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Commit dd2a06c0 authored by John Helly's avatar John Helly Committed by Matthieu Schaller
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Lightcone outputs

parent 94e73ee9
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1 merge request!1354Lightcone outputs
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with 461 additions and 7 deletions
......@@ -52,7 +52,7 @@ AC_DEFINE([_GLIBCXX_INCLUDE_NEXT_C_HEADERS],1,[Hack for min() and max() using g+
# Enable POSIX and platform extension preprocessor macros.
AC_USE_SYSTEM_EXTENSIONS
# Check for compiler version and vendor.
# Check for C compiler version and vendor.
AX_COMPILER_VENDOR
AX_COMPILER_VERSION
......@@ -1397,6 +1397,34 @@ if test "$enable_velociraptor_orphans" = "yes"; then
AC_DEFINE([HAVE_VELOCIRAPTOR_ORPHANS], 1, [Orphan particles should be written out])
fi
# Check if lightcone output is on.
AC_ARG_ENABLE([lightcone],
[AS_HELP_STRING([--enable-lightcone],
[Activate lightcone outputs.],
)],
[enable_lightcone="$enableval"],
[enable_lightcone="no"]
)
if test "$enable_lightcone" = "yes"; then
# Check for healpix for lightcone maps. May require cfitsio
# This sets CHEALPIX_LIBS and CHEALPIX_CFLAGS and #defines HAVE_CHEALPIX.
# It also adds a --with-cfitsio flag in case cfitsio is installed in a
# different location from healpix.
GV_FIND_LIBRARY([cfitsio], [CFITSIO], [cfitsio], [cfitsio], [ffclos])
TMP_LIBS=${LIBS}
LIBS="${CFITSIO_LIBS} ${LIBS}"
GV_FIND_LIBRARY([chealpix], [CHEALPIX], [chealpix], [chealpix], [ang2vec])
LIBS=${TMP_LIBS}
have_chealpix=${USE_CHEALPIX}
CHEALPIX_LIBS="${CHEALPIX_LIBS} ${CFITSIO_LIBS}"
AC_DEFINE([WITH_LIGHTCONE], 1, [Enable lightcone outputs])
if test "$have_chealpix" != "yes"; then
AC_MSG_ERROR([Lightcone output requires the HEALPix C API. Please configure with --with-chealpix.])
fi
else
have_chealpix="no"
fi
# Check for floating-point execeptions
AC_CHECK_FUNC(feenableexcept, AC_DEFINE([HAVE_FE_ENABLE_EXCEPT],[1],
[Defined if the floating-point exception can be enabled using non-standard GNU functions.]))
......@@ -1614,6 +1642,7 @@ with_subgrid_stars=none
with_subgrid_star_formation=none
with_subgrid_feedback=none
with_subgrid_sink=none
with_subgrid_extra_io=none
case "$with_subgrid" in
yes)
......@@ -1630,6 +1659,7 @@ case "$with_subgrid" in
with_subgrid_feedback=GEAR
with_subgrid_black_holes=none
with_subgrid_sink=none
with_subgrid_extra_io=none
enable_fof=no
;;
QLA)
......@@ -1642,6 +1672,7 @@ case "$with_subgrid" in
with_subgrid_feedback=none
with_subgrid_black_holes=none
with_subgrid_sink=none
with_subgrid_extra_io=none
enable_fof=no
;;
QLA-EAGLE)
......@@ -1666,6 +1697,7 @@ case "$with_subgrid" in
with_subgrid_feedback=EAGLE
with_subgrid_black_holes=EAGLE
with_subgrid_sink=none
with_subgrid_extra_io=none
enable_fof=yes
;;
EAGLE-XL)
......@@ -1678,6 +1710,7 @@ case "$with_subgrid" in
with_subgrid_feedback=EAGLE
with_subgrid_black_holes=EAGLE
with_subgrid_sink=none
with_subgrid_extra_io=EAGLE
enable_fof=yes
;;
*)
......@@ -2169,6 +2202,35 @@ case "$with_tracers" in
;;
esac
# Extra fields added to snapshots at i/o time
AC_ARG_WITH([extra_io],
[AS_HELP_STRING([--with-extra-io=<function>],
[chemistry function @<:@none, EAGLE default: none@:>@]
)],
[with_extra_io="$withval"],
[with_extra_io="none"]
)
if test "$with_subgrid" != "none"; then
if test "$with_extra_io" != "none"; then
AC_MSG_ERROR([Cannot provide with-subgrid and with-extra_io together])
else
with_extra_io="$with_subgrid_extra_io"
fi
fi
case "$with_extra_io" in
none)
AC_DEFINE([EXTRA_IO_NONE], [1], [No extra_io function])
;;
EAGLE)
AC_DEFINE([EXTRA_IO_EAGLE], [1], [Extra i/o fields taken from the EAGLE model])
;;
*)
AC_MSG_ERROR([Unknown extra-io choice: $with_extra_io])
;;
esac
# Stellar model.
AC_ARG_WITH([stars],
[AS_HELP_STRING([--with-stars=<model>],
......@@ -2592,6 +2654,9 @@ DX_DOXYGEN_FEATURE(OFF)
DX_INIT_DOXYGEN(SWIFT, doc/Doxyfile, doc/)
AM_CONDITIONAL([HAVE_DOXYGEN], [test "$ac_cv_path_ac_pt_DX_DOXYGEN" != ""])
# Check if using EAGLE extra I/O
AM_CONDITIONAL([HAVEEAGLEEXTRAIO], [test "${with_extra_io}" = "EAGLE"])
# Check if using QLA cooling
AM_CONDITIONAL([HAVEQLACOOLING], [test "$with_cooling" = "QLA"])
AM_CONDITIONAL([HAVEQLAEAGLECOOLING], [test "$with_cooling" = "QLA-EAGLE"])
......@@ -2693,6 +2758,7 @@ AC_MSG_RESULT([
- MPI : $have_mpi_fftw
- ARM : $have_arm_fftw
GSL enabled : $have_gsl
HEALPix C enabled : $have_chealpix
libNUMA enabled : $have_numa
GRACKLE enabled : $have_grackle
Special allocators : $have_special_allocator
......@@ -2700,6 +2766,7 @@ AC_MSG_RESULT([
Pthread barriers : $have_pthread_barrier
VELOCIraptor enabled : $have_velociraptor
FoF activated: : $enable_fof
Lightcones enabled : $enable_lightcone
Hydro scheme : $with_hydro
Dimensionality : $with_dimension
......@@ -2725,8 +2792,9 @@ AC_MSG_RESULT([
Star feedback model : $with_feedback_name
Sink particle model : $with_sink
Black holes model : $with_black_holes
Radiative transfer : $with_rt
Radiative transfer : $with_rt$rt_extra_msg
Extra i/o : $with_extra_io
Atomic operations in tasks : $enable_atomics_within_tasks
Individual timers : $enable_timers
Task debugging : $enable_task_debugging
......
......@@ -93,6 +93,16 @@ GRACKLE
~~~~~~~
GRACKLE cooling is implemented in SWIFT. If you wish to take advantage of it, you will need it installed.
HEALPix C library
~~~~~~~~~~~~~~~~~~~
This is required for making light cone HEALPix maps. Note that by default HEALPix builds a static library which cannot be used to build the SWIFT shared library. Either HEALPix must be built as a shared library or -fPIC must be added to the C compiler flags when HEALPix is being configured.
CFITSIO
~~~~~~~
This may be required as a dependency of HEALPix.
Initial Setup
-------------
......
.. Light Cones
John Helly 29th April 2021
.. _lightcone_adding_outputs_label:
Adding New Types of Output
~~~~~~~~~~~~~~~~~~~~~~~~~~~
New particle properties can be added to the particle light cones as follows:
* Add a field to the ``lightcone_<type>_data`` struct in ``lightcone_particle_io.h`` to store the new quantity
* Modify the ``lightcone_store_<type>`` function in ``lightcone_particle_io.c`` to set the new struct field from the particle data
* in ``lightcone_io_make_output_fields()``, add a call to ``lightcone_io_make_output_field()`` to define the new output
Here, <type> is the particle type: gas, dark_matter, stars, black_hole or neutrino.
To add a new type of HEALPIX map:
* Add a function to compute the quantity in ``lightcone_map_types.c``. See ``lightcone_map_total_mass()`` for an example.
* Add a new entry to the ``lightcone_map_types`` array in lightcone_map_types.h. This should specify the name of the new map type, a pointer to the function to compute the quantity, and the units of the quantity. The last entry in the array is not used and must have a NULL function pointer to act as an end marker.
.. Light Cones
John Helly 29th April 2021
.. _lightcone_algorithm_description_label:
Light Cone Output Algorithm
~~~~~~~~~~~~~~~~~~~~~~~~~~~
In cosmological simulations it is possible to specify the location of
an observer in the simulation box and have SWIFT output information
about particles in the simulation as they cross the observer's past
light cone.
Whenever a particle is drifted the code checks if any periodic copy of
the particle crosses the lightcone during the drift, and if so that
copy of the particle is buffered for output. As an optimization, at the
start of each time step the code computes which periodic copies of the
simulation box could contribute to the light cone and only those copies
are searched. When drifting the particles in a particular cell the list of
replications is further narrowed down using the spatial extent of the
cell.
Particles can be output directly to HDF5 files or accumulated to healpix
maps corresponding to spherical shells centred on the observer.
.. Light Cones
John Helly 29th April 2021
.. _Light_Cones_label:
Light Cone Outputs
==================
This section describes the light cone outputs
and related parameters
.. toctree::
:maxdepth: 2
:caption: Contents:
algorithm_description
lightcone_particle_output
lightcone_healpix_maps
running_with_lightcones
adding_outputs
.. Light Cones
John Helly 29th April 2021
.. _lightcone_healpix_maps_label:
Light Cone HEALPix Maps
~~~~~~~~~~~~~~~~~~~~~~~
SWIFT can accumulate particle properties to HEALPix maps as they
cross the observer's past light cone. Each map corresponds to a
spherical shell centred on the observer. When a particle crosses
the lightcone its distance from the observer is calculated and the
particle's contribution is added to a buffer so that at the end of
the time step it can be added to the corresponding HEALPix map.
Maps can be generated for multiple concentric shells and multiple
quantities can be accumulated for each shell. The HEALPix map for a
shell is allocated and zeroed out when the simulation first reaches
a redshift where particles could contribute to that map. The map is
written out and deallocated when the simulation advances to a point
where there can be no further contributions. In MPI runs the pixel
data for the maps are distributed across all MPI ranks.
Updates to the maps are buffered in order to avoid the need for
communication during the time step. At the end of the step if any
MPI rank has a large amount of updates buffered then all pending
updates will be applied to the pixel data.
For gas particles, the HEALPix maps are smoothed using a projected
version of the same kernel used for the hydro calculations. Other
particle types are not smoothed.
The code writes one output file for each spherical shell. In MPI mode
all ranks write to the same file using parallel HDF5. If maps of
multiple quantities are being made they will be written to a single
file as separate 1D datasets with one element per pixel.
.. Light Cones
John Helly 29th June 2021
.. _lightcone_particle_output_label:
Light Cone Particle Output
~~~~~~~~~~~~~~~~~~~~~~~~~~
SWIFT can output particles to HDF5 output files (similar to the
snapshots) as they cross the observer's light cone. During each time
step, any particles which cross the light cone are added to a buffer.
If this buffer is large at the end of the step then its contents
are written to an output file. In MPI runs each MPI rank writes its
own output file and decides independently when to flush its particle
buffer.
A new output file is started whenever restart files are written. This
allows the code to automatically continue from the point of the restart
dump if the run is interrupted. Any files written after the restart
dump will be overwritten when the simulation is resumed, preventing
duplication of particles in the light cone output.
The output files have names of the form ``basename_XXXX.Y.hdf5``, where
XXXX numbers the files written by a single MPI rank and Y is the index
of the MPI rank.
The output files contain one HDF5 group for each particle type. Within
each group there are datasets corresponding to particle properties in
a similar format to the snapshots.
.. Light Cones
John Helly 29th April 2021
.. _lightcone_running_label:
Running SWIFT with Light Cone Output
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
To produce light cone particle output swift must be configured
with ``--enable-lightcone``. Additionally, making HEALPix maps
requires the HEALPix C library. If using MPI then parallel HDF5
is also required.
One lightcone is produced for each ``LightconeX`` section in the
parameter file, where X=0-7. This allows generation of up to 8
light cones. See :ref:`Parameters_light_cone` for details.
SWIFT must be run with the ``--lightcone`` flag to activate light
cone outputs, otherwise the Lightcone sections in the parameter file
are ignored.
......@@ -975,6 +975,182 @@ be processed by the ``SpecWizard`` tool
range_when_shooting_down_y: 100. # Range along the y-axis of LoS along y
range_when_shooting_down_z: 100. # Range along the z-axis of LoS along z
.. _Parameters_light_cone:
Light Cone Outputs
---------------------
One or more light cone outputs can be configured by including ``LightconeX`` sections
in the parameter file, where X is in the range 0-7. It is also possible to include a
``LightconeCommon`` section for parameters which are the same for all lightcones. The
parameters for each light cone are:
* Switch to enable or disable a lightcone: ``enabled``
This should be set to 1 to enable the corresponding lightcone or 0 to disable it.
Has no effect if specified in the LightconeCommon section.
* Directory in which to write light cone output: ``subdir``
All light cone output files will be written in the specified directory.
* Base name for particle and HEALPix map outputs: ``basename``.
Particles will be written to files ``<basename>_XXXX.Y.hdf5``, where XXXX numbers the files
written by a single MPI rank and Y is the MPI rank index. HEALPix maps are written to files
with names ``<basename>.shell_X.hdf5``, where X is the index of the shell. The basename must
be unique for each light cone so it cannot be specified in the LightconeCommon section.
See :ref:`lightcone_adding_outputs_label` for information on adding new output quantities.
* Location of the observer in the simulation box, in internal units: ``observer_position``
* Size of in memory chunks used to store particles and map updates: ``buffer_chunk_size``
During each time step buffered particles and HEALPix map updates are stored in a linked
list of chunks of ``buffer_chunk_size`` elements. Additional chunks are allocated as needed.
The map update process is parallelized over chunks so the chunks should be small enough that
each MPI rank typically has more chunks than threads.
* Maximum amount of map updates (in MB) to send on each iteration: ``max_map_update_send_size_mb``
Flushing the map update buffer involves sending the updates to the MPI ranks with the affected
pixel data. Sending all updates at once can consume a large amount of memory so this parameter
allows updates to be applied over multiple iterations to reduce peak memory usage.
* Redshift range to output each particle type: ``z_range_for_<type>``
A two element array with the minimum and maximum redshift at which particles of type ``<type>``
will be output as they cross the lightcone. ``<type>`` can be Gas, DM, DMBackground, Stars, BH
or Neutrino. If this parameter is not present for a particular type then that type will not
be output.
* The number of buffered particles which triggers a write to disk: ``max_particles_buffered``
If an MPI rank has at least max_particles_buffered particles which have crossed the lightcone,
it will write them to disk at the end of the current time step.
* Size of chunks in the particle output file
This sets the HDF5 chunk size. Particle outputs must be chunked because the number of particles
which will be written out is not known when the file is created.
* Whether to use lossy compression in the particle outputs: ``particles_lossy_compression``
If this is 1 then the HDF5 lossy compression filter named in the definition of each particle
output field will be enabled. If this is 0 lossy compression is not applied.
* Whether to use lossless compression in the particle outputs: ``particles_gzip_level``
If this is non-zero the HDF5 deflate filter will be applied to lightcone particle output with
the compression level set to the specified value.
* HEALPix map resolution: ``nside``
* Name of the file with shell radii: ``radius_file.txt``
This specifies the name of a file with the inner and outer radii of the shells used to make
HEALPix maps. It should be a text file with a one line header and then two comma separated columns
of numbers with the inner and outer radii. The units are determined by the header. The header must
be one of the following:
``# Minimum comoving distance, Maximum comoving distance``,
``# Minimum redshift, Maximum redshift``, or
``# Maximum expansion factor, Minimum expansion factor``. Comoving distances are in internal units.
The shells must be in ascending order of radius and must not overlap.
* Number of pending HEALPix map updates before the buffers are flushed: ``max_updates_buffered``
In MPI mode applying updates to the HEALPix maps requires communication and forces synchronisation
of all MPI ranks, so it is not done every time step. If any MPI rank has at least
``max_updates_buffered`` pending updates at the end of a time step, then all ranks will apply
their updates to the HEALPix maps.
* Which types of HEALPix maps to create: ``map_names_file``
This is the name of a file which specifies what quantities should be accumulated to HEALPix maps.
The possible map types are defined in the lightcone_map_types array in ``lightcone_map_types.h``.
See :ref:`lightcone_adding_outputs_label` if you'd like to add a new map type.
* Whether to distribute HEALPix maps over multiple files: ``distributed_maps``
If this is 0 then the code uses HDF5 collective writes to write each map to a single file. If this
is 1 then each MPI rank writes its part of the HEALPix map to a separate file.
The file contains two columns: the first column is the name of the map type and the second is the
name of the compression filter to apply to it. See io_compression.c for the list of compression
filter names. Set the filter name to ``on`` to disable compression.
* Whether to use lossless compression in the HEALPix map outputs: ``maps_gzip_level``
If this is non-zero the HDF5 deflate filter will be applied to the lightcone map output with
the compression level set to the specified value.
The following shows a full set of light cone parameters for the case where we're making two
light cones which only differ in the location of the observer:
.. code:: YAML
LightconeCommon:
# Common parameters
subdir: lightcones
buffer_chunk_size: 100000
max_particles_buffered: 1000000
hdf5_chunk_size: 10000
# Redshift ranges for particle types
z_range_for_Gas: [0.0, 0.05]
z_range_for_DM: [0.0, 0.05]
z_range_for_DMBackground: [0.0, 0.05]
z_range_for_Stars: [0.0, 0.05]
z_range_for_BH: [0.0, 0.05]
z_range_for_Neutrino: [0.0, 0.05]
# Healpix map parameters
nside: 512
radius_file: ./shell_radii.txt
max_updates_buffered: 100000
map_names_file: map_names.txt
max_map_update_send_size_mb: 1.0
distributed_maps: 0
# Compression options
particles_lossy_compression: 0
particles_gzip_level: 6
maps_gzip_level: 6
Lightcone0:
enabled: 1
basename: lightcone0
observer_position: [35.5, 78.12, 12.45]
Lightcone0:
enabled: 1
basename: lightcone1
observer_position: [74.2, 10.80, 53.59]
An example of the radius file::
# Minimum comoving distance, Maximum comoving distance
0.0, 50.0
50.0, 100.0
150.0, 200.0
200.0, 400.0
400.0, 1000.0
An example of the map names file::
TotalMass on
SmoothedGasMass on
UnsmoothedGasMass on
DarkMatterMass on
.. _Parameters_eos:
Equation of State (EoS)
......
......@@ -27,6 +27,7 @@ difference is the parameter file that will need to be adapted for SWIFT.
FriendsOfFriends/index
VELOCIraptorInterface/index
LineOfSights/index
LightCones/index
EquationOfState/index
ExternalPotentials/index
Neutrinos/index
......
......@@ -15,12 +15,12 @@
# along with this program. If not, see <http://www.gnu.org/licenses/>.
# Add the source directory and the non-standard paths to the included library headers to CFLAGS
AM_CFLAGS = -I$(top_srcdir)/src -I$(top_builddir)/examples $(HDF5_CPPFLAGS) $(GSL_INCS) $(FFTW_INCS) $(NUMA_INCS) $(OPENMP_CFLAGS)
AM_CFLAGS = -I$(top_srcdir)/src -I$(top_builddir)/examples $(HDF5_CPPFLAGS) $(GSL_INCS) $(FFTW_INCS) $(NUMA_INCS) $(OPENMP_CFLAGS) $(CHEALPIX_CFLAGS)
AM_LDFLAGS = $(HDF5_LDFLAGS) $(HDF5_LIBS) $(FFTW_LIBS) $(NUMA_LIBS) $(TCMALLOC_LIBS) $(JEMALLOC_LIBS) $(TBBMALLOC_LIBS) $(GRACKLE_LIBS) $(GSL_LIBS) $(PROFILER_LIBS)
# Extra libraries.
EXTRA_LIBS = $(HDF5_LIBS) $(FFTW_LIBS) $(NUMA_LIBS) $(PROFILER_LIBS) $(TCMALLOC_LIBS) $(JEMALLOC_LIBS) $(TBBMALLOC_LIBS) $(GRACKLE_LIBS) $(VELOCIRAPTOR_LIBS) $(GSL_LIBS)
EXTRA_LIBS = $(HDF5_LIBS) $(FFTW_LIBS) $(NUMA_LIBS) $(PROFILER_LIBS) $(TCMALLOC_LIBS) $(JEMALLOC_LIBS) $(TBBMALLOC_LIBS) $(GRACKLE_LIBS) $(VELOCIRAPTOR_LIBS) $(GSL_LIBS) $(CHEALPIX_LIBS)
# Programs.
bin_PROGRAMS = cooling_rates
......
......@@ -20,13 +20,15 @@ MYFLAGS =
# Add the source directory and the non-standard paths to the included library headers to CFLAGS
AM_CFLAGS = -I$(top_srcdir)/src -I$(top_srcdir)/argparse $(HDF5_CPPFLAGS) \
$(GSL_INCS) $(FFTW_INCS) $(NUMA_INCS) $(GRACKLE_INCS) $(OPENMP_CFLAGS)
$(GSL_INCS) $(FFTW_INCS) $(NUMA_INCS) $(GRACKLE_INCS) $(OPENMP_CFLAGS) \
$(CHEALPIX_CFLAGS)
AM_LDFLAGS = $(HDF5_LDFLAGS)
# Extra libraries.
EXTRA_LIBS = $(GSL_LIBS) $(HDF5_LIBS) $(FFTW_LIBS) $(NUMA_LIBS) $(PROFILER_LIBS) \
$(TCMALLOC_LIBS) $(JEMALLOC_LIBS) $(TBBMALLOC_LIBS) $(GRACKLE_LIBS)
$(TCMALLOC_LIBS) $(JEMALLOC_LIBS) $(TBBMALLOC_LIBS) $(GRACKLE_LIBS) \
$(CHEALPIX_LIBS)
# MPI libraries.
MPI_LIBS = $(PARMETIS_LIBS) $(METIS_LIBS) $(MPI_THREAD_LIBS) $(FFTW_MPI_LIBS)
......
......@@ -41,6 +41,7 @@ SPH:
# Parameters governing the snapshots
Snapshots:
subdir: snapshots
basename: snap
delta_time: 1.02
scale_factor_first: 0.02
......
Small LCDM cosmological simulation generated by C. Power. Cosmology
is WMAP9 and the box is 100Mpc/h in size with 64^3 particles.
We use a softening length of 1/25th of the mean inter-particle separation.
The ICs have been generated to run with Gadget-2 so we need to switch
on the options to cancel the h-factors and a-factors at reading time.
We generate gas from the ICs using SWIFT's internal mechanism and set the
temperature to the expected gas temperature at this redshift.
This example is intended to be run with the EAGLE-XL model in order to
produce lightcone outputs including gas, stars and black holes. Note
that the resulting output will not be at all realistic due to the extremely
poor mass resolution and the minimum overdensity for star formation has
to be be reduced to allow any star formation.
To configure the code appropriately, the following flags should be included:
./configure \
--with-hydro=sphenix \
--with-subgrid=EAGLE-XL \
--with-kernel=wendland-C2 \
--with-chealpix \
--enable-lightcone
MD5 checksum of the ICs:
08736c3101fd738e22f5159f78e6022b small_cosmo_volume.hdf5
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/CoolingTables/COLIBRE/UV_dust1_CR1_G1_shield1.hdf5
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/CoolingTables/EAGLE/coolingtables.tar.gz
tar -xvzf coolingtables.tar.gz
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/YieldTables/EAGLE/photometry.tar.gz
tar -xf photometry.tar.gz
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/YieldTables/EAGLE/yieldtables.tar.gz
tar -xf yieldtables.tar.gz
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/ICs/small_cosmo_volume.hdf5
#!/bin/bash
wget http://virgodb.cosma.dur.ac.uk/swift-webstorage/CoolingTables/COLIBRE/X_Ray_tables.13072021.hdf5
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