The IMF impact on the ULF oscillations in the magnetospheric polar cusps
Ultra-low-frequency (ULF) oscillations of the magnetospheric cusps are observed permanently in the near-mid sector of auroral oval in the form of so-called IPCL. In this paper, we posed the question: do electromagnetic waves incident on cusp from the foreshock (it is a special region of cosmic plasm...
Main Authors: | , |
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Format: | Report |
Language: | unknown |
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arXiv
2018
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Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.1805.02256 https://arxiv.org/abs/1805.02256 |
Summary: | Ultra-low-frequency (ULF) oscillations of the magnetospheric cusps are observed permanently in the near-mid sector of auroral oval in the form of so-called IPCL. In this paper, we posed the question: do electromagnetic waves incident on cusp from the foreshock (it is a special region of cosmic plasma existing before the front of the magnetosphere) affect the IPCL regime? We have proposed a method of experimental investigation, which is based on the idea of the foreshock position dependence on the interplanetary magnetic field (IMF) orientation. A hypothesis has been put forward on the existence of a specific effect of the IPCL north-south asymmetry. We tested our hypothesis using IPCL observation data from the Hornsund (Spitsbergen) and Davis (Antarctica) observatories. We found confirmation of the hypothesis at a high confidence level of statistical significance. Keywords: magnetosphere, ultra-low-frequency oscillations, north-south asymmetry. : 9 pages, 2 figures |
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