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小波变换在河西地区水文和气候周期变化分析中的应用 总被引：35，自引：1，他引：35
小波时—频分析由于其局部优化性质而优于傅立叶分析。应用 Meyer小波 ,对甘肃河西地区近 50 a来年径流量、年降水量和年平均气温做周期分析 ,发现河西地区水文气象序列的变化周期基本在 35a、2 2 a、1 1 a、5～ 6a和 2～ 3a左右的时间尺度上浮动。而这些基本周期正是太阳黑子活动周期或海—气相互作用的周期 ,说明河西地区水文、气象序列的周期变化受天体运动变化的影响。天体运动直接影响降水和气温的周期变化 ,进而在一定的下垫面条件下 ,影响径流的周期变化。 相似文献
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利用连续小波分析和经验模态分解方法,对我国北方地区(33°～41°N,108°～115°E)1470 ～2002年每年夏季降水量指数的时间序列进行了周期成分分析,探索全球气候变暖下的该地区降水量的多尺度变化特征.小波分析表明,降水量指数的可能周期有2.57a,4.83a,10.65a,23.25a,48.56a,68.30a和105.90a的周期,在95％置信水平有统计意义的周期是2.57a和23.25a的周期.这些周期和自然因素导致的周期相联系,不仅包含了气候系统内部(平流层准2a振荡和厄尔尼诺/南方涛动)的非线性作用,还包含了气候系统外(主要是太阳活动)受强迫的周期变化,且二者在原始降水量中所在比重相当,共同反映了原始降水量的绝大部分变化.降水量不只是在百年尺度上受太阳活动的驱动,在数十年尺度上也受到太阳活动的影响.我国北方地区的夏季降水量指数和夏季温度指数同相位反相关,全球增温并没有明显地改变二者之间的反相关关系.近百年来全球变暖期间,夏季降水量出现明显的新特征:短周期成分(小于30a的周期)的振幅比以往要显著大,而长周期成分的振幅比以往要显著小,同时呈现降水量逐年减少的长期变化趋势. 相似文献
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以太阳活动为中心,以长期和超长期水文预报为目标,用数理统计分析方法,分析太阳黑子、埃尔尼诺事件(El Ni?o event)对松花江区域水文影响特征与其水、旱灾害发生的基本规律。揭示了“埃尔尼诺”和太阳活动11年周期的联系,把1810年～1991年间的太阳活动按强度划分为强弱两段,给出了强弱两段中事件产生不同水文影响的黑子数临界值,建立以黑子数为参数的“同年”水文计算的方程式。分析了1898年以来强弱两段中事件影响松花江流域发生水、旱灾害的规律性;用降水量为指标分析旱涝规律,揭示了降水量按磁周期时段呈丰、枯水周期性变化的规律。研究结果为长期水文预报提供了途径。 相似文献
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利用辽宁省1956～2018年的降水量和太阳黑子相对数资料分析了辽宁西部、中北部、东南部地区夏季降水量与太阳黑子相对数的关系。结果表明:(1)1960年代以来,辽宁省中北部和东南部夏季降水量距平系列变化过程相似,西部地区与它们相比,在1980年代中期和2010～2013年有一定差异。三个区域的降水量距平系列均为减小趋势,但只有东南部的趋势达到0.05显著水平。(2)太阳黑子相对数序列与西部、中北部、东南部地区夏季降水量序列呈显著负相关。(3)从多年平均来看,西部、中北部、东南部地区夏季降水量的极大值多在太阳活动的极小年(m年)及其前后;各分区夏季降水量极小值多分布在M年及其前后。 相似文献
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近1 000年长江中下游旱涝与气候变化关系 总被引：7，自引：2，他引：7
文章利用旱涝灾害历史记载与现代器测降水资料重建长江中下游旱涝灾害等级序列 ,并通过相关分析与波谱分析、交叉谱分析等分别探讨了长江中下游旱涝灾害发生与东太平洋海水表面温度 (SST)以及太阳活动 (太阳黑子数 )的关系。结果表明 ,长江中下游涝灾多发生于气候过渡期 ,即涝灾在气候由一种气候状态向另一种气候状态转变时期多发。谱分析与交叉谱分析结果表明 ,长江中下游旱涝灾害等级序列在 10～ 11年周期上与太阳黑子数存在相关 ,但两者有近 1年的滞后性。长江中下游旱涝灾害与SST的相关关系分析表明 ,SST正距平年份 ,往往对应着长江中下游的涝灾 ;而SST负距平年份往往对应着长江中下游旱灾。因而可以认为 ,SST与太阳活动变化(太阳黑子数量变化 )在不同周期频度上对长江中下游旱涝灾害具有明显影响。 相似文献
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德令哈降水中δ18O年际变化与水汽输送 总被引：1，自引：0，他引：1
根据德令哈地区1992—2001年的降水中δ18O数据及降水时刻所记录的相关气象参数,并对比中国气象局气象资料和NCEP/NCAR格点气象数据,利用相关、回归等分析方法分别对该地区降水中δ18O与温度、降水量以及水汽通量之间的关系进行分析,并讨论了降水量与大气环流的变化关系,揭示了影响该地区降水中δ18O变化的气象因素,特别是与水汽来源之间的关系。研究结果表明,德令哈降水中δ18O年际变化表现出一定程度的“温度效应”,但与温度的相关性要低于季节尺度。不同类型汽团的水汽输送是影响降水中δ18O年际变化的另一个重要原因。 相似文献
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Gnevyshev’s hypothesis of time space organization of sunspot activity over the solar surface like impulses is considered. Using numerical simulation it was shown that complex solar cycle shape can be explained by distribution of impulses in the northern and southern hemispheres. For long solar cycles, impulses at higher latitudes breaking Sp?rer’s law were found. Comparison of the time-latitude diagrams of solar magnetic fields and impulses has shown that each wave of new polarity to the poles is accompanied by impulse of sunspot activity. 相似文献
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Prediction of sunspot cycle is a vital activity in space mission planning and various engineering decision making. In the present study, the sunspot cycle prediction has been carried out by a hybrid model which employs multivariate regression technique and the binary mixture of Laplace distribution (BMLD) function. The Expectation Maximization (EM) algorithm is being applied to the multivariate regression analysis to obtain a robust prediction of the sunspot cycle. Sunspot cycle 24 has been predicted using this technique. Multivariate regression model has been derived based on the available cycles 1 to 23. This model could predict cycle 24 as an average of previous cycles. Prediction from this model has been refined to capture the cycle characteristics such as bimodal peak at the high solar activity period by incorporating a predicted peak sunspot number from the BMLD model. This revised prediction has shown more accuracy in forecasting the major discrete features of sunspot cycle like maximum amplitude, the Gnevyshev gap, time duration from peak to peak amplitude, and the epoch of peak amplitude. This refined prediction shows that cycle 24 will be having a peak amplitude of 78 with an uncertainty of ±25. Moreover, the present forecast says that, cycle 24 will be having double peak with a strong second peak compared to the first peak. This hypothesis is found to be true with the realized data of cycle 24. Further, this techniques have been validated by predicting sunspot cycles 22 and 23. A preliminary level prediction of sunspot cycle 25 also been carried out using the technique presented here. Present study predicts that, cycle 25 also will be a modest cycle like the present cycle 24, and the peak amplitude may vary in a band of 75–95. 相似文献
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Long period variations in the occurrence of prolonged intervals of calm magnetic field conditions are studied using index
Ap of magnetic activity. The solar-cycle variation in occurrence is compared with the sunspot number. Anomalous behaviour
for solar cycle 20, observed in other solar parameters, are shown to be manifested in the occurrence frequency of quiet intervals.
Spectral characteristics of occurrence indicates a dominant long period variation of about 30 years and a more feeble 11-year
oscillation 相似文献
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The shift between the solar activity cycles in the northern and southern hemispheres of the Sun is studied using data on sunspot number and area. The data obtained are compared with archival information on episodes of appreciable solar-cycle asymmetry. The small phase shift between recent activity cycles in the northern and southern solar hemispheres differs considerably from the shift for episodes of appreciable deviations from dipolar symmetry in the sunspot distribution detected with various degrees of confidence in archival astronomical data from the 17th–19th centuries. The current time shift between the hemispheres is insignificant, about 6–7 months. This shift has changed its sign twice in recent solar history; this probably corresponds to more or less periodic variations with a timescale close to the duration of the Gleissberg cycle. 相似文献
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SCL与中国东部气候年代际变化 总被引：3，自引：2，他引：1
据宇地磁耦合原理,利用太阳黑子周期长度(SCL)的变化及其与地磁场(文中主要考虑地热)的关系,模拟计算并重建了中国东部历史时期的气温序列变化,除了个别时段外,模拟曲线与修正后的竺可桢曲线十分相似;分析了2500a来中国东部气候的年代际变化.结果表明,该曲线能较好地再现2500a来中国东部气候的冷暖变化.对竺氏曲线中有争议的几个冷暖时段,如公元150—350年的温暖期、1050—1150年的小气候适宜期等,模拟结果与后来研究者分析的结果相合.中唐至五代的气候冷暖交替变化不稳定.该曲线也能清晰地反映出小冰期中国东部气候各个时段的变化以及现代气候的变化趋势。 相似文献
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The probability distributions and fractal dimension of sunspot cycles associated with ENSO phenomena
Asma Zaffar Shaheen Abbas Muhammad Rashid Kamal Ansari 《Arabian Journal of Geosciences》2018,11(3):63
Various methods have been used to secure the certainty of significant relations among the sunspot cycles and some of the terrestrial climate parameters such as temperature, rainfall, and ENSO. This study investigates the behavior of ENSO cycles and mean monthly sunspot cycles. Sunspot cycles range from 1755 to 2016 whereas, ENSO cycles range from 1866 to 2012. In this regard, the appropriateness of distributions is investigated with the help of Kolmogorov-Smirnov D, Anderson-Darling, and chi-square tests. It is found that most of the sunspot cycle follows generalized Pareto distribution whereas, generalized extreme value distribution was found appropriate for ENSO cycles. Probability distribution is used to analyze the behavior of each sunspot cycle and ENSO cycle separately. Probability distribution indicates the tail behavior of each cycle; tail explored correlation cycles. Furthermore, self-similar and self-affine fractal dimension methods are used to compute Hurst exponents to determine the persistency of the available data. Fractal dimension has an ability to study the complexity involved in sunspot and ENSO cycles. The fractal dimension and Hurst exponent describe persistency (smoothness) and complexity of data. Hurst exponent measures long-term behavior of time series, making it more helpful for forecasting. This is the measure of regularity or irregularity (chaos) of the time function in the form of their persistency or anti-persistency, respectively. Hurst exponents are computed using rescaled range analysis method and box counting methods. Both these methods are suitable for long-term forecasting. The results of this study confirm that during the period 1980–2000, ENSO cycles were very active. Simultaneously, ENSO was active for the periods 1982–1983, 1986–1987, 1991–1993, 1994–1995, and 1997–1998; these periods include two strongest periods of the century viz., 1982–1983 and 1997–1998. Sunspot cycles and ENSO cycles both were found to be persistent. Self-similar fractal dimensions exhibited a better persistency and a better correlation as compared to self-affine fractal dimension. This research is a part of a larger research project investigating the correlation of sunspot cycles and ENSO cycles, and the influence of ENSO cycles on variations of the local climatic parameters which in turn depends on solar activity changes. 相似文献
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《Quaternary Research》2014,81(3):508-512
Understanding precipitation variation, drought and flood history, and their associated forcing mechanisms are important to human society. In this study, five moisture-sensitive tree-ring width chronologies are used to represent variations in precipitation over the past millennium on the Northeastern Tibetan Plateau (NETP). We find a strong coherency between chronologies in the NETP, indicating a common response to regional climate during the last millennium. The first principal component of the five chronologies (PC1) correlates significantly with regional precipitation and can thus be used as an indicator of regional precipitation variations. Dry spells, even more severe than the 1920s drought, occurred during AD 1139–1152, 1294–1309, 1446–1503 and 1708–1726. Previous studies in this area using other proxies also identified these droughts. Multi-Taper spectral analysis demonstrates significant periodicities at 205 yr and 73 yr, plus a range of ~ 2 yr cycles, suggesting possible linkage with solar variation and the Pacific Decadal Oscillation (PDO). PC1 also shows coherent patterns with solar irradiance variation: the precipitation tends to reach low values during the well-known solar minimum. 相似文献
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Using data of the extended Greenwich sunspot catalog for 1874–2006, annual average values of some quantities characterizing
the latitude distribution of sunspot activity have been calculated. The quantity describing the width of the sunspot formation
zone is closely correlated with the corresponding Wolf numbers. A latitude characteristic has been found that demonstrates
in a particular time interval in the fourth year after the maximum of the current 11-year cycle a high correlation with the
Wolf number at the maximum of the next cycle. This time interval is characterized by extreme differences between the speeds
of the motion of the mean latitude and the upper boundary of the sunspot formation zone. A model displaying good stability
and enabling forecasting of the amplitudes of the next 11-year cycles is constructed based on the found correlation. According
to these forecasts, the activity of the next (24th) cycle will be 20–30% higher than in the previous one. 相似文献