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Electromagnetic Fields and Waves: Including Electric Circuits

Paul Lorrain, Dale R. Corson

Chapter 38

Radiation Ii - all with Video Answers

Educators


Chapter Questions

01:01

Problem 1

The radiation field of a long wire carrying a step current Figure 38-13(a) shows a long wire that carries a current that varies as in Fig. 38-13(b). Beyond $\rho_{2}=c t$ there is no field. Inside $\rho_{1}=c(t-\tau)$ the field is that of a steady current $I_{0}$. In the shaded region,
$$
\boldsymbol{A}=\frac{\mu_{0} I}{2 \pi} \ln \frac{C}{\rho} \hat{\boldsymbol{z}}
$$
where $C$ is the length of the wire, as in Prob. 37-1.
(a) Calculate $\boldsymbol{E}$ and $\boldsymbol{B}$ in the shaded region.
(b) Show that Maxwell's equations apply.
(c) Sketch curves of $E$ and $B$ as functions of $\rho$ at a given instant, between $\rho=0$ and $\rho=\rho_{2}$. There are discontinuities at $\rho=\rho_{1}$ and at $\rho=\rho_{2}$, because we have assumed that $d^{2} I / d t^{2}$ is infinite at $t=0$ and at $t=\tau$.

Dominador Tan
Dominador Tan
Numerade Educator
05:02

Problem 2

A charge $Q$ oscillates along the $z$-axis, and $z=z_{m}$ exp j\omegat.
What is the dipole moment of an equivalent oscillating dipole? You can find the equivalence in the following way. If the currents are the same, then the $A$ 's are the same. Then the $V$ 's are the same, from the Lorentz condition (Sec. 37.1). Then the $\boldsymbol{E}$ 's and $\boldsymbol{H}$ 's are the same.

Nick Johnson
Nick Johnson
Numerade Educator
04:34

Problem 3

Show that the electric field of an electric dipole has three components: one that depends on the positions of the charges, one that depends on their velocities, and one that depends on their accelerations.

Linda Winkler
Linda Winkler
Numerade Educator
01:02

Problem 4

What fraction of the total power in the field of an electric dipole is radiated within $45^{\circ}$ of the equatorial plane?

Ajay Singhal
Ajay Singhal
Numerade Educator
07:01

Problem 5

The electric and magnetic energy densities in the field of an electric dipole
Calculate the ratio of the time-averaged electric energy density to the time-averaged magnetic energy density in the field of an electric dipole (a) for $r \ll \lambda$, (b) for $r=\lambda$, and (c) for $r \gg \lambda$.

Oleksandr Sulyma
Oleksandr Sulyma
Numerade Educator
01:52

Problem 6

The Poynting vector and the energy density in the field of an electric dipole
Show that, for $r \gg \lambda$, the magnitude of the Poynting vector in the field of an electric dipole is equal to the energy density multiplied by $c$.

Carlos Henrique De Lima
Carlos Henrique De Lima
Numerade Educator
01:39

Problem 7

All light sources should be black, for the following reason. Take the sun, for example. A cone in the retina of the eye collects radiation emanating from a very large number of atoms. These sources are incoherent.
At any given instant there is a near-infinite number of phasors in the complex plane, all of different magnitudes and different phases, rotating at different velocities. Their vector sum is clearly zero.
The same reasoning applies to any object, say a white wall, illuminated with incoherent light. The radiation that reaches a given cone comes from an area that is a large number of wavelengths in diameter. There again, the net field at the cone should be zero, and the wall should appear black.
To explain this paradox, consider $N$ waves of a single frequency and of a given linear polarization but of random amplitudes and phases. The number $N$ is very large. For the $i$-th wave, $E_{i}=E_{m i} \exp j\left(\omega t-\alpha_{i}\right)$ at the cone, and the net $E$ is the sum of the $E_{i}$ 's.
Now the eye is sensitive, not to $E$ but to $\mathscr{S}$, and thus to $E E^{*}$. Show that $\mathscr{S}_{\mathrm{av}}=\sum \mathscr{S}_{i} .$ This means that the net energy flux is equal to the sum of the energy fluxes of the individual waves. ${ }^{\dagger}$

Suzanne W.
Suzanne W.
Numerade Educator
02:04

Problem 8

Consider a particular class of astronomical objects, say quasars. Assume that they are all identical and distributed uniformly in a Euclidean universe.
Show that, if $N$ is the number of objects whose radio-frequency flux is greater than $\mathscr{S}$ at the earth, then a plot of $\log N$ against $\log \mathscr{S}$ should be a straight line whose slope is $-1.5 .$ The slope for quasars is, in fact, larger. This is possibly a measure of cosmological evolution.

Salamat Ali
Salamat Ali
Numerade Educator
02:39

Problem 9

The atmosphere scatters sunlight. Draw a sketch showing the sun, the earth, and a vector $\boldsymbol{E}$ on a ray of scattered light. Explain why skylight is polarized. The light is only partially polarized because it is scattered many times.

Narayan Hari
Narayan Hari
Numerade Educator