2020
DOI: 10.1007/978-3-030-10475-7_156-1
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Electromagnetic Pulsations and Magnetic Storms

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“…They noted a clear ULF wave perturbation with period ∼5 minutes triggered by the frontal shock, but such response was not clearly seen in either of the inclined shocks, even in the case of the strong inclined shock impact. Oliveira and Raeder (2014) attributed this effect to an effective excitation of cavity modes (Samson et al, 1992;Hughes, 1994;Lakhina and Tsurutani, 2020) in the magnetosphere-ionosphere system by the symmetric compression caused by the frontal shock. The inclined shocks, on the other hand, were not able to trigger these cavity modes due to the asymmetric magnetospheric compressions.…”
Section: Ultra-low Frequency Wavesmentioning
confidence: 99%
“…They noted a clear ULF wave perturbation with period ∼5 minutes triggered by the frontal shock, but such response was not clearly seen in either of the inclined shocks, even in the case of the strong inclined shock impact. Oliveira and Raeder (2014) attributed this effect to an effective excitation of cavity modes (Samson et al, 1992;Hughes, 1994;Lakhina and Tsurutani, 2020) in the magnetosphere-ionosphere system by the symmetric compression caused by the frontal shock. The inclined shocks, on the other hand, were not able to trigger these cavity modes due to the asymmetric magnetospheric compressions.…”
Section: Ultra-low Frequency Wavesmentioning
confidence: 99%