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  2. 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 ...

  3. Stellar wind - Wikipedia

    en.wikipedia.org/wiki/Stellar_wind

    The Sun's wind is called the solar wind. These winds consist mostly of high-energy electrons and protons (about 1 keV) that are able to escape the star's gravity because of the high temperature of the corona. Stellar winds from main-sequence stars do not strongly influence the evolution of lower-mass stars such as the Sun.

  4. 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.

  5. Bow shock - Wikipedia

    en.wikipedia.org/wiki/Bow_shock

    Bow shock occurs when the magnetosphere of an astrophysical object interacts with the nearby flowing ambient plasma such as the solar wind. For Earth and other magnetized planets, it is the boundary at which the speed of the stellar wind abruptly drops as a result of its approach to the magnetopause.

  6. Polar wind - Wikipedia

    en.wikipedia.org/wiki/Polar_wind

    The polar wind or plasma fountain is a permanent outflow of plasma from the polar regions of Earth's magnetosphere. [2]: 29 Conceptually similar to the solar wind, it is one of several mechanisms for the outflow of ionized particles. Ions accelerated by a polarization electric field known as an ambipolar electric field is believed to be the ...

  7. Wind - Wikipedia

    en.wikipedia.org/wiki/Wind

    Wind is the natural movement of air or other gases relative to a planet's surface. Winds occur on a range of scales, from thunderstorm flows lasting tens of minutes, to local breezes generated by heating of land surfaces and lasting a few hours, to global winds resulting from the difference in absorption of solar energy between the climate ...

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

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

    It is recommended to name the SVG file “Map prevailing winds on earth.svg”—then the template Vector version available (or Vva) does not need the new image name parameter. Summary Description Map prevailing winds on earth.png

  9. Planetary boundary layer - Wikipedia

    en.wikipedia.org/wiki/Planetary_boundary_layer

    In addition to the surface layer, the planetary boundary layer also comprises the PBL core (between 0.1 and 0.7 of the PBL depth) and the PBL top or entrainment layer or capping inversion layer (between 0.7 and 1 of the PBL depth). Four main external factors determine the PBL depth and its mean vertical structure: the free atmosphere wind speed;

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