Fundamentals of Physics Extended (10th Edition)

Published by Wiley
ISBN 10: 1-11823-072-8
ISBN 13: 978-1-11823-072-5

Chapter 32 - Maxwell's Equations; Magnetism of Matter - Problems - Page 970: 54a

Answer

$h=1.66 \times 10^3 \mathrm{~km} .$

Work Step by Step

At a distance $r$ from the center of the Earth, the magnitude of the magnetic field is given by $$ B=\frac{\mu_0 \mu}{4 \pi r^3} \sqrt{1+3 \sin ^2 \lambda_w}, $$ where $\mu$ is the Earth's dipole moment and $\lambda_m$ is the magnetic latitude. The ratio of the field magnitudes for two different distances at the same latitude is $$ \frac{B_2}{B_1}=\frac{r_1^3}{r_2^3} . $$ With $B_1$ being the value at the surface and $B_2$ being half of $B_1$, we set $r_1$ equal to the radius $R_e$ of the Earth and $r_2$ equal to $R_e+h$, where $h$ is altitude at which $B$ is half its value at the surface. Thus, $$ \frac{1}{2}=\frac{R_c^3}{\left.\mid R_e+h\right]^3} . $$ Taking the cube root of both sides and solving for $h$, we get $ h=\left(2^{1 / 3}-1\right) R_e=\left(2^{1 / 3}-1\right)(6370 \mathrm{~km})=1.66 \times 10^3 \mathrm{~km} . $
Update this answer!

You can help us out by revising, improving and updating this answer.

Update this answer

After you claim an answer you’ll have 24 hours to send in a draft. An editor will review the submission and either publish your submission or provide feedback.