Unpolarized light of intensity \(I_{0}\) is incident on a series of five polarizers, each rotated \(10.0^{\circ}\) from the preceding one. What fraction of the incident light will pass through the series?

Malus's law is fundamental when understanding how the intensity of light changes as it passes through a polarizing filter. Imagine light as a wave, oscillating in all directions. A polarizer is like a fence with vertical slats; it only allows waves that move parallel to the slats to pass. Mathematically, Malus's law is expressed with the elegant equation: \[I = I_0 \times \text{cos}^2(\theta)\]where \(I\) is the intensity of the polarized light, \(I_0\) the initial intensity, and \(\theta\) the angle between the light's initial polarization direction and the polarizing filter's axis. If the light is unpolarized, like sunlight on a clear day, a single filter cuts its intensity in half—a simple concept to visualize. Any subsequent polarization depends on both the reduced intensity and the angle between the polarizers.
In practice, if you were wearing polarized sunglasses and look at the sky at a 90-degree angle to the sun, the sky would appear darker. That's Malus's law in action, minimizing glare and easing the strain on your eyes. Fully grasp Malus's law, and you'll understand why photographers use polarizing filters to enhance contrast and colors in their pictures.

When considering the intensity of light after it passes through a polarizer, it's crucial to understand that polarization filters light based on its plane of vibration. In our exercise, light's path through a series of polarizers is a journey of diminishing brightness. Each polarizer allows only the light oscillating in a specific direction to pass through, reducing its intensity.
To calculate the intensity after each polarizer, we apply Malus's Law recursively. The intensity after the first polarizer is set—but what about subsequent ones? They depend on the angles. If you place polarizers at 90-degree angles to each other, no light passes through. Conversely, at 0 degrees, the intensity remains unchanged. An angle in between, like the \(10^{\text{o}}\) in our example, results in a gradual decrease in intensity, reflected beautifully in the compounded effect of \[\text{cos}^2(10^{\text{o}})\] terms.
Understanding how to measure the diminishing intensity can be applied outside the classroom too. For instance, if you're trying to reduce glare on a water surface to see the aquatic life beneath, adjusting the angle of your polarized sunglasses uses this same principle to optimize clarity.

Unpolarized light is the maverick of waves: it vibrates in numerous planes perpendicular to the direction it travels. This is the typical state of light emitted by the sun, light bulbs, and flames. Before human intervention, there is no order to this light; it's a chaotic dance of waves. By introducing a polarizer, we essentially invite the light to a formal ball. The polarizer—analogous to a dance instructor—teaches the light to only oscillate in one direction (plane).
Our exercise demonstrates the initial halving of the intensity of unpolarized light when it first encounters a polarizer. It's not unlike bringing a sunny field into the dappled shade. Subsequent polarizers further refine the light's behavior, like repeated dance lessons enhancing the elegance of the ballroom dancers' moves. Each polarizer the light encounters is an opportunity to impose further polarization—and reduce its intensity.
Whether it's creating crisp laser beams, reducing glare on car windshields, or improving the visual quality on LCD screens, the role of unpolarized light's transformation through polarization is an ever-present tool in technology and daily life. Grasping the journey from unpolarized to polarized light illuminates, quite literally, countless phenomena in both the natural and constructed worlds.