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| Content Provider | Springer Nature Link |
|---|---|
| Author | Sedykh, Pavel A. Pomarev, Evgenij A. |
| Copyright Year | 2012 |
| Abstract | The structurally adequate model of the geomagnetosphere consists of the following modules: A. Bow shock as a source of power for magnetospheric processes. B. The generation of magnetospheric convection. C. The plasma pressure distribution in the magnetosphere and electron-proton precipitations into the ionosphere. D. The magnetosphere-ionosphere coupling. Field-aligned currents. Essentially, each module presented in an analytical form is a model of a particular process described in physical terms. It has an input and output to couple with other modules. When combined, the modules comprise a single large physically adequate model describing a phenomenon in such a way that we understand its essence and contribution of each physical process into the overall picture. |
| Starting Page | 1079 |
| Ending Page | 1093 |
| Page Count | 15 |
| File Format | |
| ISSN | 00393169 |
| Journal | Studia Geophysica et Geodaetica |
| Volume Number | 56 |
| Issue Number | 4 |
| e-ISSN | 15731626 |
| Language | English |
| Publisher | Springer Netherlands |
| Publisher Date | 2012-09-22 |
| Publisher Place | Dordrecht |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | solar wind bow shock convection of plasma magnetosphereionosphere coupling Geophysics/Geodesy Structural Geology Meteorology/Climatology |
| Content Type | Text |
| Resource Type | Article |
| Subject | Geochemistry and Petrology Geophysics |
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