清代江苏省冬季冷暖等级序列的重建及特征分析

通过对历史文献资料的收集整理,重建了清代江苏省冬季逐年冷暖等级序列,并利用Morlet复小波变换分析方法对序列进行了多时间尺度特征的综合分析。结果表明:(1)整个清代江苏省冬季气候变化大致可分为2个冷时段(1644—1730年、1821—1900年)和1个暖时段(1731—1820年);(2)重建的冷暖等级序列存在多尺度下的周期变化特征,其中有较明显的周期变化尺度是38～42 a、18～20 a、13～15 a和8 a,38～42 a和8 a特征时间尺度的周期变化相对具有全域性,18～20 a尺度的周期变化在1690—1790年之间比较明显,13～15 a尺度的周期变化在1720年之前和1830年之后比较明显;(3)重建序列的第1主周期为42 a,第2、3、4主周期依次是20 a、 8 a和3 a;在42 a尺度下,清代江苏省冬季气候可划分为6个偏冷时段和6个偏暖时段。     

基于小波变换的大安地区年降水量变化特征

基于小波分析的方法,对吉林省大安地区1959—2007年的年降水量序列的变化特征进行了分析。经分析表明,大安地区年降水量在其计算时域内各时间尺度分布不均匀,具有明显的局部化特征;其中4～6 a尺度主要发生在1959—1969年和1984年之后,10～12 a尺度主要发生在1965—1999年,20～25a尺度在整个计算时域内均有发生。不同时间尺度下,降水量偏多、偏少交替变化也不相同。此外,分析结果显示该地区年降水量具有4 a、10 a和21 a左右的主周期,其中4 a周期为第一主周期。     

钦州市降雨及入海河流径流演变规律与趋势分析

依据钦州市58a平均降雨量和3条入海河流控制站径流量长序列资料,采用滑动平均、线性回归、Spearman、M-K及R/S法综合分析降雨径流的趋势性及突变特征。结果表明,钦州市降雨量总体呈弱增加趋势,增加率为0.742mm/10a,而茅岭江、钦江、大风江流域径流量存在总体减少趋势,减少率分别为0.2×108m~3/10a、1.1×108m~3/10a、0.4×108m~3/10a。运用复Molet小波分析多时间尺度周期性,降雨量序列存在5个时间尺度,22a和15a时间尺度分别为序列第一、三主周期;径流量序列存在3个时间尺度,其中22a和8a时间尺度分别为径流量序列第一、二主周期。     

地层形变与地下水位分层监测数据的交叉小波分析

地面沉降通常由于地下水的超采而引发,其发生发展相对于地下水位的变化具有一定滞后性。如何获取准确的地面沉降滞后时间一直是地面沉降研究的重要课题。基于北京平各庄地面沉降监测站2008—2018年地面沉降和地下水位长时间序列的分层监测数据,采用Mann-Kendall趋势检验、连续小波变换、交叉小波变换等方法,分析了不同层位地层形变对地下水位动态的滞后特征。结果表明:中–深层承压水具有1 a左右的主震荡周期,潜水和浅部承压水在大部分时域无显著周期;深部严重沉降层的形变量具有1 a左右的主震荡周期,地下水位与形变量共振周期显著,地层由浅到深形变时滞分别为(16.58±8.91)、(7.16±7.09)和(9.66±6.62) d;浅部弱沉降层中,埋深在32~63 m地层形变量具有1 a左右的主震荡周期,与中层承压水存在显著共振周期,形变时滞为(32.02±9.67) d,其他地层形变量与地下水位无显著周期及相关性。研究成果为构建地面沉降精细化模型、提高地面沉降预测精度以及研究更有效的地面沉降防控措施提供了新的技术思路。      

济南泉域地下水位动态及其对降水响应的交叉小波分析

利用1988—2009年济南泉域8个地下水位动态观测点不同时段观测资料及1998—2009年降水数据,采用连续小波变换、交叉小波变换方法对济南泉域地下水位动态的多时间尺度特征、相互关系及其对降水的响应进行了分析。结果表明:①济南泉域地下水位动态存在显著的0.82～1.16 a的主振荡周期,低频部分仅在部分年份存在1.95～3.09 a的振荡周期;②含水岩组富水性对地下水位动态存在影响,研究区主径流方向上弱富水性地段地下水位动态时滞较强富水性地段长,强富水性地段4个观测孔地下水位波动时序基本一致;③地下水位动态对降水的响应滞后明显,为73.06～134.42 d,总体表现为地下水径流路径越长,响应越滞后;④基于地下水位动态与基于降水—地下水位动态交叉小波变换得到的观测点对水位动态的滞后时间多数一致,同一径流路径上局部点对滞后时间之和与全局点对有很好的对应关系。交叉小波分析可定量评价泉域地下水位动态及其与降水的相关关系。     

新疆伊犁地区巩乃斯河流域1972～2015年气温及降水时间序列的变化特征及趋势分析

为了更好的指导巩乃斯河流域水资源的开发利用,对其水文气象变化规律的研究有至关重要的作用。本文借助1972～2015年逐年平均气温、降水资料,运用滑动平均法、M-K(Mann-Kendall)检验法和小波分析法,对巩乃斯河流域气温与降水序列的演变趋势、突变情况和周期性变化特征进行分析研究。结果表明:(1)基于M-K检验法,分析各序列的演变趋势,发现巩乃斯河流域年平均气温与年降水量总体都有显著的增加趋势,其中年平均气温与降水的变化倾向率分别为0.65℃/10a与17.2 mm/10a,突变时间点分别表现在1991年与1982年上;(2)基于小波分析法,分析各序列的周期变换特性,发现研究区未来的年平均气温整体呈上升趋势,降雨量呈减少趋势,其中年平均气温序列的变化第一、二主周期表现在22年与29年的时间尺度上;年平均降水量则在时间尺度为27年与8年上出现变化的第一、二主周期。     

小波变换在河西地区水文和气候周期变化分析中的应用

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。     

青海德令哈地区近400年来的降水量变化与太阳活动

使用多种数学统计方法分析了德令哈地区降水量变化与太阳活动之间的关系,发现近400年来降水量的长期变化与太阳黑子周期长度(SCL)和太阳黑子周期上升支长度之间存在着较好的反相关关系,当SCL偏短、太阳黑子周期上升支长度偏短时,太阳活动偏强,德令哈地区降水量偏多,反之偏少。功率谱和小波分析发现降水量序列中存在着与太阳活动的多种周期相一致的周期,对降水量与太阳活动在不同时间尺度上周期变化之间的关系进行了详细分析。交叉小波分析发现太阳活动主要在百年左右尺度的周期变化上影响德令哈地区降水量的长期变化,太阳活动周期变化的信号越强,对降水量变化的影响越大。文章最后对太阳活动影响德令哈地区降水量变化的可能机制进行了探讨。     

1644-2004年中国洪涝灾害主周期的变化

采用1644-1839年、1840-1949年中国洪涝受灾县数和1950-2004年中国洪涝受灾面积资料,经过去趋势标准化处理后,采用滑动功率谱和Butterworth滤波器进行了分析,得出:1644-2004年间中国洪涝受灾范围变化是不同时间尺度周期振荡的综合结果,主要包含80年的世纪周期和50年、30年、20年尺度的年代际周期。中国洪涝受灾范围变化的主周期在不同时段内存在明显的变化,1833年以前世纪周期变化显著;1834-1920年在世纪周期变化的背景下叠加了显著的20年尺度波动;1921年以后年代际尺度周期变化显著,其中1947年前后发生了主周期从20年尺度到30年尺度的变化。     

基于小波变换的北京地区1724～2009年降水量多尺度分析

基于小波分析方法,对1724~2009年北京气象站年降水量序列的变化特征进行了分析。结果表明,北京地区年降水量在其计算时域内各时间尺度分布不均匀,具有明显的局部化特征;其中,19~23a的时间尺度,震荡中心分别在1889年和1979年;35~37a左右的时间尺度主要发生在1920~1928年、1950~1960年和1983~1991年;83~87a的时间尺度在整个计算时域上均有发生,1769~1859年间表现明显。分析结果显示北京地区年降水量具有21a、35a和86a左右的主周期,其中86a左右的周期振荡最强,为第一主周期。计算的趋势表明,未来10余年北京仍属于降水偏少的时期。     

Wavelet-based variability of Yellow River discharge at 500-, 100-, and 50-year timescales

Water scarcity in the Yellow River, China, has become increasingly severe over the past half century. In this paper, wavelet transform analysis was used to detect the variability of natural, observed, and reconstructed streamflow in the Yellow River at 500-, 100-, and 50-year timescales. The periodicity of the streamflow series and the co-varying relationships between streamflow and atmospheric circulation indices/sunspot number were assessed by means of continuous wavelet transform (CWT) and wavelet transform coherence (WTC) analyses. The CWT results showed intermittent oscillations in streamflow with increasing periodicities of 1–6 years at all timescales. Significant multidecadal and century-scale periodicities were identified in the 500-year streamflow series. The WTC results showed intermittent interannual covariance of streamflow with atmospheric circulation indices and sunspots. At the 50-year timescale, there were significant decadal oscillations between streamflow and the Arctic Oscillation (AO) and the Pacific Decadal Oscillation (PDO), and bidecadal oscillations with the PDO. At the 100-year timescale, there were significant decadal oscillations between streamflow and Niño 3.4, the AO, and sunspots. At the 500-year timescale, streamflow in the middle reaches of the Yellow River showed prominent covariance with the AO with an approximately 32-year periodicity, and with sunspots with an approximately 80-year periodicity. Atmospheric circulation indices modulate streamflow by affecting temperature and precipitation. Sunspots impact streamflow variability by influencing atmospheric circulation, resulting in abundant precipitation. In general, for both the CWT and the WTC results, the periodicities were spatially continuous, with a few gradual changes from upstream to downstream resulting from the varied topography and runoff. At the temporal scale, the periodicities were generally continuous over short timescales and discontinuous over longer timescales.     

The properties of long-term sunspot oscillations

It is shown that neglecting the motion of sunspots in the plane of the sky in pixels of SOHO MDI magnetograms obtained for the vertical direction results in false periods of 700–1300 min in the long-term oscillations of the magnetic fields of sunspots observed near the central meridian (the Y artefact). The oscillation mode proposed by Efremov, Parfinenko, and Solov’ev in 2012 to be the lowest-frequency sunspot mode is an artefact. A proposed technique for monitoring this artefact using wavelet transforms can be used to study oscillation periods in the range 15 min < T < 500 min. The observational dependence of the oscillation frequency of the sunspot magnetic field on the field strength is constructed using observations of 45 sunspots. This dependence shows a multimode behavior that is consistent with earlier ground observations. One interpretation of this dependence based on the existence of four geometrical oscillation modes detected earlier is proposed.     

Trend analysis of hydroclimatological variables in Urmia lake basin using hybrid wavelet Mann–Kendall and Şen tests

This paper investigates monthly, seasonal, and annual trends in rainfall, streamflow, temperature, and humidity amounts at Urmia lake (UL) basin and analyzes the interaction between these variables and UL’s water level fluctuation during the 1971–2013 period. Two new methods including nonparametric hybrid wavelet Mann–Kendall test and ?en’s methodology have been used to determine potential trends in the variables and their dominant periods. The results showed significant decreasing trends in the water level and streamflow series, moderate decreasing trend in the rainfall and relative humidity series, and increasing trends in the observed temperature data. The 8- , 12-month, and 2-year periods were detected as the dominant periods of the variables in monthly, seasonal, and annual timescales, respectively. The results from the interaction analysis revealed that the main factor influencing the water level at UL is decreasing trend in the streamflow series. Both the monthly series of UL’s water level and the streamflow series of the stations indicated two start points of significant decreasing trend in 1973 and 1998. Furthermore, a comparative analysis among the applied methods indicated a good agreement between the results of hybrid wavelet Mann–Kendall test and ?en’s trend analyzing method.     

Contribution of cross time-frequency analysis in assessment of possible relationships between large-scale climatic fluctuations and rainfall of northern central Algeria

This paper is proposed for the investigation of possible relationships between the large-scale atmospheric circulation phenomena such as the North Atlantic Oscillation (NAO), Southern Oscillation (SOI), Mediterranean Oscillation (MO), Western Mediterranean Oscillation (WeMO) and rainfall of Sebaou river watershed (Northern central Algeria), covering a period of 39 years at monthly scale. Several time and scale-based methods were used: correlation and spectral analysis (CSA), continuous wavelet transform (CWT), multiresolution wavelet analysis (MRWA), cross wavelet analysis (XWT), wavelet coherence transform (WCT) and cross multiresolution wavelet analysis (CMRWA). The rainfall analysis by CSA and CWT has been clearly demonstrating the dominance of 1 year and 1–3-year modes, which they explain 30 to 51% and 25 to 28% of the variance respectively. However, the indices have shown that inter-annual fluctuations up to long-term explain between 60 and 90%. CWT and MRWA indicated significant fluctuations materialising a dry period more marked between the 1980s and 1990s with strong trend towards drier conditions starting from the 1980s, explained by the decadal components D7 and the approximation A7. In addition to the annual component, the XWT spectrums reveal strong coefficients for the SOI between 1992–2005 and 1986–2000 for the modes of 5–10 years and higher than 10 years respectively and less intense for NAO. The WCT between NAO and rainfall indicated the most significant relationship for 1 year, 1–3 years and 3–5 years approximately from the early 1980s corresponding to the dry period. However, the SOI affects rainfall only locally and with significant values more or less localised in the time-frequency space between MO, WeMO and rainfall, but this influence could be significant for low-frequency events. CWMRA shows that the components of 5–10 years and higher than 10 years are the most effective to represent climate index-rainfall significant relationships, where change in Daubechies wavelet properties can improve the correlation across the scales. Furthermore, has indicated that the short-term processes dominate the relationship index-rainfall, which masks the long-term phenomena whose influence can sometimes be very distant. As such, the rainfall variability of the study area has shown fairly significant links, at least locally with large-scale atmospheric circulation phenomena.     

A climatological study of the relations among solar activity,galactic cosmic ray and precipitation on various regions over the globe

We apply Fourier and wavelet analyses to the precipitation and sunspot numbers in the time series (1901–2000) over Australia (27°S, 133°E), Canada (60°N, 95°W), Ethiopia (8°N, 38°E), Greenland (72°N, 40°W), United Kingdom (54°N, 2°W), India (20°N, 77°E), Iceland (65°N, 18°W), Japan (36°N, 138°E), United States (38°N, 97°W), South Africa (29°S, 24°E) and Russia (60°N, 100°E). Correlation analyses were also performed to find any relation among precipitation, sunspot numbers, temperature, and cloud-cover at the same spatial and temporal scale. Further correlations were also performed between precipitation with electron and proton fluence at the time interval, 1987–2006. All these parameters were considered in annual and seasonal scales. Though correlation study between precipitation and other parameters do not hint any linear relation, still the Fourier and wavelet analyses give an idea of common periodicities. The 9–11 year periodicity of sunspot numbers calculated by Fourier transform is also confirmed by wavelet transform in annual scale. Similarly, wavelet analysis for precipitation also supports the short periods at 2–5 years which is verified by Fourier transform in discontinuous time over different geographic regions.     

近1 000年长江中下游旱涝与气候变化关系

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。     

Short-period variations in the proper motions of sunspots from SOHO (MDI) observations

Short-period (1–60 min) variations in the coordinates of the centers of gravity of isolated sunspots are analyzed. The sunspot coordinated were determined using two sets of observational data—magnetograms and intensities—obtained by SOHO (MDI) on December 6, 1998, from 01:00 to 21:57 UT with temporal resolution 60 s and spatial resolution 0.6″/pixel. A slow drift in the sunspot coordinates was removed using a low-frequency filter with a 61-min integration window. The guiding errors (RMS～0.014″) were determined by analyzing correlated motions in pairs of sunspots, and were removed from the time series before determining the sunspot proper motions. Based on the calculated power spectra for the sunspot proper motions, two period intervals containing appreciable power were identified. One coincides with the well-known 5-min acoustic solar oscillations. The concentration of power in this interval is greater for the coordinate variations derived the magnetograms than those derived from the intensities; the harmonic amplitude for some peaks reaches ～±30 km. The other spectral interval corresponds to periods exceeding 30 min. Overall, the rms short-period variations in the sunspot proper motions are 9.9±2.2 and 16.7±7.6 km (0.014″±0.003″ and 0.024″±0.010″) for the magnetogram and intensity data, respectively.     

Form of the latitude distribution of sunspot activity

The spatial (latitude) distribution of sunspots is studied, including its dependence on solar activity. It is shown that the latitude distributions of sunspots for a given year can be approximately described by the normal law, with its variance being a linear function of the current level of solar activity. Thus, an increase in activity is accompanied by an expansion of the zone of solar activity, in good agreement with earlier results. As the solar activity increases, the width of the zone of sunspot generation and the latitude maximum of the sunspot density grow somewhat more slowly than the number of sunspots, in agreement with observations. The results obtained can be used to reconstruct the spatial distributions of sunspots in the past, interpret the magnetic activity of stars, and address the requirements of the dynamo theory in the form of constraints imposed on models of cyclicity.     

太行山东缘典型岩溶泉流量变化特征及规律分析

为揭示太行山东缘小南海泉流量变化特征及规律,基于小南海泉1971-2016年的流量资料,采用R/S分析法、Mann-Kendall趋势分析法和小波分析法,探讨小南海泉流量变化规律及特征。结果表明:小南海泉年流量呈显著下降趋势,年变化幅度为0.05 m3·s-1;未来泉流量的变化趋势和过去一致,具有持续性特征,且持续性强烈;泉流量的变化存在约15、27年的主周期与6年的次周期。降水量的减少和气温的增加是导致泉流量减少的主要气象因素,且这种暖干化现象会持续发展。泉流量对降雨的响应存在一定的滞后,流量与前五个月的月降水量均呈高度相关,其中与前2月的降水相关性最高,研究成果可为小南海泉水资源合理开发和保护提供依据。