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  2. Atmospheric circulation - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_circulation

    The winds that flow to the west (from the east, easterly wind) at the ground level in the Hadley cell are called the trade winds. Though the Hadley cell is described as located at the equator, it shifts northerly (to higher latitudes) in June and July and southerly (toward lower latitudes) in December and January, as a result of the Sun's ...

  3. Hodograph - Wikipedia

    en.wikipedia.org/wiki/Hodograph

    A hodograph is a diagram that gives a vectorial visual representation of the movement of a body or a fluid. It is the locus of one end of a variable vector, with the other end fixed. [1] The position of any plotted data on such a diagram is proportional to the velocity of the moving particle. [2] It is also called a velocity diagram.

  4. Wind - Wikipedia

    en.wikipedia.org/wiki/Wind

    In outer space, solar wind is the movement of gases or charged particles from the Sun through space, while planetary wind is the outgassing of light chemical elements from a planet's atmosphere into space. The strongest observed winds on a planet in the Solar System occur on Neptune and Saturn.

  5. File:Map prevailing winds on earth.png - Wikipedia

    en.wikipedia.org/wiki/File:Map_prevailing_winds...

    Besides the westerlies, and trade winds, the large surfaces of land also effect the wind, causing cyclones, hurricanes and other deviations to the normal direction of trade wind File usage The following 10 pages use this file:

  6. Prevailing winds - Wikipedia

    en.wikipedia.org/wiki/Prevailing_winds

    Prevailing winds are strongly influenced by Earth's overall atmospheric circulation, in addition to smaller-scale and shorter-lived weather phenomena. In meteorology, prevailing wind in a region of the Earth's surface is a surface wind that blows predominantly from a particular direction. The dominant winds are the trends in direction of wind ...

  7. Magnetopause - Wikipedia

    en.wikipedia.org/wiki/Magnetopause

    The solar wind is supersonic and passes through a bow shock where the direction of flow is changed so that most of the solar wind plasma is deflected to either side of the magnetopause, much like water is deflected before the bow of a ship. The zone of shocked solar wind plasma is the magnetosheath. At Earth and all the other planets with ...

  8. Planetary wind - Wikipedia

    en.wikipedia.org/?title=Planetary_wind&redirect=no

    Print/export Download as PDF; Printable version; In other projects Appearance. move to sidebar hide. From Wikipedia, the free encyclopedia ... w/index.php?title ...

  9. Jet stream - Wikipedia

    en.wikipedia.org/wiki/Jet_stream

    The path of the jet typically has a meandering shape, and these meanders themselves propagate eastward, at lower speeds than that of the actual wind within the flow. Further, the meanders can split or form eddies. [25] Each large meander, or wave, within the jet stream is known as a Rossby wave (planetary wave).

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