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Horizontal resolution increase |
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On Tuesday 26 January 2010, ECMWF upgraded the horizontal resolution of its deterministic forecasting system and the Ensemble Prediction System (EPS), including the monthly extension to 32 days. A new cycle of the IFS model has been introduced to implement the higher resolution upgrade. This cycle is labelled 36r1. The main contents of Cycle 36r1 are:
These upgrades
The model number identifier (generating process identification number - GRIB Section 1, Product Definition Section, Octet 6) has been changed:
The model number identifier for the European Shelf (Mediterranean) wave model and the ocean model has not been changed and remains set to 204 and 2, respectively. The new cycle was implemented in operations on Tuesday 26 January 2010.
This document will be updated as required and was last changed on 29.01.2010. For a record of changes made to this page please refer to Document versions. A printable version Further information and advice regarding the upgrade can be obtained from News29 January 2010
22 January 2010
13 January 2010
1 December 2009 A new version of the ECMWF model that includes a major resolution upgrade has been tested extensively for all seasons in 2009. The higher-resolution system has been run in experimental suite (e-suite) mode since 15 July 2009. The final configuration, IFS cycle 36r1, has been run since 1 October 2009. The e-suite is now running in step with operations in near-real time. The planned implementation date is Tuesday 26 January 2010. 5 November 2009 The pre-operational testing is progressing well. However, last week the test suite was restarted with a modification to the IFS code. This modification consists of a correction to the radiation scheme, affecting the reflection of short-wave radiation by clouds. 16 October 2009 The e-suite for the IFS cycle 36r1 deterministic T129L91 forecasts has been run since 25 September 2009. 4 September 2009
TimetableThe implementation of the horizontal resolution increase is planned as follows:
The timetable given here represents our current expectations and may have to be reviewed in light of the actual progress made. This cycle of the IFS model is primarily to implement the higher resolution upgrade. No other significant meteorological changes are planned for this model change. This cycle will be labelled 36r1. Further information regarding previous changes to the IFS model can be found at: http://www.ecmwf.int/products/data/technical/model_id/.
Resolution changesAtmospheric model
Wave model
The resolution of the European Shelf (Mediterranean) model was upgraded independently on 13 October 2009.
Ocean modelThere were no changes made to the resolution of the ocean model used in the monthly extension of the EPS to 32 days.
Gaussian definitionsDescriptions of the Gaussian Grids for N640, N320 and N160 used with the higher resolution model are available. For a catalogue containing the descriptions of all other Gaussian Grids as well as the correspondence between the three types of grid resolutions (Spherical Harmonic, Gaussian Grid and Latitude-Longitude) please refer to: http://www.ecmwf.int/products/data/technical/gaussian/. The figure shows the grid spacing and orography fields over the United Kingdom and Ireland for the N400 (left) and N640 (right) Gaussian grids (click on the images for larger versions).
Land-sea mask and orography fields at reduced Gaussian resolutions N640, N320 and N160 are available for download:
Impact on usersField sizesThe size of the fields produced by the model have increased by a factor of 2.56. When retrieving data via MARS or dissemination, if users do not specify any spectral truncation or grid resolutions, fields are provided at model resolution. In particular, users should be aware of the increase in memory needed to process the increased resolution fields. For example, the coefficient file used to interpolate T1279 spectral fields to a 0.125 x 0.125 regular latitude-longitude grid is about 4 GBytes in size. This is 4 times more larger than the coefficient file used to interpolate T799 spectral fields to a 0.225 x 0.225 regular latitude-longitude grid. A standard MARS retrieval of a T1279 spectral fields to a 0.125 x 0.125 regular latitude-longitude grid will, therefore, need about 4 times more memory. It may not be possible for users to run such retrievals interactively on ecgate. In this case, retrievals will need to be submitted to the LoadLeveler batch system. The memory and CPU limits of the various LoadLeveler classes on ecgate have been reviewed to cater for the increased resources needed. Users running their retrievals on the HPCF may need to alter the memory requirement using the "#@ resources = ConsumableMemory" LoadLeveler directive.
DisseminationThere are a number of issues that need to be addressed before the implementation of the resolution upgrade:
All results from the e-suite are available from the MARS archive under version number 0046 (EXPVER=0046). ECMWF have migrated all Member States' dissemination requirements to the higher resolution system to provide products that are compatible with the current operational products, i.e.at the same horizontal resolution as currently disseminated. Spectral data from the deterministic Global wave model is disseminated at the new spectral resolution of 36 directions and 36 frequencies only. On Tuesday 8 December 2009, a dissemination test data set was made available on ECPDS as version number 0046 based on current operational dissemination requirements. The data set comprises one full day (00, 06, 12 and 18UTC) of e-suite dissemination data (deterministic, EPS, Boundary Condition, global wave and wave EPS, and limited-area wave suites). Please contact Dragan Jokic Users will be able to request data at higher resolution after implementation of the new cycle. Member State jobsMember State users will be responsible for testing and checking the output of their jobs that use the new higher resolution data sets. In particular:
These tests can be carried out using the e-suite test data. On ecgate, the default user versions of EMOSLIB, MAGICS and Metview can all handle the increased horizontal resolution fields. Member State jobs submitted through the ECaccess time-critical (option-1) mechanism need to be tested and adapted by Member State users themselves. Please contact User Support
Member State projectsThose responsible for Member State projects (e.g., COSMO-LEPS, NORLAMEPS) as well as the common applications (HIRLAM, FLEXTRA, meso-nh, COSMO/LM, etc) running at ECMWF will need to:
Boundary Condition projectThe same resolution changes as for the main deterministic forecast applies also to the BC project forecast runs. The impact on field sizes and dissemination is as described above. Test data sets for the Boundary Condition project at the higher resolution (T1279 L91) are stored in MARS and can be used for technical testing purposes (see Test data sets from pre-operational e-suite ).
EPSgramsThe EPSgram facility has been upgraded or the implementation of the higher resolution model upgrade. The interfaces are fully compatible and the upgrade transparent to the user. The coordinates of the nearest grid point in the EPSgrams have changed.
Other issuesUsers with other issues that are not covered here are urged to contact User Support
SoftwareEMOS LibraryGRIB decodingA new version of the EMOS library (release 000370) is available on the Linux PC/Cluster, IBM servers, and IBM HPCF/C1A/C1B and includes support for the horizontal resolution model upgrade. This has been the default version since 7 September 2009. Both double and single precision versions of the library are available on each platform. Please check that your codes work correctly with the 000370 version of the library and report any problems to User Support The 000370 version of the library includes several changes needed for the resolution upgrade, notably
and is sufficient for users needing only to decode the increased resolution fields. Users are encouraged to use the GRIB API Library to decode higher resolution model data - see GRIB API. Field interpolationUsers needing to interpolate the increased horizontal need to use version 000371 of the EMOS Library. This version is also available on all computing platforms at ECMWF and can be accessed as follows.
The truncation can be controlled using the truncation option in INTIN. For further information about the interpolation routines available in EMOSLIB see: http://www.ecmwf.int/publications/manuals/libraries/interpolation/. Note that high resolutions need more resources to carry out the required processing. For more information about changes to the EMOS library, please refer to: http://www.ecmwf.int/publications/manuals/libraries/emoslib/. For Member State users an export (web downloadable) version of the new EMOS library versions 000370 and 000371 are available at: http://www.ecmwf.int/products/data/software/download/interpolation.html. Member States are encouraged to install and test these versions locally.
GRIB APIAlthough GRIBEX will continue to work, users are encouraged to use the GRIB API Library to decode higher resolution model data. The latest version 1.8.0 of the GRIB API Library is available for download at: http://www.ecmwf.int/products/data/software/grib_api.html
MARSUsers should also be aware of the effect of the RESOL directive when retrieving spectral fields in spherical harmonics form. If the RESOL directive is not specified then fields will be retrieved at the new higher resolution. If RESOL is specified then triangular truncation of retrieved data will, as usual, take place accordingly before any selected post-processing . Spectral fields are automatically truncated before interpolation to grid fields to reduce data volumes and spurious ‘aliased’ values. For a table detailing the default truncations please refer to the MARS User Guide. Note that high resolutions need more resources (memory, CPU and disk space) to carry out the required processing. See Impact on users - Field sizes above for information about memory requirements.
MAGICS and Magics++MAGICS 6 applications need to be re-linked with EMOS library version 000370 to cope with the new Gaussian definition. A new MAGICS 6 export version (MAGICS 6.12-export) with a fix to allow direct visualisation of T1279 spectral fields was made available to Member State users on 14 October 2009 and can be ordered from: http://www.ecmwf.int/products/data/software/magics.html. However, only a small code change is required; for most installers it will be easier to update their MAGICS 6 installation by following the advice given at: This fix is not required if your application is visualising data on the Gaussian or regular latitude-longitude grids. Users are encouraged to migrate their MAGICS applications to Magics++.
MetviewMetview version 3.11.5-export using EMOS Library cycle 000370, and including the fix to allow direct visualisation of T1279 spectral fields, was made available on 7 September 2009 and can be ordered from: http://www.ecmwf.int/products/data/software/metview.html.
Test data sets from pre-operational e-suiteThe IFS cycle 36r1 e-suite for the deterministic T1279L91 forecasts was run from 1 October 2009 to 26 January 2010. All results are stored in MARS and can be used for technical test purposes by Member States users. The version number of the e-suite is 0046 (MARS parameter EXPVER=46). The IFS cycle 36r1 e-suite for the EPS T639L62 / T319L62 Leg A / Leg B / C forecasts was run from 3 October 2009 to 3 November 2009 and 24 November 2009 to 26 January 2010. All results are also stored in MARS. The version number of the e-suite is 0046 (MARS parameter EXPVER=46). These data sets are available only to registered ECMWF users with access to MARS or WebMARS.
The quality of these data sets is not guaranteed. Please report any problems you find with this data to User Support
Changes to the dissemination scheduleThere were no changes to the dissemination schedule.
Document versions
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