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The Coriolis Effect Quin és correcte ? In the iner5al frame of reference (upper part of the picture), the black object moves in a straight line, without significant fric5on with the disc. However, the observer (red dot) who is standing in the rota5ng (non‐ iner5al) frame of reference (lower part of the picture) sees the object as following a curved path due to the Coriolis and centrifugal forces present in this frame. • In physics, the Coriolis effect is a deflec5on of moving objects when they are viewed in a rota5ng reference frame. • In a reference frame with clockwise rota5on, the deflec5on is to the leJ of the mo5on of the object; in one with counter‐clockwise rota5on, the deflec5on is to the right. • The mathema5cal expression for the Coriolis force appeared in an 1835 paper by French scien5st Gaspard‐ Gustave Coriolis, in connec5on with the theory of water wheels, and also in the 5dal equa5ons of Pierre‐Simon Laplace in 1778. • Even earlier, Italian scien5sts Giovanni BaYsta Riccioli and his assistant Francesco Maria Grimaldi described the effect in connec5on with ar5llery in the 1651 Almagestum Novum, wri5ng that rota5on of the Earth should cause a cannon ball fired to the north to deflect to the east.[1] • Early in the 20th century, the term Coriolis force began to be used in connec5on with meteorology. • The Coriolis effect is caused by the rota5on of the Earth and the iner5a of the mass experiencing the effect. • Newton's laws of mo5on govern the mo5on of an object in a (non‐ accelera5ng) iner5al frame of reference. • When Newton's laws are transformed to a rota5ng frame of reference, the Coriolis and centrifugal forces appear. • Both forces are propor5onal to the mass of the object. The Coriolis force is propor5onal to the rota5on rate and the centrifugal force is propor5onal to its square. • The Coriolis force acts in a direc5on perpendicular to the rota5on axis and to the velocity of the body in the rota5ng frame and is propor5onal to the object's speed in the rota5ng frame. • This force is termed either iner5al force, fic55ous force or pseudo force.[2] It allows the applica5on of simple Newtonian laws to a rota5ng system. • It is a correc5on factor that does not exist in a true non‐accelera5ng "iner5al" system. • Perhaps the most commonly encountered rota5ng reference frame is the Earth. • Because the Earth completes only one rota5on per day, the Coriolis force is quite small, and its effects generally become no5ceable only for mo5ons occurring over large distances and long periods of 5me, such as large‐scale movement of air in the atmosphere or water in the ocean. • Such mo5ons are constrained by the 2‐dimensional surface of the earth, so only the horizontal component of the Coriolis force is generally important. • This force causes moving objects on the surface of the Earth to appear to veer to the right in the northern hemisphere, and to the leJ in the southern. • Rather than flowing directly from areas of high pressure to low pressure, as they would on a non‐rota5ng planet, winds and currents tend to flow to the right of this direc5on north of the equator, and to the leJ of this direc5on south of it. • This effect is responsible for the rota5on of large cyclones (see Coriolis effects in meteorology). Eötvös Effect • The prac5cal impact of the Coriolis effect is mostly caused by the horizontal accelera5on component produced by horizontal mo5on. • There are other components of the Coriolis effect. Eastward‐traveling objects will be deflected upwards (feel lighter), while westward‐traveling objects will be deflected downwards (feel heavier). • This is known as the Eötvös effect. This aspect of the Coriolis effect is greatest near the equator. The force produced by this effect is similar to the horizontal component, but the much larger ver5cal forces due to gravity and pressure mean that it is generally unimportant dynamically. • In addi5on, objects traveling upwards or downwards will be deflected to the west or east respec5vely. This effect is also the greatest near the equator. Since ver5cal movement is usually of limited extent and dura5on, the size of the effect is smaller and requires precise instruments to detect. Geostrophic wind • The geostrophic wind is the theore5cal wind that would result from an exact balance between the Coriolis effect and the pressure gradient force. • This condi5on is called geostrophic balance. • The geostrophic wind is directed parallel to isobars (lines of constant pressure at a given height). This balance seldom holds exactly in nature. • The true wind almost always differs from the geostrophic wind due to other forces such as fric5on from the ground. Thus, the actual wind would equal the geostrophic wind only if there were no fric5on and the isobars were perfectly straight. • Despite this, much of the atmosphere outside the tropics is close to geostrophic flow much of the 5me and it is a valuable first approxima5on. • Air naturally moves from areas of high pressure to areas of low pressure, due to the pressure gradient force. • As soon as the air starts to move, however, the Coriolis "force" deflects it. • The deflec5on is to the right in the northern hemisphere, and to the leJ in the southern hemisphere. • As the air moves from the high pressure area, its speed increases, and so does its Coriolis deflec5on. • The deflec5on increases un5l the Coriolis and pressure gradient forces are in geostrophic balance: at this point, the air flow is no longer moving from high to low pressure, but instead moves along an isobar. • (Note that this explana5on assumes that the atmosphere starts in a geostrophically unbalanced state and describes how such a state would evolve into a balanced flow. In prac5ce, the flow is nearly always balanced.) • The geostrophic balance helps to explain why, in the northern hemisphere, low pressure systems (or cyclones) spin counterclockwise and high pressure systems (or an;cyclones) spin clockwise, and the opposite in the southern hemisphere. • Flow of ocean water is also largely geostrophic. • Just as mul5ple weather balloons that measure pressure as a func5on of height in the atmosphere are used to map the atmospheric pressure field and infer the geostrophic wind, measurements of density as a func5on of depth in the ocean are used to infer geostrophic currents. • Satellite al5meters are also used to measure sea surface height anomaly, which permits a calcula5on of the geostrophic current at the surface. • The effect of fric5on, between the air and the land, breaks the geostrophic balance. • Fric5on slows the flow, lessening the effect of the Coriolis force. • As a result, the pressure gradient force has a greater effect and the air s5ll moves from high pressure to low pressure, though with great deflec5on. • This explains why high pressure system winds radiate out from the center of the system, while low pressure systems have winds that spiral inwards. • The geostrophic wind neglects fric5onal effects, which is usually a good approxima5on for the synop5c scale instantaneous flow in the midla5tude mid‐troposphere. • Although ageostrophic terms are rela5vely small, they are essen5al for the 5me evolu5on of the flow and in par5cular are necessary for the growth and decay of storms. • Quasigeostrophic and Semigeostrophic theory are used to model flows in the atmosphere more widely. These theories allow for divergence to take place and for weather systems to then develop. Cyclonic gyres • In meteorology, a cyclone is an area of closed, circular fluid mo5on rota5ng in the same direc5on as the Earth. • This is usually characterized by inward spiraling winds that rotate an5clockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere of the Earth. • Most large‐scale cyclonic circula5ons are centered on areas of low atmospheric pressure. • The largest low‐pressure systems are cold‐core polar cyclones and extratropical cyclones which lie on the synop5c scale. • Warm‐core cyclones such as tropical cyclones, mesocyclones, and polar lows lie within the smaller mesoscale. • Subtropical cyclones are of intermediate size.