Characteristics of counter-Sq SFE (SFE*) at the dip equator CPMN stations

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Ionosphere: Solar Radiation And Cosmic Ray Effects, Ionosphere: Equatorial Ionosphere, Ionosphere: Current Systems (2721), Ionosphere: Electric Fields (2712), Ionosphere: Ionosphere/Magnetosphere Interactions (2736)

Scientific paper

The solar flare effect (SFE) at dip equatorial latitudes sometimes shows the counter-S q variation around local noon. In this paper, we refer to this type of SFE as SFE*. Observations obtained by the Circum-pan Pacific Magnetometer Network (CPMN) reveal some previously unknown characteristics of SFE*. Some of these features are the following: (1) the counter-S q SFE variation is observed in limited longitude (local time) and latitude sectors (i.e., LT ≈ 1030-1300, ∣DipLat.∣ $\lesssim$ 1.5°), (2) outside this limited region, the amplitude of SFE(H) and preflare S q (H) have a linear relationship, and (3) SFE* is observed during the significant depression of the horizontal magnetic field at dip equatorial latitudes, which indicates the presence of westward electric fields whose origin remains to be understood.

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