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Home : Our Work : Areas of Research : Plasma Physics

    Plasma Physics

Phone: (202) 767-5635

 

Overview

The Plasma Physics Division conducts broad theoretical and experimental programs of basic and applied research in plasma physics, laboratory discharge, and space plasmas, intense electron and ion beams and photon sources, atomic physics, pulsed power sources, laser physics, advanced spectral diagnostics, and nonlinear systems. 

The effort of the Division is concentrated on a few closely coordinated theoretical and experimental programs. Considerable emphasis is placed on large-scale numerical simulations related to plasma dynamics; ionospheric, magnetospheric, and atmospheric dynamics; nuclear weapons effects; inertial confinement fusion; atomic physics; plasma processing; nonlinear dynamics and chaos; free electron lasers and other advanced radiation sources; advanced accelerator concepts; and atmospheric laser propagation.

Core Capabilities 

  • Radiation Hydrodynamics - The principal emphasis is in the development and application of theoretical models and state-of-the-art numerical simulations combining magnetohydrodynamics, high energy density physics, atomic and radiation physics, and spectroscopy.
  • Laser Plasma - Primary areas of research include physics underpinnings of laser fusion, high-energy-gain laser-inertial- fusion target designs, experiments and simulations of laser-matter interactions at high intensity, advancing the science and technologies of high-energy krypton fluoride and argon fluoride lasers, advancing the technologies of durable high-repetition-rate pulse power and electron-beam diodes for laser pumping and other applications, laser fusion as a power source.
  • Space and Laboratory Plasmas - Space research includes theoretical, numerical, and laboratory and space experimental investigations of the dynamic behavior of the near-Earth space plasmas and radiation belts, and the modification of space plasmas for strategic effects on HF communications, satellite navigation, over-the-horizon radar, and UHF satellite communications.  Applications-oriented plasma research is performed in the production, characterization, and use of low-temperature plasmas and related technology for applications to advance capabilities across the Navy and DOD.  Pulsed-power investigations include electromagnetic launch science and technology and research on directed energy systems for the U.S. Navy.
  • Pulsed Power Physics - Experimental and theoretical research is performed to advance pulsed power driven accelerator technology in areas relevant to defense applications. Research concerns the production, transport, characterization, and modeling of pulsed plasmas and intense high-power, charged particle beams using terawatt-class hundred-kilojoule pulsed power systems that employ capacitive or inductive energy storage and advanced switching. 
  • Directed Energy Physics - Research encompasses the integration of theoretical/computational and experimental research relevant to DOD, ONR, DARPA, and DoE in the areas of ultra-high field laser physics, atmospheric propagation of intense lasers, advanced radiation and accelerator physics, laser-generated plasma-microwave interactions, and dynamics of nonlinear systems. 

Facilities Fact Sheets

  • Electra Experimental Lab Facility - Electron beam pumped laser.  [ Download PDF]
  • NIKE KrF Laser Target Facility.  [Download PDF]
  • Space Plasma Simulation Chamber.  [Download PDF]

Plasma Physics News

NEWS | Dec. 11, 2025

Naval Research Laboratory Scientists Uncover Electric Field Link That Triggers Magnetic Reconnection in Space

By Jameson Crabtree, U.S. Naval Research Laboratory Corporate Communications

Scientists at the U.S. Naval Research Laboratory (NRL) have identified an electric field mechanism in Earth’s magnetotail that could help predict when disruptive space weather events are about to occur.

When the solar wind, a stream of charged particles from the sun, compresses Earth’s
magnetic field, it can generate sharply localized electric fields in the magnetotail, the region of space where Earth’s magnetic field is stretched away from the sun. NRL researchers have now confirmed that these electric fields cause a distinctive asymmetric motion of particles around the magnetic field causing agyrotropy, a sign that a magnetic reconnection event may be imminent.

“We’ve found that this electric field isn’t just a bystander, it’s a crucial ingredient that sets the stage for reconnection,” said Ami M. DuBois, Ph.D., a research physicist at NRL’s Plasma Physics Division. “Understanding how it interacts with charged particles can give us a clearer picture of when powerful space weather events are likely to occur.”

Magnetic reconnection occurs when magnetic field lines break and reconnect, releasing vast amounts of energy that can disrupt satellite operations, GPS, and electrical infrastructure on Earth. The new study confirms that electric fields created during magnetotail compression distort the natural circular motion of particles, forcing them into elongated paths that may signal reconnection is about to begin.

“When a solar storm hits Earth’s magnetosphere, the magnetotail gets compressed and high-energy plasma can be flung back toward Earth, disrupting satellites and the services they provide,”.

“Normally, electrons swirl around in circular paths,” she said. “However, when a strong electric field develops across regions in the magnetotail, those paths stretch out and become asymmetric. This non-circular behavior causes agyrotropy and is thought to be an early warning sign that a reconnection event is coming.”

Using data from NASA’s Magnetospheric Multiscale (MMS) mission, DuBois and NRL colleagues in the Plasma Physics Division Chris Crabtree, Ph.D., Emily Lichko, Ph.D., and Gurudas Ganguli, Ph.D., analyzed compressed current sheets in the magnetotail and confirmed that the perpendicular electric field plays a direct role in creating agyrotropy. Their results demonstrate a strong correlation between the field strength and the level of distortion observed in the electron orbit.

DuBois credited NASA’s MMS mission with enabling the discovery. “MMS is the first mission with super high time resolution meant to study magnetic reconnection, so we can really resolve the details inside very thin current sheets and study the dynamics around these sharply localized electric fields,” she said.

“As the magnetotail is compressed, the current sheets compress too, that’s what generates this electric field, and it grows as compression increases. It pops up before reconnection happens, and it affects the waves we see in the plasma, as well as the agyrotropic signatures in particle distributions,” DuBois said.

Existing methods for detecting this agyrotropy don’t account for the electric field’s influence. By incorporating this effect into new models, the team’s findings could enable scientists to more accurately predict space weather events before they impact satellites and ground-based systems.

DuBois compared the path forward to improvements in terrestrial weather. “Space-weather prediction is heavily model-based. The more real physics we add, the better the forecasts get, just like when Doppler radar and new science improved hurricane and tornado forecasts on Earth,” she said. “With the right sensors in the magnetotail, a detector for this agyrotropy signature could trigger alerts so operators might briefly power down vulnerable satellites or adjust operations until the event passes.”

“It’s not just satellites,” DuBois added. “Human spaceflight can be affected as well; for example, the International Space Station could benefit from timely alerts.”

Next, the team plans to turn their agyrotropy indicator into a predictive index by deriving the governing equations and validating them against additional MMS datasets.

This work builds on decades of NRL leadership in plasma physics, uniting long-standing theory and laboratory experiments on compressed boundary layers with today’s space measurements. “We’re putting together pieces that others have often studied separately: electric fields, waves, and particle signatures into one big-picture understanding,” DuBois said.

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.