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  2. Atmospheric super-rotation - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_super-rotation

    Atmospheric super-rotation is a phenomenon where a planet's atmosphere rotates faster than the planet itself. This behavior is observed in the atmospheres of Venus , Titan , Jupiter , and Saturn. Venus exhibits the most extreme super-rotation, with its atmosphere circling the planet in four Earth days, much faster than the planet's own rotation ...

  3. Super-rotation - Wikipedia

    en.wikipedia.org/wiki/Super-rotation

    Download QR code; Print/export Download as PDF; ... move to sidebar hide. Super-rotation can mean: Atmospheric super-rotation, in which a planet's ...

  4. Atmospheric radiative transfer codes - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_radiative...

    An atmospheric radiative transfer model, code, or simulator calculates radiative transfer of electromagnetic radiation through a planetary atmosphere. Methods [ edit ]

  5. Rossby number - Wikipedia

    en.wikipedia.org/wiki/Rossby_number

    For a figure showing spatial and temporal scales of motions in the atmosphere and oceans, see Kantha and Clayson. [ 8 ] When the Rossby number is large (either because f is small, such as in the tropics and at lower latitudes; or because L is small, that is, for small-scale motions such as flow in a bathtub ; or for large speeds), the effects ...

  6. Atmospheric circulation - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_circulation

    The atmospheric circulation can be viewed as a heat engine driven by the Sun's energy and whose energy sink, ultimately, is the blackness of space. The work produced by that engine causes the motion of the masses of air, and in that process it redistributes the energy absorbed by the Earth's surface near the tropics to the latitudes nearer the ...

  7. Day length fluctuations - Wikipedia

    en.wikipedia.org/wiki/Day_length_fluctuations

    This spin-down time is the characteristic time for the transfer of atmospheric axial angular momentum to Earth's surface and vice versa. The zonal wind-component on the ground, which is most effective for the transfer of axial angular momentum between Earth and atmosphere, is the component describing rigid rotation of the atmosphere. [8]

  8. Atmospheric model - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_model

    In atmospheric science, an atmospheric model is a mathematical model constructed around the full set of primitive, dynamical equations which govern atmospheric motions. It can supplement these equations with parameterizations for turbulent diffusion, radiation , moist processes ( clouds and precipitation ), heat exchange , soil , vegetation ...

  9. Atmospheric circulation of exoplanets - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_circulation_of...

    Atmospheric circulation of a planet is largely specific to the planet in question and the study of atmospheric circulation of exoplanets is a nascent field as direct observations of exoplanet atmospheres are still quite sparse. However, by considering the fundamental principles of fluid dynamics and imposing various limiting assumptions, a ...