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・ Inverse quadratic interpolation
・ Inverse Raman effect
・ Inverse ratio ventilation
・ Inverse relation
・ Inverse resolution
・ Inverse scattering problem
・ Inverse scattering transform
・ Inverse search
・ Inverse second
・ Inverse semigroup
・ Inverse square root potential
・ Inverse Symbolic Calculator
・ Inverse synthetic aperture radar
・ Inverse system
・ Inverse transform sampling
Inverse trigonometric functions
・ Inverse Warburg Effect
・ Inverse-chi-squared distribution
・ Inverse-gamma distribution
・ Inverse-square law
・ Inverse-variance weighting
・ Inverse-Wishart distribution
・ Invershin
・ Invershin railway station
・ Inversija
・ Inversion
・ Inversion (artwork)
・ Inversion (discrete mathematics)
・ Inversion (evolutionary biology)
・ Inversion (geology)


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Inverse trigonometric functions : ウィキペディア英語版
Inverse trigonometric functions

In mathematics, the inverse trigonometric functions (occasionally called cyclometric functions〔For example 〕) are the inverse functions of the trigonometric functions (with suitably restricted domains). Specifically, they are the inverses of the sine, cosine, tangent, cotangent, secant, and cosecant functions. They are used to obtain an angle from any of the angle's trigonometric ratios. Inverse trigonometric functions are widely used in engineering, navigation, physics, and geometry.
==Notation==
There are several notations used for the inverse trigonometric functions.
The most common convention is to name inverse trigonometric functions using an arc- prefix, e.g., , , , etc. This convention is used throughout the article.
When measuring in radians, an angle of θ radians will correspond to an arc whose length is rθ, where r is the radius of the circle. Thus, in the unit circle, "the arc whose cosine is x" is the same as "the angle whose cosine is x", because the length of the arc of the circle in radii is the same as the measurement of the angle in radians. Similar, in computer programming languages (also Excel) the inverse trigonometric functions are usually called asin, acos, atan.
The notations , , , etc., as introduced by John Herschel in 1813, are often used as well, but this convention logically conflicts with the common semantics for expressions like , which refer to numeric power rather than function composition, and therefore may result in confusion between multiplicative inverse and compositional inverse. The confusion is somewhat ameliorated by the fact that each of the reciprocal trigonometric functions has its own name—for example, = . Nevertheless, certain authors advise against using it for its ambiguity.
Another convention used by a few authors is to use a majuscule (capital/upper-case) first letter along with a −1 superscript, e.g., , , , etc., which avoids confusing them with the multiplicative inverse, which should be represented by , , etc.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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