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Determination of the Topology Skeleton of Magnetic Fields in a Solar Active Region 被引量:4
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作者 Hui Zhao Jing-Xiu Wang +2 位作者 Jun Zhang Chi-Jie Xiao Hai-Min Wang 《Chinese Journal of Astronomy and Astrophysics》 CSCD 2008年第2期133-145,共13页
Magnetic topology has been a key to the understanding of magnetic energy release mechanism. Based on observed vector magnetograms, we have determined the threedimensional (3D) topology skeleton of the magnetic field... Magnetic topology has been a key to the understanding of magnetic energy release mechanism. Based on observed vector magnetograms, we have determined the threedimensional (3D) topology skeleton of the magnetic fields in the active region NOAA 10720. The skeleton consists of six 3D magnetic nulls and a network of corresponding spines, fans, and null-null lines. For the first time, we have identified a spiral magnetic null in Sun's corona. The magnetic lines of force twisted around the spine of the null, forming a 'magnetic wreath' with excess of free magnetic energy and resembling observed brightening structures at extraultraviolet (EUV) wavebands. We found clear evidence of topology eruptions which are referred to as catastrophic changes of topology skeleton associated with a coronal mass ejection (CME) and an explosive X-ray flare. These results shed new lights on the structural complexity and its role in explosive magnetic activity. The concept of flux rope has been widely used in modelling explosive magnetic activity, although their observational identity is rather obscure or, at least, lacking of necessary details up to date. We suggest that the magnetic wreath associated with the 3D spiral null is likely an important class of the physical entity of flux ropes. 展开更多
关键词 sun magnetic fields -- sun solar corona -- sun activity
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ENSO Index Variations and Links with Solar and Volcanic Activity
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作者 Valentina V. Zharkova Irina Vasilieva 《Natural Science》 2024年第4期25-44,共20页
In this paper, we investigated the Oceanic Niño Index (ONI), for simplicity called in this paper an El Nino Southern Oscillation (ENSO) index in 1950-2023 by applying the wavelet spectral transform and the IBM SP... In this paper, we investigated the Oceanic Niño Index (ONI), for simplicity called in this paper an El Nino Southern Oscillation (ENSO) index in 1950-2023 by applying the wavelet spectral transform and the IBM SPSS correlations analysis. ONI follows the three months’ current measurements of the average temperature of the sea surface in the East-Central tropical part of the Pacific Ocean nearby the international line of the date change over the average sea surface temperature over the past 30 years. The ENSO index is found to have a strong (>87%) correlation with the Global Land-Ocean Temperature (GLOT). The scatter plots of the ENSO-GLOT correlation with the linear and cubic fits have shown that the ENSO index is better fit by the cubic polynomial increasing proportionally to a cubic power of the GLOT variations. The wavelet analysis allowed us to detect the two key periods in the ENSO (ONI) index: 4 - 5 years and 12 years. The smaller period of 4.5 years can be linked to the motion of tectonic plates while the larger period of 12 years is shown to have a noticeable correlation of 25% with frequencies of the underwater (submarine) volcanic eruptions in the areas with ENSO occurrences. Not withholding any local terrestrial factors considered to contribute to the ENSO occurrences, we investigated the possibility of the volcanic eruptions causing ENSO to be also induced by the tidal forces of Jupiter and Sun showing the correlation of the underwater volcanic eruption frequency with the Jupiter-Earth distances to be 12% and with the Sun-Earth distances, induced by the solar inertial motion, in January, when the Earth is turned to the Sun with the southern hemisphere where the ENSO occurs, to become 15%. Hence, the underwater volcanic eruptions induced by tidal forces of Jupiter and Sun can be the essential additional factors imposing this 12 year period of the ENSO (ONI) index variations. 展开更多
关键词 sun: magnetic field sun: solar activity sun: Inertial Motion Earth: Temperature Earth: Sea Level Earth: Ice Area
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A logistic model for magnetic energy storage in solar active regions 被引量:6
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作者 Hua-Ning Wang Yan-Mei Cui Han He 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2009年第6期687-693,共7页
Previous statistical analyses of a large number of SOHO/MDI full disk longitudinal magnetograms provided a result that demonstrated how responses of solar flares to photospheric magnetic properties can be fitted with ... Previous statistical analyses of a large number of SOHO/MDI full disk longitudinal magnetograms provided a result that demonstrated how responses of solar flares to photospheric magnetic properties can be fitted with sigmoid functions. A logistic model reveals that these fitted sigmoid functions might be related to the free energy storage process in solar active regions. Although this suggested model is rather simple, the free energy level of active regions can be estimated and the probability of a solar flare with importance over a threshold can be forecast within a given time window. 展开更多
关键词 sun photosphere -- sun magnetic field -- sun solar activity
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Periodicities in Solar Activity, Solar Radiation and Their Links with Terrestrial Environment
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作者 Valentina V. Zharkova Irina Vasilieva +1 位作者 Simon J. Shepherd Elena Popova 《Natural Science》 CAS 2023年第3期111-147,共37页
Solar magnetic activity is expressed via variations of sunspots and active regions varying on different timescales. The most accepted is an 11-year period supposedly induced by the electromagnetic solar dynamo mechani... Solar magnetic activity is expressed via variations of sunspots and active regions varying on different timescales. The most accepted is an 11-year period supposedly induced by the electromagnetic solar dynamo mechanism. There are also some shorter or longer timescales detected: the biennial cycle (2 - 2.7 years), Gleisberg cycle (80 - 100 years), and Hallstatt’s cycle (2100 - 2300 years). Recently, using Principal Component Analysis (PCA) of the observed solar background magnetic field (SBMF), another period of 330 - 380 years, or Grand Solar Cycle (GSC), was derived from the summary curve of two eigenvectors of SBMF. In this paper, a spectral analysis of the averaged sunspot numbers, solar irradiance, and the summary curve of eigenvectors of SBMF was carried out using Morlet wavelet and Fourier transforms. We detect a 10.7-year cycle from the sunspots and modulus summary curve of eigenvectors as well a 22-year-cycle and the grand solar cycle of 342 - 350-years from the summary curve of eigenvectors. The Gleissberg centennial cycle is only detected on the full set of averaged sunspot numbers for 400 years or by adding a quadruple component to the summary curve of eigenvectors. Another period of 2200 - 2300 years is detected in the Holocene data of solar irradiance measured from the abundance of 14C isotope. This period was also confirmed with the period of about 2000 - 2100 years derived from a baseline of the solar background magnetic field, supposedly, caused by the solar inertial motion (SIM) induced by the gravitation of large planets. The implication of these findings for different deposition of solar radiation into the northern and southern hemispheres of the Earth caused by the combined effects of the solar activity and solar inertial motion on the terrestrial atmosphere is also discussed. 展开更多
关键词 sun: magnetic field sun: solar activity sun: sunspots sun: solar Dynamo
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Terrestrial Temperature, Sea Levels and Ice Area Links with Solar Activity and Solar Orbital Motion
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作者 Valentina V. Zharkova Irina Vasilieva 《Natural Science》 2023年第9期233-255,共23页
This paper explores the links between terrestrial temperature, sea levels and ice areas in both hemispheres with solar activity indices expressed through averaged sunspot numbers together with the summary curve of eig... This paper explores the links between terrestrial temperature, sea levels and ice areas in both hemispheres with solar activity indices expressed through averaged sunspot numbers together with the summary curve of eigenvectors of the solar background magnetic field (SBMF) and with changes of Sun-Earth distances caused by solar inertial motion resulting from the gravitation of large planets in the solar system. Using the wavelet analysis of the GLB and HadCRUTS datasets two periods: 21.4 and 36 years in GLB, set and the period of about 19.6 years in the HadCRUTS are discovered. The 21.4-year period is associated with variations in solar activity defined by the summary curve of the largest eigenvectors of the SBMF. A dominant 21.4-year period is also reported in the variations of the sea level, which is linked with the period of 21.4 years detected in the GLB temperature and the summary curve of the SBMF variations. The wavelet analysis of ice and snow areas shows that in the Southern hemisphere, it does not show any links to solar activity periods while in the Northern hemisphere, the ice area reveals a period of 10.7 years equal to a usual solar activity cycle. The TSI in March-August of every year is found to grow with every year following closely the temperature curve, because the Sun moves closer to the Earth orbit owing to gravitation of large planets (solar inertial motion, SIM), while the variations of solar radiation during a whole year have more steady distribution without a sharp TSI increase during the last two centuries. The additional TSI contribution caused by SIM is likely to secure the additional energy input and exchange between the ocean and atmosphere. 展开更多
关键词 sun: magnetic field sun: solar activity sun: Inertial Motion Earth: Temperature Earth: Sea Level Earth: Ice Area
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太阳磁场探测现状与展望 被引量:10
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作者 邓元勇 甘为群 +4 位作者 颜毅华 杨尚斌 白先勇 侯俊峰 陈洁 《红外与激光工程》 EI CSCD 北大核心 2020年第11期222-228,共7页
磁场是当今太阳物理最重要的观测量,与太阳磁场观测研究相关的科学问题是当今太阳物理、日地物理的前沿和热点。文中简要回顾了太阳磁场观测的发展历程、现状以及面临的困难,并结合国内在太阳磁场观测研究中取得的成就,探讨了国内在未... 磁场是当今太阳物理最重要的观测量,与太阳磁场观测研究相关的科学问题是当今太阳物理、日地物理的前沿和热点。文中简要回顾了太阳磁场观测的发展历程、现状以及面临的困难,并结合国内在太阳磁场观测研究中取得的成就,探讨了国内在未来的竞争中可能的突破口。基于空间探测的优势,笔者认为深空探测将在有关太阳磁场的重大科学难题的突破方面发挥决定性作用。 展开更多
关键词 太阳 太阳磁活动 太阳磁场测量 空间探测
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太阳磁场演变的起因之一——太阳的回磁效应 被引量:7
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作者 董士仑 《天体物理学报》 CSCD 1997年第1期86-90,共5页
本文指出太阳绕太阳系质心的角动量变率与黑子数年均值紧密相关 ;在 1 90 0 1 980年 (Zurich黑子数系统较稳定 ) ,当迟滞时间~ 2年 ,相关系数高达 0 .81 ,线性相关置信水平远高于 99.9% .并指出按太阳的回磁效应 ,可由太阳绕太阳系... 本文指出太阳绕太阳系质心的角动量变率与黑子数年均值紧密相关 ;在 1 90 0 1 980年 (Zurich黑子数系统较稳定 ) ,当迟滞时间~ 2年 ,相关系数高达 0 .81 ,线性相关置信水平远高于 99.9% .并指出按太阳的回磁效应 ,可由太阳绕太阳系质心运动确定太阳基本磁偶极矩 ;它是太阳磁场演变 (太阳总体活动 )在太阳系内的起因之关键纽带 .推测太阳内大部分物质的自转速度应该非常小 ;直接观测的较差自转 ,仅是表层现象 .本文叙述的基本理论 ,在对地球和其它行星乃至各种旋转天体或星系的磁性进行分析时 。 展开更多
关键词 太阳 磁场 太阳活动 回磁效应
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中尺度磁绳结构的行星际观测
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作者 宋其武 吴德金 《天文学报》 CSCD 北大核心 2004年第4期381-388,共8页
由磁绳结构主导、平均尺度约二、三十个小时的行星际磁云是日冕物质抛射在行星际膨胀、传播的体现.最近,Moldwin等人报道在太阳风中还观测到一些尺度在几十分钟的小尺度磁绳结构,并认为太阳风中的磁绳结构在尺度分布上可能具有双峰特征... 由磁绳结构主导、平均尺度约二、三十个小时的行星际磁云是日冕物质抛射在行星际膨胀、传播的体现.最近,Moldwin等人报道在太阳风中还观测到一些尺度在几十分钟的小尺度磁绳结构,并认为太阳风中的磁绳结构在尺度分布上可能具有双峰特征.在全面检视了WIND卫星(1995年-2000年)和ACE卫星(1998年-2000年)的观测资料后,发现了在行星际太阳风中一些尺度为几个小时的中尺度磁绳结构.利用初步整理的其中28个中尺度磁绳结构事件,认为太阳风中的磁绳结构在尺度分布上可能是连续的,这对行星际太阳风中磁绳结构物理起源的研究可能提出重要的物理限制. 展开更多
关键词 行星际 太阳风 中尺度 观测资料 磁云 日冕物质抛射 卫星 连续 平均 双峰
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Effect of Volcanic Activities and CO_2 Concentration on Summer Temperature in Middle Stratosphere,North Hemisphere 被引量:1
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作者 曲维政 邓声贵 +3 位作者 黄菲 刘应辰 樊婷 白燕 《Journal of Earth Science》 SCIE CAS CSCD 2010年第3期272-283,共12页
Successive filtration and comparison show that the stratosphere air temperature in 10 hPa-layer of the Northern Hemisphere (NH) in July continuously increases,which is associated to the increases in greenhouse gases... Successive filtration and comparison show that the stratosphere air temperature in 10 hPa-layer of the Northern Hemisphere (NH) in July continuously increases,which is associated to the increases in greenhouse gases mostly CO2,volcanic activities,and solar activity,demonstrating the follows.(a) The increase in CO2 concentration is largely consistent with that of the stratosphere air temperature in 10 hPa-layer of the NH in July.However,the increase in the air temperature is not in a linear pattern,during which several cooling events interrupt.The cooling events between late 1960s and late 1970s are remarkable ones and so is the one before mid 1990s.Analysis shows that these events are induced by volcanic activities and solar activity.(b) The CO2-free variation in the stratosphere air temperature in 10 hPa-layer of the NH is consistent with that of the solar magnetic index.The wave crests and wave troughs of the two curves are consistent in phase,and the curve of solar magnetic index leads the other slightly.In other words,when the solar magnetic pole is southward,a warming in the NH stratosphere corresponds;and on the contrary,the northward solar magnetic pole corresponds to a cooling event.The variation in solar magnetic polarity strongly impacts the variation in the stratosphere temperature. 展开更多
关键词 volcanic activity climate variation solar activity solar magnetic field CO2 concentration greenhouse effect
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10 TeV宇宙线的太阳阴影研究
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作者 张天津 木钧 《云南大学学报(自然科学版)》 CAS CSCD 1999年第1期12-16,共5页
利用1995年10月至1997年9月间西藏空气簇射阵列采集到的数据,再一次观测到了10TeV宇宙线的太阳阴影;仔细分析了1990年6月至1997年9月间观测到的10TeV宇宙线的太阳阴影位置,对其位置的偏移及变化行为... 利用1995年10月至1997年9月间西藏空气簇射阵列采集到的数据,再一次观测到了10TeV宇宙线的太阳阴影;仔细分析了1990年6月至1997年9月间观测到的10TeV宇宙线的太阳阴影位置,对其位置的偏移及变化行为给出了定性的解释;结合相同时期的太阳表面平均磁场强度,进一步证实了日影偏离度与太阳平均磁场的关联;利用较为完整的宇宙线成分测量数据,对日影偏离度与太阳平均磁场强度间的定量关系作了成分上的修正. 展开更多
关键词 宇宙线 太阳阴影 太阳活动 太阳平均磁场
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