Assessment of the auroral electrojet index performance under various geomagnetic conditions
Assessment of the auroral electrojet index performance under various geomagnetic conditions
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DOI:
10.1016/j.jastp.2012.09.017
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发表时间:
2013
影响因子:
1.9
通讯作者:
K. Liou;Kazue Takahashi;B. Anderson;M. Nosé;T. Iyemori
中科院分区:
文献类型:
--
作者:
K. Liou;Kazue Takahashi;B. Anderson;M. Nosé;T. Iyemori
Saturation of the auroral electrojet (AE) index during storm times is a phenomenon that has been known but not fully understood. To address this puzzle, here we correlate the (provisional) AE index with net field-aligned current (Net-dB) index, which is a data product derived with magnetic field measurements from the Iridium satellite constellation (Anderson et al., 2010), with an assumption that AE is largely measuring convection driven by the field-aligned currents represented by the Net-dB index. The Net-dB index has a time resolution of ∼45min and is currently available from February 18, 1999, to May 31, 2008. It is found that, for the entire data period, there is a good linear correlation (r=0.74) between the AE index, when averaging over the Net-dB index time grids, and the Net-dB index, suggesting that statistically ∼55% of the ionospheric Hall currents correlate with large scale convection as reflected in the field-aligned currents. It is also found that the correlation decreases during storm times, with a clear decreasing trend toward a more negative Sym-H. For large storms (Sym-H<−100nT), the correlation becomes weak (r<0.4). Two correlation peaks are identified: a major peak (r=0.73) occurring at Sym-H>30nT and a secondary peak (r=0.66) at Sym-H∼−50 to −30nT. A further study shows that the variations of the AE–Net-dB correlation are associated with the location of the field-aligned currents into and out of the ionosphere relative to the ground magnetometer stations, as expected often but not demonstrated in the past.