@article{3017978,
    title = "Quasi-periodic emissions (15- 80 min ) from the poles of Jupiter as a principal source of the large-scale high-latitude magnetopause boundary layer of energetic particle",
    author = "Karanikola, I. and Athanasiou, M. and Anagnostopoulos, G.C. and Pavlos, G.P. and Preka-Papadema, P.",
    journal = "Planetary and Space Science",
    year = "2004",
    volume = "52",
    number = "5-6",
    pages = "543-559",
    issn = "0032-0633",
    doi = "10.1016/j.pss.2003.10.002",
    keywords = "Acceleration;  Anisotropy;  Boundary layers;  Electron emission;  Magnetic field measurement;  Magnetosphere;  Planets;  Protons, Jovian particle dynamics;  Magnetopause boundary layers;  Quasi-periodic emission, Astrophysics",
    abstract = "In this study, we concentrate on the examination of the quasi-periodic behavior of 0.5-1.6 MeV (∼40-400 keV) protons (electrons) and of relativistic (> 16 MeV) electrons, observed at Jupiter by two different experiments onboard Ulysses, the HI-SCALE and COSPIN, respectively, within the large-scale south duskside magnetopause boundary layer (MPBL) of energetic particles, from ∼20:00 UT, day 41, to 12:00 UT, day 43. During those times, the observations confirm the transition of Ulysses to an important magnetospheric region with particle intensities comparable to the magnetodisk levels. A careful analysis of high time-resolution intensity, anisotropy and spectral measurements suggests the following: (1) The quasi-periodic ∼40 min (QP-40) energetic electron (> ∼40 keV) and proton (> ∼0.5 MeV) emissions from the south pole were a characteristic phenomenon in the south duskside MPBL; an almost continuous QP 40-min variation has been confirmed in energetic electron observations. (2) When the QP-40 modulation was not evident in energetic particle intensities, it was still detectable in spectral and anisotropy observations. (3) The QP-40 emission is a principal, but not the only periodic, energetic electron and proton emission; other periodicities (∼15, ∼20, ∼30, ∼50, ∼60, ∼80 min) were also significant in energetic particle spectral and anisotropy observations. We infer that QP-40 emissions along with other periodic emissions (∼15, ∼20, ∼30, ∼50, ∼60, ∼80 min) were the principal source of the large-scale high-latitude MPBL of energetic particles during Ulysses outbound pass of Jupiter. © 2003 Elsevier Ltd. All rights reserved."
}