Ionosphere modeling in the context of Algerian Satellite-based Augmentation System

2019 ◽  
Vol 193 ◽  
pp. 105092
Author(s):  
Elhadi Takka ◽  
Aichouche Belhadj-Aissa ◽  
Jianguo Yan ◽  
Biao Jin ◽  
Azzedine Bouaraba
Keyword(s):  
2008 ◽  
Vol 60 (11) ◽  
pp. e25-e28 ◽  
Author(s):  
Chang-Ki Hong ◽  
Dorota A. Grejner-Brzezinska ◽  
Jay Hyoun Kwon

Sensors ◽  
2019 ◽  
Vol 19 (13) ◽  
pp. 2947 ◽  
Author(s):  
Zhengxie Zhang ◽  
Shuguo Pan ◽  
Chengfa Gao ◽  
Tao Zhao ◽  
Wang Gao

The distribution of total electron content (TEC) in the ionosphere is irregular and complex, and it is hard to model accurately. The polynomial (POLY) model is used extensively for regional ionosphere modeling in two-dimensional space. However, in the active period of the ionosphere, the POLY model is difficult to reflect the distribution and variation of TEC. Aiming at the limitation of the regional POLY model, this paper proposes a new ionosphere modeling method with combining the support vector machine (SVM) regression model and the POLY model. Firstly, the POLY model is established using observations of regional continuously operating reference stations (CORS). Then the SVM regression model is trained to compensate the model error of POLY, and the TEC SVM-P model is obtained by the combination of the POLY and the SVM. The fitting accuracies of the models are verified with the root mean square errors (RMSEs) and static single-frequency precise point positioning (PPP) experiments. The results show that the RMSE of the SVM-P is 0.980 TECU (TEC unit), which produces an improvement of 17.3% compared with the POLY model (1.185 TECU). Using SVM-P models, the positioning accuracies of single-frequency PPP are improved over 40% compared with those using POLY models. The SVM-P is also compared with the back-propagation neural network combined with POLY (BPNN-P), and its performance is also better than BPNN-P (1.070 TECU).


Author(s):  
Stephen W. Bougher ◽  
Pierre-Louis Blelly ◽  
Michael Combi ◽  
Jane L. Fox ◽  
Ingo Mueller-Wodarg ◽  
...  

2002 ◽  
Vol 20 (6) ◽  
pp. 817-822 ◽  
Author(s):  
N. K. Sethi ◽  
K. K. Mahajan

Abstract. High resolution electron density profiles (Ne) measured with the Arecibo (18.4 N, 66.7 W), Incoherent Scatter radar (I. S.) are used to obtain the bottomside shape parameters B0, B1 for a solar maximum period (1989–90). Median values of these parameters are compared with those obtained from the IRI-2001 model. It is observed that during summer, the IRI values agree fairly well with the Arecibo values, though the numbers are somewhat larger during the daytime. Discrepancies occur during winter and equinox, when the IRI underestimates B0 for the local times from about 12:00 LT to about 20:00 LT. Furthermore, the IRI model tends to generally overestimate B1 at all local times. At Arecibo, B0 increases by about 50%, and B1 decreases by about 30% from solar minimum to solar maximum.Key words. Ionosphere (equational ionosphere; modeling and forecasting)


1992 ◽  
Vol 97 (A6) ◽  
pp. 8591 ◽  
Author(s):  
M. V. Codrescu ◽  
R. G. Roble ◽  
J. M. Forbes
Keyword(s):  

2013 ◽  
pp. 1-40
Author(s):  
Michael Schmidt ◽  
Denise Dettmering ◽  
Florian Seitz
Keyword(s):  
B Spline ◽  

2008 ◽  
Vol 139 (1-4) ◽  
pp. 107-141 ◽  
Author(s):  
Stephen W. Bougher ◽  
Pierre-Louis Blelly ◽  
Michael Combi ◽  
Jane L. Fox ◽  
Ingo Mueller-Wodarg ◽  
...  

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