The randomisation of the temperature is described here.
This section describes how the magnetic field, inclination, azimuth and line-of-sight velocity are randomised.
There are three options implemented: 1, 2 or 3 Nodes. The Nodes have the same meaning as in SIR (1 Node = Constant with height, 2 Nodes = Linear with height, 3 Nodes = parabolic with height).
For example, atmospheres for the magnetic field can look like this: