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陈鹏  陈家君 《大地测量与地球动力学》2014,34(2):105-110

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Variation of the 0+ ion density during low and high solar activity as measured by the SR0SS-C2 satellite     

《Atmósfera》2014,27(3):227-237

The O⁺ ion density measured by the SROSS-C2 satellite during solar minima (year 1995, F_10.7 = 77) and maxima (year 2000, F_10.7 = 181) has been analyzed for studying diurnal, seasonal, latitudinal and geomagnetic variations. The study region covers an area encompassed between 5-3 5° N latitude and 65-95° E longitude over India at a ~500 km altitude (F2 region). The year 2000 shows significant enhancement in the annual average of O⁺ ion density and attainment of post sunset secondary enhancement compared to 1995. Attributed to photoionization, daytime shows a maximum ionization compared to nighttime. However, attainment of post sunset secondary maxima is attributed to the strong pre-reversal enhancement in the vertical E x B drift. The effect of geomagnetic activity Kp through the E x B drift dynamic movement on O⁺ ion density distribution studies indicates periodicities of seven and nine days in 1995 and 2000, respectively, and polynomial dependency of the O⁺ ion density on geomagnetic activity Kp. Further on, stratification of the O⁺ ion density according to latitude (5-35° N) indicates high density in mid-latitudes (12-24° N) compared to high and low latitudes, except in the winter of 1995, which shows a distinct trend (i.e., density decreases with increasing latitude).  相似文献   

基于二维经验模态分解的地磁基准图制备边界补偿方法          下载免费PDF全文

赵玉新  常帅  李旺 《地球科学》2014,39(11):1617-1624

针对采用矩谐分析方法构建地磁基准图的边界震荡问题, 提出一种基于二维经验模态分解的区域地磁异常数据边界补偿方法.采用二维经验模态分解方法对区域地磁异常数据进行多尺度分解, 对分解所得小尺度本征模态函数分量, 利用总体Hilbert变换法进行瞬时频率和瞬时幅值特征提取, 通过自采样和特征匹配进行边界补偿; 将大尺度分量之和作为趋势项, 利用三角函数方法建立模型并计算边界之外的大尺度磁异常值.实验证明, 相比当前已有方法, 可以更加有效地抑制对区域地磁异常数据进行矩谐分析的边界震荡问题, 稳定提高构建地磁基准图的准确性.   相似文献   

地磁测量中日变观测的常见问题     

高建尽  武同元 《北京测绘》2014,(6):106-108

地磁日变观测质量主要与仪器性能和观测点的环境有关。本文重点研究了目前在地磁日变测量中主要采用的HC90D氦光泵磁力仪的信号失锁问题,日变站的选址二个对于最终观测精度影响很大的问题,并提出了具体的解决方法。  相似文献   

地磁匹配导航算法研究   总被引：4，自引：0，他引：4  

王向磊  孙付平  陈坡 《测绘工程》2009,18(3):37-39

提出一种MonteCarlo方法和均方差算法（MSD）相结合的匹配算法，并将本算法用于地磁匹配导航中。该方法根据惯性导航系统指示的位置从地磁图上提取参考地磁数据，将地磁测量数据进行若干次随机干扰后和参考地磁数据使用MSD算法进行匹配，得到若干个匹配位置，取其均值作为最终匹配位置。仿真结果表明本算法可行。  相似文献   

Analysis of plasma and field conditions during some intensely geo-effective transient solar/interplanetary disturbances of solar cycle 23     

Yatendra Pal Singh  Munendra Singh  Badruddin 《Journal of Astrophysics and Astronomy》2006,27(2-3):361-366

The problem of solar wind-magnetosphere coupling is investigated for intense geomagnetic storms (Dst < -100nT) that occurred during solar cycle 23. For this purpose interplanetary plasma and field data during some intensely geo-effective transient solar/interplanetary disturbances have been analysed. A geomagnetic index that represents the intensity of planetary magnetic activity at subauroral latitude and the other that measures the ring current magnetic field, together with solar plasma and field parameters (V, B, Bz, σB, N, and T) and their various derivatives (BV,-BVz, BV², -BzV², B²V, Bz²V, NV²) have been analysed in an attempt to study mechanism and the cause of geo-effectiveness of interplanetary manifestations of transient solar events. Several functions of solar wind plasma and field parameters are tested for their ability to predict the magnitude of geomagnetic storm.  相似文献   

Paleomagnetic Excursions Recorded in the Yanchi Playa in Middle Hexi Corridor, NW China Since the Last Interglacial     

YANGTaibao YUYongtao LIJijun ANCongrong LIUJinfeng ZHANGJunyan 《山地科学学报》2004,1(2):128-142

Paleomagnetic determinations on lithologieal profiles of two paralleled long drillin gcores covering the past 130 kyr B.P., GT40 and GT60,from the Yanchi Playa in the arid Northwestern China indicate that a series of pronounced paleomagnetic excursions have been documented. By correlating our results with published regional and worldwide reports 4 excursion events out of 10 apparent reversal signals (labeled from GT-1 to GT-10) were identified as excursion events coeval with the Mono Lake Event (28.4 kyr-25.8 kyr), Laschamp Event (43.3 kyr-40.5kyr), Gaotai Event (82.8 kyr-72.4 kyr) and the Blake Event (127.4 kyr-113.3 kyr), respectively. GT-9 correlates with the above-mentioned Gaotai Event,GT-7 and GT-6 correspond to two stages of the Laschamp Event and GT-5 to the Mono Lake Event. It is noteworthy that the so-called Gaotai Event has not been reported as a pronounced paleomagnetic excursion in the Northwestern China. Every magnetic excursion event corresponds to paleointensity minima, anteceding those established abrupt paleoclimatic change events, such as the Younger Drays and the Heinrich Events (H1-H6). Here, we tentatively propose that these geomagnetic excursions/reversals can be viewed as precursors to climate abruptness. During the transitional stages when the earth‘s magnetic field shifted between a temporal normal and a negative period, the earth‘s magnetic paleointensity fell correspondingly to a pair of minima. Although more precise chronology and more convincing rock magnetic parameter determinations are essentially required for further interpretation of their intricate coupling mechanism, these results may have revealed, to some extent, that the earth‘s incessantly changing magnetic field exerts an strong influence on the onset of saw-tooth shaped abrupt climate oscillations through certain feedback chains in arid Central Asia or even North Hemispheric high latitude regions.  相似文献   

Influence of coronal mass ejection on geomagnetic activity during 1988–1993     

Shrivastava  Pankaj Kumar  Singh  G. N. 《Earth, Moon, and Planets》2002,91(1):1-8

The most rapid and dramatic evolution in the solar corona occurs in events now known as Coronal Mass Ejections (CMEs). There have considerable importance for our understanding of the evolution of the mass and energy injected into the interplanetary medium. In this work, we have studied the relation of CMEs with geomagnetic activity for the period of 1988 to 1993. Not all CMEs are capable of producing geomagnetic disturbances. Our study indicates that the maximum chance of a geomagnetic disturbance occurs two to three days after a CME in association with B-type solar flares.  相似文献   

冕洞与太阳活动周及地磁活动的演化关系     

罗葆荣  段长春 《天文学报》1997,38(4):386-393

本文用1970－1995年的冕洞资料，分析了冕洞的分布规律，磁场极性的演化特征和冕洞的地磁效应，以及它们与太阳黑子周期的演化关系，得到了一些有意义的结论。特别指出赤道冕洞和极区冕洞具有相反的演化规律和不同的特征。  相似文献   

用曲面插值方法建立海洋局部地磁场模型   总被引：2，自引：0，他引：2  

刘辉  赵建虎  李娟 《海洋测绘》2009,29(3):28-30

地磁场模型是地磁场的数学表达式，国内外已有多种建立地磁场模型的方法，对于局部地磁场模型来说，应用比较多的是多项式方法和曲面样条函数方法。讨论了基于曲面样条函数建立局部地磁场模型的原理和方法，并在实测数据基础上对模型的精度进行了验证。  相似文献