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。     

上海大气折射指数振动及其与降水量和太阳黑子的关系

用交叉谱分析方法研究近地面大气折射指数N单位平均值、月降水总量与太阳黑子相对数之间多频振动特征。结果发现:初夏,N单位与太阳黑子(或降水量)在准5年及准2年(或准7年、准4年及准3年)周期附近有十分密切的关系;初秋,N单位与太阳黑子在准5年、准2年周期附近密切相关;N单位与降水量除在短周期准3年、准2年附近有密切关系外,在长周期准35年附近亦有较密切的关系。     

2500多年来的太阳活动与温度变化

利用Schove推算出的2500多年太阳黑子极值出现的年份得到了2500多年来的太阳黑子周期长度,将其与北半球部分地区温度对比,发现太阳黑子周期长时北半球温度低,太阳黑子周期短时北半球温度高;快周期持续时间越长暖期持续时间也越长,反之亦然。最后,利用太阳黑子周期长度和万年尺度的温度变化趋势拟合了2500多年来的温度变化,它与我国温度和极区温度有一定的可比性。     

华北北部地区地震与太阳活动关系的统计研究

使用时间序列分析和相关分析方法,分析华北北部地区1970～2006年地震与太阳黑子、耀斑的相关性,得到的结论是,太阳活动与以中小地震为主的地震样本不存在统计关系。这个结论与以往的研究不同,本文对此做了初步分析。     

华东地区中强地震与太阳黑子数时间变化的呼应

安徽地区、江苏—山东南部地区中等地震优势分布于太阳黑子数时间变化的“峰区”，亦即为5级以上地震易发时段。黄海地区中等地震优势分布于太阳黑子数的“谷区”。     

The Effect of Relative Sunspot Numbers,Solar Flare Numbers and Variable Component of 10.7 cm Solar Flux on The Seasonal Variation of 6300 Å Line Intensity at Calcutta

The paper presents the seasonal variation of 6300 Å line intensity at Calcutta with relative sunspot number, solar flare number and variable component of 10.7 cm solar flux. A study has been made and important results have been obtained which are as follows. (i) Intensity of 6300 Å line shows periodic variation with relative sunspot number, solar flare number and variable component of 10.7 cm solar flux during the period 1984–1986 which is the secondary peak of the descending phase of 21st solar cycle. (ii) 6300 Å line intensity at Cachoeira Paulista station, taken by Sahai et al. (1988), also shows periodic variation with solar parameters during the period 1978–1980 which is the peak phase of the solar cycle. (iii) A possible explanation of such a type of variation is also presented.     

Wavelet Analysis of the Schwabe Cycle Properties in Solar Activity

Properties of the Schwabe cycles in solar activity are investigated by using wavelet transform. We study the main range of the Schwabe cycles of the solar activity recorded by relative sunspot numbers, and find that the main range of the Schwabe cycles is the periodic span from 8-year to 14-year. We make the comparison of 11-year‘s phase between relative sunspot numbers and sunspot group numbers. The results show that there is some difference between two phases for the interval from 1710 to 1810, while the two phases are almost the same for the interval from 1810 to 1990.     

Relationship between Rotating Sunspots and Flares

Active Region (AR) NOAA 10486 was a super AR in the declining phase of solar cycle 23. Dominated by the rapidly rotating positive polarity of an extensive δ sunspot, it produced several powerful flare-CMEs. We study the evolution and properties of the rotational motion of the major poles of positive polarities and estimate the accumulated helicity injected by them. We also present two homologous flares that occurred in the immediate periphery of the rotating sunspots. The main results are as follows: i) anticlockwise rotational motions are identified in the main poles of positive polarities in the AR; the fastest of them is about 220° for six days. ii) The helicity injection inferred from such rotational motion during the interval from October 25 to 30 is about − 3.0×10⁴³ Mx², which is comparable that calculated by the local correlation tracking (LCT) method (− 5.2×10⁴³ Mx²) in the whole AR. It is suggested that both methods reveal the essential topological properties of the AR, even if the former includes only the major poles and the fine features of the magnetic field are neglected. iii) It is found that there is a good spatial and temporal correspondence between the onset of two homologous CME-associated flares and the rotational motion of sunspots. This suggests that the rotational motions of sunspots not only relate to the transport of magnetic energy and complexity from the low atmosphere to the corona but may also play a key role in the onset of the homologous flares. Electronic Supplementary Material The online version of this article () contains supplementary material, which is available to authorized users.     

中国大陆MS≥7.0地震与太阳黑子活动之间关系的统计检验

利用1900—2017年间中国大陆地区64次M_S≥7.0地震资料,根据太阳黑子11年周期变化计算了它们的相位角,分析了它们的相位角分布,利用统计检验方法对它们与太阳黑子11年周期变化之间的关系进行了检验。结果是:中国大陆地区M_S≥7.0地震中约66%发生在太阳黑子11年周期变化的谷值点前2年—后3年的时段内,在α=0.001显著性水平下通过显著性检验。2019年底太阳黑子11年周期变化将达谷值点,因此,2018—2022年为中国大陆地区M_S7.0地震易发时段。