Current model details
Model version | Implement. date | Time range [Days/Hours] | Resolution (original) | Resolution (original) [km] | Resolution (archived) [° ] | Ens. Size | Runs [UTC] | Ensemble assimilation method | Perturbed Obs.? | Perturbed initial cond.? | Model uncertainty? | Size of 1 run [GB] | Official model changes link | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
BoM (ammc) | d 0-10 | 0,45 x 0.5 (800 x 600) | 17 | 0/6/12/18 | 23.5 | |||||||||
CMA (babj) | d 0-15 | 0.5° x 0.5° | 50 | as original | 30 | 0/12 | 41 | |||||||
CPTEC (sbsj) | d 0-15 | 0.9375° x 0.9375° ( 384 x 192, GG ) | 104 | as original | 15 | 0/12 | 7 | |||||||
ECCC (cwao) | d 0-16 | Yin-Yang grid | 39 | 1 x 1 (360 x 181) | 21 | 0/12 | 4 | |||||||
ECMWF (ecmf) | CY47R1 | 30/06/2020 | d 0-15 | O640 L91 (d 0-15) | 16 | as original | 51 | 0/12 | Ensemble of 4DVar | Yes - based on a variety of approaches | 2 day SVs at T42 | SPPT on scales 500km 6h, 1000km 3d , 2000km 30d | 710 | link |
IMD (vabb) | d 0-10 | T1534 L64 (3072 x 1536 RGG) | 12 | 0.12 x 0.12 (3000 x 1501) | 21 | 0/12 | 242 | |||||||
JMA (rjtd) | d 0-11 | 1.25° x 1.25° (288 x 145, TL479 L100) | 139 | as original | 27 | 0/12 | 4.7 | |||||||
KMA (rksl) | d 0-10 | 0.3° x 0.45° (800 x 600) | 33 | as original | 25 | 0/12 | 52 | |||||||
M-F (lfpw) | h 0-72/0-108 | TL538 L60 c2.4 | 15-87** | 1.5 x 1.5 (240 x 121) | 35 | 6/18 | 0.8/1.2 | |||||||
NCEP (kwbc) | d 0-16 | TL1534/382 (after day 10) L64 | 12/55 | 1 x 1 (360 x 181) | 21 | 0/6/12/18 | 5.1 | |||||||
NCMRWF (dems) | d 0-10 | 0.117° x 0.175° (ACG, N1024) | 13 | 0.18 x 0.12 (2000 x 1501) | 12 | 0/12 | 268 | |||||||
UKMO (egrr) | h 0-174 | 0.187° x 0.28125° (1280 x 960, ACG , N640) | 21 | as original | 18 | 0/6/12/18 | 63 |
- GG = Gaussian grid
- RGG = reduced Gaussian grid
- ACG = Arakawa C grid
- ORGG = octahedral reduced Gaussian grid
- SV = sigular vector
- SSPT = stochastically perturbed physics tendencies
- ** because of the stretching (2.4) the horizontal resolution ranges from 15 (over France) to 87 km depending on the location
- *1 it has been agreed to provide if possible the additional high resolution forecast outputs (type=fc in MARS) interpolated to the same resolution as ensemble