A point plotted using the spherical coordinate system

In mathematics, the spherical coordinate system is a coordinate system for representing geometric figures in three dimensions using three coordinates: the radial distance of a point from a fixed origin, the zenith angle from the positive z-axis, and the azimuth angle from the positive x-axis.

Notation

Several different conventions exist for representing the three coordinates. In accordance with the International Organisation for Standardisation (ISO 31-11), in physics they are typically notated as (r, θ,φ ) for radial distance, zenith, and azimuth, respectively.

In (American) mathematics, the notation for zenith and azimuth are reversed as φ is used to denote the zenith angle and θ is used to denote the azimuthal angle. A further complication is that some mathematics texts list the azimuth before the zenith, but this convention is left-handed and should be avoided. The "math" convention has the advantage of being most compatible in the meaning of θ with the traditional notation for the two-dimensional polar coordinate system and the three-dimensional cylindrical coordinate system, while the "physics" convention has broader acceptance geographically. Some users of the "physics" convention also use φ for polar coordinates to avoid the first problem (as is the standard ISO for cylindrical coordinates). Other notation uses � for radial distance.Eric W. Weisstein (2005-10-26). Spherical Coordinates. MathWorld. Retrieved on 2007-04-10. The notation convention of the author of any work pertaining to spherical coordinates should always be checked before using the formulas and equations of that author. This article uses the standard convention.

Definition

The coordinate surfaces of the spherical coordinates (r, θ, φ). The red sphere shows the points with r=2, the blue cone shows the points with θ=45°, and the yellow half-plane shows the points with φ=-60°. The z-axis is vertical and the x-axis is highlighted in green. The three surfaces intersect at the point P with those coordinates (shown as a black sphere); the Cartesian coordinates of P are roughly (0.707, -1.225, 1.414).

The three coordinates (r, θ, φ) are defined as:

• r ≥ 0 is the distance from the origin to a given point P.
• 0 ≤ θ ≤ Ï€ is the angle between the positive z-axis and the line formed between the origin and P.
• 0 ≤ φ < 2Ï€ is the angle between the positive x-axis and the line from the origin to the P projected onto the xy-plane.

φ is referred to as the azimuth, while θ is referred to as the zenith, colatitude or polar angle.

θ and φ lose significance when r = 0 and φ loses significance when sin(θ) = 0 (at θ = 0 and θ = π).

To plot a point from its spherical coordinates, go r units from the origin along the positive z-axis, rotate θ about the y-axis in the direction of the positive x-axis and rotate φ about the z-axis in the direction of the positive y-axis.

Coordinate system conversions

As the spherical coordinate system is only one of many three-dimensional coordinate systems, there exist equations for converting coordinates between the spherical coordinate system and others.

Cartesian coordinate system

Further information: Cartesian coordinate system

The three spherical coordinates are obtained from Cartesian coordinates by:

$r=\backslash sqrt\{x^2\; +\; y^2\; +\; z^2\}$

$\{\backslash theta\}=\backslash arctan\; \backslash left(\; \backslash frac\{\backslash sqrt\{x^2\; +\; y^2\}\}\{z\}\; \backslash right)=\backslash arccos\; \backslash left(\; \{\backslash frac\{z\}\{\backslash sqrt\{x^2\; +\; y^2\; +\; z^2\}\}\}\; \backslash right)$

$\{\backslash varphi\}=\backslash arctan\; \backslash left(\; \{\backslash frac\{y\}\{x\}\}\; \backslash right).$

Note that the arctangent must be defined suitably so as to take account of the correct quadrant of $y/x$. The atan2 or equivalent function accomplishes this for computational purposes.

Conversely, Cartesian coordinates may be retrieved from spherical coordinates by:

$\{x\}=r\; \backslash ,\; \backslash sin\backslash theta\; \backslash ,\; \backslash cos\backslash varphi\; \backslash quad$

$\{y\}=r\; \backslash ,\; \backslash sin\backslash theta\; \backslash ,\; \backslash sin\backslash varphi\; \backslash quad$

$\{z\}=r\; \backslash ,\; \backslash cos\backslash theta.\; \backslash quad$

Geographic coordinate system

Further information: Geographic coordinate system

The geographic coordinate system is an alternate version of the spherical coordinate system, used primarily in geography though also in mathematics and physics applications. In geography, � is usually dropped or replaced with a value representing elevation or altitude.

Latitude $\{\backslash delta\}\backslash ,$ is the complement of the zenith or colatitude, and can be converted by:

$\{\backslash delta\}=90^\backslash circ\; -\; \backslash theta$, or

$\{\backslash theta\}=90^\backslash circ\; -\; \backslash delta$,

though latitude is typically represented by θ as well. This represents a zenith angle originating from the xy-plane with a domain -90° ≤ θ ≤ 90°. The longitude is measured in degrees east or west from 0°, so its domain is -180° ≤ φ ≤ 180°.

Cylindrical coordinate system

Further information: Cylindrical coordinate system

The cylindrical coordinate system is a three-dimensional extrusion of the polar coordinate system, with an z coordinate to describe a point\'s height above or below the xy-plane. The full coordinate tuple is (r, φ, z).

Cylindrical coordinates may be converted into spherical coordinates by:

$r=\backslash sqrt\{\backslash rho^2+z^2\}$

$\{\backslash theta\}=\backslash arctan\backslash frac\{\backslash rho\}\{z\}$

$\{\backslash varphi\}=\backslash varphi\; \backslash quad$

Spherical coordinates may be converted into cylindrical coordinates by:

$\backslash rho\; =\; r\; \backslash sin\; \backslash theta\; \backslash ,$

$\backslash varphi\; =\; \backslash varphi\; \backslash ,$

$z\; =\; r\; \backslash cos\; \backslash theta\; \backslash ,$

Applications

The geographic coordinate system applies the two angles of the spherical coordinate system to express locations on Earth, calling them latitude and longitude. Just as the two-dimensional Cartesian coordinate system is useful on the plane, a two-dimensional spherical coordinate system is useful on the surface of a sphere. In this system, the sphere is taken as a unit sphere, so the radius is unity and can generally be ignored. This simplification can also be very useful when dealing with objects such as rotational matrices.

Spherical coordinates are useful in analyzing systems that are

ymmetrical about a point; a sphere that has the Cartesian equation x² + y² + z² = c² has the very simple equation r = c in spherical coordinates. An example is in solving a triple integral with a sphere as its domain.

The surface element for a spherical surface is

$\backslash mathrm\; dS=r^2\backslash sin\backslash theta\backslash ,\backslash mathrm\; d\backslash theta\backslash ,\backslash mathrm\; d\backslash varphi$

The volume element is

$\backslash mathrm\; dV=r^2\backslash sin\backslash theta\backslash ,\backslash mathrm\; dr\backslash ,\backslash mathrm\; d\backslash theta\backslash ,\backslash mathrm\; d\backslash varphi$

Spherical coordinates are the natural coordinates for describing and analyzing physical situations where there is spherical symmetry, such as the potential energy field surrounding a sphere (or point) with mass or charge. Two important partial differential equations, Laplace\'s equation and the Helmholtz equation, allow a separation of variables in spherical coordinates. The angular portions of the solutions to such equations take the form of spherical harmonics.

Another application is ergonomic design, where r is the arm length of a stationary person and the angles describe the direction of the arm as it reaches out.

The concept of spherical coordinates can be extended to higher dimensional spaces and are then referred to as hyperspherical coordinates.

Kinematics

In spherical coordinates the position of a point is written,

$\backslash mathbf\{r\}\; =\; \backslash rho\; \backslash mathbf\{e\}\_\backslash rho$

its velocity is then,

$\backslash mathbf\{v\}\; =\; \backslash dot\backslash rho\; \backslash mathbf\{e\}\_\backslash rho\; +\; \backslash rho\backslash dot\backslash theta\; \backslash mathbf\{e\}\_\backslash theta\; +\; \backslash rho\backslash dot\backslash phi\backslash sin\backslash theta\; \backslash mathbf\{e\}\_\backslash phi$

and its acceleration is,

$\backslash mathbf\{a\}\; =\; \backslash left(\; \backslash ddot\backslash rho\; -\; \backslash rho\backslash dot\backslash theta^2\; -\; \backslash rho\backslash dot\backslash phi^2\backslash sin^2\backslash theta\; \backslash right)\backslash mathbf\{e\}\_\backslash rho$

$+\; \backslash left(\; \backslash rho\backslash ddot\backslash theta\; +\; 2\backslash dot\backslash rho\backslash dot\backslash theta\; -\; \backslash rho\backslash dot\backslash phi^2\backslash sin\backslash theta\backslash cos\backslash theta\; \backslash right)\; \backslash mathbf\{e\}\_\backslash theta$

$+\; \backslash left(\; \backslash rho\backslash ddot\backslash phi\backslash sin\backslash theta\; +\; 2\backslash dot\backslash rho\backslash dot\backslash phi\backslash sin\backslash theta\; +\; 2\backslash rho\backslash dot\backslash theta\backslash dot\backslash phi\backslash cos\backslash theta\; \backslash right)\; \backslash mathbf\{e\}\_\backslash phi$

Notes

See also

• Vector fields in cylindrical and spherical coordinates
• Del in cylindrical and spherical coordinates
• List of canonical coordinate transformations
• Sphere
• Hypersphere
• Orthogonal coordinates
• Two dimensional orthogonal coordinate systems

• Three dimensional orthogonal coordinate systems

Bibliography

• Morse PM, Feshbach H (1953). Methods of Theoretical Physics, Part I. New York: McGraw-Hill, p. 658. ISBN 0-07-043316-X, LCCN 52-11515. 

• Margenau H, Murphy GM (1956). The Mathematics of Physics and Chemistry. New York: D. van Nostrand, pp. 177–178. LCCN 55-10911. 

• Korn GA, Korn TM (1961). Mathematical Handbook for Scientists and Engineers. New York: McGraw-Hill, pp. 174–175. LCCN 59-14456, ASIN B0000CKZX7. 

• Sauer R, Szabó I (1967). Mathematische Hilfsmittel des Ingenieurs. New York: Springer Verlag, pp. 95–96. LCCN 67-25285. 

• Moon P, Spencer DE (1988). "Spherical Coordinates (r, θ, ψ)", Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions, corrected 2nd ed., 3rd print ed., New York: Springer-Verlag, pp. 24–27 (Table 1.05). ISBN 978-0387184302. 

External links

MathWorld description of spherical coordinates

This article is licensed under the GNU Free Documentation License. It uses material from Wikipedia

This article is licensed under the GNU Free Documentation License. It uses material from Wikipedia