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利用MPAS(Model for Prediction Across Scales)和北京大学浅水模式(PKU_SWM)对余弦钟和Rossby-Haurwitz波理想个例进行了模拟。结果表明:在余弦钟测试中,MPAS能更好的模拟出余弦钟的基本形态,但模拟结果的绝对误差较大;网格分辨率提高后,MPAS模拟效果提升得更明显。在Rossby-Haurwitz波测试中,MPAS模拟的槽脊位置和强度更加接近于初始分布形态,PKU_SWM模拟的槽脊的强度偏强,位置偏西,MPAS模拟效果整体要优于PKU_SWM;网格分辨率提高后,两模式模拟效果都有较大的提升。  相似文献   
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利用不同水平分辨率下的中尺度数值模式WRF模拟1319号超强台风"天兔",以研究模式水平分辨率对台风强度和微结构(包括动力和微物理)的影响。模拟结果表明:不同水平分辨率(1 km、2 km、3 km、4km、5 km)模拟的台风路径差异不大,且均与实况基本相同;不同水平分辨率对台风强度和微结构的模拟效果影响较大,其中以对10 m最大风速、垂直运动和降水强度的影响为最大。将模式水平分辨率提高到1 km有助于改善台风强度和微结构的模拟效果。在较低分辨率下,台风非对称性较明显、眼墙倾斜程度较大和海表水汽通量较小等结构特征共同使得台风强度较小。  相似文献   
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Typhoon Usagi (1319) was simulated by using the Advanced Weather Research and Forecasting numerical model (WRF) with different horizontal resolution to understand the impact of horizontal resolution on the intensity and characteristics of typhoon’s microstructures (including dynamic and microphysical structure). The simulated results show that the improvement of horizontal resolution from 5 km to 1 km has little impact on the track which is comparable to real results, but has a significant impact on the intensity and microstructures, and especially, the impact on wind speed at 10 m height, the vertical movement and precipitation intensity is the greatest. When the resolution is increased to 1 km, the intensity and characteristics of typhoon’s microstructures can be simulated better. In lower resolution simulations, some structural characteristics, including more asymmetrical and more outward tilted eyewall, and less water vapor flux on sea surface, work together to weaken typhoon intensity.  相似文献   
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Based on high-fidelity numerical simulation by using the Weather Research and Forecast (WRF) model, we analyzed the formation and replacement mechanism of the concentric eyewall of Super Typhoon Muifa (1109) from the aspects of the potential vorticity (PV), dynamic/ thermodynamic structure change, sea surface flux, and water vapor content. Observational data and sensitivity tests were also adopted to verify the results. We found that: (1) The abnormal increase of the PV in the rain zone is mainly due to the condensation latent heat. Sufficient water vapor conditions are beneficial to the formation of the outer eyewall structure, and when the environmental water vapor content is larger, the intensity of the outer eyewall becomes greater. (2) After the formation of the typhoon’s outer eyewall, in the area where the outer eyewall is located, the increase of inertial stability contributes to the decrease of the intensity of the inner eyewall. When the intensity of the outer eyewall is larger, the divergence and subsidence motion in the upper layer of the outer eyewall has a greater weakening effect on the intensity of the inner eyewall. (3) The increase of potential temperature of the outer eyewall is mainly due to the condensation latent heat release and the warming of dry air subsidence motion in the moat area. (4) The increase of sea surface heat flux can prolong the concentric eyewall replacement process.  相似文献   
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