Artigo Revisado por pares

High‐latitude ionospheric equivalent currents during strong space storms: Regional perspective

2014; American Geophysical Union; Volume: 13; Issue: 1 Linguagem: Inglês

10.1002/2014sw001139

ISSN

1542-7390

Autores

Liisa Juusola, A. Viljanen, Max van de Kamp, E. I. Tanskanen, Heikki Vanhamäki, Noora Partamies, Kirsti Kauristie,

Tópico(s)

Geomagnetism and Paleomagnetism Studies

Resumo

Abstract Geomagnetically induced currents (GIC) are a space weather phenomenon that can interfere with power transmission and even cause blackouts. The primary drivers of GIC can be represented as ionospheric equivalent currents. We used International Monitor for Auroral Geomagnetic Effects (IMAGE) magnetometer data from 1994–2013 to analyze the extreme behavior of the time derivative of the equivalent current density (|Δ J eq |/Δ t ) together with the occurrence of modeled GIC in the European high‐voltage power grids (1996–2008). Typically, when intense |Δ J eq |/Δ t occurred, geomagnetic activity extended to latitudes <60°, K p ≥ 8, and modeling suggested large GIC in the European high‐voltage power grids. Intense, although short‐lived, |Δ J eq |/Δ t also occurred when geomagnetic activity was confined to latitudes >60°. In such cases, typically 5≤ K p <8, and modeling suggested that there were no large GIC in the European high‐voltage power grids. Intense |Δ J eq |/Δ t and GIC occurred preferentially before midnight or at dawn and were rare after noon. There was a seasonal peak in October and a minimum around midsummer. Intense |Δ J eq |/Δ t and GIC occurred preferentially in the declining phase of the solar cycle and were rare around solar minima. A longer perspective (1975–2013) was obtained by comparison with the time derivative of the magnetic field from the IMAGE station Nurmijärvi (NUR, MLAT ∼57°). NUR data indicated that the quietness of summer months may have been due to a coincidental lack of intense storms during the shorter period. NUR data agreed with the increased activity in the declining phase but demonstrated that extreme events could also occur during solar minima.

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