Washington D.C. –
For 11 years, the
VLA Low-band Ionosphere and Transient Experiment, known as VLITE, has quietly recorded the low-frequency radio sky every time the
National Science Foundation’s Very Large Array (VLA) observes.
A collaboration between the U.S. Naval Research Laboratory
(NRL) and the National Radio Astronomy Observatory
(NRAO), VLITE operates alongside the VLA without interrupting its primary science mission. While astronomers study distant galaxies and black holes, VLITE collects a parallel stream of low-frequency data, building one of the most extensive continuous records of the dynamic radio sky.
The data has practical implications. Variations in space weather can affect satellite communications, GPS, radar and long-distance radio systems.
Originally conceived as an opportunistic add-on, VLITE has become a sustained observing program with both scientific and operational value.
“VLITE was designed to take advantage of opportunity,” said Tracy Clarke, Ph.D., an NRL research astronomer and VLITE lead. “We thought it might last a few years, but eleven years later it’s still ongoing. The longer it ran the more valuable it became. Time reveals scientific discoveries that you can’t anticipate.”
Monitoring the Ionosphere Across a Solar Cycle
Because VLITE observes at low radio frequencies, its signals are shaped both by distant astrophysical sources and by Earth’s ionosphere, the charged upper atmosphere that affects radio propagation.
Over 11 years, VLITE has recorded data spanning an entire solar cycle, capturing periods of both high and low solar activity.
“There are disturbances that occur when the sun is quiet and others that occur when it’s active,” said Joe Helmboldt, Ph.D., an ionospheric scientist in
NRL’s Remote Sensing Division. “If you want reliable statistics, you have to observe across that full range of conditions.”
That extended coverage has enabled researchers to move beyond isolated case studies.
“We’ve gone from studying single events to identifying the physical processes that generate those disturbances,” Helmboldt said. “Short-term experiments show what’s happening at a moment in time. VLITE shows how the ionosphere behaves over years.”
Precision Sources and Navigation Potential
VLITE also monitors millisecond pulsars, rapidly rotating neutron stars that emit extremely stable radio pulses.
“Millisecond pulsars are among the most precise natural timing sources known,” said Emil Polisensky, NRL Ph.D., who supports VLITE’s transient detection and cataloging efforts. “Long-term monitoring helps us better understand their stability and potential applications.”
Because some pulsars are more stable than atomic clocks, they can serve as natural navigation beacons.
“You can use them analogously to GPS satellites,” Polisensky said. “In principle, a spacecraft could navigate around Earth, the Moon or even deeper into the solar system using pulsars.”
As the number of VLITE antennas expands from 18 to 23 by the end of this year, the system’s sensitivity will increase, improving its ability to detect rare and faint objects.
“Greater sensitivity means we can find more exotic sources,” Polisensky said.
Turning Signals into Science
Each time VLITE collects data, Wendy Peters’ computer code goes to work. She is an NRL data processing and imaging pipeline developer. The custom code she developed automatically processes incoming signals, calibrates them, and prepares them for archiving.
Within about 48 hours, the data are stored and made available to researchers at a pace that requires constant monitoring as observations continue around the clock.
“The system doesn’t stop,” Peters said. “As new data comes in, the code has to keep up processing, organizing, and ensuring everything is accessible and reliable.”
Over 11 years, that steady flow has grown into a vast, searchable archive, sustained through continuous refinement and disciplined software engineering.
A Model of Efficient Collaboration
VLITE operates through a long-running partnership between NRL and NRAO. While the VLA conducts its primary observations, VLITE collects low-frequency data simultaneously, an approach known as commensal observing.
“The beauty of commensal observing is efficiency,” Clarke said. “We’re expanding scientific return from existing infrastructure. We’ve maintained it and invested in it. The VLITE approach is being evaluated internationally as a framework for similar systems.”
Over more than a decade, VLITE has accumulated tens of thousands of hours of observing time and repeatedly imaged nearly the entire sky visible to the VLA. The resulting archive includes millions of processed data products that support studies of astrophysical transients, ionospheric structure and celestial reference frame source stability.
Training the Next Generation
VLITE has also provided research opportunities for students, including a
Naval Research Enterprise Internship Program participant who contributed to the discovery of a millisecond pulsar.
“As a scientist, you want to pass on what you’ve learned,” Peters said. “Helping students experience discovery firsthand is one of the most rewarding parts of this work.”
Students working with VLITE
gain experience analyzing large datasets, writing code and conducting original research.
Looking Ahead
The VLITE team is now developing polarization imaging capabilities, which would enhance detection of certain transient events and pulsars.
“There are many transient phenomena that are highly polarized,” Polisensky said. “Polarization imaging would make searching for new millisecond pulsars significantly more effective.”
VLITE demonstrates how sustained engineering and collaboration can expand scientific insight without competing for observing time.
“We’ve built something that continues to deliver value year after year,” Helmboldt said. “That consistency is what makes it powerful.”
After 11 years VLITE continues to listen, capturing a dynamic universe in motion and reinforcing the value of long-term vision, sustained collaboration and quiet innovation.
“We’ve got a small team, but they are a remarkable group of people that have been able to make this a success.” said Clarke, “I’m really proud of that.”
About the U.S. Naval Research Laboratory
NRL is a scientific and engineering command dedicated to research that drives innovative advances for the U.S. Navy and Marine Corps from the seafloor to space and in the information domain. NRL, located in Washington, D.C. with major field sites in Stennis Space Center, Mississippi; Key West, Florida; Monterey, California, and employs approximately 3,000 civilian scientists, engineers and support personnel.
NRL offers several mechanisms for collaborating with the broader scientific community, within and outside of the Federal government. These include Cooperative Research and Development Agreements (CRADAs), LP-CRADAs, Educational Partnership Agreements, agreements under the authority of 10 USC 4892, licensing agreements, FAR contracts, and other applicable agreements.
For more information, contact NRL Corporate Communications at
NRLPAO@us.navy.mil.