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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. Planetary boundary layer - Wikipedia

    en.wikipedia.org/wiki/Planetary_boundary_layer

    The reduction in velocity near the surface is a function of surface roughness, so wind velocity profiles are quite different for different terrain types. [5] Rough, irregular ground, and man-made obstructions on the ground can reduce the geostrophic wind speed by 40% to 50%. [9] [10] Over open water or ice, the reduction may be only 20% to 30%.

  4. General circulation model - Wikipedia

    en.wikipedia.org/wiki/General_circulation_model

    Atmospheric models calculate winds, heat transfer, radiation, relative humidity, and surface hydrology within each grid and evaluate interactions with neighboring points. [1] A general circulation model (GCM) is a type of climate model. It employs a mathematical model of the general circulation of a planetary atmosphere or ocean.

  5. 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 ...

  6. Wind - Wikipedia

    en.wikipedia.org/wiki/Wind

    Planets require large magnetic fields in order to reduce the ionization of their upper atmosphere by the solar wind. [153] Other phenomena caused by the solar wind include geomagnetic storms that can knock out power grids on Earth, [ 157 ] the aurorae such as the Northern Lights , [ 158 ] and the plasma tails of comets that always point away ...

  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

    Planetary wind. Add languages. Add links. Article; ... Upload file; Special pages; ... Get shortened URL; Download QR code; Print/export Download as PDF; Printable ...

  9. Westerlies - Wikipedia

    en.wikipedia.org/wiki/Westerlies

    The westerlies (blue) and trade winds (yellow and brown) The general atmospheric circulation. Trade winds (red), westerlies (white) and the South Pacific anticyclone (blue) [1] The westerlies, anti-trades, [2] or prevailing westerlies, are prevailing winds from the west toward the east in the middle latitudes between 30 and 60 degrees latitude.