TY - JOUR
T1 - Empirical orthogonal function analysis and modeling of the ionospheric peak height during the years 2002-2011
AU - Lin, Jian
AU - Yue, Xinan
AU - Zeng, Zhen
AU - Lou, Yidong
AU - Shen, Xuhui
AU - Wu, Yun
AU - Schreiner, William S.
AU - Kuo, Ying Hwa
PY - 2014/5
Y1 - 2014/5
N2 - The ionospheric peak electron density height (hm) is one of the most important ionospheric parameters characterizing high-frequency radio wave propagation conditions. In this paper, a global hm model based on the empirical orthogonal function (EOF) analysis method is constructed by using Global Navigation Satellite Systems ionospheric radio occultation measurements from COSMIC and CHAMP as well as global ionosonde data during the years 2002-2011. The variability of hm can be well represented by the several EOF base functions Ek and the corresponding coefficients Pk. The rapid convergence of EOF decomposition makes it possible to use only the first four EOFs components, which express 99.133% of total variance in this study, to construct the empirical model. The variations of h m with respect to the magnetic latitude, local time, season, and solar cycle have been studied, and the EOF-based hm model has been validated through comparisons with the International Reference Ionosphere (IRI) model and other observation. The evaluations indicate that the EOF and IRI model give better hmF2 at middle and high latitudes than those at low latitudes. Since the limited data were used in the EOF model during high solar activity years, its accuracy degrades to some extent. During nighttime of spring, summer, and winter in the auroral zone, the hm derived from the EOF model may range from 90 to 150 km because of the reduction of h m, which is due to particle precipitation, whereas the IRI model does not include this reduction. During the periods of low solar activity, the F2 peak heights (hmF2) from the EOF model are in good agreement with the observed data, while the IRI model tends to overestimate the hmF2 in the middle and high latitudes. Key Points A global hm model has been constructed by EOF analysis using observed data The hm model can capture the main features with only a few EOF series The hm model agrees better with the observed data than IRI model
AB - The ionospheric peak electron density height (hm) is one of the most important ionospheric parameters characterizing high-frequency radio wave propagation conditions. In this paper, a global hm model based on the empirical orthogonal function (EOF) analysis method is constructed by using Global Navigation Satellite Systems ionospheric radio occultation measurements from COSMIC and CHAMP as well as global ionosonde data during the years 2002-2011. The variability of hm can be well represented by the several EOF base functions Ek and the corresponding coefficients Pk. The rapid convergence of EOF decomposition makes it possible to use only the first four EOFs components, which express 99.133% of total variance in this study, to construct the empirical model. The variations of h m with respect to the magnetic latitude, local time, season, and solar cycle have been studied, and the EOF-based hm model has been validated through comparisons with the International Reference Ionosphere (IRI) model and other observation. The evaluations indicate that the EOF and IRI model give better hmF2 at middle and high latitudes than those at low latitudes. Since the limited data were used in the EOF model during high solar activity years, its accuracy degrades to some extent. During nighttime of spring, summer, and winter in the auroral zone, the hm derived from the EOF model may range from 90 to 150 km because of the reduction of h m, which is due to particle precipitation, whereas the IRI model does not include this reduction. During the periods of low solar activity, the F2 peak heights (hmF2) from the EOF model are in good agreement with the observed data, while the IRI model tends to overestimate the hmF2 in the middle and high latitudes. Key Points A global hm model has been constructed by EOF analysis using observed data The hm model can capture the main features with only a few EOF series The hm model agrees better with the observed data than IRI model
KW - Ionosphere
KW - Modeling
UR - https://www.scopus.com/pages/publications/84902449349
U2 - 10.1002/2013JA019626
DO - 10.1002/2013JA019626
M3 - Article
AN - SCOPUS:84902449349
SN - 2169-9380
VL - 119
SP - 3915
EP - 3929
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 5
ER -