共查询到20条相似文献，搜索用时 15 毫秒
1.
地磁活动是太阳爆发现象引起地球近地空间磁场扰动的重要空间天气过程之一.地球磁场的变化具有多种时间尺度,其中从数十年到数世纪的长时间地磁场变化主要是由地核磁场引起的,而从数秒到数年的短时间地磁变化与太阳活动有关.近年来,越来越多的统计研究表明,地磁活动与太阳活动和地球气候变化之间存在着显著的相关性.地球磁场和地球大气系统的耦合现象驱动着人们探索地磁活动对地球天气和气候系统影响的研究.本文的目的就是综述国内外地磁变化对气候影响的研究进展,介绍我们最新的研究成果,探索地磁活动对气候要素的影响特征和可能机理过程,为深入研究地磁活动对地球天气和气候的影响提供基础和依据,以期对地磁活动和气候要素关系有进一步的认识. 相似文献
2.
The effect of solar/geomagnetic activity and QBO phase on the distribution of winds prevailing in the winter periods (January–March)
in the Northern Hemisphere at the altitude of 850 mb was studied. Analysis has shown that the zonal flow over the North Atlantic
under high geomagnetic activity intensifies and under low solar/geomagnetic activity weakens. Flow deviations, associated
with geomagnetic activity, are more marked under the QBO-east phase, and flow deviations, associated with solar activity,
are more marked under the QBO-west phase. The results reported by Venne and Dartt (1990) concerning the wind distribution
in the winter (February–March) Northern Hemisphere under high and low solar activity and a QBO-west phase, have been confirmed,
and supplemented with wind distributions under high and low geomagnetic activity. 相似文献
3.
There are limited homogeneous instrumental observations of the sunspot magnetic fields, but the Earth is a sort of a probe reacting to interplanetary disturbances which are manifestation of the solar magnetic fields. We find correlations between some parameters of geomagnetic activity (the geomagnetic activity “floor”—the minimum value under which the geomagnetic activity cannot fall in a sunspot cycle, and the rate of increase of the geomagnetic activity with increasing sunspot number), and sunspot magnetic fields (the sunspot magnetic field in the cycle minimum, and the rate of increase of the sunspot magnetic field from cycle minimum to cycle maximum). Based on these correlations we are able to reconstruct the sunspot magnetic fields in sunspot minima and maxima since sunspot cycle 9 (mid 19th century). 相似文献
4.
Frédéric Ouattara Christine Amory-Mazaudier 《Journal of Atmospheric and Solar》2009,71(17-18):1736-1748
Legrand and Simon [1989. Solar cycle and geomagnetic activity: a review for geophysicists. Part I. The contributions to geomagnetic activity of shock waves and of the solar wind. Annales Geophysicae 7(6), 565–578] classified one century (1868–1978) of geomagnetic activity, using the Mayaud's Aa index, in four classes related to solar activity: (1) the magnetic quiet activity due to slow solar wind flowing around the magnetosphere, (2) the recurrent activity related to high wind speed solar wind, (3) the fluctuating activity related to fluctuating solar wind and (4) the shock activity due to shock events (CME). In this paper, we use this classification to analyse the solar–geomagnetic activity from 1978 to 2005. We found that during the last three decades the level of geomagnetic quiet activity estimated by Aa indices is decreasing: 2003 is the year of the smallest level of quiet geomagnetic activity since 1868. We compare Legrand and Simon's classification with new in situ solar wind data [Richardson, I.G., Cliver, E.W., Cane, H.V., 2000. Sources of geomagnetic activity over the solar cycle: relative importance of coronal mass ejections, high-speed streams, and slow solar wind. Journal of Geophysical research 105(A8), 18,200–18,213; Richardson, I.G., Cane, H.V., 2002. Sources of geomagnetic activity during nearly three solar cycles (1972–2000). Journal of Geophysical Research 107(A8), 1187] and find a rather good agreement. The differences are only due to minor definitions of the extent of the classes. An attempt is made at defining a more precise standard classification of solar phenomena and at defining time scales of these to understand more precisely the geomagnetic signatures of solar activity. 相似文献
5.
Summary The analyses of various types of geomagnetic and atmospheric manifestations have disclosed certain associations. The agreement in the occurrence of the increased spectral densities as regards geomagnetic activity and the variations of atmospheric pressure over the geomagnetic pole proves the relation between their periodicities. The results imply that the changes in the intensity of corpuscular radiation, indicated by geomagnetic activity, affect the pressure patterns over the geomagnetic pole and polar region significantly, so that a pronounced modification of the general circulation may take place, as shown schematically in Figs 14a,b.Dedicated to Prof. RNDr. Emil Buchar, DrSc., Corresponding Member of the Czechoslovak Academy of Sciences, on the Occasion of His 75th Birthday 相似文献
6.
7.
Summary With the aid of 36 monthly and a double 12-month running average, graphs of the smoothed run of geomagnetic activity were constructed from the monthly values of the geomagnetic activity index aa for the period 1868–1978 and they were then used to determine the run of the geomagnetic activity, expressed during a uniform period and devoid of the secular variation of geomagnetic activity, for the individual 11-year cycles Nos 12–20 and the average runs for even and odd cycles, as well as for the whole period of the 9 cycles. The analysis and comparison of the graphs substantiates and renders more accurate the tendency, observed earlier, towards a regular alternation of geomagnetic activity cycles with double and single maxima. Wheareas a saddle-like shape with a maximum in the neighbourhood of the first and third quarter of the cycle is characteristic of the shape of the even cycle, the second maximum being, as a rule, the main one, the odd cycle is characterized by a peak-like shape with the main maximum in the vicinity of the cycle's centre. 相似文献
8.
A. E. Levitin L. I. Gromova S. V. Gromov L. A. Dremukhina 《Geomagnetism and Aeronomy》2014,54(3):292-299
A new method for determining geomagnetic activity based on calculation of the hourly amplitudes of geomagnetic field variations at ground-based observatories has been developed. Observations performed in 2009, when unusually low solar and geomagnetic activity was registered, were used as a reference level. The described method was used to estimate the energy of local geomagnetic activity; such energy is estimated for observatories in the Earth’s Northern and Southern hemispheres, and a total estimation is made for both hemispheres and for the entire Earth’s surface during large magnetic storms. These are used to compare characteristics of magnetic storm intensity based on the classical Kp and Dst indices and calculated energy estimate. 相似文献
9.
Summary Using a more detailed geomagnetic activity Kp index, the finding in [3] that geomagnetic activity increases after the CMP of coronal holes, was verified; it was shown using individual activity patterns, that coronal holes apparently do not form a homogeneous class of phenomena, which must be respect in considerations of emissions of fast solar wind streams. 相似文献
10.
J. A. Joselyn 《Surveys in Geophysics》1984,6(3-4):419-424
The Space Environment Services Center (SESC) provides real-time information on the state of the solar-terrestrial environment. In particular, the geomagnetic field is closely monitored. Summaries of geomagnetic activity are issued daily, as are forecasts for each of the next three days. Customers are alerted when activity rises above selected thresholds of theK- andA-indices. This present geomagnetic reporting and forecasting format is no longer the most appropriate for the expanding number of agencies and industries which the SESC serves. These customers need more detailed information about the geographic distribution of geomagnetic activity stated in plainer language. The proposed new format would quantitatively describe geomagnetic activity in terms of 6 qualitative categories: quiet, unsettled, active, minor storm, major storm, and severe storm. Summaries and forecasts would be made for 2 specific latitude zones: mid-latitudes (20–50 deg geomagnetic) and high-latitudes (50–80 deg geomagnetic). The format adapts well to longer-range (27-day) forecasts. 相似文献
11.
Summary Relatively good correlation between such remote phenomena as microseisms, geomagnetic activity and ionospheric absorption of radio waves has been observed. These phenomena are probably connected by a considerably increased penetration of energetic particles into the atmosphere under conditions of geomagnetic activity. 相似文献
12.
13.
日冕物质抛射(CME)的规模和对地有效性是地磁暴预报中重点关注的特征.本项研究的目的是通过对行星际高能质子通量和能谱的特征与演化规律的分析,得到CME对粒子的加速能力,评估CME可能对地磁场造成的影响.在工作中,统计分析了ACE/EPAM的1998-2010年的质子数据,对质子能谱进行了拟合,得到了能谱指数,并对能谱指数及其变化特征所对应的CME和地磁暴进行了相关统计.通过研究发现:(1)能谱指数随着太阳活动水平而变化,高年最大,达到-2.6,而且涨落幅度也达到±0.4,而在太阳活动低年则稳定在-3.0左右;(2)CME对粒子的加速对应着能谱指数的升高,幅度达到20%时,CME引起地磁暴的可能性较大;(3)冕洞高速流到达地球时,高能质子通量也会升高,但能谱指数同时会有下降;(4)以2004年全年的能谱指数为例,对能谱指数在地磁暴预报中的应用进行了评估,结论认为,能谱指数的升高是CME引发地磁暴的必要条件,可以作为地磁暴预报的参数使用. 相似文献
14.
地磁垂直分量Z日变幅逐日比及其与磁暴和地震的关系 总被引：1，自引：0，他引：1
地磁垂直分量Z日变幅逐日比是基于变化磁场在地球电导率的作用下会产生一个与变化磁场相反的感应磁场, 该感应磁场不仅包含了外空磁场的信息, 还包含了地下电导率的信息。 因此, 相对于地磁场其他成分来说Z分量更多地反应了地下活动的变化, 逐日比是利用前后两日地磁Z分量日变幅相比来提取该异常现象, 但磁暴可能会对逐日比异常判定产生影响。 我们取1984年至今江苏区域范围达到逐日比异常判定指标的29个事件结合磁暴以及该异常事件之后和地震的对应关系进行统计分析。 研究发现, 无磁暴时逐日比异常和预测范围内地震对应关系达到0.77, 有磁暴时逐日比异常和地震对应关系为0.25。 综合分析认为逐日比异常事件发生后, 若该日无磁暴或者Dst指数小于异常第二日, 那么该异常为地震前兆的可能性大概为0.8, 反之则该异常有可能是磁暴的影响而不是来自于地下活动的影响, 需结合其他前兆分析方法进行综合分析, 该研究增强了逐日比异常判定地震地磁前兆信息的可靠性。 相似文献
15.
The possible contribution of solar and geomagnetic activity to changes in the characteristics of the main components of the climatic system—the ocean and the atmosphere—is considered and discussed. The mechanisms and models of the solar activity impact on thermobaric and climatic characteristics of the troposphere are presented. Based on a complex analysis of hydrometeorological data, it has been shown that changes in the temperature of the troposphere and the World Ocean reflect a response both to individual helio-geophysical perturbations and to long-term changes (1854–2015) of solar and geomagnetic activity. It is established that the climatic response to the influence of solar and geomagnetic activity is characterized by considerable spatio-temporal heterogeneity, is of a regional nature, and depends on the general circulation of the atmosphere. The largest contribution of solar activity to the global climate changes was observed in the period 1910–1943. 相似文献
16.
This work investigated an interrelationship between the monthly means of time derivatives of horizontal geomagnetic field, dH/dt, sunspot number, R z , and aa index for the period of substorms (from ?90 to ?1800 nT) during the years 1990–2009. A total of 232 substorms were identified during the period of study. The time derivative of horizontal geomagnetic field, dH/dt, used as a proxy for geomagnetically induced current (GIC) exhibited high positive correlation with sunspot number (0.86) and aa index (0.8998). The obtained geomagnetic activity is in 92.665% explicable by the combined effect of sunspot number and aa index. The distribution of substorms as a function of years gives a strong support for the existence of geomagnetic activity increases, which implies that as the sunspot number increases the base level of geomagnetic activity increases too. 相似文献
17.
2005年11月26日九江——瑞昌MＳ5.7地震发生前,震中及其周围地区的地磁基本场测量和相应的ldquo;2005.0中国地磁基本场曲面样条模型rdquo;显示,震中周围100 km范围内存在显著的ldquo;2005.0九江——瑞昌地磁基本场水平分量异常rdquo;. 而该异常在ldquo;1970.0中国地磁基本场曲面样条模型rdquo;中并不存在. 2005年12月在震中及其周围地区的21个测点上进行了地磁重复测量, 并建立了ldquo;局部修订2005.0中国地磁基本场曲面样条模型rdquo;. 该模型显示,震后ldquo;2005.0九江——瑞昌地磁基本场水平分量异常rdquo;明显减弱. 因此认为,ldquo;2005.0九江——瑞昌地磁基本场水平分量异常rdquo;是地震地磁前兆异常现象. 相似文献
18.
乌鲁木齐地磁台地磁场变化特征 总被引：2，自引：2，他引：0
根据乌鲁木齐地磁台有史以来的地磁观测资料,对该地区地磁场的长期变,短期变及其磁暴活动规律进行了总结分析,这对进一步认识乌鲁木齐地磁台地磁场各要素的变化规律及征,为地震震预报提供有实用价值的第一手资料都是十分有意义的。 相似文献
19.
利用新建中山站高频雷达2010年4月到2011年2月的观测数据,研究了中山站高频雷达回波的日变化特征以及地磁活动的影响. 研究结果表明,中山站高频雷达回波具有明显的日变化特征且受地磁活动影响较大. 雷达回波发生率的峰值在地磁活动较小时处于日侧;随着地磁活动的增强,峰值减小并向夜侧移动. 另外,平均多普勒视线速度具有明显的昼夜分布,夜侧主要为正向速度,即朝向雷达,日侧主要为负向速度,即远离雷达;随着地磁活动的增强,平均回波强度和平均多普勒视线速度的峰值都会增加,而多普勒谱宽则会减小. 相似文献
20.
Diurnal and semiannual variations in geomagnetic activity are considered. We prove that there exists an inner magnetospheric source of magnetic activity, which depends on the angle φ between the planes of the magnetotail plasma sheet and the geomagnetic equator. It is shown that diurnal and semiannual variations in magnetic activity result from changes in the value of this angle. 相似文献