Statistics on Registered PWRF 3.5.1, 3.4.1 and 3.3.1 users as of March 4, 2014
Polar WRF 3.5 was tested with Arctic simulations for 1998 and 2012. The results are in a manuscript submitted to Monthly Weather Review. See Hines et al. (2014) below. The updated version 3.5.1 has also been tested and shown to produce results very similar to 3.5. Polar WRF version 3.5.1 was sent to registered users on February 24, 2014. Future plans include updating Polar WRF for WRF version 3.6 and providing time-dependent data sets of sea ice concentration, sea ice thickness, snow depth on sea ice, and Arctic sea ice albedo through this website. These sea ice fields can be processed through the WRF preprocessing program metgrid into WRF sea surface fields. WRF 3.5/3.5.1 are compatible with these sea ice fields, however, gridded time and space-depedent fields of sea ice thickness, snow cover and albedo have not been easily obtainable by numerical weather prediction community.
Based on extensive experience with mesoscale modeling in the polar regions by the Polar Meteorology Group of the Byrd Polar Research Center at The Ohio State University, the Weather Research and Forecasting model (WRF) has been modified for use in the Polar Regions (referred to as the Polar WRF). A development approach is adopted similar to that used previously to implement the Polar version of the PSU/NCAR fifth generation mesoscale model (Polar MM5). The key modifications for Polar WRF are:
Testing of Polar WRF over Arctic and Antarctic surfaces provides guidance on best choice of physics options. See the publications for guidance.
Model evaluations through Polar WRF simulations over Greenland and the Arctic Ocean (SHEBA site) have been performed, and the results are described in the articles provided below. Development studies have been performed for Arctic land (ARM sites in Alaska), and Antarctica.
Polar WRF is used by forecasters as part of the National Science Foundation sponsored Antarctic Mesoscale Prediction System (AMPS; link provided below) to meet the operational and logistic needs of the United States Antarctic Program (USAP). Under a collaborative project with the Polar Meteorology Group, AMPS simulations are performed at the National Center for Atmospheric Research twice per day (00Z and 12Z initializations), and cover progressively finer domains ranging from 45-km (covering most of the Southern Hemisphere) to 1.7-km (covering the region immediately surrounding McMurdo Station, the base of USAP operations). A 45-km resolution version of the Polar WRF is run here at the Byrd Polar Research Center twice per day for 5 days.
Disclaimer: Polar WRF code is released and supported solely by the PMG and is currently based on standard WRF version 18.104.22.168 (released November 2008), WRF version 3.1.1 (released July 2009), WRF version 3.2.1 (released August 23, 2010), or WRF version 3.3.1 (released September 2011) or WRF version 3.4.1 (released August 2012); contact Dr. David Bromwich for details. The Polar WRF code cannot be guaranteed to work under all circumstances, so feedback will help iron out any remaining kinks. We will provide assistance with code use to the level consistent with our ongoing responsibilities.
October 18, 2012
WRF Model Version 3.4.1 was released by NCAR on August 16, 2012. The most recent polar modifications (primarily sea ice related) have been ported to WRF 3.4.1 and the resulting code run through a series of validation tests - this is Polar WRF 3.4.1 that is NOW available to the scientific community.
Extensive testing of Polar WRF including version 3.3.1 in Antarctica completed. See Bromwich et al. (2013) below.
November 2, 2011:
Polar WRF 3.3.1 is available. Tested for limited periods over Greenland, Arctic Ocean, and Alaska.
April 25, 2011:
WRF 3.3 was released to the community by NCAR on April 6, 2011. The Polar Meteorology Group will port all polar modifications to this release and provide a tar file of changes to interested users. Release date of Polar WRF 3.3 is yet to be decided. A suite of test simulations for Arctic sea ice (SHEBA case), the Greenland Ice Sheet, and Antarctic will be performed to verify the reliability of the modified codes.
August 23, 2010 : Polar WRF 3.2.1 is available:
WRF 3.2 was released to the community by NCAR on April 2, 2010. The Polar Meteorology Group has ported all polar modifications to this release and provides a tar file of changes to interested users as of August 2010. A suite of test simulations for Arctic sea ice (SHEBA case), the Greenland Ice Sheet, and Antarctic are performed to verify the reliability of the modified codes.
The modifications to WRF code for polar applications are available upon request from the Polar Meteorology Group to interested researchers.
October 5, 2009: Polar WRF 3.1.1 is available:
WRF Version 3.1.1 was released by NCAR on July 31, 2009 with fractional sea ice now as a standard option in the downloadable code from NCAR. The Polar WRF modifications have now been updated for WRF 3.1.1 as of October 5, 2009. Important new features include the posibility of variable specified sea ice thickness and variable specified snow depth on sea ice. These features have been added in preparation for the Arctic System Reanalysis. Users should expect colder Arctic near-surface atmospheric temperatures and reduced ground heat flux. If you are still using WRF 22.214.171.124, with that previous upgrade in that standard release the Morrison mixed-phase microphysics (developed especially for Arctic stratus clouds and tested by Bromwich et al. ) became a standard option. All other polar physics for WRF 2.2 was implemented into WRF 126.96.36.199, and the modified code was tested fairly extensively. The fractional sea ice description developed by the Polar Meteorology Group (PMG; Le-Sheng Bai and Keith Hines) has been ported to the surface driver included in WRF 188.8.131.52, as well as the modifications to the NOAH LSM required for ice sheets, as described by Hines and Bromwich (2008).
April 9, 2009
WRF 3.1 has been released to the community by NCAR. The fractional sea ice developed by the Polar Meteorology Group is now a standard option within WRF. To use fractional sea ice set the "fractional_seaice" option to 1 in the WRF runtime namelist. Also, set the WPS initialization to ensure that the correct fractional sea ice data values (variable name SEAICE, it's best to include it in the metgrid variable table) are input to your model run. This is a contribution to the International Polar Year (March 2007-March 2009).
September 17, 2009
The full polar physics used with WRF 184.108.40.206 is being ported into a publicly-available modifications tar file for use with the most recent version of WRF, version 3.1.1. This will include the modified surface energy balance over permanent ice sheets, and modified heat transfer within permanent ice. New additions to the Noah LSM will be variable thickness of sea ice and variable snow cover on sea ice. Expected availability of Polar WRF 3.1.1 tar file is late September/early October 2009.
Future for Polar WRF: Polar WRF is a research modification of the standard WRF code and new capabilities will continue to be added. The polar capabilities in standard WRF will likely lag behind those available in the Polar WRF code from the Polar Meteorology Group (not necessarily supported by NCAR). The goals for the next phase of Polar WRF development target more detailed specified sea-ice description within the NOAH LSM, including variable ice thickness and surface albedo, along with a representation of Arctic melt ponds.
Based upon request, Polar WRF has been sent to the following individuals:
If you would like to use Polar WRF, please fill out our registration form to obtain the source code.
Watch this location for further updates that will be issued when needed. We appreciate your interest and trust you will acknowledge our efforts on behalf of the scientific community in presentations and publications. Please keep us informed as to manuscripts on Polar WRF so that we can maintain an online archive of relevant publications. Research supported by US federal funding, primarily from the National Science Foundation.