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  Analysis of the Sporadic-E Layer Behavior in Different American Stations during the Days around the September 2017 Geomagnetic Storm

Resende Chagas, L. C., Zhu, Y., Arras, C., Denardini, C. M., Chen, S. S., Moro, J., Barros, D., Chagas, R. A. J., Da Silva, L. A., Andrioli, V. F., Marchezi, J. P., Carrasco, A. J., Wang, C., Li, H., Liu, Z. (2022): Analysis of the Sporadic-E Layer Behavior in Different American Stations during the Days around the September 2017 Geomagnetic Storm. - Atmosphere, 13, 10, 1714.
https://doi.org/10.3390/atmos13101714

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Resende Chagas, Laysa Cristina1, Author
Zhu, Yajun1, Author
Arras, Christina2, Author              
Denardini, Clezio M.1, Author
Chen, Sony S.1, Author
Moro, Juliano1, Author
Barros, Diego1, Author
Chagas, Ronan A. J.1, Author
Da Silva, Lígia A.1, Author
Andrioli, Vânia F.1, Author
Marchezi, José P.1, Author
Carrasco, Alexander J.1, Author
Wang, Chi1, Author
Li, Hui1, Author
Liu, Zhengkuan1, Author
Affiliations:
1External Organizations, ou_persistent22              
21.1 Space Geodetic Techniques, 1.0 Geodesy, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_146025              

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 Abstract: The development of sporadic-E (Es) layers over five Digisonde stations in the American sector is analyzed. This work aims to investigate the dynamic of such layers during the days around the geomagnetic storm that occurred on 8 September 2017. Therefore, a numerical model (MIRE) and Radio Occultation (RO) technique are used to analyze the E layer dynamics. The results show a downward movement in low-middle latitudes due to the wind components that had no significant changes before, during, and after the geomagnetic storm. In fact, our data and simulations showed weak Es layers over Boulder, Cachoeira Paulista, and Santa Maria, even though the winds were not low. However, the RO data show the terdiurnal and quarterdiurnal influence in the Es layer formation, which can explain this behavior. In addition, we observed an atypical Es layer type, slant Es layer (Ess), during the main phase of the magnetic storm over Boulder. The possible cause of the Ess layers was gravity waves. Another interesting point is the spreading Es layer occurrence associated with the Kelvin–Helmholtz Instability (KHI). Finally, it is confirmed that the disturbed electric field only influenced the Es layer dynamics in regions near the magnetic equator.

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 Dates: 2022-10-182022
 Publication Status: Finally published
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 Identifiers: DOI: 10.3390/atmos13101714
GFZPOF: p4 T1 Atmosphere
OATYPE: Gold Open Access
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Title: Atmosphere
Source Genre: Journal, SCI, Scopus, oa
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Pages: - Volume / Issue: 13 (10) Sequence Number: 1714 Start / End Page: - Identifier: CoNE: https://gfzpublic.gfz-potsdam.de/cone/journals/resource/191024
Publisher: MDPI