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Aerosol vertical distribution and interactions with land/sea breezes over the eastern coast of the Red Sea from lidar data and high-resolution WRF-Chem simulations

机译:从LIDAR数据和高分辨率WRF-Chem模拟的红海东海岸陆地/海风的气溶胶垂直分布和互动

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With advances in modeling approaches and the application of satellite and ground-based data in dust-related research, our understanding of the dust cycle has significantly improved in recent decades. However, two aspects of the dust cycle, namely the vertical profiles and diurnal cycles, are not yet adequately understood, mainly due to the sparsity of direct observations. Measurements of backscattering caused by atmospheric aerosols have been ongoing since 2014 at the King Abdullah University of Science and Technology (KAUST) campus using a micro-pulse lidar (MPL) with a high temporal resolution. KAUST is located on the eastern coast of the Red Sea and currently hosts the only operating lidar system in the Arabian Peninsula. We use the data from the MPL together with other collocated observations and high-resolution simulations (with 1.33?km grid spacing) from the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) to study the following three aspects of dust over the Red Sea coastal plains. Firstly, we compare the model-simulated surface winds, aerosol optical depth (AOD), and aerosol size distributions with observations and evaluate the model performance in representing a typical large-scale dust event over the study site. Secondly, we investigate the vertical profiles of aerosol extinction and concentration in terms of their seasonal and diurnal variability. Thirdly, we explore the interactions between dust aerosols and land/sea breezes, which are the most influential components of the local diurnal circulation in the region. The WRF-Chem model successfully reproduced the diurnal profile of surface wind speed, AOD, and dust size distributions over the study area compared to observations. The model also captured the onset, demise, and height of a large-scale dust event that occurred in 2015, as compared to the lidar data. The vertical profiles of aerosol extinction in different seasons were largely consistent between the MPL data and WRF-Chem simulations along with key observations and reanalyses used in this study. We found a substantial variation in the vertical profile of aerosols in different seasons and between daytime and nighttime, as revealed by the MPL data. The MPL data also identified a prominent dust layer at ~5–7?km during the nighttime, which likely represents the long-range transported dust brought to the site by the easterly flow from remote inland deserts. The sea breeze circulation was much deeper (~2?km) than the land breeze circulation (~1?km), but both breeze systems prominently affected the distribution of dust aerosols over the study site. We observed that sea breezes push the dust aerosols upwards along the western slope of the Sarawat Mountains. These sea breezes eventually collide with the dust-laden northeasterly trade winds coming from nearby inland deserts, thus causing elevated dust maxima at a height of ~1.5?km above sea level over the mountains. Moreover, the sea and land breezes intensify dust emissions from the coastal region during the daytime and nighttime, respectively. Our study, although focused on a particular region, has broader environmental implications as it highlights how aerosols and dust emissions from the coastal plains can affect the Red Sea climate and marine habitats.
机译:随着建模方法和卫星和地面数据在与灰尘相关的研究中的应用,近几十年来,我们对灰尘周期的理解显着改善。然而,灰尘周期的两个方面,即垂直轮廓和昼夜循环,也没有得到充分的理解,主要是由于直接观察的稀疏性。自2014年以来,由大气气溶胶造成的反向散射的测量在阿卜杜拉理工大学国王科技(KAURT)校园内持续了,使用微脉冲激光乐队(MPL),具有高时间分辨率。 Kaust位于红海的东海岸,目前举办了阿拉伯半岛的唯一运营的激光雷达系统。我们将来自MPL的数据与其他并置的观测和高分辨率模拟(带有1.33 km网格间距)的数据从天气研究和预测模型与化学(WRF-Chem)一起研究,研究以下三个方面的灰尘红海沿海平原。首先,我们将模拟模拟表面风,气溶胶光学深度(AOD)和气溶胶尺寸分布进行了观察,并评估了在研究现场代表典型的大规模尘埃事件的模型性能。其次,我们在季节性和昼夜变异性方面调查气溶胶灭绝和浓度的垂直曲线。第三,我们探讨了尘埃气溶胶和陆地/海风之间的相互作用,这是该地区局部昼夜循环的最具影响力的组成部分。与观察结果相比,WRF-Chem模型成功地再现了研究区的表面风速,AOD和灰尘尺寸分布的差。与LIDAR数据相比,该模型还捕获了2015年发生的大规模尘埃事件的发病,消亡和高度。在不同季节中的气溶胶灭绝的垂直曲线在很大程度上是在MPL数据和WRF-Chem模拟之间的一致性,以及本研究中使用的主要观察和Reanalyses。我们在不同季节和白天和夜间之间发现了气溶胶垂直轮廓的大量变化,如MPL数据所透露。 MPL数据还在夜间〜5-7 km识别出突出的粉尘层,这可能代表从远程内陆沙漠中的东方流向该网站带来的远程运输粉尘。海风循环比土地微风循环更深(〜2 km)(〜1 km),但两条微风系统突出地影响了研究现场的尘埃气溶胶的分布。我们观察到海风沿着撒拉维特山脉的西坡向上推动尘埃气溶胶。这些海风最终与来自附近的内陆沙漠的东北贸易风相撞,从而在山上海平面的高度〜1.5 km的高度造成升高的尘埃。此外,海洋和陆地布雷兹分别在白天和夜间分别加剧了沿海地区的尘埃排放。我们的研究虽然专注于特定地区,但具有更大的环境影响,因为它突出了沿海平原的气溶胶和尘埃如何影响红海气候和海洋栖息地。

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