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PARAMETRIC SURFACE

A 'parametric surface' is a surface defined by a parametric equation, involving two parameters, most commonly (''s'', ''t'') or (''u'',''v''). Typically they will be surfaces in three dimensions. They are of great use in such vector calculus applications as Stokes' theorem.
The simplest example of a parametric surface is the ''x''-''y'' plane. Here the surface is defined by the equation
:S:mathbf{R}^2mapstomathbf{R}^3, S:(s,t) o(s,t,0).,
The mapping ''S'' is a 'parameterization' of the surface and the variables, ''s'', ''t'' are said to be the 'parameters' of the mapping. Any pair of value of ''s'' and ''t'' will give a point on the surface.
Another example of a parametrized surface is the (capless) cylinder given by
:r(u, v) = Big(x(u, v), y(u, v), z(u, v) Big) = Big(a cos(u), a sin(u), v Big),
Considering the equation as representing a circle in the plane, it is evident that this represents a cylinder. It is then allowed to take on values of ''z''.
Many different parameterizations can give the same surface, for example the parametrisation
:S(s,t)=(s+t,s-t,0),
also gives the ''x''-''y'' plane.
Surfaces can be defined in other ways, the plane can be defined as an algebraic surface which is the set of zeros of a polynomial equation. The ''x''-''y'' plane can be defined as the zeros of the function
:f:mathbf{R}^3mapstomathbf{R}, f(x,y,z)=z,
giving the surface
:f^{-1}(0), z=0.,
This can be generalised to the zeros of any implicit function. Other methods for defining surfaces include minimal surfaces defined through a process of minimising energy, soap bubbles are an example of this.
The unit sphere can be parameterized by
:s( heta,phi) = (sin heta ; cos phi, sin heta ; sin phi, cos heta),
where 0 leq heta leq pi, and -pi < phi leq pi , are the two parameters. This parametrisation breaks down at the north and south poles where the more than one set of parameters give the same point.

Contents
Local differential geometry
Directional derivatives
Surface area
First fundamental form
Second fundamental form
Curvature
See also
Web links

Local differential geometry


The local shape of a surface can be characterised by considering the partial derivatives of the parametrisation.
Notation: here lower case letters will be used for points and curves in the parameter space, which will be taken to be the plane, upper case will be used for points and curves on the surface. Likewise lower case vectors ec u will be tangent vectors in the plane and upper case vectors ec U will be the corresponding tangent vectors to the surface in 'R'3.
For any point on a parameterized surface ''S''(''s'',''t''), two tangent vectors are defined by taking the partial derivatives ec U={partial Soverpartial s} and ec V={partial Sover partial t}. Provided neither ec U, ec V are zero and they are not parallel then they define a tangent plane. The tangent plane will have a normal vector ec N= ec U imes ec V which will be at right angles to any tangent vectors, this can be made into a 'unit normal' vector by dividing by its length. The tangent plane does not depend on the particular parametrisation chosen, and the unit length normal vector will only change up to sign (that is point in the opposite direction).
Directional derivatives

The partial derivatives can be expanded to give a directional derivative, a map from the set of tangent vectors at a point, ''p'', in the plane to the set of tangent vectors to the surface at ''S''(''p''). If ec w=(lpha,eta) is a tangent vector in the plane then its directional derivative will be
:dSlangle ec w
angle=lpha ec U+eta ec V=lpha {partial Soverpartial s}+eta{partial Soverpartial t}.
A parametrised curve in the plane which has tangent vector ec w will be mapped to a curve on the surface with tangent vector dSleftlangle ec w
ight
angle.
The second directional derivative is constructed by differentiating the first directional derivative. This will give a bi-linear map on pairs of tangent vectors. If ec u=(lpha,eta), ec v=(gamma,delta) then
:d^2Slangle ec u, ec v
angle=lphagamma{partial^2Soverpartial s^2}+(lphadelta+etagamma){partial^2Soverpartial spartial t}+etadelta{partial^2Soverpartial t^2}
higher derivatives can be constructed in a similar fashion.
Surface area

The surface area can also be calculated by integrating the length of the normal vector over the uv rectangle bounding the area in question. In other words, to find the surface area of the rectangle bounded by ale ule b And c le vle d where ec r(u,v)=langle x(u,v),y(u,v),z(u,v)
angle, evaluate
:
int_{a}^{b}int_{c}^{d}left | rac{partial ec r}{partial v} imes rac{partial ec r}{partial u}
ight |;partial v;partial u.

As simple as this formula may seem, every symbol stands for an operation so complex that it often leads to impossible integrals which can only be approximated numerically. Typically, evaluation of the surface area is only done by a CAS, because evaluating it by hand is very time consuming. Except for simple formulas (e.g. the torus), surface area can rarely be given in exact notation.
First fundamental form

Main articles: First fundamental form

The 'first fundamental form', I_plangle ec u, ec v
angle, is an inner product and it captures the metric information about the surface. It is used to calculate distances and angles. If ec u, ec v are tangent vectors in the plane then:
I_plangle ec u, ec v
angle=dSlangle ec u
anglecdot dSlangle ec v
angle.
This form is symmetric and bilinear so I_plangle ec u, ec v
angle=I_plangle ec v, ec u
angle, I_plangle 2 ec u, ec v
angle=2I_plangle ec u, ec v
angle, etc.
If ''c'':'R'→'R'2 is a curve in the plane with tangent vector ec u at ''p'', and ''C''(''t'')=''S''(''c''(''t'')) is its image on the surface, then I_plangle ec u, ec u
angle will be the square of the speed of ''C''. If I_p=1, for all points on ''c'' then ''C'' will be a 'unit speed curve'. The length of ''C'' can be found by integrating I_plangle ec u, ec u
angle. The angle between two curves on the surface is found from I_plangle ec u, ec v
angle where ec u, ec v are the tangent vectors of the two curves in the plane.
Second fundamental form

Main articles: Second fundamental form

For a given parametrisation a continuous unit normal vector field, ec N:mathbf{R}^2mapstomathbf{R}^3 and the directional derivative d ec Nlangle ec u
angle can be found.
The 'second fundamental form', II_plangle ec u, ec v
angle, captures second derivative information. It is defined by:
:II_plangle ec u, ec v
angle=d^2Slangle ec u, ec v
anglecdot ec N.
Differentiation ec Ncdot dSlangle u
angle=0 in the direction ec v gives
:d ec Nlangle v
anglecdot dSlangle ec u
angle+ ec Ncdot d^2Slangle ec u, ec v
angle+ ec Ncdot dSlangle d ec ulangle ec v
angle
angle=0.
The last term is always zero, and the equations can be rearranged to give
:II_plangle ec u, ec v
angle=-d ec Nlangle ec u
anglecdot dSlangle ec v
angle.
It is also symmetric and bilinear.
Curvature

The surface curves can be analysed by examining the first and second fundamental forms, to give Gaussian curvature, mean curvature and principal curvature.
Let E=Ilangle ec u, ec u
angle, F=Ilangle ec u, ec v
angle, G=Ilangle ec v, ec v
angle,
l=IIlangle ec u, ec u
angle, m=IIlangle ec u, ec v
angle, n=IIlangle ec v, ec v
angle. The
'Gaussian curvature' is
:K={ln-m^2over EG-F^2}
and the 'mean curvature' is
:H={En-2Fm+Glover 2(EG-F^2)}.
These curvatures are independent of the parametrisation used, and hence important tools for analysing the surface.
The sign of the Gaussian curvature determines whether the surface is locally convex (''G''>0) or saddle shaped (''G''<0). The terms 'elliptical' and 'hyperbolic' are used for these two cases. When the Gaussian curvature is zero the surface is 'parabolic'. In general parabolic points form a curve on the surface called the parabolic line. The Gaussian curvature is intimately connected with the Gauss map.
The equation
:IIlangle ec u, ec u
angle=kappa Ilangle ec u, ec u
angle
generally has two eigenvectors ec p and ec q with corresponding eigenvalues kappa_p, kappa_q. Let ec P=dslangle ec p
angle, ec Q=dslangle ec q
angle, choose ec p, ec q so that ec P, ec Q are of unit length.
ec P, ec Q are called the 'principal directions' and kappa_p, kappa_q are the 'principal curvatures'. It can be shown that the principal directions are orthogonal, and
:Ilangle ec p, ec p
angle=1, Ilangle ec p, ec q
angle=0, Ilangle ec q, ec q
angle=1,
IIlangle ec p, ec p
angle=kappa_p, IIlangle ec p, ec q
angle=0, IIlangle ec q, ec q
angle=kappa_q.
Hence, the Gaussian curvature is G=kappa_pkappa_q and the mean curvature is H={1over 2}(kappa_p+kappa_q). The principal directions are the directions of maximum and minimum curvature for curves on the surface. If both have the same sign the surface will be locally convex (ellipitical) and if they have opposite signs then the surface will be saddle shaped (hyperbolic). Parabolic points occur when one of the principal curvatures is zero.
There can be points where the eigenvector-equation is degenerate. Here all directions are principal and the principal curvatures are equal. At such points called umbilics the surface is locally spherical. Generally these occur at isolated points in the ellipitical region.

See also



Spline (mathematics)

Web links



Java applets demonstrate the parametrization of a helix surface

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