What is the significance of rotation in equations?

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This is sort of a homework question but I'm not looking for an answer. I'm just trying to understand exactly what's going on. It says "Among all the equations of the form [the general second order linear homogeneous partial differential equation], show that the only ones that are unchanged under all rotations (rotationally invariant) havce the form a(uxx + uyy) + bu =0.

What exactly does it mean for an equation to be rotated? I don't understand what's going on here very well.
 
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I would guess it means if you rotate the coordinate system through an arbitrary angle, the form of the equation stays the same, i.e. you don't get a uxy term.
 
Let x= x'cos(\theta)+ y' sin(\theta), y= -x'sin(\theta)+ y'cos(\theta), so that x'= xcos(\theta)- ysin(\theta) and y'= xsin(\theta)+ ycos(\theta), and use the chain rule to replace u_{xx} and u_{yy} with derivatives in terms of x' and y' rather than x and y.

For example, u_x= u_x'(x'_x)+ u_y'(y'_x)= cos(\theta)u_x'+ sin(\theta)u_y'.
 
Are there any good visualization tutorials, written or video, that show graphically how separation of variables works? I particularly have the time-independent Schrodinger Equation in mind. There are hundreds of demonstrations out there which essentially distill to copies of one another. However I am trying to visualize in my mind how this process looks graphically - for example plotting t on one axis and x on the other for f(x,t). I have seen other good visual representations of...
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