Radius of curvature (applications)


Radius of curvature (applications)

The distance from the center of a sphere or ellipsoid to its surface is its radius. The equivalent "surface radius" that is described by radial distances at points along the body's surface is its radius of curvature (more formally, the radius of curvature of a curve at a point is the radius of the osculating circle at that point).With a sphere, the radius of curvature equals the radius. With an oblate ellipsoid (or, more properly, an oblate spheroid), however, not only does it differ from the radius, but it varies, depending on the direction being faced. The extremes are known as the "principal radii of curvature".

Explanation

Imagine driving a car on a curvy road on a completely flat plain (so that the geographic plain is a geometric plane). At any one point along the way, lock the steering wheel in its position, so that the car thereafter follows a perfect circle. The car will, or course, deviate from the road, unless the road is also a perfect circle. The radius of that circle the car makes is the radius of curvature of the curvy road at the point at which the steering wheel was locked. The more sharply curved the road is at the point you locked the steering wheel, the smaller the radius of curvature.

Formula

If gamma : mathbb{R} ightarrow mathbb{R}^n is a parameterized curve in mathbb{R}^n then the radius of curvature at each point of the curve, ho : mathbb{R} ightarrow mathbb{R}, is given by

: ho = frac{sqrt{|gamma'^2(t)| ; |gamma"^2(t)| - (gamma'(t) cdot gamma"(t))^2

or, omitting the parameter ("t") for readability,

: ho = frac{|gamma'|^3}{sqrt{|gamma'|^2 ; |gamma"|^2 - (gamma' cdot gamma")^2.

Elliptic, latitudinal components

The radius extremes of an oblate spheroid are the equatorial radius, or semi-major axis, "a", and the polar radius, or semi-minor axis, "b". The "ellipticalness" of any ellipsoid, like any ellipse, is measured in different ways (e.g., eccentricity and flattening), any and all of which are trigonometric functions of its "angular eccentricity", o!varepsilon,!:

:egin{matrix}{}_{color{white}.}\o!varepsilon=arccos!left(frac{b}{a} ight)=2arctan!left(sqrt{frac{a-b}{a+b, ight).\{}^{color{white}.}end{matrix},!

The primary parameter utilized in identifying a point's vertical position is its latitude.A latitude can be expressed either directly or from the arcsine of a trigonometric product, the "arguments" (i.e., a function's "input") of the factors being the arc path (which defines, and is the azimuth at the equator of, a given great circle, or its elliptical counterpart) and the transverse colatitude, which is a corresponding, vertical latitude ring that defines a point along an arc path/great circle. The relationship can be remembered by the terms' initial letter, L-A-T::::sin(oldsymbol{L})=cos(oldsymbol{A})sin(oldsymbol{T}).,!
Therefore, along a north-south arc path (which equals 0°), the primary quadrant form of latitude equals the transverse colatitude's at a given point.As most introductory discussions of curvature and their radius identify position in terms of latitude, this article will too, with only the added inclusion of a "0" placeholder for more advanced discussions where the arc path is actively utilized: F(L) ightarrow F(0,L)=F(A,T).,!There are two types of latitude commonly employed in these discussions, the planetographic (or planetodetic; for Earth, the customized terms are ""ge"ographic" and ""ge"odetic") and reduced latitudes, phi,! and eta! (respectively):

:egin{matrix}{}_{color{white}.}\eta&=&arctan(cos(o!varepsilon) an(phi));\\phi&=&arctan(sec(o!varepsilon) an(eta)).\{}^{color{white}.}end{matrix},!

The calculation of elliptic quantities usually involves different elliptic integrals, the most basic integrands being E'(0,L),! and its complement, C'(0,L),!:

:egin{matrix}{}_{color{white}.}\E'(0,phi)=C'(0,frac{pi}{2}-phi)!!&=&!!!!!!asqrt{1-(cos(0)sin(phi)sin(o!varepsilon))^2},\\qquad=quadfrac{ab}{C'(0,eta)}!!!&=&!!asqrt{cos^2(o!varepsilon)+(cos(phi)sin(o!varepsilon))^2},\\&=&!!!!!!!!sqrt{(acos(phi))^2+(bsin(phi))^2},qquad\\&=&!!!!!!!!absqrt{left(frac{sin(phi)}{a} ight)^2+left(frac{cos(phi)}{b} ight)^2};qquad\{}^{color{white}.}end{matrix},!

:egin{matrix}{}_{color{white}.}\C'(0,eta)=E'(0,frac{pi}{2}-eta)!!&=&!!asqrt{cos^2(o!varepsilon)+(cos(0)sin(eta)sin(o!varepsilon))^2},\\qquad=quadfrac{ab}{E'(0,phi)}!!!&=&!!!!!!!asqrt{1-(cos(eta)sin(o!varepsilon))^2},qquadqquadquad\\&=&!!!!!!sqrt{(asin(eta))^2+(bcos(eta))^2},qquadqquadquad\\&=&!!!!!!!!absqrt{left(frac{cos(eta)}{a} ight)^2+left(frac{sin(eta)}{b} ight)^2};qquadqquadquad\{}^{color{white}.}end{matrix},!

Thus E'(0,phi)C'(0,eta)=ab,!.

Curvature

A simple, if crude, definition of a circle is "a curved line bent in equal proportions, where its endpoints meet". Curvature, then, is the state and degree of deviation from a straight line—i.e., an "arced line".There are different interpretations of curvature, depending on such things as the planular angle the given arc is dividing and the direction being faced at the surface's point.What is concerned with here is "normal curvature", where "normal" refers to orthogonality, or perpendicularity.There are two principal curvatures identified, a maximum, "κ1", and a minimum, "κ2".

Meridional maximum

::kappa_1=frac{E'^3(0,phi)}{(ab)^2}=frac{ab}{C'^3(0,eta)};,!

:The arc in the meridional, north-south vertical direction at the planetographic equator possesses the maximum curvature, where it "pinches", thereby being the least straight.

Perpendicular minimum

::kappa_2=frac{E'(0,phi)}{a^2}=frac{cos(o!varepsilon)}{C'(0,eta)};,!

:The perpendicular, horizontally directed arc contains the least curvature at the equator, as the equatorial circumference is——at least in mathematical definition——perfectly circular.

The spot of least curvature on an oblate spheroid is at the poles, where the principal curvatures converge (as there is only one facing direction——towards the planetographic equator!) and the surface is most flattened.

Merged curvature

:There are two universally recognized blendings of the principal curvatures: The arithmetic mean is known as the "mean curvature", "H", while the squared geometric mean——or simply the product——is known as the "Gaussian curvature", "K":

::H=frac{kappa_1+kappa_2}{2};qquadKappa=kappa_1kappa_2;,!

Principal radii of curvature

A curvature's radius, "RoC", is simply its reciprocal:

:mathrm{RoC} = frac{1}mathrm{curvature};qquad mathrm{curvature} = frac{1}mathrm{RoC};,!

Therefore, there are two principal radii of curvature: A vertical, corresponding to "κ1", and a horizontal, corresponding to "κ2". Most introductions to the principal radii of curvature provide explanations independent to their curvature counterparts, focusing more on positioning and angle, rather than shape and contortion.

Meridional radius of curvature

:The vertical radius of curvature is parallel to the "principal vertical", which is the facing, "central meridian" and is known as the "meridional radius of curvature, M" (alternatively, "R1" or "p"):

::M=widehat{M}(0,phi)=;frac{(ab)^2}{E'^3(0,phi)};=frac{1}{kappa_1}=;frac{C'^3(0,eta)}{ab};= ilde{M}(0,eta);,!:::"(Crossing the planetographic equator, {}_{M=bcos(o!varepsilon)=frac{b^2}{a,!.}"

Normal radius of curvature

:The horizontal radius of curvature is perpendicular (again, meaning "normal" or "orthogonal") to the central meridian, but parallel to a great arc (be it spherical or elliptical) as it crosses the "prime vertical", or "transverse equator" (i.e., the meridian 90° away from the facing principal meridian——the "horizontal meridian"), and is known as the "transverse (equatorial)", or normal, "radius of curvature, N" (alternatively, "R2" or "v"):

::N=widehat{N}(0,phi)=;frac{a^2}{E'(0,phi)};=frac{1}{kappa_2}=;frac{a}{b}C'(0,eta);= ilde{N}(0,eta);,!:::"(Along the planetographic equator, which is an ellipsoid's"::: "only true great circle, {}_{N=bsec(o!varepsilon)=a},!.)"

Polar convergence

:Just as with the curvature, at the poles "M" and "N" converge, resulting in an equal radius of curvature:::::M=N=asec(o!varepsilon)=frac{a^2}{b}.,!

Merged radius of curvature

:There are two possible, basic "means":

::*"Mean radius of curvature", which is the arithmetic mean::::frac{M+N}{2}=frac{frac{1}{kappa_1}+frac{1}{kappa_2{2}=frac{M}{2}!cdot!left(1+frac{a^4}{(bN)^2} ight)=frac{N}{2}!cdot!left(frac{(bN)^2}{a^4}+1 ight);,!

::*"Radius of mean curvature", which is the harmonic mean::::frac{2}{frac{1}{M}+frac{1}{N=frac{2}{kappa_1+kappa_2}=frac{1}{H}=frac{2M}{1+frac{(bN)^2}{a^4=frac{2N}{frac{a^4}{(bN)^2}+1}.,!

:If these means are then arithmetically and harmonically averaged together, with the results reaveraged until the two averages converge, the result will be the arithmetic-harmonic mean, which equals the geometric mean and, in turn, equals the square root of the "inverse of Gaussian curvature"!

::sqrt{M!N}=sqrt{frac{1}{Kappa=sqrt{frac{1}{kappa_1kappa_2=frac{b}{a^2}N^2;,!

:While, at first glance, the squared form may be regarded as either the "radius of Gaussian curvature", "radius of Gaussian curvature2" or "radius2 of Gaussian Curvature", none of these terms quite fit, as Gaussian Curvature is the product of two curvatures, rather than a singular curvature.

Applications and examples

*For the use in differential geometry, see Cesàro equation.

Radius of curvature is also used in a three part equation for bending of beams.

ee also

*Radius of curvature (optics)
*Bend radius
*Curvature
*Diameter

External links

* [http://www.fas.org/irp/agency/nima/nug/gloss_t.html USIGS Glossary] (Definitions of "transverse" terms)
* [http://www.geom.uiuc.edu/zoo/diffgeom/surfspace/concepts/curvatures/prin-curv.html The Geometry Center: Principal Curvatures]
* [http://www-math.mit.edu/18.013A/HTML/chapter15/section03.html 15.3 Curvature and Radius of Curvature]
* [http://mathworld.wolfram.com/PrincipalCurvatures.html MathWorld: Principal Curvatures]
* [http://mathworld.wolfram.com/PrincipalRadiusofCurvature.html MathWorld: Principal Radius of Curvature]
* [http://www.brown.edu/Students/OHJC/hm4/k.htm The History of Curvature]


Wikimedia Foundation. 2010.

Look at other dictionaries:

  • Radius of curvature (optics) — Radius of curvature has specific meaning and sign convention in optical design. A spherical lens or mirror surface has a center of curvature located in (x, y, z) either along or decentered from the system local optical axis. The vertex… …   Wikipedia

  • Radius of curvature — may refer to: Radius of curvature (mathematics) Radius of curvature (optics) Radius of curvature (applications), in geodesy and materials science The reciprocal of the curvature, in differential geometry Radius, for a sphere (lingo) The radius of …   Wikipedia

  • Curvature — In mathematics, curvature refers to any of a number of loosely related concepts in different areas of geometry. Intuitively, curvature is the amount by which a geometric object deviates from being flat, or straight in the case of a line, but this …   Wikipedia

  • Curvature of Riemannian manifolds — In mathematics, specifically differential geometry, the infinitesimal geometry of Riemannian manifolds with dimension at least 3 is too complicated to be described by a single number at a given point. Riemann introduced an abstract and rigorous… …   Wikipedia

  • Curvature form — In differential geometry, the curvature form describes curvature of a connection on a principal bundle. It can be considered as an alternative to or generalization of curvature tensor in Riemannian geometry. Contents 1 Definition 1.1 Curvature… …   Wikipedia

  • Radius — For other uses, see Radius (disambiguation). Circle illustration In classical geometry, a radius of a circle or sphere is any line segment from its center to its perimeter. By extension, the radius of a circle or sphere is the length of any such… …   Wikipedia

  • Scalar curvature — In Riemannian geometry, the scalar curvature (or Ricci scalar) is the simplest curvature invariant of a Riemannian manifold. To each point on a Riemannian manifold, it assigns a single real number determined by the intrinsic geometry of the… …   Wikipedia

  • Mean curvature — In mathematics, the mean curvature H of a surface S is an extrinsic measure of curvature that comes from differential geometry and that locally describes the curvature of an embedded surface in some ambient space such as Euclidean space. The… …   Wikipedia

  • Principal curvature — Saddle surface with normal planes in directions of principal curvatures In differential geometry, the two principal curvatures at a given point of a surface are the eigenvalues of the shape operator at the point. They measure how the surface… …   Wikipedia

  • Minimum railway curve radius — 90 foot (27.43 m) radii on the elevated 4 ft 8 1⁄2 in (1,435 mm) Chicago L . There is no room for longer radii at this street intersection The minimum railway curve radius, the shortest design radius, has an… …   Wikipedia


Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”

We are using cookies for the best presentation of our site. Continuing to use this site, you agree with this.