Detecting non-stationarity of precipitation across coastal-terrestrial Virginia

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Xiaomin Yang, Xixi Wang, Zhaoyi Cai
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Abstract

Since the industrial revolution, the Earth's ambient temperature has been rising at an accelerating pace, partially due to the release of greenhouse gases (e.g., carbon dioxide) into the atmosphere. Consequently, precipitation may become nonstationary, leading to new patterns of watershed hydrology with more frequent and/or severe floods and droughts. Non-stationarity occurs when one or more of precipitation characteristics exhibit step changes, temporal trends, and/or variance deviations. The objective of this study was to detect historical variations in precipitation characteristics across coastal and terrestrial Virginia, USA. Thirteen indices were selected to represent precipitation characteristics for amount, intensity, spell, maximum, and exceedance. A modified Mann-Kendall technique was applied to detect step changes and/or temporal trends in these indices on an annual basis. The results indicated that most rain gauges showed a statistically significant step change in one or more indices between 1948 and 2019, with more step increases than step decreases. This indicates that precipitation across Virginia has exhibited non-stationarity, which must be considered for water management. This phenomenon is likely true for most coastal regions worldwide.

Abstract Image

探测弗吉尼亚沿海-陆地降水的非稳态性
自工业革命以来,地球的环境温度一直在加速上升,部分原因是温室气体(如二氧化碳)释放到大气中。因此,降水可能变得不稳定,导致流域水文出现新的模式,洪水和干旱更加频繁和/或严重。当一种或多种降水特征出现阶跃变化、时间趋势和/或方差偏差时,就会出现非稳态现象。本研究的目的是探测美国弗吉尼亚州沿海和陆地降水特征的历史变化。选择了 13 个指数来代表降水量、强度、峰值、最大降水量和超标降水量的特征。采用改进的 Mann-Kendall 技术来检测这些指数每年的阶跃变化和/或时间趋势。结果表明,1948 年至 2019 年间,大多数雨量计的一个或多个指数都出现了统计学意义上的阶跃变化,阶跃增加的指数多于阶跃减少的指数。这表明弗吉尼亚州各地的降水呈现出非稳态性,在水资源管理中必须考虑到这一点。这种现象可能在全球大多数沿海地区都存在。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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