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Frontiers of Earth Science

ISSN 2095-0195

ISSN 2095-0209(Online)

CN 11-5982/P

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2018 Impact Factor: 1.205

Front. Earth Sci.    2022, Vol. 16 Issue (2) : 277-290    https://doi.org/10.1007/s11707-020-0854-9
RESEARCH ARTICLE
Effects of local and non-local closure PBL schemes on the simulation of Super Typhoon Mangkhut (2018)
Zixi RUAN1,2, Jiangnan LI1,2(), Fangzhou LI1, Wenshi LIN1
1. School of Atmospheric Sciences, and Guangdong Province Key Laboratory for Climate Change and Natural Disaster Studies, Sun Yat-sen University, Zhuhai 519082, China
2. Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai), Zhuhai 519082, China
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Abstract

With the convection-permitting simulation of Super Typhoon Mangkhut (2018) with a 3 km resolution for 10.5 days using mesoscale numerical model, Weather Research and Forecasting Model Version 4.1 (WRFV4.1), the influences of local closure QNSE planetary boundary layer (PBL) scheme and non-local closure GFS planetary boundary layer scheme on super typhoon Mangkhut are mainly discussed. It is found that in terms of either track or intensity of typhoon, the local closure QNSE scheme is better than the non-local closure GFS scheme. Local and non-local closure PBL schemes have a large influence on both the intensity and the structure of typhoon. The maximum intensity difference of the simulated typhoon is 50 hPa. The intensity of typhoon is closely related to its variations in structure. In the rapid intensification stage, the typhoon simulated by the QNSE scheme has a larger friction velocity, stronger surface latent heat flux, sensible heat flux and vapor flux, related to a higher boundary height and stronger vertical mixing. The latent heat flux and sensible heat flux on the surface conveyed energy upward for the typhoon while the water vapor was transported upward through vertical mixing. While the water vapor condensed, the latent heat was released, which further warmed the typhoon eyewall, strengthening the convection. The stronger winds also intensified the vertical mixing and the warm-core structure, further strengthened the typhoon. The differences in surface layer schemes dominated the differences between the two simulations.

Keywords typhoon      planetary boundary layer scheme      WRF model     
Corresponding Author(s): Jiangnan LI   
About author: Tongcan Cui and Yizhe Hou contributed equally to this work.
Online First Date: 01 June 2021    Issue Date: 26 August 2022
 Cite this article:   
Zixi RUAN,Jiangnan LI,Fangzhou LI, et al. Effects of local and non-local closure PBL schemes on the simulation of Super Typhoon Mangkhut (2018)[J]. Front. Earth Sci., 2022, 16(2): 277-290.
 URL:  
https://academic.hep.com.cn/fesci/EN/10.1007/s11707-020-0854-9
https://academic.hep.com.cn/fesci/EN/Y2022/V16/I2/277
Fig.1  Comparison of the simulated track of TC with observation (OBS) based on the CMA's TC database.
Fig.2  Simulated distance error (left, unit: km) and angle error (right, unit: °).
Fig.3  Comparison of simulated minimum sea level pressure of TC with observation.
Fig.4  Comparison of simulated maximum surface wind of TC with observation.
Assessment QNSE GFS
R 0.919496 0.83056
BIAS/hPa −14.0431 −38.0171
NBIAS/% −1.47856 −4.00272
RMSE/hPa 19.5743 44.3034
NRMSE/% 2.06083 4.66459
Tab.1  Assessment statistics of simulated minimum sea level pressure of TC
Assessment QNSE GFS
R 0.955226 0.823218
BIAS/(m·s−1) 6.64404 15.9988
NBIAS/% 14.9462 35.9904
RMSE/(m·s−1) 8.556 19.5313
NRMSE/% 19.2473 43.9371
Tab.2  Assessment statistics of simulated maximum surface wind of TC
Fig.5  Time variation of simulated regional average (within a radius of 150 km from TC center) (a) surface sensible heat flux (HFX), (b) surface latent heat flux (LH), (c) surface water vapor flux (QFX), (d) surface friction velocity (U*) and (e) boundary layer height (PBLH) during the mature stage (from 00:00 of 10th to 00:00 of 13th, the same below).
Fig.6  Simulated surface sensible heat fluxes (unit: W/m2) of TC at 00:00 on 13 September, 2018.
Fig.7  Simulated surface latent heat fluxes (unit: W/m2) of TC at 00:00 on 13 September, 2018.
Fig.8  Simulated water vapor fluxes (unit: 104kg·m2·s1) of TC at 00:00 on 13 September, 2018.
Fig.9  Simulated azimuthally-averaged vertical velocity (unit: m/s) of TC inner core at 00:00 on 13 September, 2018 at radius-height.
Fig.10  Simulated azimuthally-averaged tangential wind speed (unit: m/s) of TC inner core at 00:00 on 13 September, 2018 at radius-height.
Fig.11  Simulated azimuthally-averaged radial wind speed (unit: m/s) of TC inner core at 00:00 on 13 September, 2018 at radius-height.
Fig.12  Simulated time variation of vertical-averaged and azimuthally-averaged radar reflectivity factor (unit: dBz) of TC inner core during the mature stage.
Fig.13  Simulated time variation of vertical-averaged and azimuthally-averaged tangential wind speed (unit: m/s) of TC inner core during the mature stage.
Fig.14  Simulated time variation of vertical-averaged and azimuthally-averaged radial wind speed (unit: m/s) of TC inner core during the mature stage.
Fig.15  Simulated time variation of vertical-averaged and azimuthally-averaged vertical velocity (unit: m/s) of TC inner core during the mature stage.
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