Equatorial ionospheric electrodynamics during solar flares

• Autores: Zhang, Ruilong, Liu, Libo, Le, Huijun, Chen, Yiding
• Formato: artículo
• Fecha de Publicación: 2017
• Institución: Instituto Geofísico del Perú
• Repositorio: IGP-Institucional
• Lenguaje: inglés
• OAI Identifier: oai:repositorio.igp.gob.pe:20.500.12816/3784
• Enlace del recurso: http://hdl.handle.net/20.500.12816/3784; https://doi.org/10.1002/2017GL073238
• Nivel de acceso: acceso abierto
• Materia: EEJ; EIA; Equatorial electric field; Solar flare; http://purl.org/pe-repo/ocde/ford#1.05.01

Previous investigations on ionospheric responses to solar flares focused mainly on the photoionization caused by the increased X‐rays and extreme ultraviolet irradiance. However, little attention was paid to the related electrodynamics. In this letter, we explored the equatorial electric field (EEF) and electrojet (EEJ) in the ionosphere at Jicamarca during flares from 1998 to 2008. It is verified that solar flares increase dayside eastward EEJ but decrease dayside eastward EEF, revealing a negative correlation between EEJ and EEF. The decreased EEF weakens the equatorial fountain effect and depresses the low‐latitude electron density. During flares, the enhancement in the Cowling conductivity may modulate ionospheric dynamo and decrease the EEF. Besides, the decreased EEF is closely related to the enhanced ASY‐H index that qualitatively reflects Region 2 field‐aligned current (R2 FAC). We speculated that solar flares may also decrease EEF through enhancing R2 FAC that leads to an overshielding‐like effect.