On an oriented 2-manifold, a
Riemannian metric induces a complex structure using the passage to
isothermal coordinates. If the Riemannian metric is given locally as : ds^2 = E \, dx^2 + 2F \, dx \, dy + G \, dy^2, then in the complex coordinate
z =
x + i
y, it takes the form : ds^2 = \lambda|dz +\mu \, d\overline{z}|^2, where :\lambda = \frac14 \left( E + G + 2\sqrt{EG - F^2} \right),\ \ \mu = \frac1{4\lambda} (E - G + 2iF), so that
λ and
μ are smooth with
λ > 0 and |
μ| ds^2 = \rho (du^2 + dv^2) with
ρ > 0 smooth. The complex coordinate
w =
u + i
v satisfies :\rho \, |dw|^2 = \rho |w_z|^2 \left| dz + {w_{\overline{z}}\over w_z} \, d\overline{z}\right|^2, so that the coordinates (
u,
v) will be isothermal locally provided the
Beltrami equation : {\partial w\over \partial \overline{z}} = \mu {\partial w\over \partial z} has a locally diffeomorphic solution, i.e. a solution with non-vanishing Jacobian. These conditions can be phrased equivalently in terms of the
exterior derivative and the
Hodge star operator . and will be isothermal coordinates if , where is defined on differentials by . Let be the
Laplace–Beltrami operator. By standard elliptic theory, can be chosen to be
harmonic near a given point, i.e. , with non-vanishing. By the
Poincaré lemma has a local solution exactly when . This condition is equivalent to , so can always be solved locally. Since is non-zero and the square of the Hodge star operator is −1 on 1-forms, and must be linearly independent, so that and give local isothermal coordinates. The existence of isothermal coordinates can be proved by other methods, for example using the
general theory of the Beltrami equation, as in , or by direct elementary methods, as in and . From this correspondence with compact Riemann surfaces, a classification of closed orientable Riemannian 2-manifolds follows. Each such is conformally equivalent to a unique closed 2-manifold of
constant curvature, so a
quotient of one of the following by a
free action of a
discrete subgroup of an
isometry group: • the
sphere (curvature +1) • the
Euclidean plane (curvature 0) • the
hyperbolic plane (curvature −1). File:Orange Sphere.png|genus 0 File:Orange Torus.png|genus 1 File:Orange Genus 2 Surface.png|genus 2 File:Orange Genus 3 Surface.png|genus 3 The first case gives the 2-sphere, the unique 2-manifold with constant positive curvature and hence positive
Euler characteristic (equal to 2). The second gives all flat 2-manifolds, i.e. the
tori, which have Euler characteristic 0. The third case covers all 2-manifolds of constant negative curvature, i.e. the
hyperbolic 2-manifolds all of which have negative Euler characteristic. The classification is consistent with the
Gauss–Bonnet theorem, which implies that for a closed surface with constant curvature, the sign of that curvature must match the sign of the Euler characteristic. The Euler characteristic is equal to 2 – 2
g, where
g is the genus of the 2-manifold, i.e. the number of "holes". ==Methods of proof==