A localized magnetic field $H$ in an electrically conducting medium of permeability $\mu$ and conductivity $\sigma$ will diffuse through the medium in the $x$ -direction at a rate given by
$$
\frac{\partial H}{\partial t}=\frac{1}{\mu \sigma} \frac{\partial^{2} H}{\partial x^{2}}
$$
Show that the time of decay of the field is given approximately by $L^{2} \mu \sigma$, where $L$ is the extent of the medium, and show that for a copper sphere of radius $1 \mathrm{~m}$ this time is less than $100 \mathrm{~s}$.
$$
\begin{aligned}
&\mu(\text { copper })=1 \cdot 26 \times 10^{-6} \mathrm{Hm}^{-1} \\
&\sigma(\text { copper })=5 \cdot 8 \times 10^{7} \mathrm{~S} \mathrm{~m}^{-1}
\end{aligned}
$$
(If the earth's core were molten iron its field would freely decay in approximately $15 \times 10^{3}$ years. In the sun the local field would take $10^{10}$ years to decay. When $\sigma$ is very high the local field will change only by being carried away by the movement of the medium-such a field is said to be 'frozen' into the medium - the field lines are stretched and exert a restoring force against the motion.)