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1.
2015年尼泊尔地震的震前电离层异常探测 总被引：2，自引：0，他引：2
提出了一种基于奇异谱分析的电离层异常探测的方法。通过对尼泊尔地震震中周围GIM格网点TEC时间序列的探测,发现在2015年4月23日震中东部区域出现电离层正异常。进一步利用二维电离层地图分析异常空间分布,发现出现电离层正异常的区域为25°N-37.5°N,90°E-110°E,时间为2015年4月23日UT9:00-15:00。利用中国陆态网数据计算异常区域卫星穿刺点轨迹STEC变化情况,发现2015年4月23日穿刺点轨迹进入异常区域后STEC值比前后几天明显增大,而离开异常区域后又恢复正常。采用CIT(computerized ionosphere tomography)方法详细地呈现了电离层异常的三维形态,发现4月23日UT9:00-15:00在震中东部区域出现电离层正异常,峰值位于约30°N,115°E,高度范围为100~500 km,且异常峰值随高度变化与电离层本身垂直密度分布规律相一致。 相似文献
2.
3.
基于北斗GEO卫星独有的静地特性,本文利用其观测数据提取电离层TEC进行磁暴期间电离层TEC时空变化研究。同时利用全球电离层格网图GIM值进行试验对比,结果表明：北斗GEO卫星提取的TEC与GIM模型值变化趋势一致,并且前者可更有效地监测电离层的细微扰动变化。在此次磁暴发生期间,亚太地区电离层TEC变化及扰动响应特征在纬度方向差异明显。其中南北半球较高纬度区域,电离层TEC在磁暴主相阶段主要表现为正响应扰动,而赤道及北半球较低纬度区域,电离层TEC在磁暴主相及恢复相阶段均产生了强度更大、持续时间更长的正响应扰动。结合现有研究,认为造成此次电离层异常扰动的激励因素主要为东向快速穿透电场的增强及热层中性成分的变化。试验结果也证明了GEO卫星可以精准有效地监测在磁暴发生时电离层TEC的变化规律及不同空间位置处TEC产生的扰动响应特征。 相似文献
4.
针对2015-04-25尼泊尔Mw 7.8地震,利用NOAA卫星遥感射出长波辐射(OLR)数据和IGS(International GNSS Service)提供的全球IONEX总电子含量(TEC)数据,并考虑太阳和地磁活动水平的条件下,分别对OLR数据采用标准差阈值法和对电离层TEC数据采用四分位距法进行了异常探测。结果显示,2015-04-22在震中附近地区卫星遥感OLR出现异常增强现象;同时,2015-04-23在震中附近电离层TEC出现显著正异常现象,而且出现磁共轭现象。 相似文献
5.
For about 40 years, ionospheric variations [including total electron content (TEC)] have been observed from time to time during large earthquakes. The TEC is the integrated electron density between a ground beacon and a satellite. It is a by-product of the International DORIS Service (IDS), which is also used for precise orbit determination of altimetric satellites. This paper reports the study of TEC variations observed by the DORIS station Cibinong, Indonesia (CICB, latitude: 6.48°S; longitude: 106.85°E) at the time of the Sumatra–Andaman earthquake (magnitude 9.2), which occurred on December 26, 2004. Numerous and intense aftershocks followed for several months after the main shock. An analysis was done to compare the variation of the TEC intensity observed by several satellites with the occurrence of these earthquakes. For comparison, the same study was also performed for another earthquake occurred very close to CICB but at a very different time. The main result is that the DORIS data show a TEC perturbation during night time close to the epicenter prior to the main Sumatra–Andaman earthquake event. 相似文献
6.
利用GPS研究电离层,具有其他探测技术所没有的全天候、高分辨率、大范围等优点.本文采用双频GPS数据提取区域电离层电子浓度总含量（TEC）,并结合全球电离层地理（GIM）数据,借助滑动四分位距法建立TEC背景值.研究了台风“莫兰蒂”对其经过区域及登陆地点电离层TEC的影响.分析表明,台风登陆厦门前一天,厦门地区电离层TEC发生了较强的正扰动,登陆后第二天,TEC发生了小尺度的负扰动;台风临近台湾岛前,东南沿海和台湾岛区域电离层出现了大范围的正异常扰动,其值为15～20 TECU,持续时间10 h.结合厦门和台湾岛的地形,推测此次TEC异常原因是由于台风所激发的声重力波传播到电离层高度,造成了电离层的异常扰动. 相似文献
7.
基于IGS全球电离层TEC地图数据,提取到汶川地震上空TEC时间序列。使用移动Chapman－Miller太阳日变化分析方法,研究了地震前后15天TEC异常现象。结果显示,地震前6天（除5月9日外） TEC都出现了不同程度的减小现象,5月9日TEC周日峰值出现延迟现象;5月3日,即地震前第9天出现了TEC增大现象。离发震时刻较远的4月29日出现了TEC减小现象;震后3天也出现了明显的减少现象。排除磁暴等因素后,认为这些异常现象可能是汶川地震引起的地震－电离层耦合效应。 相似文献
8.
采用IGS发布的GIM数据,提出了一种结合滑动时窗法和临近格网点电离层TEC相关性分析法的联合分析方法,研究了震前电离层异常变化与地震的关系。通过分析震区附近5个格网点TEC的异常变化情况,发现震前电离层TEC发生明显异常变化,且格网点之间的TEC序列相关性受地震显著影响;通过分析二维电离层图的TEC异常空间分布,发现震前三天震中附近分别出现6h、12h和6h的异常。最后利用电离层层析的方法,对电离层异常时刻进行了电子密度的反演,进一步分析了电子密度在电离层异常时刻的分布情况。 相似文献
9.
2014年鲁甸6.5级地震震前TEC异常分析 总被引：2，自引：0，他引：2
2014年8月3日云南省鲁甸发生了6.5级地震.针对震前电离层异常问题,利用IGS提供的全球电离层数据,采用滑动四分位法对鲁甸地震震中及其周围格网点的TEC进行异常探测,发现震前3d、6d和13 d电离层有明显的异常,其中震前3d、6d的异常最为显著.在进一步分析了太阳地磁活动及这几天的全球TEC异常分布后,认为这3d的电离层异常可能与震前的孕育地震有关.另外,这3d的TEC异常分布区域都满足在经度方向跨度和纬度方向跨度长度比约为3:1,且异常的峰值点并不位于震中的正上方,而是位于震中偏向赤道方向,同时赤道共轭区域也存在异常,但范围和幅度都较小. 相似文献
10.
利用GPS双频观测数据分析了仪器偏差对计算电离层TEC的影响,结果表明忽略仪器偏差的影响不能正确反映测站上空电离层总电子含量的变化规律。验证了短期内仪器偏差的稳定性,并在此基础上研究了2005年太阳活动低峰年区域电离层VTEC的周年变化规律,揭示了电离层VTEC半年变化、季节性变化及冬季异常等现象。 相似文献
11.
电离层参量的提取是开展电离层研究的基础,而数据同化技术则是获取电离层参量的一种重要手段。以NeQuick模型的输出作为背景场,Kalman滤波作为同化算法,利用数据同化技术实现区域电离层TEC重构,结果表明,数据同化方法重构的倾斜总电子含量（TEC）和垂直TEC与实测值较为一致。相比NeQuick模型及全球电离层地图（GIM）数据,数据同化方法重构得到的TEC的平均误差和标准差均有明显的降低,实测数据验证了数据同化技术在区域TEC重构中的精度和可靠性。 相似文献
12.
Experimental analysis was performed using multiplicative algebraic reconstruction technique (MART) to map the ionosphere over Brazil. Code and phase observations from the global navigation satellite system (GNSS) together with the international reference ionosphere (IRI) enabled the estimation of ionospheric profiles and total electron content (TEC) over the entire region. Twenty-four days of data collected from existing ground-based GNSS receivers during the recent solar maximum period were used to analyze the performance of the MART algorithm. The results were compared with four ionosondes. It was demonstrated that MART estimated the electron density peak with the same degree of accuracy as the IRI model in regions with appropriate geometrical coverage by GNSS receivers for tomographic reconstruction. In addition, the slant TEC, as estimated with MART, presented lower root-mean-square error than the TEC calculated by ionospheric maps available from the International GNSS Service (IGS). Furthermore, the daily variations of the ionosphere were better represented with the algebraic techniques, compared to the IRI model and IGS maps, enabling a correlation of the elevation of the ionosphere at higher altitudes with the equatorial ionization anomaly intensification. The tomographic representations also enabled the detection of high vertical gradients at the same instants in which ionospheric irregularities were evident. 相似文献
13.
We consider disturbances of total electron content (TEC) of the high-latitude ionosphere provided by the GPS global navigation satellite system before and during the magnetic storm on April 5, 2010. Simultaneously, we examine magnetic data from all available magnetometer arrays in the northern hemisphere, augmented with data from scanning photometers and riometers. The substorm onset, during both non-storm and storm periods, is found to cause significant enhancement of TEC scintillations characterized by the TEC time derivative dTEC. Comparison of 2D maps of the spectral power of magnetic fluctuations in the Pc5 band (1–10 mHz) and dTEC during substorms shows a good spatial and temporal correspondence between them. Both magnetic and ionospheric fluctuations tend to concentrate inside the auroral oval, the boundaries of which are determined from the OVATION model. The time–space evolution of TEC scintillations is rather similar to that of ultra-low-frequency magnetic fluctuations, but not to that of the ionospheric electrojet. GPS signal phase slips, resulting in non-physical TEC jumps (>1 TECu/min), occur predominantly inside the auroral oval and in the vicinity of its equatorward boundary. 相似文献
14.
利用2000~2012年的IGS电离层TEC数据,研究了南北半球电离层TEC的非对称性。首先对南北半球TEC日平均值的不对称指数(AI)进行了研究,结果表明,AI的极大值的绝对值集中在0.4左右,极小值的绝对值集中在0.3左右,表明南北半球电离层TEC存在数值上的非对称性;通过傅里叶变换,发现AI存在1 a和1/3 a周期;每年北半球电离层TEC高于南半球电离层TEC的时间比例均大于50%,平均值为58%,表明了南北半球电离层TEC存在时间上的非对称性。然后进一步分析了南北半球TEC年平均值的差异,发现了北半球TEC年平均值高于南半球的规律,2000~2012年的南北半球TEC年平均值的不对称指数在0.036左右。最后从全球大气分布及运动规律的南北非对称性和热层年度变化赤道非对称性两个角度,对南北半球电离层TEC的非对称性产生的原因做了初步分析。 相似文献
15.
Application of SWACI products as ionospheric correction for single-point positioning: a comparative study 总被引：1，自引：0，他引：1
In Global Navigation Satellite Systems (GNSS) using L-band frequencies, the ionosphere causes signal delays that correspond with link related range errors of up to 100 m. In a first order approximation the range error is proportional to the total electron content (TEC) of the ionosphere. Whereas this first order range error can be corrected in dual-frequency measurements by a linear combination of carrier phase- or code-ranges of both frequencies, single-frequency users need additional information to mitigate the ionospheric error. This information can be provided by TEC maps deduced from corresponding GNSS measurements or by ionospheric models. In this paper we discuss and compare different ionospheric correction methods for single-frequency users. The focus is on the comparison of the positioning quality using dual-frequency measurements, the Klobuchar model, the NeQuick model, the IGS TEC maps, the Neustrelitz TEC Model (NTCM-GL) and the reconstructed NTCM-GL TEC maps both provided via the ionosphere data service SWACI (http://swaciweb.dlr.de) in near real-time. For that purpose, data from different locations covering several days in 2011 and 2012 are investigated, including periods of quiet and disturbed ionospheric conditions. In applying the NTCM-GL based corrections instead of the Klobuchar model, positioning accuracy improvements up to several meters have been found for the European region in dependence on the ionospheric conditions. Further in mid- and low-latitudes the NTCM-GL model provides results comparable to NeQuick during the considered time periods. Moreover, in regions with a dense GNSS ground station network the reconstructed NTCM-GL TEC maps are partly at the same level as the final IGS TEC maps. 相似文献
16.
Patricia Doherty joins the regular contributors of this column to discuss the correlation between measurements of solar 10.7
cm radio flux and ionospheric range delay effects on GPS. Mrs. Doherty has extensive experience in the analysis of ionospheric
range delays from worldwide systems and in the utilization and development of analytical and theoretical models of the Earth's
ionosphere.
Ionospheric range delay effects on GPS and other satellite ranging systems are directly proportional to the Total Electron
Content (TEC) encountered along slant paths from a satellite to a ground location. TEC is a highly variable and complex parameer
that is a function of geographic location, local time, season, geomagnetic activity, and solar activity. When insufficiently
accounted for, ionospheric TEC can seriously limit the performance of satellite ranging applications. Since the ionosphere
is a dispersive medium, dual-frequency Global Positoning System (GPS) users can make automatic corrections for ionospheric
range delay by computing the apparent difference in the time delays between the two signals. Single-frequency GPS users must
depend on alternate methods to account for the ionospheric range delay. Various models of the ionosphere have been used to
provide estimates of ionospheric range delay. These models range from the GPS system's simple eight-coefficient algorithm
designed to correct for approximately 50% rms of the TEC, to state-of-the-art models derived from physical first principles,
which can correct for up to 70 to 80% rms of the TEC but at a much greater computational cost.
In an effort to improve corrections for the day-to-day variability of the ionosphere, some attempts have been made to predict
the TEC by using the daily values of solar 10.7 cm radio flux (F10,7). The purpose of this article is to show that this type of prediction is not useful due to irregular, and sometimes very
poor, correlation between daily values of TEC and F10.7. Long-term measurements of solar radio flux, however, have been shown to be well correlated with monthly mean TEC, as well
as with the critical frequency of the inonospheric F2 region (foF2), which is proportional to the electron density at the
peak of the ionospheric F2 region. ? 2000 John Wiley & Sons, Inc. 相似文献
17.
Single layer ionosphere models are frequently used for ionospheric modeling and estimation using GPS measurements from a network of GPS reference stations. However, the accuracies of single layer models are inherently constrained by the assumption that the ionospheric electrons are concentrated in a thin shell located at an altitude of about 350 km above Earths surface. This assumption is only an approximation to the physical truth because the electrons are distributed in the entire ionosphere region approximately from 50 to 1,000 km. To provide instantaneous ionospheric corrections for the real-time GPS positioning applications, the ionospheric corrections need to be predicted in advance to eliminate the latency caused by the correction computation. This paper will investigate ionospheric total electron content (TEC) predictions using a multiple-layer tomographic method for ionospheric modeling over a local area GPS reference network. The data analysis focuses on the accuracy evaluation of short-term (5 min in this study) TEC predictions. The results have indicated that the obtainable TEC prediction accuracy is at a level of about 2.8 TECU in the zenith direction and 95% of the total electron content can be recovered using the proposed tomography-based ionosphere model. 相似文献
18.
为提高电离层总电子含量（total electronic content，TEC）扰动探测参考背景值的预测精度，提出了多尺度自回归移动平均（autoregressive moving average，ARMA）残差修正模型。通过对比该方法、ARMA模型、四分位距法（inter quartile range，IQR）及滑动时窗法对TEC背景值的预测精度，结果显示修正模型预测的TEC背景值平均相对精度为89.78%，分别比ARMA模型、IQR及滑动时窗法高5.18%、1.41%和1.42%，且预测值的残差绝对值小于等于3.0 TECU的百分比为91.67%，明显优于其他3种方法，说明修正模型探测震前TEC异常是可行的。利用该方法探测2013-04-20芦山县Mw7.0级地震震前电离层TEC扰动情况，验证了该方法的有效性。实验结果表明，震前第9天和第13天电离层明显的正异常和震前第1~4天明显的负异常极可能是孕育地震引起的，且正异常主要出现在08:00-10:00 UT，而负异常主要集中在0:00-14:00 UT。 相似文献
19.
GAMIT／GLOBK是全球应用最广泛的高精度GPS数据处理软件之一,不仅在高精度定位方面得到应用,而且在全球地壳板块运动监测、电离层监测和GPS气象学等领域也得到广泛应用。本文介绍了在Windows7系统下实现Ubunru Kylin16.04桌面版系统的安装,并在Ubuntu Kylin系统平台下安装、更新最新版GAMIT／GLOBK10.60,并利用中国及其周边IGS站观测数据进行基线解算和网平差,验证了软件安装的正确性。 相似文献
20.
High-frequency variability of the ionosphere, or irregularities, constitutes the main threat for real-time precise positioning techniques based on Global Navigation Satellite Systems (GNSS) measurements. Indeed, during periods of enhanced ionospheric variability, GNSS users in the field—who cannot verify the integrity of their measurements—will experience positioning errors that can reach several decimeters, while the nominal accuracy of the technique is cm-level. In the frame of this paper, a climatological analysis of irregularities over the European mid-latitude region is presented. Based on a 10 years GPS dataset over Belgium, the work analyzes the occurrence rate (as a function of the solar cycle, season and local time) as well as the amplitude of ionospheric irregularities observed at a single GPS station. The study covers irregularities either due to space weather events (solar origin) or of terrestrial origin. If space weather irregularities are responsible for the largest effects in terms of ionospheric error, their occurrence rate highly depends on solar activity. Indeed, the occurrence rate of ionospheric irregularities is about 9 % during solar maximum, whereas it drops to about 0 % during medium or low solar activity periods. Medium-scale ionospheric disturbances (MSTIDs) occurring during daytime in autumn/winter are the most recurrent pattern of the time series, with yearly proportions slightly varying with the solar cycle and an amplitude of about 10 % of the TEC background. Another recurrent irregularity type, though less frequent than MSTIDs, is the noise-like variability in TEC observed during summer nighttime, under quiet geomagnetic conditions. These summer nighttime irregularities exhibit amplitudes ranging between 8 and 15 % of the TEC background. 相似文献