EISCAT雷达观测到的极区电离层等离子体反常对流          下载免费PDF全文

马淑英  刘鹏  刘会欣  徐继生  K Schlegel 《地球物理学报》2001,44(4):446-453,T001

综合分析EISCAT雷达与卫星当地测量数据,并利用磁层磁场模式对磁力线进行追踪,研究了发生在极光椭圆朝极盖边界附近电离层中,一例反常的背离太阳流动的强等离子体对流事件,及相关的太阳风-磁层-电离层耦合过程.结果表明,磁暴期间IMFBz指向南时观测到这一反常高速对流,及其相应的等离子体性态特征,很可能是向阳侧磁层顶磁重联过程在电离层中的印记.  相似文献   

Local time variation of geomagnetic transfer functions   总被引：1，自引：0，他引：1  

Masahiko Takeda 《Geophysical Journal International》1997,130(3):765-770

The local time (LT) variation of the geomagnetic transfer function at the 32-min period was examined for observatories distributed worldwide. Two distinct variation types (types 1 and 2) were found in the real part of A. Type 1 is conspicuous at lower latitudes and its seasonal variation is small, whereas type 2 is found at higher latitudes and has its maximum in summer. These two types of LT variation are seen globally and are conspicuous when solar activity is high. The amplitudes of both types of variation vary from 0.018 to 0.078, and are independent of the mean values at each observatory. These values are relatively small, but the amplitude of Chambon la Foret is larger than the mean value, which shows that Au changes its sign in local time. The amplitudes of type 1 and 2 variations decrease and increase with geomagnetic latitude, respectively. These features suggest that they are generated by some global external fields. The most probable cause is the Sq field, although the Dp field may contribute to type 1 variation. On the other hand, for the islands of the Pacific Ocean at low latitudes, such as Honolulu and Chichijima, the type 1 variation appears not in the real but in the imaginary part of A, which suggests that currents induced in the ocean also contribute to the local time variation.  相似文献   

1987年9月23日日环食引起的电离层扰动          下载免费PDF全文

李利斌  万卫星 《地球物理学报》1990,33(4):384-390

本文利用武汉电离层观象台的高频多普勒台阵、TEC台阵和加密频高图等多种观测资料,分析了1987年9月23日发生在我国境内的日环食的电离层效应,简要地讨论了光食过程的电离层变化,着重研究了食后电离层扰动以及这种效应的高度演变和传播特征.结果表明:1.在不同高度上电离层的光化过程的弛豫时间不同,光食效应有明显的高度差异;2.食后出现了电离层行扰,这种扰动的特性随高度变化十分复杂,但不同高度上扰动的水平传播方向都指向日食中心带.这种扰动的激发源不在环食中心带内,它的激发可能与日食时大范围的大气冷却收缩所引起的低层大气运动的不稳定性有关.  相似文献   

Undifferenced Cycle Slip Estimation of Triple-Frequency BeiDou Signals with Ionosphere Prediction     

Bofeng Li  Yanan Qin  Zhen Li  Lizhi Lou 《Marine Geodesy》2016,39(5):348-365

With the rapid development of BeiDou satellite navigation system (BDS), high-quality service has been provided in the Asia-Pacific region currently, which will be extended to the whole world very soon. BDS is the first Global Navigation Satellite System that all satellites broadcast the triple-frequency signals. The triple-frequency signals in theory can improve the cycle slip detection that is one of the preconditions in precise positioning by making use of carrier phase. This paper discusses the development of a cycle slip detection method for undifferenced BDS triple-frequency observations in kinematic scenario. In this method, two geometry-free extra-wide-lane combinations and one geometry-free narrow-lane (NL) combinations are employed. The key is to mitigate the between-epoch ionospheric biases in the geometry-free NL combinations. We propose to predict the ionospheric biases of current epoch by using those from its consecutive foregoing epochs. The method is tested with extensive experiments in varying observation scenarios. The results show that in case of sampling interval as small as 5 s, the between-epoch ionospheric biases can be ignored and the correct cycle slips can be determined. Meanwhile in case of lower sampling frequency, one needs to compensate the ionospheric biases of current epoch by using the predicted ionospheric biases. The presented method can correctly detect all cycle slips even if they are as small as 1 cycle.  相似文献   

不同TEC分布模式对星载SAR立体定位精度的影响及校正     

赵玲  周杨  靳国旺  薛武 《测绘科学技术学报》2016,(6):599-604

基于SAR成像模型和R-D定位模型,分析了电离层对星载SAR立体定位精度的影响,提出了相应的校正方法,并进行了仿真实验。实验表明对于特定波长的SAR信号,不同TEC分布模式组合对SAR立体像对定位精度的影响不同,校正效果也不同:当两幅影像对应的TEC分布均匀且大小相同时,电离层对SAR立体定位精度的影响小到可以忽略;当两幅影像由于拍摄季节不同导致TEC不同时,电离层影响很大,特别是距离向精度,其影响程度与两幅影像对应的TEC差值正相关,此时定向参数精化法校正效果很好;当电离层发生扰动时,电离层影响随着扰动程度的增大而增大,定向参数精化法有一定效果,但当电离层扰动很大时,校正效果明显减弱,还需要通过斜距直接校正法等其他方法予以校正。  相似文献   

Klobuchar电离层模型精化进展     

刘宸  李海峰  冯绪  鲍亚东  宋华标 《测绘科学技术学报》2017,(5):455-460

电离层延迟是卫星导航定位的重要误差源之一。采用合适的电离层延迟模型可以有效地减弱电离层延迟误差对定位结果的影响。目前在导航定位中运用最广泛的是Klobuchar模型,但Klobuchar模型的修正率只有50%~60%。为了满足日益增长的导航定位精度的需求,不同的精化模型被提出。本文介绍了Klobuchar模型在GPS和BDS系统中的应用,比较了在两个系统应用时的差异。回顾概括了文献在Klobuchar模型的参数精化和模型精化两个方面的研究,并对各种精化模型进行了对比总结。模型精化的结果优于参数精化,未来对于Klobuchar模型的精化更趋向于模型精化。  相似文献   

基于CMONOC GPS数据的SSA电离层预测模型研究     

史坤朋  郭金运  张永明  狄文强 《大地测量与地球动力学》2019,39(11):1153-1158

利用基于CMONOC的GPS观测数据反演中国大陆区域高精度的RIM，并将奇异谱分析(SSA)方法应用于TEC预报，判断不同序列长度对预测结果的影响，并根据w-correlation选取合适的RC迭代阶数和窗口长度。结果发现，当TEC时间序列长度为27 d，窗口长度为序列长度的1/3、迭代SSA分解的前5项时，预测效果最好。提取RIM中心网格点的TEC数据，分别以年积日1~27、101~127、201~227、301~327等4个时段的TEC序列为原始数据，基于SSA进行7 d的预测，同时建立ARMA预测模型。结果显示，相较于ARMA预测，SSA方法总体预测精度提高约10%，预测时段更长。进一步对4个时段RIM中2 911个网格点处的TEC进行预测，发现RMSE随着纬度减小而增大，预测相对精度呈现中纬度比高、低纬度略高的特点，但无论哪种精度指标，SSA预测模型均优于ARMA预测模型。  相似文献   

卫星导航服务的全球电离层时变特性分析   总被引：2，自引：0，他引：2  

冯建迪  王正涛  赵珍珍 《测绘科学》2015,40(2):13-17

针对电离层对无线电波应用技术的影响,该文利用IGS提供的1998年—2012年的全球电离层TEC数据,结合相应的太阳活动数据,采用时间序列分析、相关性分析以及等值线图等数理统计的方法,分析了全球电离层的时变特性;分析了电离层TEC、F10.7和太阳黑子数的相关性,发现3者之间的相关系数高度线性相关。通过电离层日变化规律的研究发现:电离层TEC日极大值出现的时刻集中在当地时间12时至16时,其中14时占38.47%,12时占26.58%,16时占19.05%;夜间TEC值与太阳活动强度密切相关,在太阳活动低峰年,夜间全球电离层TEC平均值在5TECU左右,在太阳活动高峰年,夜间全球电离层TEC平均值在17TECU左右,最大值可达24TECU。最后,从日地距离和太阳活动强度两个方面,讨论了全球电离层TEC季节变化规律以及成因。  相似文献   

Reconstruction of nonmonotonic electron density profiles of the Martian topside ionosphere     

H. Zou  E. Nielsen  X.-D. Wang 《Planetary and Space Science》2010,58(10):1391-1399

One of the problems in reconstructing the real ionosphere from an ionogram is the occurrence of a ‘valley,’ where electron density decreases with altitude and make a non-monotonic profile. For the case of the Earth ionosphere, the ordinary and extraordinary ray data, accompanied with an empirical model, based on the observations, are necessary to obtain a mathematical solution for a ‘valley,’ such as the region between the E and F layers. MARSIS/MEX is a topside sounder designed to observe the ionosphere of Mars. Some ‘valley’ structures were found in the ionograms measured by MARSIS. The echoes of the extraordinary ray are not available owing to the absence of the strong magnetic field on Mars. Therefore, it is difficult to have a mathematical solution for the valleys in the Martian ionosphere. In this paper, a least square method with a simple model is presented to solve the ‘valley’ problem in the topside ionosphere of Mars. The electron density profiles with ‘valleys’ observed by the Radio Occultation experiment onboard MGS are used to rebuild the virtual depths at MARSIS frequencies. The reconstructed electron density profile by the least square method with a simple model from the rebuilt virtual depth curve is compared with the original electron density profile. It is proved that this method can reproduce small valleys in the profile of the Martian ionosphere well.  相似文献   

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杨马陵  邓柏昌  赵文化  黄江 《大地测量与地球动力学》2009,29(6):13-17

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