*If you're already familiar with the Bezier formulation of curves, then you shouldn't feel overwhelmed by the topics presented here. If you're not, read the previous article "The Practical Guide to Bezier Curves".*This article is a primer for the next article in this series. I believe this article and its companions to be essential to understanding a very common and powerful set of curves and surfaces.

# Disclaimer

**The information presented here might seem new to anyone familiar with traditional B-spline formulations. It's not meant as a replacement to the mathematical methods, which are almost certainly more efficient. This article is meant, however, to introduce the concepts behind B-splines in a more intuitive manner than simply deciphering things through equations. This graphical approach is mathematically equivalent to the traditional definitions of B-splines with full generality preserved.**

# What is a B-spline?

You can think of a B-spline as just a series of Bezier curves joined together with a certain degree of continuity. What determines how these curves are joined? The answer is the knot vector. For example, the knot vector or a degree-3 B-spline \( U = \{ 0,0,0,0,1,2,2,2,2 \} \) says that this B-spline consists of 2 Bezier curves with parameter domains \([0,1]\) and \([1,2]\), they have Bezier end conditions (meaning that the control points at the ends of the curve are on the curve), and that the continuity of the curves at u=1 is \(C^2\). How did we know all that just from the knot vector? To understand this, we have to introduce a notation invented by Dr. Lyle Ramshaw called*polar form*.

# Polar Form

Polar form is a kind of notation that allows us to associate the values in the knot vector to specific control points. This allows us to perform mathematical operations on the B-spline using graphical techniques. There are 4 rules that summarize how to use polar form.- For a degree-n Bezier curve defined on a parameter interval [a,b], the control points of the curve are labeled as \( P_i = P(u_1,u_2,\cdots,u_n)\), where \( u_j = \begin{cases}a,& j \leq n-i \\ b,& otherwise \end{cases} \).
- For a degree-n B-spline with a knot vector \( \{ t_1,t_2,t_3,t_4,\cdots \} \), the polar form of each control point is a group of n adjacent knots. In polar form, the first and last knot values give us no information, so we leave them off. For example, a "regular" degree-3 B-spline would have a knot vector like \( U = \{ 0,0,0,0,1,2,2,2,2 \} \), but in polar form we would see the knot vector as \( U = \{ 0,0,0,1,2,2,2 \} \). For this example, the control points would be labeled as: \( P_0 = P(0,0,0)\),\( P_1 = P(0,0,1)\),\( P_2 = P(0,1,2)\),\( P_3 = P(1,2,2)\),\( P_4 = P(2,2,2) \).
- All combinations of the polar values are equivalent. For example, \( P(1,0,0,2) = P(0,1,0,2) = P(0,0,1,2) = P(2,1,0,0) = \cdots \) and so on.
- Given 2 polar values that only differ by one value, such as \( P_1 = P(u_1,u_2,u_3,\cdots,a) \) and \( P_2 = P(u_1,u_2,u_3,\cdots,b) \), we can find a value \( P_3 = P(u_1,u_2,u_3,\cdots,c) \) by linear interpolation: \( P_3 = \frac{(b-c)P_1+(c-a)P_2}{b-a} \).