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Magnetospheric response of two types in PSc geomagnetic pulsations to interaction with interplanetary shock waves

Vladimir A. ParkhomovPolar Geophysical Institute, Apatity, Russia,Vladimir ParhomovBaikal State UniversityN. L. BorodkovaИнститут космических исследований РАНNatalia L. BorodkovaPolar Geophysical Institute, Apatity, Russia,A. G. IakhninПолярный геофизический институтAleksandr YahninPolar Geophysical InstituteTero RaitaBaikal State University, Irkutsk, Russia,Б. ЦэгмэдИнститут астрономии и геофизики АН МонголииСергей ХомутовInstitute of Astronomy and Geophysics AS Mongolia, Ulaanbaatar, Mongolia,Sergey KhomutovInstitute of Astronomy and Geophysics AS Mongolia, Ulaanbaatar, Mongolia,Александр ПашининInstitute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia,Александр ПашининPolar Geophysical Institute, Apatity, Russia,Виталий ЧиликинInstitute of Cosmophysical Research and Radio Wave Propa-gation FEB RAS, Paratunka, Kamchatskii Krai, Russia,Vitaliy ChilikinBaikal State UniversityАлексей МочаловPolar Geophysical Institute, Apatity, Russia,Aleksey MochalovInstitute of Astronomy and Geophysics AS Mongolia, Ulaanbaatar, Mongolia,
2018en
ABI

Annotatsiya

Using the June 22, 2015 event as an example, we present new data confirming the presence of a precursor of the sudden magnetic impulse caused by a powerful interplanetary shock wave (ISW). The precursor in the form of a train of oscillations (broadband pulse) with a falling frequency in the range 0.25÷11 Hz with a duration of ~20 s, which had a spectral resonance structure, was recorded globally by a network of induc-tion magnetometers at 18:33:27 UT. No significant phase delays of the signals were detected in four fre-quency bands at widely spaced observatories. It is sug-gested that the impulse can be excited in the Earth — ionosphere waveguide by a pulsed electric field which occurs in the ionosphere due to the short-term impact of ISW on the magnetosphere.

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