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Waves in the presence of an applied magnetic field: cyclotron resonance                 13

                    Medium 1            Medium 2               Medium 3
                    Vacuum              Conductor              Vacuum
                   Incident wave        Forward
                                      travelling wave
                                                             Transmitted
                                                               wave          Fig. 1.6
                                                                             Incident electromagnetic wave
               Reflected wave           Backward
                                                                             transmitted to medium 3. The
                                                                             amplitude of the wave decays in
                                       travelling wave
                                                                             medium 2 but without any energy
                                    ωτ   < <  1  ω  >  ω p                   absorption taking place.

            converted into heat. The energy balance in the most general case is

                       energy in the wave = energy in the transmitted wave
                                        + energy in the reflected wave
                                        + energy absorbed.

               A good example of the phenomena enumerated above is the reflection of
            radio waves from the ionosphere. The ionosphere is a layer which, as the name
            suggests, contains ions. There are free electrons and positively charged atoms,
            so our model should work. In a metal, atoms, and electrons are closely packed;
            in the ionosphere, the density is much smaller, so that the critical frequency
            ω p is also smaller. Its value is a few hundred MHz. Thus, radio waves below
            this frequency are reflected by the ionosphere (this is why short radio waves
            can be used for long-distance communication) and those above this frequency
            are transmitted into space (and so can be used for space or satellite commu-
            nication). The width of the ionosphere also comes into consideration, but at
            the wavelengths used (it is the width in wavelengths that counts) it can well be
            regarded as infinitely wide.


            1.6 Waves in the presence of an applied magnetic field:
            cyclotron resonance

            In the presence of a constant magnetic field, the characteristics of electromagn-
            etic waves will be modified, but the solution can be obtained by exactly the
            same technique as before. The electromagnetic eqns (1.22) and (1.23) are still
            valid for the a.c. quantities; the equation of motion should, however, contain
            the constant magnetic field, which we shall take in the positive z-direction. The
            applied magnetic field, B 0 , may be large, hence v × B 0 is not negligible; it is a
            first-order quantity. Thus, the linearized equation of motion for this case is  In order to satisfy this vector equa-
                                                                             tion, we need both the v x and v y
                                                                             components. That means that the
                                   ∂v  v
                               m     +    = e(E E E + v × B 0 ).      (1.56)  current density, and through that
                                   ∂t  τ
                                                                             the electric and magnetic fields,
               Writing down all the equations is a little lengthy, but the solution is not  will also have both x and y com-
            more difficult in principle. It may again be attempted in the exponential form,  ponents.
            and ∂/∂z and ∂/∂t may again be replaced by ik and –iω, respectively. All the
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