Solar-Terrestrial Physics (Sep 2018)

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

  • Parkhomov V.A.,
  • Borodkova N.L.,
  • Yahnin A.G.,
  • Tero Raita,
  • Tsegmed B.,
  • Khomutov S.Yu.,
  • Pashinin A.Yu.,
  • Chilikin V.E.,
  • Mochalov A.A.

DOI
https://doi.org/10.12737/stp-43201808
Journal volume & issue
Vol. 4, no. 3
pp. 52 – 66

Abstract

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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 induction magnetometers at 18:33:27 UT. No significant phase delays of the signals were detected in four frequency bands at widely spaced observatories. It is suggested 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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