|
A natural equation is an equation which specifies a curve independent of any choice of coordinates or parameterization. The study of natural equations began with the
following problem: given two functions of one parameter, find the space curve for which the functions are the curvature and torsion.
Euler gave an integral solution for plane curves (which always have torsion ). Call the
angle between the tangent line to the curve and the x-axis the tangential
angle, then
 |
(1)
|
where is the curvature. Then the equations
where is the torsion,
are solved by the curve with parametric
equations
The equations and are called
the natural (or intrinsic)
equations of the space curve. An equation expressing a plane curve in terms of and radius
of curvature (or ) is called
a Cesàro equation, and
an equation expressing a plane curve in terms of and is called a Whewell equation.
Among the special planar cases which can be solved in terms of elementary functions are the circle,
logarithmic spiral, circle involute, and epicycloid.
Enneper showed that each of these is the projection of a helix
on a conic surface of revolution
along the axis of symmetry. The above cases correspond to the cylinder, cone,
paraboloid, and sphere.
Cesàro, E. Lezioni di Geometria Intrinseca. Napoli, Italy, 1896.
Euler, L. Comment. Acad. Petropolit. 8, 66-85, 1736.
Gray, A. Modern Differential Geometry of Curves and Surfaces with Mathematica,
2nd ed. Boca Raton, FL: CRC Press, pp. 138-139, 1997.
Melzak, Z. A. Companion to Concrete Mathematics, Vol. 2. New York:
Wiley, 1976.
Struik, D. J. Lectures on Classical Differential Geometry. New York:
Dover, pp. 26-28, 1988.
|