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Obi. (sash) Back of a woman wearing a kimono with the obi tied in the tateya musubi style. An obi ( 帯) is a belt of varying size and shape worn with both traditional Japanese clothing and uniforms for Japanese martial arts styles. Originating as a simple thin belt in Heian period Japan, the obi developed over time into a belt with a number of ...
The medium size individual equipment belt (NSN 8465-00-001-6488) is for soldiers with waists measuring under 30 inches (76 cm) and size large (NSN 8465-00-001-6487) is for those with waists measuring 30 inches (76 cm) or over. The length of the belt is adjusted at each end by means of adjusting clamps which slide along the belt when opened. [3]
The angular speed is inversely proportional to size, so the larger the one wheel, the less angular velocity, and vice versa. Actual pulley speeds tend to be 0.5–1% less than generally calculated because of belt slip and stretch. In timing belts, the inverse ratio teeth of the belt contributes to the exact measurement. The speed of the belt is:
The joint European standard for size labelling of clothes, formally known as the EN 13402 Size designation of clothes, is a European standard for labelling clothes sizes. The standard is based on body dimensions measured in centimetres, and as such, and its aim is to make it easier for people to find clothes in sizes that fit them.
The belts are named after James Van Allen, who is often credited with their discovery. [1] Earth's two main belts extend from an altitude of about 640 to 58,000 km (400 to 36,040 mi) [2] above the surface, in which region radiation levels vary. The belts are in the inner region of Earth's magnetic field. They trap energetic electrons and protons.
Currently most of the objects of mass between 10 9 kg to 10 12 kg (less than 1000 teragrams (Tg)) listed here are near-Earth asteroids (NEAs). The Aten asteroid 1994 WR12 has less mass than the Great Pyramid of Giza, 5.9 × 10 9 kg. For more about very small objects in the Solar System, see meteoroid, micrometeoroid, cosmic dust, and ...
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