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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!



Blazing a trail: SaraniaSat-led Team Shapes the Future of Space-Based Analytics

Blazing a trail: SaraniaSat-led Team Shapes the Future of Space-Based Analytics

10/13/2025

On July 24, 2025, a unique international partnership of SaraniaSat, NV5 Geospatial Software, BruhnBruhn Innovation (BBI), Netnod, and Hewlett Packard Enterprise (HPE) achieved something unprecedented: a true demonstration of cloud-native computing onboard the International Space Station (ISS) (Fig. 1). Figure 1. Hewlett... Read More >

NV5 at ESA’s Living Planet Symposium 2025

NV5 at ESA’s Living Planet Symposium 2025

9/16/2025

We recently presented three cutting-edge research posters at the ESA Living Planet Symposium 2025 in Vienna, showcasing how NV5 technology and the ENVI® Ecosystem support innovation across ocean monitoring, mineral exploration, and disaster management. Explore each topic below and access the full posters to learn... Read More >

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 >

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3.2

IDL's HISTOGRAM function

Anonym

IDL's HISTOGRAM function

IDL's HISTOGRAM function is one of the most versatile functionsI can think of. It can be very fast and efficient for a number of common tasks.

1. Plotting a histogram is an effective way to investigate statisticalproperties of data. A probability density graph quickly shows the distribution:

IDL> a = randomn(seed, 100000)+15.5+3*randomn(seed, 100000)

IDL> p = plot(location,histogram(a,nbins=1000,location=location),'r')

histogram plot

From the histogram, you could quickly conclude that asuitable range for BYTSCL might be MIN=10.0, MAX=20.0.

2. Finding percentiles in a programmatic way can be doneusing lookups in the cumulative histogram, for example if you want to find the5% and 95% in a dataset:

IDL> a = randomn(seed, 100000)+15.5+3*randomn(seed, 100000)

IDL> location[value_locate(total(histogram(a,nbins=1000,location=location),/cumulative)/a.length,[0.05,0.95])]

      10.285119       20.638901

Which shows that about 90% of the values are between 10.29and 20.64.

3. Finding the most common number in an array of integers.

IDL> arr = [3,7,34,5,8,8,5,31,5,8]

IDL> location[where(histogram(arr) eq max(histogram(arr,location=location)))]

       5       8

This shows a tie between 5 and 8 for the most abundant valuein the array.

4. Sorting can also be performed with HISTOGRAM. For example2-D sorting into a grid and computing the mean "F" value for eachgrid tile:

IDL> x = 45*randomu(seed, 100000)

IDL> y = 32*randomu(seed, 100000)

IDL> f = 5.5*randomn(seed, 100000) + 16

IDL> grid_index = floor(x + floor(y)*ceil(max(x)))

IDL> h = histogram(grid_index, min=0, binsize=1,reverse_indices=rev)

IDL> f_means = dblarr(ceil([max(x),max(y)]))

IDL> for i=0,h.length-1 do if h[i] gt 0 then f_means[i] = mean(f[rev[rev[i]:rev[i+1]-1]])

Check one of the values using the slower "WHERE"approach:

IDL> f_means[6,8]

      15.784905433654785

IDL> mean(f[where(floor(x) eq 6 and floor(y) eq 8)])

       15.784905

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