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231.
Jung-Hee Kim Heon-Young Chang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(8):2040-2049
We investigate the geomagnetic field variations recorded by INTERMAGNET geomagnetic observatories, which are observed while the Moon’s umbra or penumbra passed over them during a solar eclipse event. Though it is generally considered that the geomagnetic field can be modulated during solar eclipses, the effect of the solar eclipse on the observed geomagnetic field has proved subtle to be detected. Instead of exploring the geomagnetic field as a case study, we analyze 207 geomagnetic manifestations acquired by 100 geomagnetic observatories during 39 solar eclipses occurring from 1991 to 2016. As a result of examining a pattern of the geomagnetic field variation on average, we confirm that the effect can be seen over an interval of 180?min centered at the time of maximum eclipse on a site of a geomagnetic observatory. That is, demonstrate an increase in the Y component of the geomagnetic field and decreases in the X component and the total strength of the geomagnetic field. We also find that the effect can be overwhelmed, depending more sensitively on the level of daily geomagnetic events than on the level of solar activity and/or the phase of solar cycle. We have demonstrated it by dividing the whole data set into subsets based on parameters of the geomagnetic field, solar activity, and solar eclipses. It is suggested, therefore, that an evidence of the solar eclipse effect can be revealed even at the solar maximum, as long as the day of the solar eclipse is magnetically quiet. 相似文献
232.
研究迷效应和地磁场效应对中低轨道航天器表充电的影响,根据航天器表充电机制,采用薄鞘模型,根据电流收庥和轨道反演方法进行了数值模拟,给出航天器表面为导体和非导体的平衡电位,并进行了分析研究,数据结果观测和理论分析相符。 相似文献
233.
234.
G. Qin S. QiuH. Ye A. HeL. Sun X. LinH. Li X. XuH. Zeng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Three “SZ” Atmospheric Composition Detectors (ACDs) on board spacecraft “SZ-2”, “SZ-3” and “SZ-4” were launched on 10th January 2001, 26th March 2002 and 31st December 2002 separately. A large quantity of thermospheric composition data at the orbital altitude ranging from 330 to 362 km were collected from the in-situ measurement of ACDs. The spacecrafts’ lifetime was just in the second peak period of the 23rd solar cycle which includes two peaks and the solar activity value F10.7 was from 89 to 228. During this period, several intense geomagnetic disturbances happened. 相似文献
235.
M. Papailiou H. Mavromichalaki K. Kudela J. Stetiarova S. Dimitrova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Over the last years the potential effect that the geomagnetic activity may have on human physiological parameters (such as heart rate, arterial diastolic and systolic pressure) is being widely investigated with irrefutable results. As it is suggested, human health can be affected by solar activity and related geophysical changes. In this study a group of 4018 Slovak aviators was examined from January 1, 1994 to December 31, 2002, covering periods with high solar and geomagnetic activity. Specifically, medical data of mean values of arterial diastolic and systolic blood pressure, which were registered during the medical examinations of the Slovak aviators, were related to daily variations of Dst and Ap geomagnetic indices. All subjects were men (from 18 to 60 years old) in good health. Statistical significance levels (p-values) of the effect of geomagnetic activity on the aforementioned parameters up to three days before and three days after the geomagnetic event were established using the statistical method ANalysis Of VAriance (ANOVA). Statistical analysis of the arterial blood pressure variations for different levels of geomagnetic activity revealed that geomagnetic changes are connected to variations of the human physiological parameters. 相似文献
236.
V.V. Kalegaev N.A. Vlasova 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The Earth’s magnetosphere response to interplanetary medium conditions on January 21–22, 2005 and on December 14–15, 2006 has been studied. The analysis of solar wind parameters measured by ACE spacecraft, of geomagnetic indices variations, of geomagnetic field measured by GOES 11, 12 satellites, and of energetic particle fluxes measured by POES 15, 16, 17 satellites was performed together with magnetospheric modeling based in terms of A2000 paraboloid model. We found the similar dynamics of three particle populations (trapped, quasi-trapped, and precipitating) during storms of different intensities developed under different external conditions: the maximal values of particle fluxes and the latitudinal positions of the isotropic boundaries were approximately the same. The main sources caused RC build-up have been determined for both magnetic storms. Global magnetospheric convection controlled by IMF and substorm activity driven magnetic storm on December 14–15, 2006. Extreme solar wind pressure pulse was mainly responsible for RC particle injection and unusual January 21, 2005 magnetic storm development under northward IMF during the main phase. 相似文献
237.
为解决地磁匹配算法中匹配点的选取和匹配序列长度的设置问题,提出一种迭代最近等值线(ICCP)算法的地磁匹配序列生成方法。首先,分析了采样定理、地磁图分辨率、磁场起伏特征和磁传感器测量精度等对匹配序列采样间隔的约束,以及匹配序列长度与误匹配的关系;然后,在此基础上利用增量调制原理实现了匹配点的选取;最后,建立了本文方法参数优化的目标函数,并利用二进制粒子群优化(BPSO)算法对匹配序列的长度和增量调制的量阶进行寻优,使ICCP算法在保证匹配精度的前提下能够缩短匹配时间。仿真结果证明所提方法具有良好的环境适应性,对ICCP算法的精度和实时性都有明显改善。 相似文献
238.
239.
利用时序叠加法对1984年4月至1987年2月的日侧极隙纬度VLF波活动指数与磁暴活动作了统计分析。结果表明若以磁暴开始日为第0天,则VLF波活动指数在0至一2天内相对于平均值都有下降的效应,而在第2天或第4天则有明显的上升效应,并且存在着季节不对称性,其中急始型的暴始下降和缓始型的暴后上升效应均显冬大夏小的特征,冬季值约为夏季值的3倍。 相似文献
240.