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3







                           Differential geometry of surfaces

                                                        in E   3








                           3.1 Equations of surfaces

                        The classical differential geometry of curves and surfaces is presented in many text-
                        books, of which we quote several in the bibliography. Here we are concerned with
                        surfaces embedded in three-dimensional Euclidean space, which may be represented
                        by a variety of mathematical expressions in terms of rectangular cartesian co-ordinates
                        x, y, z.
                          A function of two variables f (x, y) gives a surface

                                                       z = f (x, y).                        (3.1)
                          A function of three variables F(x, y, z) gives a surface

                                                      F(x, y, z) = 0.                       (3.2)

                          Two real parameters u and v maybeused togiveasurface r = r(u, v), or, in terms
                        of three functions of two variables,

                                           x = x(u, v),  y = y(u, v),  z = z(u, v).         (3.3)
                        The parameters u and v here may be referred to as surface (or Gaussian) co-ordinates.
                          We assume that all functions are continuously differentiable unless otherwise stated.
                        In each of the above cases the functions may be defined only for a restricted range of
                        the independent variables. For example, the hemispherical surface obtained by slicing
                                                2
                                            2
                                       2
                        the unit sphere x + y + z = 1 in half through the plane Oxy and discarding the
                        part with z< 0 may be expressed as

                                                                         2
                                                                             2
                                                            2
                                       z = f (x, y) =+ 1 − x − y 2  with x + y   1
                        or
                                                                                      2
                                                                                 2
                                                   2
                                           2
                                               2
                              F(x, y, z) = x + y + z − 1 = 0 with 0   z   1and x + y   1
                        or, in terms of spherical polar co-ordinates θ, ϕ as parameters (Fig. 3.1),
                         x = sin θ cos ϕ,  y = sin θ sin ϕ,  z = cos θ,  with 0   θ   π/2,  0   ϕ   2π.
                                                                                            (3.4)
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