Knowledge (XXG)

Non-inertial reference frame

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858: 36: 871: 1134: 1309:". Similarly, a background observer can argue that the forced acceleration of the mass causes an apparent gravitational field in the region between it and the environmental material (the accelerated mass also "drags light"). This "mutual" effect, and the ability of an accelerated mass to warp lightbeam geometry and lightbeam-based coordinate systems, is referred to as 1223: 1679: 1742: 1020:
frame. This approach avoids the use of fictitious forces (it is based on an inertial frame, where fictitious forces are absent, by definition) but it may be less convenient from an intuitive, observational, and even a calculational viewpoint. As pointed out by Ryder for the case of rotating frames as used in meteorology:
1056:. The rotation of the Earth seemingly causes the pendulum to change its plane of oscillation because the surroundings of the pendulum move with the Earth. As seen from an Earth-bound (non-inertial) frame of reference, the explanation of this apparent change in orientation requires the introduction of the fictitious 1316:
Frame-dragging removes the usual distinction between accelerated frames (which show gravitational effects) and inertial frames (where the geometry is supposedly free from gravitational fields). When a forcibly-accelerated body physically "drags" a coordinate system, the problem becomes an exercise in
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exists in the accelerated frame (we reserve the word gravitational for the case in which a mass is involved). An object accelerated to be stationary in the accelerated frame will "feel" the presence of the field, and they will also be able to see environmental matter with inertial states of motion
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In flat spacetime, the use of non-inertial frames can be avoided if desired. Measurements with respect to non-inertial reference frames can always be transformed to an inertial frame, incorporating directly the acceleration of the non-inertial frame as that acceleration as seen from the inertial
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This incompatible use of the term "fictitious force" is unrelated to non-inertial frames. These so-called "forces" are defined by determining the acceleration of a particle within the curvilinear coordinate system, and then separating the simple double-time derivatives of coordinates from the
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A simple way of dealing with this problem is, of course, to transform all coordinates to an inertial system. This is, however, sometimes inconvenient. Suppose, for example, we wish to calculate the movement of air masses in the earth's atmosphere due to pressure gradients. We need the results
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In this connection, it may be noted that a change in coordinate system, for example, from Cartesian to polar, if implemented without any change in relative motion, does not cause the appearance of fictitious forces, although the form of the laws of motion varies from one type of curvilinear
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models, the accelerated body can agree that the apparent gravitational field is associated with the motion of the background matter, but can also claim that the motion of the material as if there is a gravitational field, causes the gravitational field - the accelerating background matter
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at rest in a non-inertial frame will, in general, detect a non-zero acceleration. While the laws of motion are the same in all inertial frames, in non-inertial frames, they vary from frame to frame, depending on the acceleration.
80:, is a useful starting point for translations, but translators must revise errors as necessary and confirm that the translation is accurate, rather than simply copy-pasting machine-translated text into the English Knowledge (XXG). 1067:. In that case, the prediction of the measured tension in the string based on the motion of the spheres as observed from a rotating reference frame requires the rotating observers to introduce a fictitious centrifugal force. 90: 212: 236: 66: 1093:. To avoid confusion, this distracting ambiguity in terminologies is pointed out here. These so-called "forces" are non-zero in all frames of reference, inertial or non-inertial, and do 994: 967:. In general, the expression for any fictitious force can be derived from the acceleration of the non-inertial frame. As stated by Goodman and Warner, "One might say that 997:, there are no global inertial reference frames in general relativity. More specifically, the fictitious force which appears in general relativity is the force of 1247: 1155: 902: 491: 1209:, and effectively free from obvious gravitational fields, then if an accelerated coordinate system is overlaid onto the same region, it can be said that a 1284:
In frame-based descriptions, this supposed field can be made to appear or disappear by switching between "accelerated" and "inertial" coordinate systems.
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Do not translate text that appears unreliable or low-quality. If possible, verify the text with references provided in the foreign-language article.
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That a given frame is non-inertial can be detected by its need for fictitious forces to explain observed motions. For example, the rotation of the
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relative to the rotating frame, the earth, so it is better to stay within this coordinate system if possible. This can be achieved by introducing
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holds in any coordinate system provided the term 'force' is redefined to include the so-called 'reversed effective forces' or 'inertia forces'."
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and this very large centripetal force explicitly, and yet our interest is almost always the small relative motion of the atmosphere and ocean,
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transform as vectors under rotations and translations of the coordinates (as all Newtonian forces do, fictitious or otherwise).
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Content in this edit is translated from the existing Spanish Knowledge (XXG) article at ]; see its history for attribution.
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remaining terms. These remaining terms then are called "fictitious forces". More careful usage calls these terms "
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it is often possible to explain the motion of bodies in non-inertial reference frames by introducing additional
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by James F. Price, Woods Hole Oceanographic Institution (2006). See in particular §4.3, p. 34 in the
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Reference frame that undergoes acceleration with respect to an inertial frame
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to the source of your translation. A model attribution edit summary is
1549:(Reprint of 1963 ed.). Courier Dover Publications. p. 358. 573: 419: 329: 1063:
Another famous example is that of the tension in the string between
1772:(Reprint of 1970 ed.). Courier Dover Publications. p. 4. 1049: 409: 404: 346: 1085:
A different use of the term "fictitious force" often is used in
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Discovering the Natural Laws: The Experimental Basis of Physics
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Detection of a non-inertial frame: need for fictitious forces
1657:(3rd ed.). Saunders College Publishing. p. 135. 207:{\displaystyle {\textbf {F}}={\frac {d\mathbf {p} }{dt}}} 89:
to this template: there are already 946 articles in the
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As the situation is modeled in finer detail, using the
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gravitational field becomes less realistic. In these
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Sidney Borowitz & Lawrence A. Bornstein (1968).
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Lawrence E. Goodman & William H. Warner (2001).
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a machine-translated version of the Spanish article.
127:{{Translated|es|Sistema de referencia no inercial}} 1706: 1596:"The inertial frame equations have to account for 1507: 206: 951:(also called inertial forces, pseudo-forces, and 993:inertial, but globally non-inertial. Due to the 1022: 115:accompanying your translation by providing an 60:Click for important translation instructions. 47:expand this article with text translated from 1855:I. Bernard Cohen, George Edwin Smith (2002). 1454:. Atlantica SĂ©guier Frontières. p. 286. 1390:Emil Tocaci, Clive William Kilmister (1984). 896: 8: 1075:Fictitious forces in curvilinear coordinates 1681:Mathematical Methods of Classical Mechanics 1205:If a region of spacetime is declared to be 1162:. Unsourced material may be challenged and 995:non-Euclidean geometry of curved space-time 1861:. Cambridge University Press. p. 43. 1005:Avoiding fictitious forces in calculations 903: 889: 150: 1744:A Contemporary View of Elementary Physics 1393:Relativistic Mechanics, Time, and Inertia 1266:Learn how and when to remove this message 1182:Learn how and when to remove this message 188: 182: 173: 172: 170: 1478:A Modern Approach to Classical Mechanics 1796:The Investigation of the Physical World 1362: 1201:Proper reference frame (flat spacetime) 222: 158: 1824:Louis N. Hand, Janet D. Finch (1998). 1713:. Courier Dover Publications. p.  1654:Physics for scientists & engineers 1108:" to indicate their connection to the 959:. Common examples of this include the 94: 1065:two spheres rotating about each other 585:Newton's law of universal gravitation 7: 1793:Giuliano Toraldo di Francia (1981). 1317:warped spacetime for all observers. 1160:adding citations to reliable sources 1081:Mechanics of planar particle motion 566:Mechanics of planar particle motion 174: 1570:M. Alonso & E.J. Finn (1992). 25: 1858:The Cambridge companion to Newton 1630:. Aachen Shaker. pp. 78–79. 1448:Ludwik Marian Celnikier (1993). 1221: 1132: 870: 869: 856: 189: 34: 1294:general principle of relativity 1769:Methods of analytical Dynamics 1573:Fundamental university physics 1371:"Accelerated Reference Frames" 1071:coordinate system to another. 125:You may also add the template 1: 492:Koopman–von Neumann mechanics 1747:. McGraw-Hill. p. 138. 1514:(Reprint of 1968 ed.). 917:non-inertial reference frame 560:Non-inertial reference frame 1766:Leonard Meirovitch (2004). 1347:Inertial frame of reference 1241:. The specific problem is: 1011:Inertial frame of reference 921:accelerated reference frame 487:Appell's equation of motion 357:Inertial frame of reference 138:Knowledge (XXG):Translation 97:will aid in categorization. 18:Accelerated reference frame 1909: 1832:Cambridge University Press 1729:reference laws of physics. 1705:Milton A. Rothman (1989). 1651:Raymond A. Serway (1990). 1516:Courier Dover Publications 1288:More advanced descriptions 1237:to meet Knowledge (XXG)'s 1198: 1124:Relativistic point of view 1078: 1008: 72:Machine translation, like 1684:. Springer. p. 129. 1506:Albert Shadowitz (1988). 1417:Wolfgang Rindler (1977). 1396:. Springer. p. 251. 1281:as if the field is real. 1195:Frames and flat spacetime 49:the corresponding article 1327:Rotating reference frame 1211:uniform fictitious field 1052:can be observed using a 650:Rotating reference frame 482:Hamilton–Jacobi equation 1110:generalized coordinates 1087:curvilinear coordinates 591:Newton's laws of motion 451:Newton's laws of motion 136:For more guidance, see 1678:V. I. Arnol'd (1989). 1451:Basics of Space Flight 1041: 618:Simple harmonic motion 531:Euler's laws of motion 325:D'Alembert's principle 208: 1199:Further information: 472:Hamiltonian mechanics 290:Statistical mechanics 209: 109:copyright attribution 1827:Analytical Mechanics 1624:Peter Ryder (2007). 1420:Essential Relativity 1358:References and notes 1352:Free motion equation 1248:improve this article 1156:improve this section 1114:Lagrangian mechanics 989:causes frames to be 695:Angular acceleration 687:Rotational frequency 467:Lagrangian mechanics 460:Analytical mechanics 216:Second law of motion 169: 1893:Classical mechanics 1888:Frames of reference 1627:Classical Mechanics 1475:Harald Iro (2002). 1296:, the concept of a 1036:Classical Mechanics 985:, the curvature of 957:Newton's second law 945:classical mechanics 931:with respect to an 547:Harmonic oscillator 525:Equations of motion 160:Classical mechanics 154:Part of a series on 1576:. 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Knowledge (XXG):Translation
Classical mechanics
Second law of motion
History
Timeline
Textbooks
Applied
Celestial
Continuum
Dynamics
Kinematics
Kinetics
Statics
Statistical mechanics
Acceleration
Angular momentum
Couple
D'Alembert's principle
Energy

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