Intensity of the auroral electrojets during a recovery phase of magnetic storm
| Autor: | R.N. Boroyev |
|---|---|
| Rok vydání: | 2016 |
| Předmět: |
Geomagnetic storm
Atmospheric Science 010504 meteorology & atmospheric sciences Aerospace Engineering Electrojet Astronomy and Astrophysics Storm Atmospheric sciences 01 natural sciences Physics::Geophysics Intensity (physics) Solar wind Geophysics Space and Planetary Science Electric field Physics::Space Physics 0103 physical sciences Coronal mass ejection Astrophysics::Solar and Stellar Astrophysics General Earth and Planetary Sciences Environmental science Ionosphere 010303 astronomy & astrophysics Physics::Atmospheric and Oceanic Physics 0105 earth and related environmental sciences |
| Zdroj: | Advances in Space Research. 57:2479-2486 |
| ISSN: | 0273-1177 |
| DOI: | 10.1016/j.asr.2016.04.001 |
| Popis: | In this work, the effect of solar wind velocity on the development of magnetospheric and ionospheric disturbances is studied. It is shown that at high velocity of the solar wind during a recovery phase of magnetic storm the strong auroral activity characterized by the AE index is observed. In some cases during a recovery phase of magnetic storm the value of AE index is practically comparable with the value of AE index observed during the main phase of magnetic storm. When comparing time intervals of two magnetic storms during which the values of solar wind electric fields are approximately equal to each other, it is found that auroral electrojet intensity is stronger in that storm in which the solar wind velocity is higher. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
|
Full Text from ScienceDirect