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Lecture 23: Curvilinear Coordinates (RHB 8.10)

Lecture 23: Curvilinear Coordinates (RHB )It is often convenient to work with variables other than the Cartesian coordinatesxi( =x,y,z). For example in Lecture 15 we met spherical polar and cylindrical polar are two important examples of what are calledcurvilinear Coordinates . In thislecture we set up a formalism to deal with these rather general coordinate we have effectively covered much of the materical in lectures 18 and 19 where westudied surface and volume integrals. There we considered parameterisation of surfaces andvolumes. Here we do the same thing but think about how this realises non-Cartesian Co-ordinate we change from the Cartesian Coordinates (x1,x2,x3) to the Curvilinear Coordinates ,which we denoteui, each of which are functions of thexi:-u1=u1(x1, x2, x3)u2=u2(x1, x2, x3)u3=u3(x1, x2, x3)Theuishould be single-valued, except

Lecture 23: Curvilinear Coordinates (RHB 8.10) It is often convenient to work with variables other than the Cartesian coordinates x i ( = x, y, z). For example in Lecture 15 we met spherical polar and cylindrical polar coordinates.

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Transcription of Lecture 23: Curvilinear Coordinates (RHB 8.10)