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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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Polarimetric Data Analysis with IDL

Jenny Bloom

This blog, written by Ranier M.E. Illing is the third blog of a series writing by our IDL Fellows. The IDL Fellows program is our way of supporting passionate retired IDL users who may need support to continue their work with IDL. There is continual innovation behind IDL, and this program is one of the many ways we hear about the new innovative ways people are using it on a regular basis. If you are retired and interested in becoming an IDL Fellow and sharing your research through a blog post, feel free to reach out to me to see if you qualify for the program.

When we look at the world around us, most of the information our eyes capture comes from the intensity of light. We perceive different colors based on the varying intensities in spectral bands, helping us understand the characteristics of objects and their surroundings. However, our eyes are not particularly adept at detecting another critical quality of light – polarization.

Light is more than just color and intensity. It is a wave that oscillates perpendicular to its direction. Polarization measures the coherence of this wave in time – essentially whether the wave oscillates in a fixed plane, spirals around its path, or something in between. To fully describe the properties of a light wave, scientist use four key parameters.

S0 – the total intensity of the wave
S1 – the amount of intensity oscillation in a given transverse direction
S2 – the amount of intensity oscillation at 45° to that direction
S3 – the amount of intensity oscillation around the line of sight

Linear polarization, where the wave oscillates in a fixed transverse plane, is the most common form. For instance, polarized sunglasses filter out all light that doesn’t oscillate in a horizontal plane, reducing glare and improving visual clarity.

A Closer Look at Polarization with IDL®

For our exploration of polarized data, we acquired field data images using the Ball TTP dual liquid crystal polarimeter. The raw images were processed and corrected using the PolarQL analysis system written in IDL. IDL enables us to analyze the processed images and generate a variety of polarimetric products, offering deeper insights into the data.

One particular dataset stood out. It focuses on the elimination of haze using only polarized light measurements. The study took place on the grassy knoll in front of the Ball BCH, with the TTP set up to capture imagery of Eldorado Canyon.

Discovering Hidden Layers with Linear Polarization

Figure 1 shows a sample of the linear polarized intensity gathered (calculated as S_linear=√(S_1^2+S_2^2 ) ). The vibrant color display reveals the different layers of mountain ranges, each differentiated by their linearly polarized scattered path radiance. This unique visualization allows us to see through the haze, distinguishing the various layers of landscape that might otherwise blend together.

To further explore this data, we used the interactive segmentation tool available in PolarQL.pro version 2.1. This tool allows any pair of data images to be plotted against each other as a 2D histogram. The data available for analysis include the four raw images (S0, S1, S2, S3), linearly polarized intensity, fractional polarizations, ellipticity, and more. Users can interactively select a region of interest using a box cursor, which highlights the corresponding pixels in a “show” image rendered in a red color table. The image show can be any of the available raw or processed images.

Figure 1. The first image of the two below shows the linear polarized intensity, with the vibrant color showing the layers of mountain ranges, each differentiated by their linearly polarized scattered path radiance.

Figure 2. Eldorado Canyon data analyzed using the segmentation tool in IDL. Features in the S1-S2 histogram plot pointer box are highlighted in the S0 image as green pixels.

Figure 2 shows the clear segmentation of the image by its linear polarized flux. The green section corresponds to the pixels in the cursor box connected by the arrow, clearly highlighting the segmentation of the image based on its polarization characteristics. Notice the shadowing effect – the farther mountain range’s polarization is overshadowed by the nearer mountain, indicating a significantly different polarization between the two.

Beyond Fractional Polarization

While fractional polarization is important, it can sometimes obscure clear segmentation seen in linearly polarized flux. This is because fractional polarization involves division by S0, introducing intensity features with polarization information. For example, a low polarized intensity feature that can be clearly distinguished from a high polarized intensity feature, such as the sky and the front mountains in Figure 2. However, after dividing the total intensity, the fractional polarization might become similar for both features, making it harder to distinguish.

Instead of relying solely on fraction polarization, the “most polarimetric” information can be found in the polarization angle (or more directly, S2/S1). This ratio focuses solely on the polarization of light, eliminating the need for absolute intensity calibration and providing a more accurate representation of the underlying polarimetric properties.

Polarimetric data analysis offers a powerful lens through which we can uncover hidden details in our environment, revealing insights that go beyond what is visible to the naked eye. By leveraging tools like IDL and the PolarQL analysis system, we can explore the nuances of light's polarization, enabling clearer interpretations of complex datasets.


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