Search Results - "Lysak, R. L."

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  1. 1

    Poynting Fluxes, Field‐Aligned Current Densities, and the Efficiency of the Io‐Jupiter Electrodynamic Interaction by Sulaiman, A. H., Szalay, J. R., Clark, G., Allegrini, F., Bagenal, F., Brennan, M. J., Connerney, J. E. P., Hue, V., Kurth, W. S., Lysak, R. L., Nichols, J. D., Saur, J., Bolton, S. J.

    Published in Geophysical research letters (28-05-2023)
    “…Juno's highly inclined orbits provide opportunities to sample high‐latitude magnetic field lines connected to the orbit of Io, among the other Galilean…”
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    Io's Near‐Field Alfvén Wings and Local Electron Beams Inferred From Juno/Waves by Sulaiman, A. H., Kurth, W. S., Connerney, J. E. P., Elliott, S. S., Hospodarsky, G. B., Kruegler, N. S., Lysak, R. L., Menietti, J. D., Szalay, J. R., Allegrini, F., Bolton, S. J.

    Published in Geophysical research letters (16-08-2024)
    “…Juno conducted two close Io flybys on 30 December 2023 and 03 February 2024, both at a minimum altitude of 1,500 km. Filamentary structures in the electric and…”
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    Alfvénic Dynamics and Fine Structuring of Discrete Auroral Arcs: Swarm and e‐POP Observations by Miles, D. M., Mann, I. R., Pakhotin, I. P., Burchill, J. K., Howarth, A. D., Knudsen, D. J., Lysak, R. L., Wallis, D. D., Cogger, L. L., Yau, A. W.

    Published in Geophysical research letters (28-01-2018)
    “…The electrodynamics associated with dual discrete arc aurora with antiparallel flow along the arcs were observed nearly simultaneously by the enhanced Polar…”
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    Propagation of Pi2 pulsations in a dipole model of the magnetosphere by Lysak, R. L., Song, Y., Sciffer, M. D., Waters, C. L.

    “…Localized fast flows that impinge on the inner magnetosphere from the plasma sheet are observed to oscillate on time scales of minutes. The compression ahead…”
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    Propagation of kinetic Alfvén waves in the ionospheric Alfvén resonator in the presence of density cavities by Lysak, R. L., Song, Y.

    Published in Geophysical research letters (01-10-2008)
    “…Recent observations of particle distributions that are narrow in pitch angle and broad in energy have suggested that kinetic Alfvén waves are a significant…”
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  7. 7

    Ultra-low frequency wave coupling in the ionospheric Alfvén resonator: Characteristics and implications for the interpretation of ground magnetic fields by Woodroffe, J. R., Lysak, R. L.

    “…In cold magnetospheric plasmas, ultra‐low frequency (ULF) waves occur in either the Alfvén or magnetosonic mode. Owing to the strong inhomogeneity of the…”
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  8. 8

    Magnetosphere-ionosphere coupling by Alfvén waves at midlatitudes by Lysak, R. L.

    “…Numerical modeling of magnetosphere‐ionosphere coupling by Alfvén waves has proven to be a valuable tool in describing the propagation and evolution of…”
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    Field Line Resonances in Jupiter's Magnetosphere by Lysak, R. L., Song, Y.

    Published in Geophysical research letters (28-09-2020)
    “…The arrival of the Juno satellite at Jupiter has led to an increased interest in the dynamics of the Jovian magnetosphere. Jupiter's auroral emissions often…”
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    Propagation of Alfvén waves in the magnetotail during substorms by LYSAK, R. L, SONG, Y, JONES, T. W

    Published in Annales geophysicae (1988) (18-05-2009)
    “…Recent observations from the THEMIS mission have focused attention on the timing of events in the magnetotail during magnetospheric substorms and other periods…”
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  12. 12

    On the coupling of fast and shear Alfvén wave modes by the ionospheric Hall conductance by Waters, C. L., Lysak, R. L., Sciffer, M. D.

    Published in Earth, planets, and space (01-01-2013)
    “…There are two low frequency, magnetised, cold plasma wave modes that propagate through the Earth’s magnetosphere. These are the compressional (fast) and the…”
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  13. 13

    Kinetic Alfvén waves and auroral particle acceleration: a review by Lysak, R. L.

    Published in Reviews of modern plasma physics (01-01-2023)
    “…Shear mode Alfvén waves are the carriers of field-aligned currents in the auroral zones of Earth and other planets. These waves travel along the magnetic field…”
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  14. 14

    A Numerical Model for the Interaction of Io‐Generated Alfvén Waves With Jupiter's Magnetosphere and Ionosphere by Lysak, R. L., Sulaiman, A. H., Bagenal, F., Crary, F.

    “…The interaction of Io with the corotating magnetosphere of Jupiter is known to produce Alfvén wings that couple the moon to Jupiter's ionosphere. We present…”
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    Io-Jupiter interaction: Alfvén wave propagation and ionospheric Alfvén resonator by Su, Yi-Jiun, Jones, S. T., Ergun, R. E., Bagenal, F., Parker, S. E., Delamere, P. A., Lysak, R. L.

    “…A linear, one‐dimensional gyrofluid code has been used to determine the characteristics of propagating Alfvén waves and the ionospheric Alfvén resonator on a…”
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  16. 16

    Statistical study of substorm timing sequence by Lin, Naiguo, Frey, H. U., Mende, S. B., Mozer, F. S., Lysak, R. L., Song, Y., Angelopoulos, V.

    “…Observations of timing sequences of substorms expected in various onset mechanisms are examined by using a space‐time diagram, which correlates observed space…”
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    S bursts and the Jupiter ionospheric Alfvén resonator by Ergun, R. E., Su, Y.-J., Andersson, L., Bagenal, F., Delemere, P. A., Lysak, R. L., Strangeway, R. J.

    “…This article explores a possible relationship between S bursts and trapped Alfvén waves in Jupiter's upper ionosphere. Eigenmodes of inertial Alfvén waves in…”
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    The Jovian Ionospheric Alfvén Resonator and Auroral Particle Acceleration by Lysak, R. L., Song, Y., Elliott, S., Kurth, W., Sulaiman, A. H., Gershman, D.

    “…The ionospheric Alfvén resonator (IAR) is a structure formed by the rapid decrease in the plasma density above a planetary ionosphere. This results in a…”
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  19. 19

    A mechanism of the auroral substorm expansion onset: electric discharge in the double layer by Song, Yan, Lysak, R. L.

    Published in Frontiers in astronomy and space sciences (15-11-2023)
    “…Magnetospheric substorms often occur when a significant amount of energy from the solar wind is deposited and stored in the magnetotail during the growth phase…”
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  20. 20

    Numerical Investigations of Interhemispheric Asymmetry due to Ionospheric Conductance by Lysak, R. L., Song, Y., Waters, C. L., Sciffer, M. D., Obana, Y.

    “…Due to differences in solar illumination, a geomagnetic field line may have one foot point in a dark ionosphere while the other ionosphere is in daylight. This…”
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