X

NV5 Geospatial Blog

Each month, NV5 Geospatial posts new blog content across a variety of categories. Browse our latest posts below to learn about important geospatial information or use the search bar to find a specific topic or author. Stay informed of the latest blog posts, events, and technologies by joining our email list!



Monitor, Measure & Mitigate: Integrated Solutions for Geohazard Risk

Monitor, Measure & Mitigate: Integrated Solutions for Geohazard Risk

9/8/2025

Geohazards such as slope instability, erosion, settlement, or seepage pose ongoing risks to critical infrastructure. Roads, railways, pipelines, and utility corridors are especially vulnerable to these natural and human-influenced processes, which can evolve silently until sudden failure occurs. Traditional ground surveys provide only periodic... Read More >

Geo Sessions 2025: Geospatial Vision Beyond the Map

Geo Sessions 2025: Geospatial Vision Beyond the Map

8/5/2025

Lidar, SAR, and Spectral: Geospatial Innovation on the Horizon Last year, Geo Sessions brought together over 5,300 registrants from 159 countries, with attendees representing education, government agencies, consulting, and top geospatial companies like Esri, NOAA, Airbus, Planet, and USGS. At this year's Geo Sessions, NV5 is... Read More >

Not All Supernovae Are Created Equal: Rethinking the Universe’s Measuring Tools

Not All Supernovae Are Created Equal: Rethinking the Universe’s Measuring Tools

6/3/2025

Rethinking the Reliability of Type 1a Supernovae   How do astronomers measure the universe? It all starts with distance. From gauging the size of a galaxy to calculating how fast the universe is expanding, measuring cosmic distances is essential to understanding everything in the sky. For nearby stars, astronomers use... Read More >

Using LLMs To Research Remote Sensing Software: Helpful, but Incomplete

Using LLMs To Research Remote Sensing Software: Helpful, but Incomplete

5/26/2025

Whether you’re new to remote sensing or a seasoned expert, there is no doubt that large language models (LLMs) like OpenAI’s ChatGPT or Google’s Gemini can be incredibly useful in many aspects of research. From exploring the electromagnetic spectrum to creating object detection models using the latest deep learning... Read More >

From Image to Insight: How GEOINT Automation Is Changing the Speed of Decision-Making

From Image to Insight: How GEOINT Automation Is Changing the Speed of Decision-Making

4/28/2025

When every second counts, the ability to process geospatial data rapidly and accurately isn’t just helpful, it’s critical. Geospatial Intelligence (GEOINT) has always played a pivotal role in defense, security, and disaster response. But in high-tempo operations, traditional workflows are no longer fast enough. Analysts are... Read More >

1345678910Last
«September 2025»
SunMonTueWedThuFriSat
31123456
78910111213
14151617181920
21222324252627
2829301234
567891011
11534 Rate this article:
4.5

The Wavelike Nature of Light

Diffraction, Interference and Refraction Round Out Our Overview of the Behavior of Light

Anonym

In looking at the nature of light, we have seen how light interacting with matter illuminates our world. When light rays fall up some piece of matter, they can be absorbed, reflected, or transmitted. We've seen that the reflection of light is key to how we remotely perceive the universe around us. Light photons that are absorbed by matter add to the energy of the quantum system, and matter may radiate light back out to space. Just with this information, we can say a great deal about the way light behaves. To complete the bigger picture, however, we will need to take a look at how the wavelike nature of light emerges when light flows around and through matter.

The Golden Gate Bridge refracted in rain drops acting as lenses on glass by Brocken Inaglory - Licensed under CC BY-SA 3.0 via Commons

If you've ever been to the ocean and seen water waves bending around the end of a sea wall, or watched as waves spread out from a channel, you've observed the wave phenomenon known as diffraction. Basically, wave energy bends around physical objects that it encounters. While this is easy to observe with mechanical waves in a medium such as water, diffraction of light is very subtle and not easily noticed. Light waves have such small wavelengths (~5000 Angstroms) that the amount of bending that occurs is always very small. However, there is in fact a simple way to observe diffraction of light. When light from a distant source is passed through a small pinhole or slit, what is called a diffraction pattern can be observed. If you've ever seen a distant street light through a fine window screen you may have noticed that the point light source of the street lamp appears to your eyes to form a cross. This is diffraction: the four sides of each tiny hole in the screen act like the side of a diffraction slit, and bends the light four ways to form a cross shape. The fact that diffracted light rays form patterns is due to another feature of general wave phenomena: interference.

Thomas Young's sketch of two-slit diffraction, presented to the Royal Society in 1803 - Public Domain via Commons
 

Interference is another effect that is easily observed in the realm of mechanical waves. Drop two rocks into slightly different spots of a pond and watch as the resulting waves interact with each other. Waves whose crests and troughs match up with each other in frequency are said to be in-phase. Such waves will interfere with each other constructively, meaning that they will add to each other to produce a wave that, while still of the same frequency, has twice the amplitude (wave height) of the two individual constituent waves. Waves that are completely out of phase with each other (peak lining up with trough and vice-versa) will combine with what is termed destructive interference. The two waves will cancel each other out, resulting in no wave. Interference does not create or destroy wave energy, but rather redistributes it. Thus when light waves are passed through a diffraction slit, the resulting pattern is formed by the diffracted light rays constructively and destructively interfering with each other.

Constructive and destructive interference of two waves by Haade - Licensed under CC BY-SA 3.0 via Commons

When light is able to traverse through matter of some sort, perhaps its most useful behavior emerges. Refraction is the bending of light rays as they travel across the interface between two different materials, such as air and water. The cause of this behavior is that light travels at different speeds through different materials. It is well known that the speed of light is constant in a vacuum, and it doesn't slow down much when traveling through air. But light travels only 3/4 as fast through water and only 2/3 as fast through glass. The slower light travels through a substance, the more it will be bent through refraction.

Snell's Law which describes refraction by Cristan - Public Domain via Commons
 

Large portions of the science of optics largely proceed from the very simple rules of refraction. Because translucent materials such as glass bend light rays, we can create lenses that manipulate and focus the light that passes through them to serve various purposes. The lenses in eyeglasses, microscopes and telescopes all harness the refractory behavior of light, which is only possible because light observably behaves like all waves do. Of course, light also behaves in some ways as a particle (see the photoelectric effect, for example), but that is a subject for an entirely different article. 

Two soap bubbles, illustrating iridescent colors due to thin film interference by Tagishsimon - Licensed under CC BY-SA 3.0 via Commons

Please login or register to post comments.