE authors).
Another source of unexpected differences is a change in how we compute
block boundary coordinates when an AMR Grid starts with more than one
root block (i.e. any of NBlockX,NBlockY,NBlockZ > 1), leading to
a difference in rounding errors under some scenarios.

Several code units have provisions for being threaded (OpenMP directives),
but these have not been recently tested and may require some adaptation.

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!  Fixes to FLASH 4.0 included in FLASH 4.0.1 patch  !!!!! 
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!

*** HYPRE Fix ***

* A non-symmetric matrix could be generated by our AMR HYPRE adapter
  in certain situations, leading to failure to converge in PCG solver.
  The constructed matrix was not symmetric, because there was a
  mismatch between the order in which graph edges where created and
  given values for some cells.  This only affected coarse cells that
  have finer neighboring cells across more than one cell face.

  Only changed file: source/Grid/GridSolvers/HYPRE/paramesh/gr_hypreSetupGrid.F90
  r18739

*** PFFT Fixes ***

* PFFT fixes for unusual pencil grid configurations.
  We have found errors when the global number of grid points along a
  particular dimension is not a multiple of the number of MPI ranks in
  the PFFT MPI cartesian communicator in the same dimension.  This
  situation did not always cause problems, but errors could be
  introduced in particular when using PFFT in combination with
  Multigrid ("Hybrid Multigrid") as a Poisson solver and when
  there was
* a small number of Paramesh blocks per pencil process, and/or
* a prime number of pencil processes which own Paramesh blocks at
  the refinement level of the PFFT grid.
  Fixes apply to DirectSolver and HomBcTrigSolver.
  Bug reported by: Mateusz Ruszkowski 2013-01-21

* Only MPI ranks which are part of the pencil process grid should
  access certain arrays.  In the previous implementation there are
  accesses to unallocated arrays by the MPI ranks which are not part
  of the PFFT process grid.  The patch avoids undefined behavior.

* Use the correct communicator, pfft_comm(IAXIS) instead of gr_meshComm.
  Avoids possible hang with DirectSolver.

* Change in gr_pfftInitMetaData.F90 addresses a problem with
  DirectSolver/SecondOrder_FD3p (not normally used). Added some lines
  of diagnostic output.

  r18725,r18735,r18736,r18949,r18970,r18972

  NOTE: For Hybrid Multigrid configurations, we now recommend using
  the HomBcTrigSolver variant of PFFT. To do this, eliminate explict
  references to "DirectSolver" and use "PfftSolver=HomBcTrigSolver"
  on the setup command line.

*** Barnes-Hut Tree Solver Fixes ***
* Several bug fixes of the BHTree solver. The bugs could lead to
  code crashes in case of non-cubic computational domains.
  Corrected some size calculations.
  Grid_solvePoisson now uses the poisfact argument.
  Generalized BHTree code to not assume in some places that the
  source variable is DENS_VAR.
  Contributed by: Richard Wunsch, John ZuHone
  r17970,r18021,r18825,r19041,r19097

*** Active Particles Time Advancement Fix ***
* Fixed a long-standing bug in active particle time advancement, where
  the old timestep was being used to advance the particle positions
  instead of the current one. This only affects active particles with
  mass that are being advanced using the leapfrog time advancement
  routine (without cosmology).
  Contributed by: John ZuHone
  Only changed file: ../ParticlesMain/active/massive/Leapfrog/pt_advanceLeapfrog.F90
  r18678

*** Misc Fixes related to Hydro / MHD ***

* Fixes in explicit viscosity for split (PPM) Hydro.
  Bug reported by: Elke Roediger 2012-11-07
  Only changed file: source/physics/Diffuse/DiffuseFluxBased/Diffuse_visc.F90
  r18212

* Indexing error in guard cell filling for face variables (3D Staggered Mesh MHD).
  Bug reported by: Mateusz Ruszkowski 2012-11-07
  Only changed file: .../Paramesh4dev/PM4_package/source/amr_1blk_guardcell_srl.F90
  r18220

* Modified current calculation when adding resistive fluxes for Staggered Mesh MHD.
  Only changed file: .../unsplit/MHD_StaggeredMesh/hy_uhd_addResistiveFluxes.F90
  r18170

*** Misc Infrastructure Fixes ***

* Fix for inexact block boundaries.
  When runtime parameters nBlockX, nBlockY, or nBlockZ are different
  from 1, rightmost block boundaries are computed in a way that may
  make their values differ slightly from rightmost domain
  boundaries. The preferred change (to be included in a future FLASH
  release) is to change the way block boundaries are computed, but
  that can introduce unexpected differences in checkpoint files; here
  we just modify some code to use comparison with a tolerance, instead
  of testing for exact equality, when detecting boundaries.
  r18053

* Avoid accessing optional logical dummy arguments when they are not
  present.  One must not assume short-circuit evaluation of logical
  expressions in Fortran.
  Only changed file: source/Grid/GridMain/paramesh/Grid_getListOfBlocks.F90
  r18896

!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!  Original RELEASE-NOTES file for FLASH 4.0 follows  !!!!!
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
The Flash Center is pleased to announce the release of the next
version of the FLASH code, version 4.0. FLASH 4.0 closely follows 
the architecture of FLASH3. The major changes from FLASH3 are
several new capabilities in both physics solvers and infrastructure.
A major part of the new physics capabilities were introduced to
support simulations of high-energy-Density physics (HEDP).
FLASH4 also includes four major capabilities contributed by our
external users. 

The major new capabalities in FLASH4 that were not included in FLASH 3
are (the ones marked with **  are external contributions, please see the
User's Guide for references and appropriate credit for these capabilities): 

* 3T capabilities in the split and unsplit Hydro
  solvers. There is support for non-cartesian geometry, and
  the unsplit solver also supports stationary rigid bodies.

* Upwind biased constrained transport (CT) scheme in the unsplit
  staggered mesh MHD solver.

* Full corner transport upwind (CTU) algorithm in the unsplit
  hydro/MHD solver \item Cylindrical geometry support in the unsplit
  staggered mesh MHD solver on UG and AMR. A couple of MHD
  simulation setups using cylindrical geometry. 

* Radiation diffusion

* Conduction 

* Heat exchange.

* Multi-Temperature Multi-Material Multi-Table Eos

* Opacities, ability to use hot and cold opacities.

* The laser drive with threading for performance

* A new multipole solver

* Ability to replicate mesh for multigroup diffusion or other
  similar applications.

* OpenMP threading of several important solvers at both
  coarse-grain (one block per thread) and fine-grain (threads within a
  block) levels.

* Ability to add particles during evolution

* Limited support for Chombo as an alternative AMR mesh package

* Several new HEDP simulation setups.

* Hybrid-PIC    **

* Barnes-Hut tree based gravity solver  **

* Primordial chemistry  **

* Sink Particles  **

The release also includes several new features and resolves many bugs
found in previous releases up to 4-beta. The modifications since the
4-beta release include 

* The HEDP capabilities of the code have been exercised more and are
  therefore more robust.

* Laser 3D in 2D ray tracing has been added. The code traces rays in a real 3D
  cylindrical domain using a computational 2D cylindrical domain and is based
  on a polygon approximation to the angular part. 

* New public interface Particles_addNew, which makes it possible to
  add particles to a simulation during evolution. (It has been
  possible to include multiple different types of particles in the
  same simulation since release FLASH 3.1.)

* Fixed reading of particles from checkpoint in -nofbs uniform grid. 

* All I/O implementations now support writing/reading 0
  particles and/or 0 blocks. 

* Support for particles and face variables in the same PnetCDF simulation.

* Optimization of Initialization.
  Eliminated redundant calls to orrery at simulation startup.
  Ability to run the orrery in a reduced communicator in order to
  speed up FLASH initialization.  The original orrery can be restored
  by setting the parameter use_reduced_orrery to .false..  

* Ability to avoid unnecessary calls of guard cell filling.
  Ability to avoid a subsequent guard cell fill when a unit declares
  that it only reads mesh data.  It is off by default, but can be
  turned on by setting the parameter reduceGcellFills to .true..  

There are a few other changes from the beta release :

* Removed custom region code and Grid API routines. 

* PARAMESH4DEV has become the default Grid implementation.  

* PARAMESH4DEV does not need an amr_runtime_parameters file
  any more.  The corresponding parameters are now set in
  a parameter file, like other FLASH runtime parameters. 

The following features are provided on an EXPERIMENTAL basis.
They may only work in limited circumstances and/or have not
yet been tested to our satisfaction.

* New EXPERIMENTAL configuration tool, "setup_alt".  
  Intended to be a compatible replacement for "setup" with
  a cleaner structure.

* Electron-Entropy Advection in Hydro for non-ideal Eos.  

* New cubic and quartic equation solvers have been added and
  are ready to be used. They return only real cubic and quartic roots.
  The routines are in the flashUtilites/general section and their
  names are: 'ut_cubicRealRoots' and 'ut_quarticRealRoots'. 

Known Limitations in FLASH 4.0:

* The new multipole solver is missing the ability to treat
  a non-zero minimal radius for spherical geometries, and the
  ability to specify a point mass contribution to the potential.

* Usage of the Split diffusion solver in FLASH4 is only for debugging
  purposes and not generally recommended for usage.
  Split diffusion has not been tested with PARAMESH.

* Some configurations of hydrodynamic test problems with Chombo grid
  show worse than expected mass and total energy conservation.  Please
  see the Chombo section in Hydro chapter of the FLASH user guide for
  details.

* We have experienced the following abort when running
  IsentropicVortex problem with Chombo Grid:
  "MayDay: TreeIntVectSet.cpp:1995: Assertion `bxNumPts != 0' failed. !!!"
  We have been in contact with the Chombo team to resolve this
  issue.

* The Absoft compiler produces erroneous results with optimization in
  gr_markRefineDerefine routine. The results are fine without
  optimization. There may be other files with similar behavior, but
  this is the only one we are aware of.

* The PG compiler fails to compile source files which contain OpenMP
  parallel regions that reference threadprivate data.  This happens in
  the threaded versions of the Multipole solver and the within block
  threaded version of split hydro.  A workaround is to remove
  "default(none)" from the OpenMP parallel region.

* The unsplit MHD solver doesn't support the mode "use_GravPotUpdate=.true."
  for 1D when self-gravity is utilized. The solver will still work if it
  is set to be .false. In this case the usual reconstruction schemes 
  will be used in computing the gravitational accelerations at the 
  predictor step (i.e., at the n+1/2 step) rather than calling the
  Poisson solver to compute them.

* The -index-reorder setup flag does not work in all the configurations.
  If you wish to use it please contact the FLASH team. 

The release is available at:

http://flash.uchicago.edu/site/flashcode/

A stripped-down version of FLASH3 that may be downloaded without a
license is also available at the same site. 
This version is essentially the FLASH framework without any
implementations.  The Flash Center is also providing support for
"add-ons" to the code. Please see the section on "What's new in this
release" in the first chapter of the User's Guide for details.
Also, a collection of stand-alone mini-apps are available for download
under the general FLASH license from the same site. 

Additionally, the FLASH testing software FlashTest, which became
available with the FLASH3 beta release, continues to be available for
download at:

http://flash.uchicago.edu/site/flashcode/

Many, but not all parts of FLASH4 are backwards-compatible with
FLASH2. There are no architectural changes from FLASH3 to FLASH4. The
Flash code group has written extensive documentation 
detailing how to make the transition from FLASH2 to FLASH3 as smooth
as possible.  The user should look to:

http://flash.uchicago.edu/site/flashcode/user_support/

The website also contains other documentation including
a User's Guide and a developer's section.  A new feature in FLASH3
documentation is the online description of the public interface
routines to various code units.

FLASH should be portable to most UNIX-like operating systems with a 
python interpreter, Fortran 90 compiler,  C compiler, and MPI library. 
It has been used in production mode, or undergone regular testing on            
the following platforms. 

-- IBM BlueGene/P and Power5

   compilers : FORTRAN90 : xlf90

               C         : xlc

-- CRAY-XT4 system

   compilers : FORTRAN90 : Portland Group Fortran 90

               C         : gcc

-- Linux

   compilers: FORTRAN90 : Portland Group Fortran 90

                          Lahey/Fujitsu Fortran 95 

                          Intel Fortran Compiler

                          gFortran (known to have trouble with versions
                              before 4.1.0)

                          NAGWare Fortran 95

                          Absoft 

              C         : gcc

                          Portland Group C Compiler

                          Intel C++ Compiler       

-- MAC-OSX

   compilers : FORTRAN90 : gFortran

               C         : gcc

FLASH uses libraries such as MPI for communication, Paramesh
and Chombo for AMR, HDF5 or PnetCDF for IO, and Hypre for linear
solvers. The source for Paramesh 4 is included in two variants in the 
distribution; the versions included in this release are
equivalent to Paramesh 4.0 and Paramesh 4.1, respectively.
Some earlier versions of HDF5, for example 1.6.1, have been known to
have issues with FLASH. We recommend using version 1.6.2 or higher of
the HDF5 library.

Two options are available to visualize FLASH output data. One is 
Fidlr, the IDL based visualization tool included in the
distribution. Fidlr requires IDL version 6.1 or higher to work correctly.
A more extensive option is VisIt, a visualization tool from LLNL,
available from

http://flash.uchicago.edu/site/flashcode/visit and
https://wci.llnl.gov/codes/visit

Visit supports FLASH data output Format.Information on using
Visit with FLASH is contained on the website above.

Development of the FLASH Code was funded by the DOE-supported
ASC/Alliance Center for Astrophysical Thermonuclear Flashes,
and continues to be funded by DOE NNSA and NSF.  We
acknowledge support received from Lawrence Livermore National
Laboratory and the University of Chicago.

All publications resulting from the use of the FLASH Code must
acknowledge the Flash Center for Computational Science.
  Addition of the following text to the paper acknowledgments
will be sufficient.

         "The software used in this work was in part developed by the
         DOE-supported Flash Center for Computational Science
         at the University of Chicago."