Showing 561 - 580 results of 580 for search '"Moon', query time: 0.06s Refine Results
  1. 561

    Impact of Jupiter’s Heating and Self-shadowing on the Jovian Circumplanetary Disk Structure by Antoine Schneeberger, Olivier Mousis

    Published 2025-01-01
    “…The existence of these shadows in Jupiter’s CPD may have influenced the composition of the building blocks of the Galilean moons, potentially shaping their formation and characteristics. …”
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    Article
  2. 562

    Hybrid Cryptography Based on Planets: Phobos & Deimos by Kraicha Ayoub, Touil Hamza, El Akkad Nabil

    Published 2025-01-01
    “…This document presents the Phobos and Deimos encryption method, inspired by Mars’ moons. By using the unique orbital properties of Phobos and Deimos, this method creates a dynamic encryption algorithm. …”
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    Article
  3. 563

    A Development Methodology for Copper End Termination Paste — Part 1: Origin of Green Defects by Umesh Kumar

    Published 2002-01-01
    “…In this paper, the influence of paste rheology on the green cosmetic defects such as mooning, peaking, etc. is discussed. Additionally, the influence of process condition such as dipping parameters, drying conditions etc., on the green cosmetic defects are discussed. …”
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  4. 564

    Thermomechanical Fatigue of Unidirectional Carbon Fiber/Epoxy Composite in Space by Ali Anvari

    Published 2020-01-01
    “…Furthermore, with applying thermal fatigue relations, thermally-safe planets, moons, and asteroids in the solar system for unidirectional carbon fiber/epoxy composite are identified.…”
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  5. 565

    Crater Dimensions on the Dwarf Planets by Veronica J. Bray, Michael F. Zeilnhofer, S. J. Robbins, P. M. Schenk, Kelsi M. Singer, O. L. White, S. A. Stern, S. D. Benecchi, K. A. Durfey, H. A. Weaver, C. B. Olkin, J. R. Spencer, the New Horizons Geology and Geophysics Investigation Team

    Published 2025-01-01
    “…The icy dwarf planets of Pluto, Charon, and Ceres provide important geologic comparisons for each other as they possess similar gravities and experience impacts of similar velocities compared to larger planets and moons. Differences in their impact craters can therefore be attributed to differences in the impactor and/or target compositions. …”
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    Article
  6. 566

    Solid–liquid phase change in planetary cores by Huguet, Ludovic, Kriaa, Quentin, Alboussière, Thierry,  Le Bars, Michael

    Published 2024-12-01
    “…In particular, they take place in the iron core of terrestrial planets and moons, profoundly influencing their dynamics and magnetic field generation. …”
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  7. 567

    Variational Methods in Optical Quantum Machine Learning by Marco Simonetti, Damiano Perri, Osvaldo Gervasi

    Published 2023-01-01
    “…As a case study, we considered the binary classification of points belonging to a certain geometric pattern (the Two-Moons Classification problem) on a plane. We think it is reasonable to expect benefits from using hybrid deep learning systems (classical + quantum), not just in terms of accelerating computation but also in understanding the underlying phenomena and mechanisms. …”
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  10. 570

    Fingerprints of surface flows on solid substrates ablated by phase change: from laboratory experiments to planetary landscapes by Carpy, Sabrina, Berhanu, Michael, Chaigne, Martin, Courrech du Pont, Sylvain

    Published 2025-02-01
    “…In this case, the fluid mechanics associated with such phase changes play a key role in the evolution of terrestrial and planetary landscapes, observed by probes orbiting planets and moons. On Earth, sea ice, glaciers and karst plateaus extend over meters or kilometers. …”
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