# Do in our atmosphere at least two positions exist where there is no wind?

If we look at a two-dimensional sphere and draw a continuous vector field on it, you can compare this with a tennis ball whose hairs you comb in a continuous way. Two points on the ball will have an undefined direction of the hair. If you comb them from up-down, or from the right to the left, or whatever way you try to comb it, two points arise where there is no direction of the balls hair.

The wind field in the atmosphere is a continuous vector field (which can be compared with the directions of the hair on the ball). The difference is that the atmosphere in which the wind field is situated is three-dimensional. But I can't imagine that this one extra degree of freedom makes any difference for the same two points.

So my question is: are there in the atmosphere of the earth (at least?) two points in which the wind field is not defined, and does this mean the same as saying that there are two positions in the atmosphere where there is no wind?

• Related and possibly answered, but I am not capable of judgement Cyclones on Earth – user154420 Jun 20 '17 at 12:09

You are right that the degree of freedom in the altitude / height in the atmosphere does not change things greatly for the implications of the hairy ball theorem for meteorology. All you need to do is apply the theorem to every constant altitude surface or any continuous deformation thereof contained in the atmosphere. The theorem then dictates that there must be at least one point somewhere on that surface where the wind vector vanishes - i.e. a cyclonic / anticyclonic eye - or a source / sink (where air flows upwards / downwards and leaves a sink / source in each constant altitude layer). The hairy ball theorem applied to the 2-sphere $\mathbb{S}^2$ simply says that there must be at least one point where the wind vector field, assuming that the field is continuous, vanishes.
You don't need two singular points as you seem to think: consider the flow lines resulting from the projection of the lines $\mathrm{Re}(z)=const$ of constant real part (or any family of parallel straight lines) on the complex plane onto the Riemann sphere through stereographic projection. There is one singular point at the North pole.