Electromagnetic induction effects by the solar quiet magnetic field at satellite altitude
We show that magnetic fields induced by a near‐earth ionospheric source can produce, at a satellite altitude of 400 km, an induced magnetic anomaly field with an amplitude of 2–3 nT at dawn and dusk local times and 3–4 nT at noon local time. Our results are based on an earth model which has an upper...
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Published in: | Geophysical research letters Vol. 27; no. 24; pp. 4009 - 4012 |
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Main Authors: | , |
Format: | Journal Article |
Language: | English |
Published: |
Washington, DC
Blackwell Publishing Ltd
15-12-2000
American Geophysical Union |
Subjects: | |
Online Access: | Get full text |
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Summary: | We show that magnetic fields induced by a near‐earth ionospheric source can produce, at a satellite altitude of 400 km, an induced magnetic anomaly field with an amplitude of 2–3 nT at dawn and dusk local times and 3–4 nT at noon local time. Our results are based on an earth model which has an upper 4 km thick shell with a laterally varying electrical conductivity representing the distribution of continents and oceans. The upper shell overlies a one‐dimensional mantle with a radially varying electrical conductivity. In some regions, the induced anomaly field does not change sign between dawn and dusk and appears static when sampled by a satellite such as MAGSAT. This induced anomaly field could explain some of the weak oceanic static anomalies observed in satellite global magnetic anomaly maps. |
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Bibliography: | ark:/67375/WNG-VBQJ4GS5-2 istex:7B3BEC4D7741F4A0C8F90B5B929DB5B4D03F86F0 ArticleID:1999GL011249 |
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1029/1999GL011249 |