Showing 1 - 5 results of 5 for search '"Voyager 2"', query time: 0.04s Refine Results
  1. 1

    Interior and Gravity Field Models for Uranus Suggest a Mixed-composition Interior: Implications for the Uranus Orbiter and Probe by Zifan Lin, Sara Seager, Benjamin P. Weiss

    Published 2025-01-01
    “…We confirm that high degrees of mixing are required for Uranus interior models to be consistent with the J _2 and J _4 gravity harmonics measured by Voyager 2. Empirical models, which have smooth density profiles that require extensive mixing, can reproduce the Voyager 2 measurements. …”
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  2. 2

    The Orbits of Uranus, Its Satellites and Rings, the Gravity Field of the Uranian System, and the Orientation of the Poles of Uranus and Its Satellites by Robert A. Jacobson, Ryan S. Park

    Published 2025-01-01
    “…Jacobson determined the orbits of the Uranian satellites, the masses of Uranus and its satellites, and the orientation of the pole of Uranus from Earth-based astrometry, Earth-based ring occultations, and observations acquired with the Voyager 2 spacecraft. Subsequent to that publication, several observers obtained new astrometry, and some of the original astrometry was rereduced against the Gaia star catalog. …”
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  3. 3

    Ariel’s Medial Grooves: Spreading Centers on a Candidate Ocean World by Chloe B. Beddingfield, Richard J. Cartwright, Lauren M. Jozwiak, Tom A. Nordheim, G. Wes Patterson

    Published 2025-01-01
    “…While medial grooves are observable in Brownie and Kewpie Chasmata, our results indicate that these features are also present below Voyager 2 Imaging Science System image resolutions in Korrigan, Pixie, and Sylph Chasmata. …”
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  4. 4

    Hybrid Simulations of Interstellar Pickup Ions at the Solar Wind Termination Shock Revisited by Joe Giacalone, M. Kornbleuth, M. Opher, M. Gkioulidou, J. Köta, E. Puzzoni, J. D. Richardson, G. P. Zank

    Published 2025-01-01
    “…In previous simulations, a relatively cold initial distribution of PUIs was assumed; and while the resulting shock-heated distribution was consistent with Voyager 2 LECP measurements at about 30 keV, the intensity of the distribution downstream of the shock in the ~1–10 keV energy range was lower than predictions based on analysis of energetic neutral atoms (ENAs) from the Interstellar Boundary Explorer-Hi and Cassini's Ion and Neutral Camera. …”
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  5. 5

    A Systematic Literature Review and Bucher Indirect Comparison: Tildrakizumab versus Guselkumab by Kristian Garn Du Jardin, Pepi Hurtado Lopez, Mette Lange, Rachael McCool, Silvia Maeso Naval, Sandra Quickert

    Published 2020-07-01
    “…Five studies met the eligibility criteria and were included in the analysis; two tildrakizumab trials (reSURFACE 1 and reSURFACE 2) and three guselkumab trials (VOYAGE 1, VOYAGE 2, and a Japanese study). There was no statistically significant difference between guselkumab and tildrakizumab for PASI 75, PASI 90, SAEs, and rate of discontinuations at either timepoint. …”
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