Vector Fields: Arrows Everywhere
A scalar field gives you a number at every point. A vector field gives you an arrow — a direction and a magnitude — at every point.
Examples
- Wind: At every point in the atmosphere, the wind has a speed and a direction. That’s a vector field.
- Ocean currents: At every point in the ocean, water flows in some direction at some speed.
- Gravity: At every point near the Earth, there’s a gravitational pull pointing downward with a specific strength.
- Electric fields: At every point around a charged particle, there’s a force that would push or pull another charge.
In each case: pick a point → get an arrow.
Each arrow shows the field’s direction and strength at that point. Longer arrows = stronger field.
Mathematical notation
A 2D vector field is a function $\mathbf{F}(x, y)$ that returns a vector at each point:
$$\mathbf{F}(x, y) = \begin{pmatrix} F_x(x, y) \\ F_y(x, y) \end{pmatrix}$$
The two components $F_x$ and $F_y$ give the arrow’s horizontal and vertical parts.
For example, the vortex field $\mathbf{F}(x, y) = (-y, x)$ points perpendicular to the line from the origin — everything swirls.
Two key questions
Once you have a vector field, two natural questions arise:
- Does the field have sources or sinks? Is stuff being created or destroyed anywhere? This leads to divergence.
- Does the field rotate? Is there swirling motion? This leads to curl.
These two operations — divergence and curl — are the mathematical heart of Maxwell’s equations.