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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!



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 >

Thermal Infrared Echoes: Illuminating the Last Gasp of a Dying Star

Thermal Infrared Echoes: Illuminating the Last Gasp of a Dying Star

4/24/2025

This blog was written by Eli Dwek, Emeritus, NASA Goddard Space Flight Center, Greenbelt, MD and Research Fellow, Center for Astrophysics, Harvard & Smithsonian, Cambridge, MA. It is the fifth blog in a series showcasing our IDL® Fellows program which supports passionate retired IDL users who may need support to continue their work... Read More >

A New Era of Hyperspectral Imaging with ENVI® and Wyvern’s Open Data Program

A New Era of Hyperspectral Imaging with ENVI® and Wyvern’s Open Data Program

2/25/2025

This blog was written in collaboration with Adam O’Connor from Wyvern.   As hyperspectral imaging (HSI) continues to grow in importance, access to high-quality satellite data is key to unlocking new insights in environmental monitoring, agriculture, forestry, mining, security, energy infrastructure management, and more.... Read More >

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Finding Red Lights with Harris Deep Learning

Barrett Sather

 

It’s been almost a year, but I finally have found the time to train a neural network with the job of finding red traffic lights in imagery using our machine learning technology that we call MEGA. In a post in late 2016 I began with example labeling and patch harvesting for the training process, and today I’d like to discuss that process and the results!

After labeling images with examples of red lights, and many more examples of what is not a red light, the MEGA neural network is trained with patches that are clipped out of the imagery. Over time, the MEGA trainer uses a convolutional network to guess at what it believes each training patch to be. Whether correct or incorrect, the weights of the network are then modified so that the model becomes more accurate as the training continues. It can be thought of as a really fancy guess and check.

Once the network has been trained, you can give it completely new imagery that it has never seen before for classification. Below is the test image that we’ll use, which was NOT used in the training (that would be cheating).

Image

This is the classification image for red lights, in which the units are the decimal probability (0.0 – 1.0) that each pixel is a red light.

Image

And here is the heatmap overlaid on the image. You’ll notice that the edges are not classified, as each step in the convolution over the image must have a full patch, so half a patch width on the edge of the image is not classified. For this model, I used a square patch size of 31 pixels.

Image

The model is correctly identifying all red lights in the scene, but is also picking up on a couple more features in the image that look similar. Specifically, it is seeing the red tail light on the black vehicle, and the corner of an orange construction sign. To improve the model, these examples could be added to the “not light” class and re-trained.

In my experience, it is much less time consuming to create a model that finds a target than a model that finds ONLY that target. It takes some time to weed out what we’ve been calling “confusers” from the classification.

As far as accuracy goes between basic feature extraction and deep learning, deep learning has an advantage here because basic feature extraction will pick up the red circle on the sign that reads "NO TURN ON RED".

If you are interested in finding out more about Harris Deep Learning technologies contact us at GeospatialInfo@NV5.com.

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