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首页> 外文期刊>International journal of remote sensing >Atmospheric boundary layer response sequence to the 2019 annular solar eclipse over a tropical rural terrain
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Atmospheric boundary layer response sequence to the 2019 annular solar eclipse over a tropical rural terrain

机译:2019年环形日食的大气边界层响应序列在热带农村地形上

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Transient alterations in the surface meteorological parameters and atmospheric boundary layer (ABL) due to annual solar eclipse occurred on 26 December 2019 have been investigated using collocated ground-based remote-sensing and in situ measurements over a tropical rural station, Gadanki (13.5 oN, 79.2 oE). This event had provided an opportunity to assess the eclipse effect on atmospheric parameters as it occurred during initial hours of the boundary layer evolution (between 08:07 IST and 11:15 IST with peak at 09:32 IST over Gadanki). As eclipse commenced, the observations showed a dramatic reduction in the incoming shortwave radiation and consequent changes in air temperature and wind patterns throughout the ABL. Nevertheless, the amplitude of the changes in various parameters is not analogous to the obscuration proportions but is significantly dictated by the background meteorological conditions such as prevalence of dense fog and cloudiness during the eclipse timings. Ceilometer and wind profiler observations have provided the high-resolution continuous signatures of clouds and fog, strong subsidence, thick layers above the ABL, and a clear change in ABL height (ABLH) during the eclipse epoch. Interestingly, the delay in the evolution of ABL due to the eclipse is clearly manifested. The ABLH, which remained shallow even after the eclipse peak, has shown a rapid increase by more than 1000 m within a short span of an hour just before and after the eclipse culmination. However, significant delay (of about 2 hours after the eclipse) is observed in the surface variables to fall in the range of their climatological values. The observations elusively suggest that commence and termination phases of eclipse analogously influenced the surface and boundary layer parameters in descending sequence (eclipse effect is subtly seen first in Ceilometer and wind profiler attributes followed by surface state variables).
机译:由于2019年12月26日发生了由于年度日常日食的表面气象参数和大气边界层(ABL)的瞬态改变已经在Gadanki(13.5 On, 79.2 OE)。本次活动提供了在边界层演变的初始小时内(08:07 IST之间的初始小时内发生的大气参数)对大气参数进行评估的机会。随着Eclipse开始,观察结果表明,进入的短波辐射剧烈降低,并且在整个ABL中的空气温度和风图案中的变化。然而,各种参数的变化的幅度与遮蔽比例没有类似的,但是由于在日食期间的浓度雾和云度普遍存在的背景气象条件明显决定。 CeiLometer和Wind剖面观测已经提供了云和雾的高分辨率连续签名,强烈的ABL上方的沉降,厚层,并在Eclipse时期期间清楚地改变ABL高度(ABLH)。有趣的是,由于日食导致ABL的演变的延迟明显表现出来。甚至在日食峰之后仍然浅的ABLH,在Eclipse Culmination之前和之后,在一小时内的短跨度范围内快速增加了1000米。然而,在表面变量中观察到在表面变量中观察到其气候值范围的显着延迟(在日食后2小时)。该观察结果表明Eclipse的开始和终止阶段类似地影响了下降序列中的表面和边界层参数(Eclipse效果首先在Ceileometer和风轮廓属性中巧妙地看出,然后是表面状态变量)。

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