Fine analysis of clouds and precipitations observed with mm-wave Doppler radar FALCON-I (Conference Presentation)

T. Takano
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引用次数: 0

Abstract

Observation of clouds and precipitations with radars in millimeter waves is one of the most fruitful method to investigate those interior structures because the sensitivities for small particles and droplets are much better than those in longer wavelengths. We have developed the cloud profiling FMCA (Frequency Modulated Continuous Wave) 95 GHz Doppler Radar, named “FALCON-I” (Fig.1; FALCON=FMCW Radar for Cloud Observations), at Chiba University. FALCON-I consists of two 1-m diameter antennas and has a spatial resolution of 0.18 degree (which corresponds to 15m at the height of 5km) and ranging resolution of typically 50m. We make regular observations at zenith with the temporal interval of 10 seconds and make scanning observations with +/- 5-degree in one direction from the zenith with the interval of 15 seconds when we want to observe spatial extent of clouds. Fig.2 shows clouds and precipitations observed with FALCON-I on 15 August 2017 at Chiba University. Time-height intensity map from 00:00-02:00 UT (09:00-11:00 JST; Fig.2a) and Doppler profile map at 00:50 UT (Fig.2b) are presented. The intensity map shows that precipitations started around 00:35 UT at the height of 5 km. The Doppler profile map shows the cloud at 5-7km in height has Doppler velocities about 0 to -2 m/s, which negative velocity means downward motion. At the bottom of the cloud i.e. 5km in height, rain droplets with the Doppler velocities of up to -6 m/s are abruptly produced within a few hundred meters in height. Terminal velocity of 6 m/s corresponds to about 2 mm diameter droplets. Rain droplets were produced intermittently in this case and one of the gropes of droplets is marked with a solid line which just started falling below the cloud bottom as shown in Fig.2b. We can recognize several groups of droplets whose inclines in Fig.2b are getting steeper with falling down. We can derive droplet number distribution N(D) from the Doppler spectra by assuming the observed velocities are terminal velocities. Successive Doppler profile maps and movies from 00:30 to 01:00 UT show dynamic phenomena in the beginning phase of precipitations such as production and acceleration of rain droplets at the bottom of the cloud, evaporation of droplets, changes of number distributions during the falling way, and so on. These results of analysis show that observations of millimeter-wave Doppler radar FALCON-I are powerful methods to investigate micro processes in clouds and precipitations. Fig.1. Cloud Profiling Doppler Radar FALCON-I consists two 1-m antennas and observes clouds and precipitations at 95GHz with high spatial resolution of 0.18 degree. Fig.2. Clouds and precipitations observed with FALCON-I on 15 August 2017 at Chiba University. Time-height intensity map from 00:00-02:00 UT (a) and Doppler profile map at 00:50 UT (b) are presented. The intensity map shows that precipitations occurred around 00:35 UT at the height of 5 km. The Doppler profile map shows the cloud at 5-7km in height has Doppler velocities about 0 to -2 m/s, which negative velocity means downward motion. At the bottom of the cloud i.e. 5km in height, rain droplets with the Doppler velocities of up to -6 m/s are abruptly produced within a few hundred meters. Terminal velocity of 6 m/s corresponds to about 2 mm diameter droplets. Rain droplets were produced intermittently in this case and falling as shown in (b).
用毫米波多普勒雷达falcon - 1观测到的云和降水的精细分析(会议报告)
利用毫米波雷达对云和降水进行观测是研究这些内部结构最有效的方法之一,因为毫米波雷达对小颗粒和液滴的灵敏度要比波长更长的雷达高得多。我们开发了云廓线FMCA(调频连续波)95 GHz多普勒雷达,命名为“falcon - 1”(图1;隼=FMCW云观测雷达),在千叶大学。猎鹰- 1由两个直径为1米的天线组成,空间分辨率为0.18度(在5公里高度对应15米),测距分辨率通常为50米。我们在天顶进行定期观测,时间间隔为10秒,当我们要观测云的空间范围时,我们从天顶开始在一个方向上进行+/- 5度的扫描观测,时间间隔为15秒。2为2017年8月15日在千叶大学用猎鹰一号观测到的云和降水。00:00-02:00 UT (09:00-11:00 JST)时高强度图;图2a)和00:50 UT时的多普勒剖面图(图2b)。强度图显示,降水开始于00:35 UT左右,高度为5km。多普勒剖面图显示,云层在5-7km高度的多普勒速度约为0 ~ -2 m/s,负速度意味着向下运动。在云的底部,即5公里的高度,在几百米的高度内突然产生多普勒速度可达-6米/秒的雨滴。终端速度为6m /s时,液滴的直径约为2mm。在这种情况下,雨滴是间歇性地产生的,其中一组水滴被标记为一条实线,它刚刚开始落在云底以下,如图2b所示。我们可以在图2b中识别出几组水滴,它们的倾斜度随着下落而变陡。假设观测到的速度为终端速度,可以从多普勒光谱推导出液滴数分布N(D)。00:00 ~ 01:00连续多普勒剖面图和影像显示了降水开始阶段的动态现象,如云底雨滴的产生和加速、水滴的蒸发、下落过程中雨滴数量分布的变化等。这些分析结果表明,falcon - 1毫米波多普勒雷达的观测是研究云和降水微过程的有力方法。云廓形多普勒雷达falcon - 1由2根1m天线组成,在95GHz波段观测云和降水,空间分辨率为0.18度。2017年8月15日在千叶大学用猎鹰一号观测到的云和降水。给出00:00-02:00 UT时高强度图(a)和00:50 UT时多普勒剖面图(b)。强度图显示,降水发生在00:35 UT左右,高度为5km。多普勒剖面图显示,云层在5-7km高度的多普勒速度约为0 ~ -2 m/s,负速度意味着向下运动。在云的底部,即5公里的高度,在几百米内突然产生了多普勒速度高达-6米/秒的雨滴。终端速度为6m /s时,液滴的直径约为2mm。在这种情况下,雨滴间歇性地产生,并降落在(b)中。
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