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Ionospheric Equatorial Anomaly Studies During Solar Storms (2005)
| Content Provider | CiteSeerX |
|---|---|
| Author | Oliveira, Re B. V. Walter, F. |
| Description | The ionosphere is the major error source in GNSS receivers. Models for single frequency time delay correction do not work at low geomagnetic latitude regions (±20º), where the ionosphere has a peculiar behavior, known as the Ionospheric Equatorial Anomaly. In order to study the global behavior of the Ionospheric Equatorial Anomaly, dynamic maps based on IONEX data have been generated. These maps allow to study the Vertical Total Electron Content behavior since January, 1999. They also show the Kp values, Sun Spot Number, and Solar Flux. In this way the effects of the solar and geomagnetic activity on the Ionospheric Equatorial Anomaly can be studied. |
| File Format | |
| Language | English |
| Publisher Date | 2005-01-01 |
| Publisher Institution | In: Union Radio-Scientifique Internationale International Union of Radio Science (URSI), Nova |
| Access Restriction | Open |
| Subject Keyword | Kp Value Low Geomagnetic Latitude Region Vertical Total Electron Content Behavior Single Frequency Time Delay Correction Solar Flux Sun Spot Number Solar Storm Peculiar Behavior Gnss Receiver Major Error Source Ionospheric Equatorial Anomaly Ionex Data Ionospheric Equatorial Anomaly Study Global Behavior Geomagnetic Activity Dynamic Map |
| Content Type | Text |
| Resource Type | Article |
