In the past few decades, the climate has undergone significant change, and through the 1990s the world has experienced a major El-Ni o. Such change is likely to affect dust storm activity in dust prone parts of the world. A significant dust prone area is Saudi Arabia. To determine whether the ENSO cycle has had any influence on synoptic conditions over Saudi Arabia and hence dust activity, dust frequency has been examined over the period covering the past three decades. In this thesis, dust events have been classified into Haze, Local Dust Events (LDEs) and Dust Storms (DSs). Dust activity for 25 cities across Saudi Arabia was analysed for frequency of each type of dust event. It was found that in general, the cities in the south and south-east experienced the most number of dust events, with Haze being the most prevalent dust event. However, there were cities, which as a result of either their altitude or surrounding topography experienced much fewer dust events than their neighbours in the same region. Spring was shown to be the most dust prone season in the northern parts whilst the southern parts experience more dust events in summer. Potential dust sources were identified using back trajectories generated by the HYSPLIT (Hybrid Single Particle Lagrangian Integrated Trajectory Model) modelling program, in conjunction with wind roses, during the days of dust in the most active dust season, spring. In the northern region, the An-Nafud Desert appears to be the main local source, while the North African deserts (Sahara), the Syrian Desert and Iraqi deserts are the main remote and neighbouring sources. In the western region, the eastern North African deserts appear to be the main sources, although dust can come from the Rakbah Plains to the east. In the central region, the Iraqi desert area is the major source dust. Gassim in the north-central region is also affected by dust from the Sahara, while Riyadh being closer to the Rub al Khali, is affected more by dust from Rub al Khali. There is also some contribution from the Ad-Dahna Desert. For the eastern region, the Iraqi desert areas on the border in the northern region are the main source of dust, while the Rub al Khali and the Ad-Dahna Desert are local sources. For the southern region, the Rub al Khali is a major local source and the eastern North African deserts are remote sources. There is also a measurable contribution from the arid areas of Yemen for Najran and Sharurah. For most cities, maximum wind speeds were always higher on dust-days (averaging 20 ms-1) than on dust-free days (averaging about 10 ms-1). The study period was classified into three time periods based on the frequency of total dust events: 1985-1994, 1995-2009 and 2010-2013. The frequency of all three types of dust events was determined for eight of the most dust prone cities in Saudi Arabia. Except for Riyadh, which has had a statistically significant increase in Haze, nearly all cities had a statistically significant decrease in dust activity for all three types of dust events. An examination of the mean sea level pressure patterns over the same period shows some subtle changes in the intensity and position of the dominant pressure systems, particularly in spring and summer. This change may be reflected in the change in dust event frequency. However, the relationship between the Southern Oscillation Index (SOI) and dust activity was found to be quite weak. The strongest correlation was found between annual DS (dust storm) frequency and the SOI, and between annual Haze and LDE frequency and rainfall over the Rub al Khali. There was also a moderate correlation between annual Haze frequency and total rainfall over Saudi Arabia. A number of case studies were examined for both Saudi Arabia and Australia, which showed similarities in preceding synoptic conditions. In all cases, there was the existence of a zone of baroclinity, which causes atmospheric instability, a major trigger for dust storms. This research will contribute to the knowledge of dust research in Saudi Arabia. The contribution to research in Saudi Arabia is based on comprehensive analysis of temporal and spatial distribution of different types of dust over the last three decades. It has found significant behavioural change in dust activity, especially in Haze and LDE related to the changing phase of the ENSO cycle and also to rainfall variation over the Rub al Khali. The airflow pathways of dust and dust-free days were identified using HYSPLIT for spring, enabling potential dust sources to be pinpointed.
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机译:在过去的几十年中,气候发生了重大变化,整个1990年代,世界经历了主要的厄尔尼诺现象。这种变化可能会影响世界上粉尘易发地区的沙尘暴活动。沙尘暴地区是一个容易生尘的地区。为了确定ENSO周期是否对沙特阿拉伯的天气状况和粉尘活动有影响,在过去的三十年中对粉尘频率进行了检查。在本文中,尘埃事件分为阴霾,局部尘埃事件(LDE)和沙尘暴(DS)。分析了沙特阿拉伯25个城市的沙尘活动,以分析每种沙尘事件的发生频率。结果发现,一般而言,南部和东南部的城市发生的灰尘事件最多,而霾是最普遍的灰尘事件。但是,有一些城市由于海拔或周围地形的原因,尘埃事件比同一地区的邻居少得多。春季被认为是北部地区最容易发生粉尘的季节,而南部地区在夏季会经历更多的粉尘事件。在春季最活跃的沙尘季节,使用HYSPLIT(混合单粒子拉格朗日综合轨迹模型)建模程序生成的后向轨迹,并结合风玫瑰,确定了潜在的粉尘源。在北部地区,安纳富德沙漠似乎是当地的主要来源,而北非沙漠(撒哈拉沙漠),叙利亚沙漠和伊拉克沙漠则是主要的偏远和邻近来源。在西部地区,北非东部沙漠似乎是主要来源,尽管粉尘可能来自东部的拉克巴平原。在中部地区,伊拉克沙漠地区是主要的粉尘源。中北部地区的加西姆也受到撒哈拉沙尘的影响,而利雅得更靠近鲁卜哈利沙漠,而鲁卜哈利沙漠的尘埃影响更大。 Ad-Dahna沙漠也有一些贡献。对于东部地区,北部地区边界上的伊拉克沙漠地区是主要的粉尘来源,而Rub al Khali和Ad-Dahna沙漠是当地的粉尘来源。对于南部地区,鲁卜哈利沙漠是当地的主要来源,而北非东部的沙漠则是偏远的来源。也门干旱地区对纳吉兰和沙鲁拉的贡献也很大。对于大多数城市,在无尘天(平均20 ms-1)的最大风速总是比无尘天(平均约10 ms-1)的高。根据总尘埃事件的发生频率,研究期分为三个时间段:1985-1994年,1995-2009年和2010-2013年。确定了沙特阿拉伯八个尘埃多发城市中所有三种尘埃事件的发生频率。除了利雅得的雾霾在统计上显着增加外,几乎所有城市在所有三种尘埃事件中的尘埃活动在统计学上均具有显着下降。对同期平均海平面压力模式的检查表明,主要压力系统的强度和位置有一些细微的变化,特别是在春季和夏季。这种变化可能反映在粉尘事件频率的变化中。但是,发现南方涛动指数(SOI)与粉尘活动之间的关系很弱。在鲁布哈利沙漠地区,年度DS(沙尘暴)频率与SOI之间,年度烟霾和LDE频率与降雨之间存在最强的相关性。沙特阿拉伯的年度烟霾发生频率与总降雨量之间也存在适度的相关性。对沙特阿拉伯和澳大利亚的许多案例研究进行了审查,结果显示在先前的天气条件下相似。在所有情况下,都存在一个斜压区,这会导致大气不稳定,这是引发沙尘暴的主要诱因。这项研究将有助于沙特阿拉伯的粉尘研究知识。对沙特阿拉伯研究的贡献是基于对过去三十年来不同类型粉尘的时空分布的综合分析。研究发现,尘埃活动的行为发生了重大变化,尤其是在霾和LDE中,与ENSO循环的变化阶段以及Rub al Khali上的降雨变化有关。使用HYSPLIT进行春季识别,确定了粉尘和无尘天的气流路径,从而查明了潜在的粉尘源。
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