The Gauss-Codazzi equations imposed on the elements of the first and the se
cond quadratic forms of a surface embedded in R-3 are integrable by the dre
ssing method. This method allows constructing classes of Combescure-equival
ent surfaces with the same "rotation coefficients." Each equivalence class
is defined by a function of two variables ("master function of a surface").
Each class of Combescure-equivalent surfaces includes the sphere. Differen
t classes of surfaces define different systems of orthogonal coordinates of
the sphere. The simplest class (with the master function zero) corresponds
to the standard spherical coordinates.