Table 1. Catalog for ensemble forecasts
(Same for all three cases)
Member
|
Surface
|
Microphysics
|
PBL
|
CU
|
1
|
Thermal
|
Kessler
|
YSU
|
KF
|
2
|
Thermal
|
WSM3
|
YSU
|
BM
|
3
|
Noah
|
Kessler
|
MRF
|
BM
|
4
|
Noah
|
Lin
|
MRF
|
Grell
|
5
|
Noah |
WSM3
|
MRF
|
KF
|
6
|
Noah |
WSM5
|
Eta
|
BM
|
7
|
Noah |
WSM5
|
YSU
|
KF
|
8
|
Noah |
Eta
|
Eta
|
Grell
|
9
|
Noah |
WSM6
|
YSU
|
Grell
|
10
|
Noah |
WSM6
|
Eta
|
KF
|
11
|
Noah |
Thompson
|
YSU
|
BM
|
12
|
RUC
|
Lin
|
Eta
|
Grell
|
13
|
RUC |
Lin
|
YSU
|
KF
|
14
|
RUC |
WSM3
|
YSU
|
Grell
|
15
|
RUC |
WSM5
|
MRF
|
BM
|
16
|
RUC |
Eta
|
YSU
|
BM
|
17
|
RUC |
Eta
|
MRF
|
KF
|
18
|
RUC |
WSM6
|
Eta
|
BM
|
19
|
RUC |
Thompson
|
MRF
|
Grell
|
20
|
RUC |
Thompson
|
Eta
|
KF
|
- IF (PBL = "YSU" or PBL="MRF") then sf_sfclay_physics = 1
(Monin-Obukhov)
IF (PBL = "Eta")
then sf_sfclay_physics = 2 (Monin-Obukhov (Janjic Eta))
- Radiation schemes are same for all 20 members.
- ra_lw_physics = 1 (RRTM scheme)
- ra_sw_physics = 1 (Dudhia scheme)
- Ensemble forecast runs employed the same initial and boundary
conditions files for each member, except that members using different
land-surface models required different initializations of the soil
variables.
* A sample script for a batch job for Typhoon Maemi