|MPAS-Atmosphere Version 5.0
7 January 2017
This major release of MPAS introduces new capabilities, options, and enhancements
to MPAS-Atmosphere, as well as many small improvements in the MPAS framework.
Significant changes to MPAS-Atmosphere include:
Updates and improvements to the MPAS framework include:
- A new physics suite, 'convection_permitting', that is suitable for applications
where convection-permitting meshes (dx < 10 km) are employed, including
variable-resolution meshes spanning hydrostatic to nonhydrostatic resolutions
- Updates to the versions of existing physics schemes
- A new vertical level distribution (selected by default when running init_atmosphere_model)
that has been used in several MPAS-Atmosphere real-time experiments, including
the prediction of tropical cyclones
- The ability to initialize the water vapor mixing ratio directly from specific
humidity rather than relative humidity
- An option to compute sub-grid-scale orography statistics for use by the GWDO scheme
directly on the native MPAS mesh from the 30-arc-second topography used for the model
- The use of "packages" to save memory by selectively allocating fields based on
run-time choices of physics suite or schemes
- Substantial performance optimizations to the dynamical solver (with contributions from
Thomas Henderson (then at NOAA), Robert Sinkovits (SDSC), John Dennis (NCAR), and Ryan Cabell (NCAR))
- The ability to obtain bit-identical results for any MPI task count (though this may
require the addition of compiler flags, e.g., '-fp-model precise' for the ifort compiler)
- An experimental hybrid-parallel capability to allow execution with MPI and OpenMP; note
that this ability does not currently offer a performance advantage and is being released
for further development by collaborators
- Complete documentation for all namelist options and fields in the Registry file;
units and description for all fields are also written as variable attributes to
all model output files
- The introduction of a new framework for including diagnostics modules in MPAS-Atmosphere
- New diagnostics: Ertel PV diagnostics (thanks to Nick Szapiro (OU)), and convective
diagnostics including CAPE and CIN
- The ability to write soundings for a specified list of locations at any specified interval
during model integration
- For data assimilation, an Incremental Analysis Update (IAU) module to reduce
initial noise by adding analysis increments over a time window (thanks to Soyoung Ha (NCAR))
- A simplified method for building single-precision executables: simply add PRECISION=single
to the compilation command-line
- Minor performance improvements, e.g., in halo communication
- Fixes to allow the infrastructure to correctly handle large meshes (>10^7 cells)
- OpenMP threading of memory initialization, buffer copying, etc.
- Minor cleanup and bug fixes throughout
|MPAS-Atmosphere Version 4.0
22 May 2015
This major release includes several significant changes to the atmosphere core, and a small number of minor changes
to the shared MPAS infrastructure that are visible to users.
Significant changes in the atmosphere core include the following:
Several minor, though notable, changes have also been included in the MPAS software infrastructure:
- A new split dynamics-transport integration scheme has been introduced, allowing scalar transport to take place on
a longer timestep than the other dynamics. Real-data testing indicates that the new scheme offers greater model
stability. This scheme, selected by default, is controlled by the new namelist options
config_split_dynamics_transport, which controls whether the new option is used, and
config_dynamics_split_steps, which sets number of dynamics sub-cycles in a timestep.
- The concept of physics suites has been introduced, allowing groups of physics parameterizations
that have been tested together to be selected with a single namelist option; this is an alternative to
individually specifying parameterization schemes. By default, MPAS-Atmosphere uses
the 'mesoscale_reference' suite, described in Section 6.1 of the Users' Guide.
- Improved support for initializing with model-level datasets, in particular, ERA-Interim model level data.
- Scale-adaptive coordinate surface smoothing.
- A new optional keyword, io_type, has been implemented in the XML stream configuration files, allowing the file format
and library to be selected on a per-stream basis. More details are available in Section 5.2 of the Users' Guide.
- In the MPAS 3.x releases, fields and global attributes showed up in output files in random order; now, the order of
the file contents is based on the order that fields and namelist options were declared in the Registry.xml file of a core.
- A few minor improvements have been made to enable MPAS-Atmosphere to run more reliably in single-precision and at high-resolution,
especially on large MPI task counts.
|MPAS-Atmosphere Version 3.3
21 January 2015
This bugfix release corrects an number of issues in the shared MPAS infrastructure:
- Fix an issue in the timekeeping library when comparing time intervals with different numbers of years or months
- Fix a memory leak when setting times in the time manager
- Add improved error messages when attempting to read from non-existent files
- Correctly catch error conditions produced by open() when opening XML files
- Fix bug in merging var_struct and var_array elements in Registry.xml files
- Set the s_d variable within time manager to avoid potential division by zero
- Remove an extra if-test to handle r0a field destruction in pools
- Avoid allocating memory for inactive package variables
- Fix for directory creation for streams when directories are nested within non-writable directories
- Permit input streams to have the same filename template
- Update infrastructure bootstrapping process to properly handle stream attributes
- Fix an issue with interval division when resetting alarms
|MPAS-Atmosphere Version 3.2
17 December 2014
This bugfix release only affects MPAS-Ocean.
|MPAS-Atmosphere Version 3.1
24 November 2014
This bugfix release corrects an error in the downward extrapolation of RH for model levels
that lie below the surface of the initial condition dataset (e.g., GFS). Without this fix,
the RH field used to compute the initial water vapor mixing ratio field may contain zero
(or possible garbage) values in the lowest model levels.
This bug was only present in v3.0, and not in earlier releases of MPAS-Atmosphere.
|MPAS-Atmosphere Version 3.0
18 November 2014
This major release includes only minor changes to the atmosphere core, and more substantial changes
to the shared MPAS infrastructure.
Changes to atmosphere-specific code include:
This release of MPAS includes two major changes to the MPAS software infrastructure, the second of which significantly
changes the model user interface.
- Support for soil moisture and soil temperature from ERA-I levels (0-7, 7-28, 28-100, and 100-25 cm);
- a significant reduction in the print statements written to the log files;
- a reduction in the set of fields written to the default model history files; and
- miscellaneous minor bugfixes.
New features in the MPAS-Ocean and MPAS-Land Ice cores may be found in the documentation for these cores.
- As a significant step in preparing the MPAS framework for support of multiple MPAS cores being compiled together
in the same executable, the internal storage of fields and namelist options has been rewritten; this change principally
affects model developers who need to access fields inside the MPAS code.
- To enable full run-time control over file input and output, a new I/O layer has been developed for MPAS. In past
releases of MPAS, control over input, restart, and history files took place in the namelist file. Now, all configuration
of model input, restart, and history files makes use of separate XML configuration files. A new chapter (Chapter 5)
has been added to the MPAS-Atmosphere Users' Guide
to describe the use of this new I/O system.
|MPAS-Atmosphere Version 2.1
6 June 2014
This bugfix release corrects two issues in MPAS-Atmosphere:
- The double-precision RRTMG long-wave table, RRTMG_LW_DATA.DBL, was inconsistent
with the version of the RRTMG code that was included in MPAS-Atmosphere.
The RRTMG_LW_DATA.DBL has been updated in the MPAS-Data repository, and the source code
includes changes in the data checkout script to download the latest version of all
WRF physics tables from this repository.
- In two places in the MPAS-Atmosphere solver, the upwinding coefficient for the 3rd-order
advection scheme, config_coef_3rd_order, was incorrectly declared as an integer rather than a real.
The bug affects the diagnosis of the covariant vertical velocity omega, resulting in the use
of a fourth-order diagnosis as opposed to the third-order diagnosis consistent with the horizontal transport.
|MPAS-Atmosphere Version 2.0
15 November 2013
The 2.0 release represents a relatively minor increment in functionality for MPAS-Atmosphere.
Improvements and new features of MPAS-Atmosphere include:
- the option to run the RRTMG long-wave and short-wave radiation codes with climatologically varying
- improved interpolation of surface update fields (sea-surface
temperatures and fractional seaice)
- the ability to run MPAS-A in single-precision. This capability has received very limited testing, and the MPAS-A group would be
interested in receiving any feedback based on user experiences with this feature. For information on building and running MPAS-A for
single-precision execution, please see this page.
- other minor corrections to code, including:
- logic changes to compute simulated radar reflectivity and other diagnostic fields at the proper time in high-frequency diagnostic files
- fix for the lower bound of a loop in the computation of horizontal advection of w when config_w_adv_order=3 (no impact on results); thanks to Bill Gustafson Jr. and Matus Martini of PNNL
- turning off the inclusion of moisture by default in the initialization for the Jablonowski and Williamson test case
The MPAS 2.0 release is the first public release to include the MPAS Land-Ice
core. For information on MPAS-Land Ice, please see
Information about new features in the MPAS-Ocean core can be found in the MPAS-Ocean documentation.
|MPAS-Atmosphere Version 1.5
4 September 2013
This release corrects an indexing error in the computation of horizontal mixing for w.
Thanks to Matus Martini for finding this bug.
|MPAS-Atmosphere Version 1.4
27 August 2013
This bugfix release introduces corrections to the hydrostatic balancing in MPAS-A real-data initialization to properly account for vertical grid stretching.
|MPAS-Atmosphere Version 1.3
23 July 2013
This bugfix release corrects syntax in the Bourne shell script used to check out physics lookup tables at build-time.
|MPAS-Atmosphere Version 1.2
23 July 2013
This bugfix release modifies Fortran USE statements to be compatible with older as well as current versions of the pg90 compiler.
|MPAS-Atmosphere Version 1.1
15 July 2013
This bugfix release only affects MPAS-Ocean.
|MPAS-Atmosphere Version 1.0
14 June 2013
MPAS Version 1.0 was released on 14 June 2013. This is the first
public release of MPAS, including the atmosphere model. MPAS-A
has undergone limited testing for NWP time-scale integrations (days to
weeks) and seasonal to year-long integrations for regional climate
applications, in addition to idealized testing including dry and moist
idealized baroclinic waves, squall-lines, supercells, and mountain-wave
simulations in 2D and 3D Cartesian geometries.
Considerations regarding this initial release:
We welcome comments, contributions, bug reports, bug fixes, and any other feedback.
- We have not tested the model for deep-atmosphere
configurations; our model top has typically been set at 30 km in real-data simulations.
- The current physics suite, taken from the WRF-NRCM
configuration with a few additional options, had not been developed for
coarse meshes [dx ~ O(100 km)]. We have observed a number of
MPAS-A failures related to physics on coarse meshes for long-term integrations with surface updates.
- We have only used GFS, CFSR, and NNRP data for
initialization of full-physics real-world cases. Real case
initializations using other data, like ERA-Interim data, are currently
- We have only limited post-processing capabilities at present, particularly with respect to visualization.
- While we have begun testing methods for interpolating the MPAS
output to latitude-longitude meshes (which would greatly expand our
post-processing capabilities), these packages are not available in this
release. We expect to make them available in the near future.
- MPAS must be run under MPI because MPAS uses PIO. We
understand that there would be some utility to having a serial build,
and this capability may appear in a later release.
- MPAS does not currently support running MPAS-Atmosphere
coupled to MPAS-Ocean. We anticipate that most coupled-model work
using MPAS-A will occur in CESM. We are, however, open to working
with others exploring coupling with other modeling systems.
and MPAS-O are standalone models; this release does not contain the
CESM configurations for MPAS-A or MPAS-O, both of which are currently
- Data assimilation using the Data Assimilation Research
Testbed (DART) with MPAS-A is under development. This capability
is not available in this release.