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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 the next power of two

Anonym
Ron Kneusel emailed our internal PWUISATAI (People Who Use IDL Sitting Around Talking About IDL) group yesterday with a clever function he saw in some CUDA C code to calculate the next power of two greater than or equal to a given integer. His IDL translation:
function next_power_2, x
   compile_opt idl2, logical_predicate

   n = x - 1 ; protects input
   n = ishft(n, -1) or n
   n = ishft(n, -2) or n
   n = ishft(n, -4) or n
   n = ishft(n, -8) or n
   n = ishft(n,-16) or n
   n = ishft(n,-32) or n
   n = ishft(n,-64) or n

   return, ++n
end
Both ISHFT and the OR operator are used here to perform bitwise operations on the input integer. Here's an example of using NEXT_POWER_2:
IDL> a = 3565946L
IDL> b = next_power_2(a)
IDL> print, b
     4194304
IDL> factor, b

            22
 4194304 = 2
I've used Ray Sterner's FACTOR, a part of the IDL astrolib, to learn that 4194304 is 222. Atle Borsholm replied to the group with an alternate take:
function n2, x

   return, ishft(1ull,total(ishft(1ull,indgen(64)) lt x, /integer))
end
that gives the same result:
IDL> b = n2(a)
IDL> print, b
     4194304
Atle commented that although his version is shorter, Ron's may be faster. I was curious, so I made a simple time test:
pro time_test_next_power_2
   compile_opt idl2

   n_iter = 1e6
   x = 275259L

   t0 = systime(/seconds)
   for i=1, n_iter do !null = next_power_2(x)
   t1 = systime(/seconds)
   print, 'NEXT_POWER_2:', t1-t0, format='(a15,f12.8,1x,"s")'

   t0 = systime(/seconds)
   for i=1, n_iter do !null = n2(x)
   t1 = systime(/seconds)
   print, 'N2:', t1-t0, format='(a15,f12.8,1x,"s")'
end
and ran it on my laptop:
IDL> time_test_next_power_2
  NEXT_POWER_2: 2.14159489 s
            N2: 2.77271295 s
So, Ron's version is slightly faster. In either case, we hope you might find these functions handy! Update: An even simpler version from a zero-padding routine I'd written long ago:
IDL> a = 3565946L
IDL> b = 2UL^ceil(alog(a)/alog(2))
IDL> print, b
     4194304
Note: I'll be out on vacation for a bit, so I have some guest bloggers lined up for the next few weeks.
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