{"title":"世界主要沙漠中太阳日照与沙尘之间的联系","authors":"J. Barkan, P. Alpert","doi":"10.2174/1874282301004010101","DOIUrl":null,"url":null,"abstract":"The annual link between the solar insolation, the surface temperature, and the dust load in the atmosphere as estimated by the TOMS Aerosol Index was compared in five major sandy deserts around the globe. A high correlation was found between the insolation and the dust in all deserts, while the correlation of dust with temperature was lower. The peaks of the insolation and the dust occurred almost simultaneously on the same date in three out of the five deserts i.e. Sahara, S.W. North American, Atacama. In the other two deserts i.e., Australian, Taklimakan, the peak of the dust occurs earlier in the year. The temperature peaks occur on a later date in all the deserts. Our conclusion is, that in the deserts of the world the radiation is the major cause of the total dust loading. Alpert et al. 2006 (1) found that the total amount of dust in the atmosphere is highly correlated with the solar insolation over the Saharan desert. Moreover, the annual maximum is reached almost on the same day, while the maximum temperature occurs a month later. This high match exists in the very great expanse of the Sahara, while in smaller areas (like the three distinct parts of the Sahara that were examined), other variables, like the local topography, the synoptic situation, etc., appear to weaken the link between dust and insolation, thus lowering the correlation. The theoretical foundation for this high correlation was discussed in detail in that paper and are summarized in chapter 2 of this paper. In this manuscript, we compare the annual link between dust, solar insolation, and the surface temperature in the Sahara and four other major sandy deserts in the world. The four other deserts examined are: the sandy part of the Australian desert, the Arizona and Sonora deserts in the Southwestern U.S and Mexico, the Taklimakan Desert in China, and the Atacama Desert in Chile. We show that in all these deserts the role of solar insolation concerning dust loading is very important, even dominant. This, in spite of the smaller areas of these deserts when compared with the Sahara, as well as their less favorable environment, such as more rugged topography, and stronger and more erratic synoptic systems. One potential application of the present findings may be the direct incorporation of the solar insolation in dust prediction models. The strong correlation of radiation and dust load dates in the major deserts around the world can further improve these models. 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The peaks of the insolation and the dust occurred almost simultaneously on the same date in three out of the five deserts i.e. Sahara, S.W. North American, Atacama. In the other two deserts i.e., Australian, Taklimakan, the peak of the dust occurs earlier in the year. The temperature peaks occur on a later date in all the deserts. Our conclusion is, that in the deserts of the world the radiation is the major cause of the total dust loading. Alpert et al. 2006 (1) found that the total amount of dust in the atmosphere is highly correlated with the solar insolation over the Saharan desert. Moreover, the annual maximum is reached almost on the same day, while the maximum temperature occurs a month later. This high match exists in the very great expanse of the Sahara, while in smaller areas (like the three distinct parts of the Sahara that were examined), other variables, like the local topography, the synoptic situation, etc., appear to weaken the link between dust and insolation, thus lowering the correlation. The theoretical foundation for this high correlation was discussed in detail in that paper and are summarized in chapter 2 of this paper. In this manuscript, we compare the annual link between dust, solar insolation, and the surface temperature in the Sahara and four other major sandy deserts in the world. The four other deserts examined are: the sandy part of the Australian desert, the Arizona and Sonora deserts in the Southwestern U.S and Mexico, the Taklimakan Desert in China, and the Atacama Desert in Chile. We show that in all these deserts the role of solar insolation concerning dust loading is very important, even dominant. This, in spite of the smaller areas of these deserts when compared with the Sahara, as well as their less favorable environment, such as more rugged topography, and stronger and more erratic synoptic systems. One potential application of the present findings may be the direct incorporation of the solar insolation in dust prediction models. The strong correlation of radiation and dust load dates in the major deserts around the world can further improve these models. 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引用次数: 4
摘要
根据TOMS气溶胶指数估算的太阳日照量、地表温度和大气中沙尘量之间的年度联系在全球五大沙漠中进行了比较。所有沙漠的日晒与沙尘有较高的相关性,而沙尘与温度的相关性较低。5个沙漠中的3个,即撒哈拉沙漠、北美西南部、阿塔卡马沙漠,日晒高峰和沙尘高峰几乎同时出现在同一天。在另外两个沙漠,即澳大利亚和塔克拉玛干沙漠,沙尘的高峰出现在一年中的早些时候。在所有的沙漠中,温度峰值都出现在较晚的日期。我们的结论是,在世界沙漠中,辐射是总沙尘负荷的主要原因。Alpert et al. 2006(1)发现大气中的尘埃总量与撒哈拉沙漠上空的太阳日晒高度相关。此外,年最高气温几乎在同一天达到,而最高气温在一个月后出现。这种高度匹配存在于撒哈拉沙漠的广大地区,而在较小的地区(如所研究的撒哈拉沙漠的三个不同部分),其他变量,如当地地形、天气情况等,似乎削弱了沙尘和日晒之间的联系,从而降低了相关性。本文详细讨论了这种高相关性的理论基础,并在第二章进行了总结。在这份手稿中,我们比较了撒哈拉沙漠和世界上其他四个主要沙漠的沙尘、太阳日照和地表温度之间的年度联系。其他四个被研究的沙漠是:澳大利亚沙漠的沙质部分,美国西南部和墨西哥的亚利桑那和索诺拉沙漠,中国的塔克拉玛干沙漠,智利的阿塔卡马沙漠。我们表明,在所有这些沙漠中,太阳日照对沙尘负荷的作用是非常重要的,甚至是主导的。尽管与撒哈拉相比,这些沙漠的面积更小,而且它们的环境也不太有利,比如更崎岖的地形,以及更强、更不稳定的天气系统。本研究结果的一个潜在应用可能是将太阳日晒直接纳入尘埃预测模型。世界主要沙漠的辐射和沙尘负荷数据的强相关性可以进一步改进这些模型。更好的沙尘事件短期和长期预报模型可以帮助处理
The Linkage Between Solar Insolation and Dust in the Major World Deserts
The annual link between the solar insolation, the surface temperature, and the dust load in the atmosphere as estimated by the TOMS Aerosol Index was compared in five major sandy deserts around the globe. A high correlation was found between the insolation and the dust in all deserts, while the correlation of dust with temperature was lower. The peaks of the insolation and the dust occurred almost simultaneously on the same date in three out of the five deserts i.e. Sahara, S.W. North American, Atacama. In the other two deserts i.e., Australian, Taklimakan, the peak of the dust occurs earlier in the year. The temperature peaks occur on a later date in all the deserts. Our conclusion is, that in the deserts of the world the radiation is the major cause of the total dust loading. Alpert et al. 2006 (1) found that the total amount of dust in the atmosphere is highly correlated with the solar insolation over the Saharan desert. Moreover, the annual maximum is reached almost on the same day, while the maximum temperature occurs a month later. This high match exists in the very great expanse of the Sahara, while in smaller areas (like the three distinct parts of the Sahara that were examined), other variables, like the local topography, the synoptic situation, etc., appear to weaken the link between dust and insolation, thus lowering the correlation. The theoretical foundation for this high correlation was discussed in detail in that paper and are summarized in chapter 2 of this paper. In this manuscript, we compare the annual link between dust, solar insolation, and the surface temperature in the Sahara and four other major sandy deserts in the world. The four other deserts examined are: the sandy part of the Australian desert, the Arizona and Sonora deserts in the Southwestern U.S and Mexico, the Taklimakan Desert in China, and the Atacama Desert in Chile. We show that in all these deserts the role of solar insolation concerning dust loading is very important, even dominant. This, in spite of the smaller areas of these deserts when compared with the Sahara, as well as their less favorable environment, such as more rugged topography, and stronger and more erratic synoptic systems. One potential application of the present findings may be the direct incorporation of the solar insolation in dust prediction models. The strong correlation of radiation and dust load dates in the major deserts around the world can further improve these models. Better models for short and long term forecasting of dust events can aid in dealing with