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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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Rapid Cloud Masking for NPP VIIRS Imagery

Anonym

Here in NV5 (formerly Exelis VIS) Tech Support, we are often asked, “How do I remove the clouds from my imagery?”

Unfortunately, when working with optical imagery, it is usually not possible to recover accurate information for the land surface under clouds. Opaque clouds block light both from reaching the surface (i.e., shadows), and also from being reflected back to the sensor. Consequently, there simply is insufficient signal at the sensor for cloud covered areas. Even the more translucent cirrus clouds interfere with the signal of reflected light from the surface in a way that makes it difficult to analyze or interpret optical imagery in these areas.

One way to approach this problem is to create a mask of the cloud covered areas, and leave those areas out of any image processing or interpretation performed on the optical data.  In fact, official cloud mask data products are generated from some optical sensor data (e.g., MODIS). One of the newer optical sensors for which cloud mask products are available is the Visible Infrared Imaging Radidometer Suite (VIIRS) sensor.  VIIRS data products are distributed by NOAA’s Comprehensive Large Array-Data Stewardship System.  The VIIRS Cloud Mask (VCM) Intermediate Products are generated using relatively sophisticated algorithms, which not only identify cloudy and clear areas, but also indicate a level of confidence in that assessment. There are a few down sides to the VIIRS cloud mask products. The spatial resolution does not match the highest resolution available for VIIRS data. Moreover, it can be challenging to identify the correct cloud mask product that corresponds to a particular VIIRS dataset. 

Noting these challenges, NV5’s own Mark Piper has adapted an algorithm developed for Landsat 7 ETM+ data to provide a simpler, though less informative and robust, alternative to the VIIRS Cloud Mask (VCM) Intermediate Product.  The advantage of this algorithm is that can be applied to a VIIRS Imagery EDR to conveniently quantify the fractional cloud cover in the scene or in a spatial subset. Dr. Piper will be presenting this work in December at the 2012 American Geophysical Union Fall Meeting.

Cloud Mask Comparison

Left: A color composite of VIIRS data over Hawaii. Right: A comparison of the official VIIRS Cloud Mask (VCM) Intermediate Product and a cloud mask generated using Dr. Piper’s algorithm.  Areas where both masks find clouds are shown in white. Areas where both masks do not find clouds are shown in gray. Areas where only the official product finds clouds are shown in cyan. Areas where only Dr. Piper’s rapid algorithm finds clouds are shown in red. (The red striping has to do with the bowtie effect.)

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