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Effects of spatial resolution on WRF v3.8.1 simulated meteorology over the central Himalaya
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Abstract. The sensitive ecosystem of the central Himalayan (CH) region, which is experiencing
enhanced stress from anthropogenic forcing, requires adequate atmospheric
observations and an improved representation of the Himalaya in the models.
However, the accuracy of atmospheric models remains limited in this region
due to highly complex mountainous topography. This article delineates the
effects of spatial resolution on the modeled meteorology and dynamics over
the CH by utilizing the Weather Research and Forecasting (WRF) model
extensively evaluated against the Ganges Valley Aerosol Experiment (GVAX)
observations during the summer monsoon. The WRF simulation is performed over a
domain (d01) encompassing northern India at 15 km × 15 km resolution and
two nests (d02 at 5 km × 5 km and d03 at 1 km × 1 km) centered over the CH, with
boundary conditions from the respective parent domains. WRF simulations reveal
higher variability in meteorology, e.g., relative humidity
(RH = 70.3 %–96.1 %) and wind speed (WS = 1.1–4.2 m s−1), compared to
the ERA-Interim reanalysis (RH = 80.0 %–85.0 %, WS = 1.2–2.3 m s−1) over northern India owing to the higher resolution. WRF-simulated
temporal evolution of meteorological variables is found to agree with
balloon-borne measurements, with stronger correlations aloft (r = 0.44–0.92) than those in the lower troposphere (r = 0.18–0.48). The
model overestimates temperature (warm bias by 2.8 ∘C) and underestimates
RH (dry bias by 6.4 %) at the surface in d01. Model results show a
significant improvement in d03 (P = 827.6 hPa, T = 19.8 ∘C,
RH = 92.3 %), closer to the GVAX observations (P = 801.4 hPa, T = 19.5 ∘C, RH = 94.7 %). Interpolating the output from the coarser domains
(d01, d02) to the altitude of the station reduces the biases in pressure and
temperature; however, it suppresses the diurnal variations, highlighting the
importance of well-resolved terrain (d03). Temporal variations in
near-surface P, T, and RH are also reproduced by WRF in d03 to an extent (r>0.5). A sensitivity simulation incorporating the feedback from
the nested domain demonstrates the improvement in simulated P, T, and RH over
the CH. Our study shows that the WRF model setup at finer spatial resolution
can significantly reduce the biases in simulated meteorology, and such an
improved representation of the CH can be adopted through domain feedback into
regional-scale simulations. Interestingly, WRF simulates a dominant easterly
wind component at 1 km × 1 km resolution (d03), which is missing in the
coarse simulations; however, the frequency of southeasterlies remains
underestimated. The model simulation implementing a high-resolution (3 s)
topography input (SRTM) improved the prediction of wind directions;
nevertheless, further improvements are required to better reproduce the
observed local-scale dynamics over the CH.
Title: Effects of spatial resolution on WRF v3.8.1 simulated meteorology over the central Himalaya
Description:
Abstract.
The sensitive ecosystem of the central Himalayan (CH) region, which is experiencing
enhanced stress from anthropogenic forcing, requires adequate atmospheric
observations and an improved representation of the Himalaya in the models.
However, the accuracy of atmospheric models remains limited in this region
due to highly complex mountainous topography.
This article delineates the
effects of spatial resolution on the modeled meteorology and dynamics over
the CH by utilizing the Weather Research and Forecasting (WRF) model
extensively evaluated against the Ganges Valley Aerosol Experiment (GVAX)
observations during the summer monsoon.
The WRF simulation is performed over a
domain (d01) encompassing northern India at 15 km × 15 km resolution and
two nests (d02 at 5 km × 5 km and d03 at 1 km × 1 km) centered over the CH, with
boundary conditions from the respective parent domains.
WRF simulations reveal
higher variability in meteorology, e.
g.
, relative humidity
(RH = 70.
3 %–96.
1 %) and wind speed (WS = 1.
1–4.
2 m s−1), compared to
the ERA-Interim reanalysis (RH = 80.
0 %–85.
0 %, WS = 1.
2–2.
3 m s−1) over northern India owing to the higher resolution.
WRF-simulated
temporal evolution of meteorological variables is found to agree with
balloon-borne measurements, with stronger correlations aloft (r = 0.
44–0.
92) than those in the lower troposphere (r = 0.
18–0.
48).
The
model overestimates temperature (warm bias by 2.
8 ∘C) and underestimates
RH (dry bias by 6.
4 %) at the surface in d01.
Model results show a
significant improvement in d03 (P = 827.
6 hPa, T = 19.
8 ∘C,
RH = 92.
3 %), closer to the GVAX observations (P = 801.
4 hPa, T = 19.
5 ∘C, RH = 94.
7 %).
Interpolating the output from the coarser domains
(d01, d02) to the altitude of the station reduces the biases in pressure and
temperature; however, it suppresses the diurnal variations, highlighting the
importance of well-resolved terrain (d03).
Temporal variations in
near-surface P, T, and RH are also reproduced by WRF in d03 to an extent (r>0.
5).
A sensitivity simulation incorporating the feedback from
the nested domain demonstrates the improvement in simulated P, T, and RH over
the CH.
Our study shows that the WRF model setup at finer spatial resolution
can significantly reduce the biases in simulated meteorology, and such an
improved representation of the CH can be adopted through domain feedback into
regional-scale simulations.
Interestingly, WRF simulates a dominant easterly
wind component at 1 km × 1 km resolution (d03), which is missing in the
coarse simulations; however, the frequency of southeasterlies remains
underestimated.
The model simulation implementing a high-resolution (3 s)
topography input (SRTM) improved the prediction of wind directions;
nevertheless, further improvements are required to better reproduce the
observed local-scale dynamics over the CH.
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