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排序方式: 共有100条查询结果,搜索用时 171 毫秒
21.
Alam E. Kherani Matheus Mascarenhas Eurico R. De Paula Jose H. A. Sobral Fernando Bertoni 《Space Science Reviews》2005,121(1-4):253-269
We present a three-dimensional simulation of collisional-interchange-instability in the equatorial-low-latitude F region of
ionosphere. The instability is responsible for the generation of large plasma density depletion or bubble. General 3D potential
and continuity equations are derived to simulate the phenomena. To understand the linear aspect of the instability, the general
3D linear growth rate is derived using 3D potential equation. The linear growth characteristics are compared with earlier
field-aligned-integrated growth analyses. The numerical simulation of bubble in the 3D spherical polar geometry is finally
presented. Distinct evolution characteristics of bubble in 3D and 2D simulation are further discussed. 相似文献
22.
I.S. Batista M.A. Abdu Paulo A.B. Nogueira R.R. Paes J.R. de Souza B.W. Reinisch V.H. Rios 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
This study reports on ionospheric disturbances that occurred in the early morning hours in the South American–Atlantic sector during a few intense/super storm events. The events were observed at latitudes close to the southern crest of the equatorial ionization anomaly (EIA) as an unusual intensification of the F region electron density peak at local times when the EIA is not usually developed. All the events were observed at pre dawn-morning hours, under conditions of northward interplanetary geomagnetic field. Large scale traveling ionospheric disturbances that are launched during highly disturbed conditions and/or equatorward surges in the thermospheric meridional winds seem to be the most probable causes of the observed disturbances. 相似文献
23.
P.V.S. Rama Rao K. VenkateshD.S.V.V.D. Prasad K. Niranjan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
The Indian sector encompasses the equatorial and low latitude regions where the ionosphere is highly dynamic and is characterized by the equatorial ionization anomaly (EIA) resulting in large latitudinal electron density gradients causing errors and uncertainties in the estimation of range delays in satellite based navigation systems. The diurnal and seasonal variations of standard deviations in the TEC data measured during the low sunspot period 2004–2005 at 10 different Indian stations located from equator to the anomaly crest region and beyond are examined and presented. The day-to-day variability in TEC is found to be lowest at the equatorial station and increases with latitude up to the crest region of EIA and decreases beyond. 相似文献
24.
GPS广域增强系统电离层延迟网格修正算法的研究 总被引:5,自引:0,他引:5
建立了一种广域增强系统地面监测网对电离层延迟的观测数据生成网格修正值算法,并在天津,长春,西安三地通过用双频接收机同时采集的电离层延迟实测数据,对广域增强系统的电离层网格修正法的修正精度进行验证,并与一般用户目前采用的Klobuchar模型修正法进行了比较,结果表明,电离层延迟网格修正法的修正精度普遍大于80%,优于Klobuchar模型修正法,是一种精度较高的电离层实时修正法。 相似文献
25.
26.
BD2系统广域差分格网电离层模型研究与应用 总被引:1,自引:0,他引:1
电离层延迟误差是影响BD2卫星导航系统定位测速精度的关键因素,如何减少电离层误差是当前卫星导航定位领域研究的热点问题.常见的电离层模型包括广域差分格网模型和Klobuchar模型,已有研究主要关注Klobuchar模型,对BD2广域差分格网模型的研究较少.本文分析比较了广域差分格网电离层模型和Klobuchar模型对电离层延迟误差的影响,并进行了真实环境下的评测.实验结果表明,使用广域差分格网电离层模型修正电离层延迟可以减小电离误差,从而提高单频接收机导航定位精度. 相似文献
27.
Geoffrey Andima Emirant B. Amabayo Edward Jurua Pierre J. Cilliers 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):264-273
Complex electrodynamic processes over the low latitude region often result in post sunset plasma density irregularities which degrade satellite communication and navigation. In order to forecast the density irregularities, their occurrence time, duration and location need to be quantified. Data from the Communication/Navigation Outage Forecasting System (C/NOFS) satellite was used to characterize the low latitude ion density irregularities from 2011 to 2013. This was supported by ground based data from the SCIntillation Network Decision Aid (SCINDA) receivers at Makerere (Geographic coordinate 32.6°E, 0.3°N, and dip latitude ?9.3°N) and Nairobi (Geographic coordinate 36.8°E, ?1.3°N, and dip latitude ?10.8°N). The results show that irregularities in ion density have a daily pattern with peaks from 20:00 to 24:00 Local Time (LT). Scintillation activity at L band and VHF over East Africa peaked in 2011 and 2012 from 20:00 to 24:00 LT, though in many cases scintillation at VHF persisted longer than that at L band. A longitudinal pattern in ion density irregularity occurrence was observed with peaks over 135–180°E and 270–300°E. The likelihood of ion density irregularity occurrence decreased with increasing altitude. Analysis of C/NOFS zonal ion drift velocities showed that the largest nighttime and daytime drifts were in 270–300°E and 300–330°E longitude regions respectively. Zonal irregularity drift velocities over East Africa were for the first time estimated from L-band scintillation indices. The results show that the velocity of plasma density irregularities in 2011 and 2012 varied daily, and hourly in the range of 50–150 m s?1. The zonal drift velocity estimates from the L-band scintillation indices had good positive correlation with the zonal drift velocities derived from VHF receivers by the spaced receiver technique. 相似文献
28.
Guoqi Liu Wengeng Huang Hua Shen Jiancun Gong 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
GPS-derived vertical TEC recorded at Xiamen (24.5°N, 118.1°E, geomagnetic latitude 13.2°N), China, during year 2006 is analyzed for the first time and compared to that predicted by ionosphere model SPIM recommend by ISO. A manifest seasonal anomaly is found with the high value during equinoctial season and low value during summer and winter season. Relative standard deviation for VTEC shows high value at around midnight and before sunrise. The correlation analysis exhibits that the variation of VTEC has a very weak relation with geomagnetic and solar activities (Dst, AP, SSN and F10.7). Comparative results reveal that the SPIM overestimates the observed VTEC at most of the time. 相似文献
29.
A.V. Mikhalev Jiyao Xu V.I. Degtyarev Wei Yuan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Analysing the initial mid-latitude aurora phase during strong geomagnetic storms we found that the initial phase of the mid-latitude aurorae observed at 630 nm emission during the strong geomagnetic storms on March 24, 1991, April 6, 2000, October 30 and November 20, 2003 is characterized by a short (∼1 h) wave-like disturbance. This disturbance corresponds to the beginning of main phase of the magnetic storms. The marked effect of the mid-latitude aurorae is analyzed using data on magnetosphere and ionosphere conditions in observation periods. The features of the dynamics of the 630 nm emission intensity and its connection with the dynamics of magnetospheric–ionospheric structures are considered. Possible excitation mechanisms of the atomic oxygen emission (630 nm) during these disturbances are discussed. 相似文献
30.
以太阳活动低年冬季为代表,利用二维中低纬电离层理论模式模拟低纬电离层f0F2夜间增强现象,探索在赤道异常驼峰纬度附近形成该现象的可能因素或物理机制,模式在给定磁子午面内解等离子体输运方程,给出电子及各离子的浓度,速度的时空分布。在所考察条件下,低纬驼峰纬度附近f0F2模式值夜间出现了明显的增强特征。 相似文献