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21.
  • Enceladus plume variability... Enceladus plume variability and the neutral gas densities in Saturn's magnetosphere
    Smith, H. T.; Johnson, R. E.; Perry, M. E. ... Journal of Geophysical Research: Space Physics, October 2010, Volume: 115, Issue: A10
    Journal Article
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    Open access

    Neutral particle dominance over charged particles in Saturn's magnetosphere was evident prior to Cassini's arrival at Saturn in 2004. The observation of active plumes emanating from the south pole of ...
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22.
  • Solar Energetic Particles P... Solar Energetic Particles Produced by a Slow Coronal Mass Ejection at ∼0.25 au
    Giacalone, J.; Mitchell, D. G.; Allen, R. C. ... The Astrophysical journal. Supplement series, 02/2020, Volume: 246, Issue: 2
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    Open access

    We present an analysis of Parker Solar Probe (PSP) IS IS observations of ∼30-300 keV n−1 ions on 2018 November 11 when PSP was about 0.25 au from the Sun. Five hours before the onset of a solar ...
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23.
  • Properties of Suprathermal-... Properties of Suprathermal-through-energetic He Ions Associated with Stream Interaction Regions Observed over the Parker Solar Probe's First Two Orbits
    Desai, M. I.; Mitchell, D. G.; Szalay, J. R. ... The Astrophysical journal. Supplement series, 02/2020, Volume: 246, Issue: 2
    Journal Article
    Peer reviewed
    Open access

    The Integrated Science Investigation of the Sun (IS IS) suite on board NASA's Parker Solar Probe (PSP) observed six distinct enhancements in the intensities of suprathermal-through-energetic (∼0.03-3 ...
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24.
  • Parker Solar Probe Encounte... Parker Solar Probe Encounters the Leg of a Coronal Mass Ejection at 14 Solar Radii
    McComas, D. J.; Sharma, T.; Christian, E. R. ... Astrophysical journal/˜The œAstrophysical journal, 02/2023, Volume: 943, Issue: 2
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    Abstract We use Parker Solar Probe (PSP) observations to report the first direct measurements of the particle and field environments while crossing the leg of a coronal mass ejection (CME) very close ...
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25.
  • Energetic Particle Increase... Energetic Particle Increases Associated with Stream Interaction Regions
    Cohen, C. M. S.; Christian, E. R.; Cummings, A. C. ... The Astrophysical journal. Supplement series, 02/2020, Volume: 246, Issue: 2
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    The Parker Solar Probe was launched on 2018 August 12 and completed its second orbit on 2019 June 19 with perihelion of 35.7 solar radii. During this time, the Energetic Particle Instrument-Hi ...
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26.
  • The Solar Wind Ion Analyzer... The Solar Wind Ion Analyzer for MAVEN
    Halekas, J. S.; Taylor, E. R.; Dalton, G. ... Space science reviews, 12/2015, Volume: 195, Issue: 1-4
    Journal Article
    Peer reviewed

    The Solar Wind Ion Analyzer (SWIA) on the MAVEN mission will measure the solar wind ion flows around Mars, both in the upstream solar wind and in the magneto-sheath and tail regions inside the bow ...
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27.
  • Energetic particle behavior... Energetic particle behavior in near-Sun magnetic field switchbacks from PSP
    Bandyopadhyay, R.; Matthaeus, W. H.; McComas, D. J. ... Astronomy & astrophysics, 06/2021, Volume: 650
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    Context. The observation of numerous magnetic switchbacks and associated plasma jets in Parker Solar Probe (PSP) during its first five orbits, particularly near the Sun, has attracted considerable ...
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28.
  • Role of magnetosheath force... Role of magnetosheath force balance in regulating the dayside reconnection potential
    Lopez, R. E.; Bruntz, R.; Mitchell, E. J. ... Journal of Geophysical Research: Space Physics, December 2010, Volume: 115, Issue: A12
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    When the interplanetary magnetic field (IMF) is southward, most of the ionospheric potential is generated by merging between the IMF and the magnetospheric field. Typically, the ionospheric potential ...
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29.
  • Global Observations of the ... Global Observations of the Interstellar Interaction from the Interstellar Boundary Explorer (IBEX)
    McComas, D.J; Allegrini, F; Bochsler, P ... Science, 11/2009, Volume: 326, Issue: 5955
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    The Sun moves through the local interstellar medium, continuously emitting ionized, supersonic solar wind plasma and carving out a cavity in interstellar space called the heliosphere. The recently ...
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  • First Measurements of Jovia... First Measurements of Jovian Electrons by Parker Solar Probe/IS⊙IS within 0.5 au of the Sun
    Mitchell, J. G.; Leske, R. A.; Nolfo, G. A. DE ... Astrophysical journal/˜The œAstrophysical journal, 07/2022, Volume: 933, Issue: 2
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    Abstract Energetic electrons of Jovian origin have been observed for decades throughout the heliosphere, as far as 11 au, and as close as 0.5 au, from the Sun. The treatment of Jupiter as a ...
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