Why can the auroral-type sporadic E layer be detected over the South America Magnetic Anomaly (SAMA) region? An investigation of a case study under the influence of the high-speed solar wind stream

Why can the auroral-type sporadic E layer be detected over the South America Magnetic Anomaly (SAMA) region? An investigation of a case study under the influence of the high-speed solar wind stream

The low-electron flux variability (increase/decrease) in the Earth’s radiation belts could cause low-energy Electron Precipitation (EP) to the atmosphere over auroral and South American Magnetic Anomaly (SAMA) regions. This EP into the atmosphere can cause an extra upper atmosphere’s ionization, for...

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Bibliographic Details
Main Authors: L. A. Da Silva, J. Shi, L. E. Vieira, O. V. Agapitov, L. C. A. Resende, L. R. Alves, D. Sibeck, V. Deggeroni, J. P. Marchezi, S. Chen, J. Moro, C. Arras, C. Wang, V. F. Andrioli, H. Li, Z. Liu
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-11-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
inner radiation belt
South America Magnetic Anomaly
auroral-type sporadic E-layers
particle precipitation
hiss waves
pitch angle scattering
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2023.1197430/full

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https://www.frontiersin.org/articles/10.3389/fspas.2023.1197430/full

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