Comparison of ionospheric characteristic parameters obtained by GPS and ionosonde with IRI model over China

被引:6
作者
Wang, Cheng [1 ,2 ]
机构
[1] Collaborat Innovat Ctr Geospatial Informat Techno, 129 Luoyu Rd, Wuhan 430079, Peoples R China
[2] Wuhan Univ, GNSS Res Ctr, 129 Luoyu Rd, Wuhan 430079, Peoples R China
基金
中国国家自然科学基金;
关键词
TEC; NmF2; hmF2; GPS; IRI model; IRI2012; TOTAL ELECTRON-CONTENT; F-REGION; DENSITY; TEC; PREDICTIONS;
D O I
10.1007/s12040-016-0694-x
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
This paper presents a comparison of ionospheric characteristic parameters obtained by a GPS network and three ionosondes at Mohe (122.4 degrees E, 53 degrees 5. N, dip angle 70.983 degrees N), Zuolingzhen (114.6 degrees E, 30.5 degrees N, dip angle 46.350 degrees N), and Fuke (109.1 degrees E, 19.5 degrees N, dip angle 27.083 degrees N) located in China with an IRI model in the year 2011. Observed NmF2 and hmF2 values at the three stations are compared with IRI2007 and IRI2012 predictions, respectively. The results show that there are clear linear correlations between the observed values and the IRI model predicted values. The IRI model gives overestimations at the three stations mostly in 2011. For the NmF2 and hmF2 values, most of the results show that the IRI2012 predicted values are closer to the observed values compared with those of IRI2007. Additionally, the GPS TEC values derived from the Crustal Movement Observation Network of China (CMONOC) are compared with the IRI2012 predictions. From the results, it is evident that the IRI2012 model predictions follow the normal trend of diurnal variation of GPS measured TEC monthly means but do not reproduce the measured data well. The IRI2012 model overestimates electron density in the latter part of spring as well as the first half of autumn and winter and underestimates electron density in early spring and the latter part of autumn. Referring to GPS TEC, the precision of the IRI2012 model predicted TEC values is similar to 5 TECU over China. It may also be noted that there are two discontinuities of IRI-TEC monthly means appearing in November and December of the year 2011. This brings a bias of similar to 3 TECU of TEC values between two adjacent months.
引用
收藏
页码:745 / 759
页数:15
相关论文
共 42 条
[1]   An overview of IRI-observational data comparison in American (Brazilian) sector low latitude ionosphere [J].
Abdu, MA ;
Batista, IS ;
deSouza, JR .
LOW AND EQUATORIAL LATITUDES IN THE INTERNATIONAL REFERENCE IONOSPHERE (IRI), 1996, 18 (06) :13-22
[2]   Equatorial F2-peak parameters in the IRI model [J].
Adeniyi, JO ;
Bilitza, D ;
Radicella, SM ;
Willoughby, AA .
DESCRIPTION OF THE LOW LATITUDE AND EQUATORIAL IONOSPHERE IN THE INTERNATIONAL REFERENCE IONOSPHERE, 2003, 31 (03) :507-512
[3]  
Adewale A. O., 2011, Indian Journal of Radio & Space Physics, V40, P21
[4]   Validation of the STORM response in IRI2000 [J].
Araujo-Pradere, EA ;
Fuller-Rowell, TJ ;
Bilitza, D .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2003, 108 (A3)
[5]  
Bagiya M S, 2009, ANN GEOPHYS
[6]   IRI-2001 model predictions compared with ionospheric data observed at Brazilian low latitude stations [J].
Bertoni, F. ;
Sahai, Y. ;
Lima, W. L. C. ;
Fagundes, P. R. ;
Pillat, V. G. ;
Becker-Guedes, F. ;
Abalde, J. R. .
ANNALES GEOPHYSICAE, 2006, 24 (08) :2191-2200
[7]   TEC derived from GPS network in India and comparison with the IRI [J].
Bhuyan, P. K. ;
Borah, Rashmi Rekha .
ADVANCES IN SPACE RESEARCH, 2007, 39 (05) :830-840
[8]   Diurnal, seasonal and latitudinal variation of electron density in the topside F-region of the Indian zone ionosphere at solar minimum and comparison with the IRI [J].
Bhuyan, PK ;
Chamua, M ;
Bhuyan, K ;
Subrahmanyam, P ;
Garg, SC .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2003, 65 (03) :359-368
[9]   International Reference Ionosphere 2007: Improvements and new parameters [J].
Bilitza, D. ;
Reinisch, B. W. .
ADVANCES IN SPACE RESEARCH, 2008, 42 (04) :599-609
[10]   Variability of foF2 in the equatorial ionosphere [J].
Bilitza, D ;
Obrou, OK ;
Adeniyi, JO ;
Oladipo, O .
IRI: QUANTIFYING IONOSPERIC VARIABILITY, 2004, 34 (09) :1901-1906