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Showing 1–9 of 9 results
Advanced filters: Author: Aymeric Spiga Clear advanced filters
  • The Martian atmosphere hosts water-ice clouds, but it is thought that any snow precipitation settles slowly, rather than in storms. Martian meteorology simulations suggest that localized convective snowstorms can occur on Mars during the night.

    • Aymeric Spiga
    • David P. Hinson
    • Franck Montmessin
    Research
    Nature Geoscience
    Volume: 10, P: 652-657
  • The InSight lander has expanded our knowledge of the atmosphere of Mars by observing various phenomena, including airglow, bores, infrasound and Earth-like turbulence.

    • Don Banfield
    • Aymeric Spiga
    • W. Bruce Banerdt
    Research
    Nature Geoscience
    Volume: 13, P: 190-198
  • Brown dwarfs are substellar objects subject to variability and colour changes. A 3D general circulation model shows that clouds explain this observed behaviour and highlights their role as a driver of atmospheric dynamics and climate.

    • Lucas Teinturier
    • Benjamin Charnay
    • Bruno Bézard
    Research
    Nature Astronomy
    Volume: 10, P: 224-233
  • A high-resolution three-dimensional global climate model of Saturn captures the small-scale dynamics of its stratosphere. It is able to reproduce the observed semi-annual equatorial oscillation and finds evidence of an interhemispheric meridional circulation that can explain the periodicity of its equatorial oscillation and the seasonal behaviour of hydrocarbon abundances.

    • Deborah Bardet
    • Aymeric Spiga
    • Sandrine Guerlet
    Research
    Nature Astronomy
    Volume: 6, P: 804-811
  • As the Perseverance rover landed on the Martian surface, the sensors on NASA’s InSight Mars lander picked up no seismic or acoustic waves. This non-detection provides information on the crust and atmosphere of Mars.

    • Benjamin Fernando
    • Natalia Wójcicka
    • Ingrid J. Daubar
    ResearchOpen Access
    Nature Astronomy
    Volume: 6, P: 59-64
  • The magnetic field measured by the InSight lander on Mars varies daily and is ten times stronger than expected. The field is inferred to originate from components of basement rocks magnetized by an ancient dynamo of Earth-like strength.

    • Catherine L. Johnson
    • Anna Mittelholz
    • William B. Banerdt
    Research
    Nature Geoscience
    Volume: 13, P: 199-204
  • Geophysical and meteorological measurements by NASA’s InSight lander on Mars reveal a planet that is seismically active and provide information about the interior, surface and atmospheric workings of Mars.

    • W. Bruce Banerdt
    • Suzanne E. Smrekar
    • Mark Wieczorek
    Reviews
    Nature Geoscience
    Volume: 13, P: 183-189