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  2. Center of pressure (fluid mechanics) - Wikipedia

    en.wikipedia.org/wiki/Center_of_pressure_(fluid...

    Center of pressure is used in sailboat design to represent the position on a sail where the aerodynamic force is concentrated.. The relationship of the aerodynamic center of pressure on the sails to the hydrodynamic center of pressure (referred to as the center of lateral resistance) on the hull determines the behavior of the boat in the wind.

  3. Aerodynamic center - Wikipedia

    en.wikipedia.org/wiki/Aerodynamic_center

    The distribution of forces on a wing in flight are both complex and varying. This image shows the forces for two typical airfoils, a symmetrical design on the left, and an asymmetrical design more typical of low-speed designs on the right. This diagram shows only the lift components; the similar drag considerations are not illustrated.

  4. Heliosphere - Wikipedia

    en.wikipedia.org/wiki/Heliosphere

    Because the solar wind and the ISM are both fluid, the heliosphere's shape and size are also fluid. Changes in the solar wind, however, more strongly alter the fluctuating position of the boundaries on short timescales (hours to a few years). The solar wind's pressure varies far more rapidly than the outside pressure of the ISM at any given ...

  5. Magnus effect - Wikipedia

    en.wikipedia.org/wiki/Magnus_effect

    Rotor ships use mast-like cylinders, called Flettner rotors, for propulsion. These are mounted vertically on the ship's deck. When the wind blows from the side, the Magnus effect creates a forward thrust. Thus, as with any sailing ship, a rotor ship can only move forwards when there is a wind blowing.

  6. The Situations and Names of Winds - Wikipedia

    en.wikipedia.org/wiki/The_Situations_and_Names...

    The Situations and Names of Winds (Ancient Greek: Περὶ θέσεως ἀνέμων; Latin: Ventorum Situs) is a spurious fragment traditionally attributed to Aristotle.

  7. 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.

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  9. Classical compass winds - Wikipedia

    en.wikipedia.org/wiki/Classical_compass_winds

    In the Hebrew Bible, there is frequent reference to four cardinal directions. [5] The names of the directions seem to be associated with physical landmarks for the ancient Israelites living in the region of Judea, e.g. East is referred to as kedem, which may derive from "edom" ("red"), and may be a reference to the color of the rising dawn, or the red sandstone cliffs of the Land of Edom to ...

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