!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.7.1 (since FLASH 4.7) !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! * Added missing FL_NONE flux limiter for time step calculations in extended MHD that use the Nernst term. * Removed deprecated local log-lambda subroutine from Spitzer magnetic resistivity unit that could cause some compile issues. * Corrected calls to PlasmaState_tau in hy_uhd_computeDtExtMHD. * Ion viscous heating in hy_uhd_ragelike now uses the correct scratch variables in hydro & MHD. * Fixed improper memory deallocations in eos_idealgamma3T when set up with multitype EoS in non-fixed block size uniform grids. * Fixed bug in implicit magnetic diffusion HYPRE solver that only allowed diffusion of MAGX. * Updates to SESAME EoS table reader to use geometric spacing in the interpolated density/temperature grids as well as a species runtime parameter to specify the double format of the table (defaults to E22.15). * Made consistent all the output of the Circuit unit (Circuit.dat) so all data uses the same time centering. * Fixed bug in Thomson Scattering diagnostic that occurred when compiled in debug mode. * Modified fast magnetosonic speed calculation in timestep computation to avoid negative numbers. !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.7 (since FLASH 4.6.2) !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! * LaserRayTrace and ThomsonScatteringMain/WithRayTracing: 3D-cylindrical ray tracing; other ray tracing changes. (experimental) * Boundary condition aware \code{LaserRaysCreate} routines that allow rays to enter from periodic/reflecting boundaries with appropriate symmetry transformations. * Support for 3D cylindrical geometry: split and unsplit Hydro, (experimental) * Reorganize flux correction for the staggered mesh MHD implementation so that MagneticResistivity can be used with conserveAngField disabled in cylindrical coordinates. * Enhancments in implicit solves: * Anisotropic thermal conduction now supports; AMR grids with PARAMESH, as well as slope limiting to avoid unphysical temperature changes. * Periodic boundary conditions are now supported in implicit HYPRE solvers. * We have added an operator split HYPRE solver for implicit magnetic diffusion on uniform grids. * We have add the full Braginskii extended-MHD terms in the generalized Ohm's law for the unsplit staggered mesh hydro solver, including: * Full Anisotropic Magnetic Resistivity * UG +AMR * $\eta_{\parallel}$ * $\eta_\perp$ * $\eta_\wedge$ * Hall * Nernst * Seebeck * cross-field term * Biermann * The Biermann solver now has a symmetrized use of SHOK_VAR (previously left-biased) * New \code{materialProperties} implementations of transport coefficents, including: * Ji \& Held - thermal conduction * Davies \& Wen - thermal electric \& resistivity * Spitzer Viscosity * New multi-species API for calculating $Z^2$ * Fixed bug in calculation of $\tau$ for Epperlein \& Haines * Consolidate older implementations to use $Z_{\text{eff}}$ * We have implemented a Current Drive Unit that implements a magnetic field boundary condition for modeling Z-pinch experiments using a variety of models for the current drive. * This includes a circuit model that can model systems like the Z-machine and CESZAR. * We have added native readers in FLASH for tabulated data, including the LANL SESAME format for EoS and the LANL TOPS format for opacities. * The unsplit hydrodynamics solver has been updated with the option for a volume-of-fluid interface capturing scheme for maintaining sharp material interfaces. Available for 1D/2D uniform grids in Cartesian geometry. * The I/O routines have been updated for compatibility with Open-MPI 3. * The python scripts, including \code{setup}, have been updated to be fully compatible with Python3. !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.6.2 (since FLASH 4.6.1) - October 2019 !!! !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! * For unsplit Hydro with curvilinear coordinates we have improved the computation of velocity divergence used in determining the strength of artificial viscosity (when use_avisc is TRUE). The effects of artificial viscosity can be expected to change, particularly in cells close to the coordinate axis in 2D cylindrical coordinates. * Corrected wrong order of operations in an MHD code path when using flux correction: energy corrections (proper accounting of magnetic energy in cells) could be applied too late in interior cells. The problem only occurred in 1D MHD configurations (with the MHD_StaggeredMesh code), which could then lead to errors in results of 3T simulations. * Corrected wrong Eos mode in Eos_wrapped calls, as well as energy adjustment, in the Biermann battery source term code. * LaserRayTrace and ThomsonScatteringMain/WithRayTracing: Improved ray tracing in situations where rays enter the computational domain in locations that have significant electron density by adding ray speed adjustment at domain entry. * Fixed some problems in Multitype EOS that showed up in tests with non-fixed-blocksize uniform grid mode. Convergence of root search should now be improved in some EOS modes. * Slightly improved time step computation for anisotropic diffusion (Uniform Grid). * FLASH now requires being compiled against MPI version 2 or higher. Some setups continue to work when compiled against an MPI-1 library, but this will not be true in general. !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.6.1 (since FLASH 4.6) - June 2019 !!!! !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! * Correct Ohmic heating term for nonideal MHD in hy_uhd_unsplitUpdate: multiplication by density was wrong. * New runtime parameter for optionally specifying laser beam intensities in 1D and 2D Cartesian simulations in a more natural way (namely by specifying the power profile of beams always by giving beam power, not power per length or area unit). * Enabling and updating XrayImaging unit, includes new unit tests. * Fix occasional generation of invalid refinement pattern by PARAMESH in 2D and 3D spherical coordinates. * Some tweaks to make setup work better with Python3; includes removing 8bit characters, TAB character consistency. * The setup command has a new option -append-parfiles to make it easier to build up a set of runtime parameter from parts kept in separate places. * Improved detection of case-insensitive file system by setup, to avoid unnecessary recompilation by make in some Docker environments. * Disabled use of 1D profile in default configuration of Sedov example. !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.6 (since FLASH 4.5) - March 2019 !!!! !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! FLASH CODE: * Implementation of new nonideal MHD effects: Hall term (Cartesian 1d/2d/3d and cylindrical 2d), and Biermann battery (Cartesian 2d/3d and cylindrical 2d) as a source term and a flux-based formulation for 3T. * Corrections on SpitzerHighZ magnetic resistivity. Now using the NRL plasma formulary equation. * New high-order reconstruction methods in unsplit Hydro / MHD solvers: - PCM: Piecewise Cubic Method, see Lee et al, JCP 341, 230, 2017 - GP: Gaussian Process, see Reyes et al., JCP 381, 189, 2019; Reyes et al., JSC 76, 443, 2018 * Added support for anisotropic thermal conduction. Anisotropic conductivities depend on the direction of a magnetic field, so anisotropic conduction is meant to be used together with MHD. Currently only available with the uniform Grid (UG) implementation. * New implementation for simulated Thomson scattering experimental diagnostic using ray tracing. (source/diagnostics/ThomsonScattering) * Implementation of X-ray imaging simulated experimental diagnostic using ray tracing. (source/diagnostics/XrayImaging) * Implementation of proton emission simulated experimental diagnostic using ray tracing. (source/diagnostics/ProtonEmission) * Enabled support for 1D cylindrical laser energy deposition. * Applied all known patches for working with HDF5 versions 1.10.x. * Compatibility updates to the setup utility so it works with Python2 and Python3 versions. * Updated various Config files for Python3 compatibility: Minimal changes necessary include replacing comparison operator '<>' by '!=', and 'xrange()' by 'range()' in Config files interpreted by Python. * PhysicalConstants unit now supports conversion of base units, e.g., call PhysicalConstant_get("amu",unitMass="g"). !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.5 (since FLASH 4.4) - December 2017 !!!! !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! * New implementation for synthetic Thomson scattering simulated diagnostic. * A new 1D simulation of a 2-temperature Supernova evolution using the flux- limiter-aware hydro treatment of radiation, and related code changes. * A new timestep limiter, which ensures that a given list of variables remains positive-definite during hydrodynamic advection. This can be used as an alternative to lowering the Hydro unit's CFL runtime parameter, and has been shown useful for 3T simulations in particular, where non-conservative equations are considered. This will obviate negative temperature errors when using 3T Hydro and MHD. See the Driver section of User's Guide for more information. * Expanded the Sedov simulation to be initialized from a quasi- analytical profile, and added diagnostic variables to keep track of various simulation error measures. * New flux limiter "vanLeeer1.5" for unsplit Hydro and MHD. * Fixed an issue in which PARAMESH block distribution failed to settle down because of message delay, reported for some machines. This is done by inserting sleep(1.) calls in extreme cases. * Implement saving of laser irradiation (to "lase" variable) for 2DCyl3D ray tracing, too. Previously was 3D only. * Ray tracing fixes: avoid stalls; improved randomness; correct an error in ray weights and beam power in 2D cylindrical rays with statistical1D grids. * Unsplit Hydro fixes for rarely used 2D POLAR geometry. * FLASH now works correctly with HDF5 versions 1.10.x. * FLASH now assumes by default that it is being compiled against MPI version 2 or higher. If you must compile against an MPI-1 library, define the preprocessor symbol FLASH_MPI1 for your Fortran compiler. * More conservative defaults in header file FortranLangFeatures.fh. * We have included detailed instructions that outline how to easily install FLASH on Windows, Mac OS, and Linux distributions, using Docker. See the "Quick Start" section in the User's Guide. OTHER: * FLASH Interface is a new graphical interface (GUI) for managing parameter files. and is now available for download. The code was developed by Christopher Walker (cnwalker@uchicago.edu). It currently supports: - Configuring and editing existing flash.par files; - Generating new flash.par files by choosing among the full set of possible parameters; - Filtering the full set of possible FLASH parameters (found in setup_params) via categories; - Searching for FLASH params by name, and viewing full descriptions of each parameter's role and function. The source code, along with download and build instructions can be found at https://github.com/cnwalker/FLASH-Interface Compiled executables for a number of operating systems can be found at http://flash.uchicago.edu/site/flashcode/FLASH-Interface/ * The PRaLine code for Proton Radiography Linear reconstruction is now included with the FLASH code tarball and is available for download at https://github.com/flash-center/PRaLine This standalone Python code was originally developed for the magnetic field reconstruction method using proton radiography, discussed in Graziani et al. 2017 (in press), https://arxiv.org/abs/1603.08617 Alemayehu Solomon Bogale (alemsolobog@uchicago.edu) restructured the code and made it suitable for public release. For more information see the README files in tools/protonRad and tools/protonRad/PRaLine !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!! New in FLASH 4.4 (since FLASH 4.3) - October 2016 !!!!! !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! * The default Hydro implementation has changed from split PPM to unsplit Hydro. The setup shortcuts +uhd, +unsplitHydro, +usm, +uhd3t, etc. should all work as before (although +uhd or +unsplitHydro can now be omitted). A new shortcut +splitHydro can be used to request a split Hydro implementation. Simulations that previously did not specify a Hydro implementation will now need to use the new shortcut +splitHydro to reproduce previous behavior. * The default Riemann solver of unsplit Hydro implementations was changed from "Roe" to "HLLC". * Updated values of many physical constants to 2014 CODATA values. This may cause differences from previously obtained results. The previous values of constants provided by the PhysicalConstants unit can be restored by replacing the file PhysicalCosntants_init.F90 with an older version; the version from FLASH4.3 is included as PhysicalConstants_init.F90.flash43. This should only be done to reproduce previous simulation results to bit accuracy. * An improved Newton-Raphson search in the 3T Multi-type Eos implemention (MTMMMT, including Eos based on IONMIX tables) can prevent some cases of convergence failure by bounding the search. This implementation follows original improvements made to the Helmholtz Eos implementation by Dean Townsley. * The optimized code variant ("orrery avoidance") implemented in our adapted Paramesh4dev code is now always enabled by default when Paramesh4dev is used, not just when +pm4dev is explicitly specified in setup. * Added new Poisson solvers (Martin-Cartwright Geometric Multigrid [1] and BiPCGStab [2], which uses multigrid as preconditioner). Combinations of homogeneous Dirichlet, Neumann, and periodic boundary conditions are supported (although not yet "isolated" boundaries for self-gravity). [1] D. Martin, K. Cartwright. Technical Report No. UCB/ERL M96/66 1996. [2] H. Van Der Vorst. SIAM J. Sci. and Stat. Comput. 1992; 13:2, pp631–644. * Added the IncompNS physics unit, which provides a solver for incompressible flow problems on rectangular domains. Multistep and Runge-Kutta explicit projection schemes are used for time integration. These methods are described in [3]-[5]. Implementations on staggered grid arrangement for both uniform grid (UG) and adaptive mesh refinement (AMR) are provided. The new Poisson solvers are employed for AMR cases, whereas the homogeneous trigonometric solver + PFFT can be used in UG. Typical velocity boundary conditions for this problem are implemented. [3] S. Armfield, R. Street. Int. J. Numer. Meth. Fluids 2002; 38, pp255-282. [4] J. Yang, E. Balaras. J. Comput. Phys. 2006; 215:1, pp12-40. [5] M. Vanella, P. Rabenold, E. Balaras. J. Comput. Phys. 2010; 229:18, pp6427-6449. * The ProtonImaging diagnostics code has been improved. Time resolved proton imaging is now possible, where protons are traced through the domain during several time steps. The original version (tracing of protons during one time step with fixed domain) is still available. * The code for Radiation-Fluxlimiter-Aware Hydro has been updated. Smoothing of the flux-limiter function within the enhanced Hydro implementation has been implemented and has been shown effective in increasing stability in 1D simulations. * Tweaks in handling some of the geometric terms in curvilinear coordinates in unsplit Hydro and MHD. * New Opacity implementations: BremsstrahlungAndThomson and OPAL. These are for gray opacities. * In addition to the new FLASH release, the publicly available Python module opacplot2 has received significant development (credit to JT Laune). It can assist in handling EoS/opacity tables, and includes command line tools to convert various table formats to IONMIX and to compare between different tables. More information can be found in the Flash Center's GitHub repository at . * Some auxiliary units: PlasmaState. See online documentation. * Some new (or changed) API routines (see online API documentation): Grid_smoothVar, Grid_subcellGeometry * The code includes stubs for several new code units for which implementations may be added in future releases (diagnostics/ProtonEmission, diagnostics/ThomsonScattering) * Fixes for various errors, reported and unreported !!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!! !!!!! 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) Helmholtz/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. An important feature of FLASH 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 4.1.3) 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."