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JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 112,
A07308,
doi:10.1029/2006JA012240,
2007
Comparison of COSMIC ionospheric measurements with ground-based observations and model predictions: Preliminary results
Jiuhou Lei
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA
Stig Syndergaard
COSMIC Project Office, University Corporation for Atmospheric Research, Boulder, Colorado, USA
Alan G. Burns
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA
Stanley C. Solomon
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA
Wenbin Wang
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA
Zhen Zeng
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA COSMIC Project Office, University Corporation for Atmospheric Research, Boulder, Colorado, USA
Raymond G. Roble
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA
Qian Wu
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA
Ying-Hwa Kuo
COSMIC Project Office, University Corporation for Atmospheric Research, Boulder, Colorado, USA
John M. Holt
Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA
Shun-Rong Zhang
Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA
David L. Hysell
Department of Earth and Atmospheric Science, Cornell University, Ithaca, New York, USA
Fabiano S. Rodrigues
Department of Earth and Atmospheric Science, Cornell University, Ithaca, New York, USA
Chien H. Lin
National Space Organization, Hsinchu, Taiwan
Abstract
Electron densities retrieved from the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) radio
occultation (RO) measurements are compared with those measured by incoherent scatter radars (ISR) and ionosondes in this paper.
These results show that electron density profiles retrieved from COSMIC RO data are in agreement with the ISR and ionosonde
measurements. The ionospheric characteristics (N mF2 and h mF2) derived from the COSMIC satellites are also compared with those calculated by the latest International Reference Ionosphere
model (IRI-2001) and the National Center for Atmospheric Research Thermosphere-Ionosphere-Electrodynamics General Circulation
Model (NCAR-TIEGCM). The comparison of the magnitude of the COSMIC N mF2 data with those calculated by the IRI model and the TIEGCM is good. However, features such as the north-south asymmetry and
longitudinal variation of the equatorial anomaly that are seen in the COSMIC data and the TIEGCM simulations are not fully
present in the IRI model. On the other hand, the TIEGCM produces a stronger winter anomaly than that seen in either the COSMIC
data or the IRI model.
Received 22
December
2006;
accepted 1
May
2007;
published 25
July
2007.
Index Terms: 2487 Ionosphere: Wave propagation (0689, 3285, 4275, 4455, 6934); 2494 Ionosphere: Instruments and techniques; 2447 Ionosphere: Modeling and forecasting; 2437 Ionosphere: Ionospheric dynamics.
Read Full Article (file size: 970916 bytes) Cited by
Citation: Lei, J., et al.
(2007),
Comparison of COSMIC ionospheric measurements with ground-based observations and model predictions: Preliminary results,
J. Geophys. Res.,
112,
A07308,
doi:10.1029/2006JA012240.
Copyright 2007 by the American Geophysical Union.
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