Spherical Coordinates -- from Wolfram MathWorld

Spherical coordinates, also called spherical polar coordinates (Walton 1967, Arfken 1985), are a system of curvilinear coordinates that are natural for describing positions on a sphere or spheroid. Define to be the azimuthal angle in the -plane from the x-axis with (denoted when referred to as the longitude), to be the polar angle (also known as the zenith angle and colatitude, with where is the latitude) from the positive z-axis with , and to be distance (radius) from a point to the origin. This is the convention commonly used in mathematics.

In this work, following the mathematics convention, the symbols for the radial, azimuth, and zenith angle coordinates are taken as , , and , respectively. Note that this definition provides a logical extension of the usual polar coordinates notation, with remaining the angle in the -plane and becoming the angle out of that plane. The sole exception to this convention in this work is in spherical harmonics, where the convention used in the physics literature is retained (resulting, it is hoped, in a bit less confusion than a foolish rigorous consistency might engender).

Unfortunately, the convention in which the symbols and are reversed (both in meaning and in order listed) is also frequently used, especially in physics. This is especially confusing since the identical notation typically means (radial, azimuthal, polar) to a mathematician but (radial, polar, azimuthal) to a physicist. The symbol is sometimes also used in place of , instead of , and and instead of . The following table summarizes a number of conventions used by various authors. Extreme care is therefore needed when consulting the literature.

The spherical coordinates are related to the Cartesian coordinates by

where , , and , and the inverse tangent must be suitably defined to take the correct quadrant of into account.

In terms of Cartesian coordinates,

The scale factors are

so the metric coefficients are

The line element is

the area element

and the volume element

The Jacobian is

The radius vector is

so the unit vectors are

Derivatives of the unit vectors are

The gradient is

and its components are

(Misner et al. 1973, p. 213, who however use the notation convention ).

The Christoffel symbols of the second kind in the definition of Misner et al. (1973, p. 209) are given by

(Misner et al. 1973, p. 213, who however use the notation convention ). The Christoffel symbols of the second kind in the definition of Arfken (1985) are given by

(Walton 1967; Moon and Spencer 1988, p. 25a; both of whom however use the notation convention ).

The divergence is

or, in vector notation,

The covariant derivatives are given by

so

The commutation coefficients are given by

so , where .

so , .

so .

so

Summarizing,

Time derivatives of the radius vector are

The speed is therefore given by

The acceleration is

Plugging these in gives

but

so

Time derivatives of the unit vectors are

The curl is

The Laplacian is

The vector Laplacian in spherical coordinates is given by

To express partial derivatives with respect to Cartesian axes in terms of partial derivatives of the spherical coordinates,

Upon inversion, the result is

The Cartesian partial derivatives in spherical coordinates are therefore

(Gasiorowicz 1974, pp. 167-168; Arfken 1985, p. 108).

The Helmholtz differential equation is separable in spherical coordinates.

See also

Azimuth, Colatitude, Great Circle, Helmholtz Differential Equation--Spherical Coordinates, Latitude, Longitude, Oblate Spheroidal Coordinates, Polar Angle, Polar Coordinates, Polar Plot, Polar Vector, Prolate Spheroidal Coordinates, Zenith Angle Explore this topic in the MathWorld classroom

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References

Anton, H. Calculus with Analytic Geometry, 2nd ed. New York: Wiley, 1984.Apostol, T. M. Calculus, 2nd ed., Vol. 2: Multi-Variable Calculus and Linear Algebra, with Applications to Differential Equations and Probability. Waltham, MA: Blaisdell, 1969.Arfken, G. "Spherical Polar Coordinates." §2.5 in Mathematical Methods for Physicists, 3rd ed. Orlando, FL: Academic Press, pp. 102-111, 1985.Beyer, W. H. CRC Standard Mathematical Tables, 28th ed. Boca Raton, FL: CRC Press, 1987.Bronshtein, I. N.; Semendyayev, K. A.; Musiol, G.; and Muehlig, H. Handbook of Mathematics, 4th ed. New York: Springer-Verlag, 2004.Gasiorowicz, S. Quantum Physics. New York: Wiley, 1974.Korn, G. A. and Korn, T. M. Mathematical Handbook for Scientists and Engineers. New York: McGraw-Hill, 1968.Misner, C. W.; Thorne, K. S.; and Wheeler, J. A. Gravitation. San Francisco, CA: W. H. Freeman, 1973.Moon, P. and Spencer, D. E. "Spherical Coordinates ." Table 1.05 in Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions, 2nd ed. New York: Springer-Verlag, pp. 24-27, 1988.Morse, P. M. and Feshbach, H. Methods of Theoretical Physics, Part I. New York: McGraw-Hill, p. 658, 1953.Walton, J. J. "Tensor Calculations on Computer: Appendix." Comm. ACM 10, 183-186, 1967.Zwillinger, D. (Ed.). "Spherical Coordinates in Space." §4.9.3 in CRC Standard Mathematical Tables and Formulae. Boca Raton, FL: CRC Press, pp. 297-298, 1995.

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Spherical Coordinates

Cite this as:

Weisstein, Eric W. "Spherical Coordinates." From MathWorld--A Wolfram Web Resource. https://mathworld.wolfram.com/SphericalCoordinates.html

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