The energy carried by an electromagnetic (E-M) wave with field intensities E, B is given by the Poynting vector, S:
S = 1/mo [E X B]
where mo denotes the
magnetic permeability, or mo = 4 π x 10-7
H/m
Physically, the Poynting vector is
the rate at which energy flows through a unit surface perpendicular to the
flow. We already saw one form based on working out the solar flux per unit area.
This was given as: P = E y H z / c
= 1300 Wm-2 .
Recall now, for any two vectors A,
B
A X B = A B
sin Θ
where Θ is the angle between them. If then A is perpendicular to B, then sin (90) = 1 so
that:
A B sin Θ =
AB
By the same token, taking the vectors E,
B perpendicular to each other, we find: S
= EB / mo
which has units of Wm-2
Recall E /
B = c, so:
B = E /c
Then: S = EH = EB / mo = (E/c) E/ mo =
E 2 /
c mo
A depiction of an EM wave in terms of the Poynting vector S and E, H is shown
below:
E-M Wave with Poynting vector (S)
Where: B
= mo H
or: S = (c /mo) B
The "time average"
is also of interest and entails taking the time average of the function: cos 2(kx
- wt)
Which
yields:
T av {cos2 (kx - wt) } = ½
The average value of S (or Intensity) can then be obtained from the maximum vector
amplitudes, viz.
I = S av = E max B max / 2 mo
or:
S av = E max 2/ 2 mo c = cB max 2 / 2 mo
Note that mo c is a very important quantity known as the "impedance of
free space", or:
mo c = Ömo / Ö εo
= 377 ohms
The respective contribution of the two field energies (associated with the
electric intensity, E, and magnetic
intensity B) can easily be shown to
be:
U E = ½ εo E2
U m= ½ (B2/ mo)
In a given volume the energy is equally shared by the two fields such that:
U E = U m = ½ εo E2 = (B2 /2 mo)
The total, instantaneous energy density of the fields is then:
U = U E + U m = 2(½ εo E2) = εo E2 = B2 /mo
Averaged over one or more cycles this leads to the total average energy per
unit volume:
U av = [εo E2 ] av =
½ εo E max 2
= B max 2 /2 mo
The
intensity of an EM wave is then:
I = S av = c U av = PA
where P denotes the radiation pressure,
or P = S/c (for complete absorption) or P = 2S/c for complete reflection of the
wave.
(In direct sunlight, one finds P R = 5 x 10-6 N/m2)
Suggested Problem:
A radio wave transmits 25 W/m 2 of power per
unit area. A plane surface of area 2.4 m x 0.7 m is perpendicular to the
direction of propagation of the wave. Calculate the radiation pressure P R
on the surface if it is assumed to be a perfect absorber.
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