Rankers Physics

Magnetic Properties of Matter: Practice Problem & Solution

13. Due to earth's magnetic field, the charged cosmic rays particles (1997)
Can never reach the pole
Can never reach the equator
Require greater kinetic energy to reach the equator than pole
Require less kinetic energy to reach the equator than pole

Solution Explained:

To solve this problem, we apply the core principles of Magnetic Properties of Matter. Understanding the underlying formula is key to arriving at the correct answer below:

At the equator, magnetic field lines are perpendicular to incoming charged particles, causing maximum magnetic deflection force. At the poles, field lines are nearly parallel, causing little to no deflection. Thus, particles require much higher energy to penetrate at the equator.

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