陈勇,段婧,王新,郭强,张小鹏. 2023. 基于FY-4A的庐山云海特征及其成因研究. 气象学报,81(6):973-984. DOI: 10.11676/qxxb2023.20220188
引用本文: 陈勇,段婧,王新,郭强,张小鹏. 2023. 基于FY-4A的庐山云海特征及其成因研究. 气象学报,81(6):973-984. DOI: 10.11676/qxxb2023.20220188
Chen Yong, Duan Jing, Wang Xin, Guo Qiang, Zhang Xiaopeng. 2023. Identifying the seas of clouds around Mt. Lu based on FY-4A satellite observations: Formation and sustenance. Acta Meteorologica Sinica, 81(6):973-984. DOI: 10.11676/qxxb2023.20220188
Citation: Chen Yong, Duan Jing, Wang Xin, Guo Qiang, Zhang Xiaopeng. 2023. Identifying the seas of clouds around Mt. Lu based on FY-4A satellite observations: Formation and sustenance. Acta Meteorologica Sinica, 81(6):973-984. DOI: 10.11676/qxxb2023.20220188

基于FY-4A的庐山云海特征及其成因研究

Identifying the seas of clouds around Mt. Lu based on FY-4A satellite observations: Formation and sustenance

  • 摘要: 利用FY-4A卫星等资料分析了2019—2021年的19次庐山白天云海过程(12个传统云海和7个瀑布云过程),研究了庐山云海特征及其形成机制,评估了卫星资料在云海识别中的应用。研究表明:FY-4A可见光云图可基本辨识庐山云海范围及宏观演变特征,但较难刻画出小尺度瀑布云的精细结构;FY-4A的云顶高度L2产品可用于庐山传统云海的识别,但较难识别瀑布云过程。非洋面海岛的庐山也存在云系尾流现象且频率较高(共3次过程),由绕流作用形成的尾流云系呈逗号状分布,做规律性摆动但无连续涡旋;该尾流型云海形成的主要因素是庐山为相对周边孤立的椭圆形山体、冷高压底部的强北风低空急流、山腰逆温层。庐山云海发生时大多受地面高压控制且位于850 hPa的高湿区或边缘区域,该区域的弱下沉运动形成的逆温层和低空充沛的水汽有利于庐山云海形成及维持。

     

    Abstract: The characteristics, recognition and formation of seas of clouds (SOC) around Mt. Lu are studied based on FY-4A observations and other data. From 2019 to 2021, 19 events of SOCs are recorded in the dataset, including 12 traditional SOCs (TSOC) and 7 small-scale SOCs with cloud waterfalls over Mt. Lu (SSOC). The FY-4A visible-channel cloud image can identify the area and development of TSOC but cannot capture the detailed structure of SSOC. The L2 cloud-top-height product of FY-4A can be used for the recognition of TSOC around Mt. Lu but cannot be used for the recognition except of SSOC. Normally the wake phenomena of SOC (WSOC) occur on islands over the sea, but three WSOC events are found in Mt. Lu, although it is located in the land. The WSOC in Mt. Lu exhibits a comma-type cloud pattern with regular fluctuations but without continuous vortexes. The formation of the WSOC in Mt. Lu is mainly caused by the isolated ellipse shape of Mt. Lu, the northernly low-level jet, and the temperature inversion layer below the mountain top. Besides, for most SOC events, Mt. Lu is under the control of high-pressure systems and located in high-humidity region, where the synoptic-scale subsidence inversion layer and sufficient moisture could play an important role in the forming and maintenance of SOCs over Mt. Lu.

     

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