| (619) |
![]() |
(626) |
Consider a typical metallic conductor such as copper, whose electrical
conductivity at room temperature is about
. Copper, therefore, acts as a good
conductor for all electromagnetic waves of frequency below about
. The skin-depth in copper for such waves is thus
![]() |
(628) |
The conductivity of sea-water is only about
. However, this is still sufficiently high for sea-water to act as
a good conductor for all radio frequency electromagnetic waves (i.e.,
GHz). The skin-depth at 1MHz (
m)
is about
m, whereas that at 1kHz (
km)
is still only about 7m. This obviously poses quite severe restrictions for
radio communication with submerged submarines. Either the submarines
have to come quite close to the surface to communicate (which is dangerous), or the communication must be performed with extremely low frequency (ELF) waves (i.e.,
Hz). Unfortunately, such waves have very large wavelengths (
), which means
that they can only be efficiently generated by gigantic
antennas.
According to Equation (625), the phase of the magnetic component of an
electromagnetic wave propagating through a good conductor lags that of the
electric component by
radians. It follows that the mean energy flux into
the conductor takes the form
![]() |
(629) |
Note, from (627), that the impedance of a good conductor is far less than
that of a vacuum (i.e.,
). This implies that the ratio of the magnetic
to the electric components of an electromagnetic wave propagating through a good conductor is far larger than that of a wave propagating through a vacuum.
Suppose that the region
is a vacuum, and the region
is
occupied by a good conductor of conductivity
. Let the wave electric and
magnetic fields in the vacuum region take the form of the incident and reflected waves specified in (607) and (608).
The wave electric and magnetic fields in the conductor are written
| (630) | |||
| (631) |
![]() |
(632) |
According to the above analysis, a good conductor reflects a normally incident
electromagnetic wave with a phase shift of almost
radians (i.e.,
). The coefficient of reflection is just less than unity, indicating that, whilst most
of the incident energy is reflected by the conductor, a small fraction of it
is absorbed.
High-quality metallic mirrors are generally coated in silver, whose conductivity
is
. It follows, from (639), that at optical
frequencies (
) the coefficient
of reflection of a silvered mirror is
. This implies that
about
of the light incident on the mirror is absorbed, rather than being reflected. This rather severe light loss can be
problematic in instruments, such as astronomical telescopes, which are used to
view faint objects.