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245<br />

Impact of convective parameterization on high ressolution precipitation<br />

climatology using WRF for Indian summer monsoon<br />

Sourav Taraphdar, P. Mukhopadhyay, B. N. Goswami and K. Krishnakumar<br />

Indian Institute of Tropical Meteorology, Pune – 411008, India. sourav@tropmet.res.in<br />

1. Introduction<br />

The Indian monsoon rainfall shows significant variability in<br />

spatial and temporal scale. The temporal variability causes<br />

intraseasonal, interannual and multi-decadal scale<br />

oscillations and spatial variability causes the heterogeneous<br />

precipitation distribution from north to south and east to<br />

west. These variabilities are caused by two types of forcing<br />

namely slowly varying large scale surface boundary<br />

conditions e. g. sea surface temperature (SST), snow cover<br />

etc. and the regional forcing from topography e. g.<br />

Himalayas and Western Ghats etc. Thus resolving the<br />

regional heterogeneity is one of the key to improve the<br />

precipitation distribution over the region (Giorgi and Mearns<br />

1991). It is also reported that higher resolution AGCM helps<br />

in improving the monsoon simulation, however very high<br />

resolution AGCM requires large computational resources.<br />

Thus the computationally less expensive strategy of running<br />

regional models embedded in AGCM gain popularity in<br />

simulating regional climate at higher resolution since mid<br />

90s.<br />

To evaluate the sensitivity of convective parameterization<br />

schemes on monsoon simulation, several attempts were<br />

made. Ratnam and Kumar (2005) simulated two contrasting<br />

years of monsoon 1987 and 1988 by a mesoscale model<br />

(MM5) at 45 km resolution with variety of cumulus<br />

parameterization schemes. They found Betts-Miller-Janjic<br />

(BMJ) and Kain-Fritsch (KF) has certain merits compared to<br />

Grell. At this resolution, large scale monsoonal features can<br />

be captured but to resolve the physiographical heterogeneity<br />

due to topography, ocean etc. of the region, higher<br />

resolution regional climate models (RCM) are required (Im<br />

et al. 2006). Thus, it remains to be seen whether the mean<br />

monsoon rainfall bias improves with a high resolution (Less<br />

than 20 km) mesoscale model. Therefore, the first objective<br />

of the present paper is to produce robust daily monsoon<br />

climatology over Indian region at high resolution by various<br />

cumulus parameterization schemes and its validation with<br />

available observed rainfall data. Along with this attempt will<br />

also be made to identify the models ability to correctly<br />

capture the underlying spatio-temporal variability of<br />

precipitation. The detail investigation of this kind only can<br />

help to decipher the weakness in the formulation of moist<br />

convection which can be improved further. To gain<br />

sufficient insight for further development that would reduce<br />

the uncertainties in the simulations, the third goal of the<br />

paper is to investigate and identify the possible sources of<br />

deviations in simulation arising from different convective<br />

closures.<br />

2. Model, data used and experimental design<br />

The non-hydrostatic, fully compressible with a terrain<br />

following sigma mass co-ordinate mesoscale model WRF-<br />

ARW version 2.2 developed by National Center for<br />

Atmospheric Research (NCAR) has been used for the<br />

present study. The model is used with two nested domains<br />

with horizontal resolutions of 45 and 15 km and 31 sigma<br />

levels with model top at 10 hPa. The model mother domain<br />

covers the large scale Indian monsoon region where the<br />

nested domain focuses mainly on the Indian land masses.<br />

The physical parameterizations schemes used in the model<br />

is with Lin microphysics, Monin-Obukhov similarity<br />

scheme for surface layer, Yonsei university scheme for<br />

PBL, RRTM scheme for long wave and Dudhia scheme<br />

for short wave in all the numerical experiments. The<br />

experiments are differing only by three convective<br />

parameterization schemes namely KF (Kain and Fritsch<br />

1993), BMJ (Betts-Miller (1986); Janjic 1994) and Grell-<br />

Devenyi (GD; Grell and Devenyi 2002).<br />

In this study, the mother domain simulations are driven by<br />

the National Center for Environmental Prediction (NCEP)/<br />

NCAR reanalysis data at a resolution of 2.5 o . The 6-hourly<br />

SST was obtained by linearly interpolating the daily SSTs<br />

of RTG and used as the slowly varying lower boundary<br />

condition for the model. The model simulation spans from<br />

1 May to 31 October for the year 2001 to 2007. The daily<br />

precipitation simulated by the model is compared with the<br />

daily gridded rainfall data of India Meteorological<br />

Department (IMD) at 1 o x1 o resolutions for the land areas<br />

and for the land-ocean area the GPCP and TRMM rainfall<br />

are used.<br />

3. Results and Discussion<br />

a. The monsoon circulation pattern<br />

It is important to examine whether the driving field in the<br />

mother domain are adequate for the nested domain<br />

particularly in connection with synoptic scale climatic<br />

features of Indian summer monsoon. So the JJAS mean<br />

wind (2001-2007) at 850 hPa for each of the three<br />

schemes and from NCEP/NCAR (NNRP) reanalysis are<br />

showed in Fig. 1. The large scale southwesterly flow over<br />

Arabian Sea and Bay of Bengal (BOB) and a cyclonic<br />

vorticity in the north of BOB are reasonably captured by<br />

all the three cumulus schemes (Figs. 1b-d) as compared to<br />

the NNRP (Fig. 1a).<br />

Figure 1. JJAS averaged mean 850 hPa wind (m s -1 )<br />

from (a) NNRP, (b) BMJ, (c) KF and (d) GD for the<br />

year 2001-2007.<br />

However the wind field by KF (Fig. 1c) over the Arabian<br />

Sea and BOB appears to be stronger than the observation<br />

(Fig. 1a). The BMJ is found to have (Fig. 1b) simulated<br />

the most realistic wind field in both the oceanic basin<br />

where as the GD (Fig. 1d) has produced a weaker wind<br />

field over BOB although the Arabian Sea branch is<br />

reasonably reproduced. The upper air (200 hpa) easterly<br />

and the Tibetan anticyclone are captured by all the three<br />

experiments with BMJ, KF and GD (Figures not shown)<br />

but with varied intensity. The center of the anticyclone is

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