Data for "Propagation of EMIC Waves from Shabansky Orbits in the Dayside Magnetosphere"

Kim, Eun-Hwa ; Shiraiwa, Syun'ichi ; Johnson, Jay ; Bertelli, Nicola ; Vines, Sarah ; Kim, Khan-Hyuk ; Engebretson, Mark ; Kim, Hyomin ; O'ffill, Carson
Issue date: 2024
Rights:
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND)
Cite as:
Kim, Eun-Hwa, Shiraiwa, Syun'ichi, Johnson, Jay, Bertelli, Nicola, Vines, Sarah, Kim, Khan-Hyuk, Engebretson, Mark, Kim, Hyomin, & O'ffill, Carson. (2024). Data for "Propagation of EMIC Waves from Shabansky Orbits in the Dayside Magnetosphere" [Data set]. Princeton Plasma Physics Laboratory, Princeton University. https://doi.org/10.34770/e3m1-rs25
@electronic{kim_eunhwa_2024,
  author      = {Kim, Eun-Hwa and
                Shiraiwa, Syun'ichi and
                Johnson, Jay and
                Bertelli, Nicola and
                Vines, Sarah and
                Kim, Khan-Hyuk and
                Engebretson, Mark and
                Kim, Hyomin and
                O'ffill, Carson},
  title       = {{Data for "Propagation of EMIC Waves from
                 Shabansky Orbits in the Dayside Magneto
                sphere"}},
  publisher   = {{Princeton Plasma Physics Laboratory, Pri
                nceton University}},
  year        = 2024,
  url         = {https://doi.org/10.34770/e3m1-rs25}
}
Description:

Full-wave simulations of electromagnetic ion cyclotron waves in a non-dipole compressed magnetic field have been conducted using the Petra-M simulation code. The manuscript investigates the effect of misalignment of the Faraday screen and electron density in the scrape-off layer on the excitation and propagation of fast helicon and slow mode waves.

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