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The impact of solar wind ULF B z fluctuations on geomagnetic activity for viscous timescales during strongly northward and southward IMF
We analyze more than 17 years of OMNI data to statistically quantify the impact of IMF B z fluctuations on AL by using higher‐order moments in the AL ‐distribution as a proxy. For strongly southward interplanetary magnetic field (IMF), the AL distribution function is characterized by a decrease of t...
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Published in: | Journal of geophysical research. Space physics 2015-11, Vol.120 (11), p.9307-9322 |
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Main Authors: | , , , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | We analyze more than 17 years of OMNI data to statistically quantify the impact of IMF
B
z
fluctuations on
AL
by using higher‐order moments in the
AL
‐distribution as a proxy. For strongly southward interplanetary magnetic field (IMF), the
AL
distribution function is characterized by a decrease of the skewness, a shift of its peak from −30 nT to −200 nT, and a broadening of the distribution core. During northward IMF, the distribution of
AL
is characterized by a significant reduction of the standard deviation and weight in the tail. Following this characterization of
AL
for southward and northward IMF, we show that IMF fluctuations enhance the driving on timescales smaller than those of substorms by shifting the peak of the probability distribution function by more than 150 nT during southward IMF, and by narrowing the distribution function by a factor of 2 during northward IMF. For both southward and northward IMF, we demonstrate that high power fluctuations in
B
z
systematically result in a greater level of activity on timescales consistent with viscous processes. Our results provide additional quantitative evidence of the role of the solar wind fluctuations in geomagnetic activity. The methodology presented also provides a framework to characterize short timescale magnetospheric dynamics taking place on the order of viscous timescales
τ
≪ 1 hour.
We quantified the AL response to southward and northward IMF on timescales
τ
≪ 1 h
Changes in AL distribution on viscous timescales are quantified by third‐ and fourth‐order moments
IMF
B
z
fluctuations are found to enhance AL activity for northward and southward IMF |
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ISSN: | 2169-9380 2169-9402 |
DOI: | 10.1002/2015JA021505 |