摘要
In this paper we present the results of the computation of the electric and magnetic fields produced in the ionosphere by the near-earth seismogenic disturbance in the vertical atmospheric electrostatic field under different ionospheric conditions. It is shown that in the nighttime ionosphere during solar minimum and inside large-scale plasma bubbles, the magnitude of the transverse electric field can attain ∼0.2 and 1.0 mV/m, respectively. The seismomagnetic effect with the magnitude of ∼13 pT is predicted in the topside daytime and nighttime ionosphere at any solar activity.
原文 | ???core.languages.en_GB??? |
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頁(從 - 到) | 1707-1713 |
頁數 | 7 |
期刊 | Advances in Space Research |
卷 | 56 |
發行號 | 8 |
DOIs | |
出版狀態 | 已出版 - 15 10月 2015 |