Within that context, just grokking R^2 or R^3 would be great progress. To be fair, the article does present the fundamental identity, uv = u.v + u /\ v, where u.v is the usual dot product (scalar denoting relative projective size) and u /\ v = |u||v|sinθi (something related to area and the plane induced by u and v). Even if the article does exemplify with R^2 by defining i = xy, and then dropping the ball: "i is interpreted to mean the plane generated by x and y". I can't grok this part :(
* This looks like (almost) a circular definition, defining uv in terms of the specific xy, where x and y are the two orthonormal R^2 vectors forming the basis. What is xy? Is it a scalar? A vector? A normal vector? How does a normal vector work in R^2?. A tensor of some dimensions? For example, assuming x = (1,0) and y = (0,1), how does one compute i = xy?
* Plane generated how? a u + b v, given any two scalars a and b?
* When moving to R^3, i'd think uv / xy define a plane. What does uvw / xyz mean?
* Minor quibble, is it sin(θ * i) or sin(θ) * i?