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| Content Provider | Springer Nature Link |
|---|---|
| Author | Botova, M. G. Namgaladze, A. A. Prokhorov, B. E. |
| Copyright Year | 2013 |
| Abstract | The results of numerical modeling by using the global upper atmosphere model of the Earth (UAM) for reproducing the peak F2 layer electron density (N $_{ m }$F2) and total electron content (TEC) during recovery period after the magnetic storm of the April 15–20, 2002 are discussed. According to the simulations, the time it takes to reach a stationary regime of N $_{ m }$F2 and TEC diurnal variations is 24 hours, much shorter then the plasmasphere refilling time. The results are compared with the predictions of the IRI-2007 empirical model and GPS data on the TEC and found in good quantitative agreement for the latitudinal variations of N $_{ m }$F2 and TEC for daytime conditions in the southern hemisphere. The worst agreement occurs in the region of the main ionospheric trough. |
| Starting Page | 606 |
| Ending Page | 610 |
| Page Count | 5 |
| File Format | |
| ISSN | 19907931 |
| Journal | Russian Journal of Physical Chemistry B |
| Volume Number | 7 |
| Issue Number | 5 |
| e-ISSN | 19907923 |
| Language | English |
| Publisher | Springer US |
| Publisher Date | 2013-11-07 |
| Publisher Place | Boston |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | total electron content peak F2-layer electron density GPS Physical Chemistry |
| Content Type | Text |
| Resource Type | Article |
| Subject | Physical and Theoretical Chemistry |
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