基于分形维数和Hurst指数方法的伊斯兰堡首都地区气候时间序列变异分析

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Ali Khan , Shahid Hussain , Ahmed Bakhet , Afshan Anwer , S.M. Murshid Raza , Sajjad Ali , Mohammed Zakarya
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引用次数: 0

摘要

本研究试图在伊斯兰堡首都地区(ICT)的地方尺度上研究气候参数的变异。气候变化可以影响温度趋势和降水模式、园艺活动、农业生产力、地下水位、可用水和基础设施。为了评估气候变化对伊斯兰堡首都地区的影响,利用巴基斯坦气象部门(PMD) 1983 - 2022年的降水、最低和最高气温资料。采用分形维数D和伤害指数H方法估算研究区月最高、最低气温和降水量。数据被分成4个子集。对数据集采用重标度极差分析法计算Hurst指数和分形维数。所得结果相应地显示出布朗随机和持续的趋势。另一方面,H在2013 - 2022年期间呈现反持续趋势,D在2013 - 2022年期间呈现随机趋势。显示持久结果的时间序列包含了长期记忆。当一个时间序列表现出随机的布朗行为时,就不会有任何延长的长期记忆。采用重标度极差分析(R/S)方法计算分形维数,结果一致,表明局部最低温度波动较小。而最高温度的Hurst指数值则表现为随机行为,即不存在相关性。计算的赫斯特指数证实了降水模式的持久结果。同样,分形维数的计算值也显示出持久的结果。因此,降水模式表现出循环行为,即降水时间序列保持长期记忆。最后,从时间序列的持续特征可以推断,局地降水型会有延长的时间效应。使用Python软件进行计算。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Climate time series variability analysis of Islamabad Capital Territory using fractal dimension and Hurst exponent methods
This study is an attempt to examine variability of climatic parameters at local scale, Islamabad Capital Territory (ICT). Climate change can affect temperature trends and precipitation patterns, horticultural activity, agricultural productivity, underground water level, portable water availability, and infrastructure.To assess the impact of climate change of Islamabad Capital Territory, the data of precipitation, minimum and maximum temperatures were obtained for the period from 1983 to 2022 from Pakistan Metrological Department (PMD). Fractal dimension D and Hurt exponent H methods were employed to estimate the monthly maximum and minimum temperatures, and precipitation of the study area. The data was portioned into 4 subsets. Rescaled range analysis method was applied on the datasets to compute values of Hurst exponent and fractal dimension. The results obtained show Brownian random and persistent tendencies, correspondingly. On the other hand, the period from 2013 to 2022 shows anti-persistent trend for H and random trend during (2013–2022) for D, respectively. The time series showing persistent results contain the long-term memory. When a time series shows random Brownian behaviour, thenthere will be no any extended long-term memory. Rescaled range analysis (R/S)method was employed to compute fractal dimensions show consistent outcomes, reveal small fluctuation in the local behaviour of minimum temperatures.Whereas, Hurst exponent values of maximum temperatures show random behavior i.e. there exists no correlation. The Hurst exponents computed confirm persistent results for precipitation pattern. Likewise, the computed values of fractal dimensions also show persistent results. Thus, the precipitation pattern shows cyclic behaviour, i.e. the precipitation time series retain long-run memory. Finally, from the persistent behavior of time series, one would infer that there will bean extended time effect on the local precipitation pattern. Python software was used to perform computations.
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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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