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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 | Oct. 22, 2024

NRL's CCOR-1 Instrument Captures Its First Images of the Sun's Atmosphere

By Emily Winget, U.S. Naval Research Laboratory Corporate Communications

U.S. Naval Research Laboratory’s (NRL) Compact Coronagraph (CCOR) instrument has successfully collected its first images of coronal mass ejections (CMEs).
 
CCOR is a small space telescope designed to observe the Sun's atmosphere. On Sept. 19, the aperture door of CCOR was opened for the first time since it was launched on National Oceanic and Atmospheric Administration’s (NOAA) GOES-19 spacecraft on June 25 from NASA’s Kennedy Space Flight Center.
 
The full sunlight directly illuminated the inside of the instrument where a cylindrical device at the center of its field of view, called an occulter, blocks the Sun and creates an artificial eclipse – just like the moon would block the solar disk during an eclipse. As a result, the CCOR does not observe the Sun but only its outer atmosphere, called the solar corona, said Arnaud Thernisien, a research physicist from the NRL Advanced Sensor Technology Section within the Space Science Division.
 
On Oct. 3, the CCOR saw a perfect illustration of the Sun’s activity called a halo. Halos appear on coronagraph images as near-circular shapes, approximately concentric with the Sun’s center. The observed halo CME resulted in some effects seen on Earth a few days later including a rare glimpse of northern lights visible across the northern United States from Washington state to Maine. Northern lights, also called auroras, are the result of Earth’s magnetosphere disturbance with solar wind.
 
Over the next few weeks, the CCOR witnessed several CMEs including another halo on Oct. 10, resulting from an active region at the surface of the sun. “Halo CMEs are of particular interest for space weather as they are generally directed towards Earth,” Thernisien said.
 
“By creating an artificial eclipse, the CCOR allows scientists to study the Sun's corona, which can produce powerful solar storms that can disrupt Earth-based technologies,” said Thernisien. “The CCOR team is thrilled to see that the instrument is performing as expected.”
 
The instrument is used by NOAA's Space Weather Prediction Center (SWPC) and DOD to detect CMEs with low latency, providing critical early warnings of solar storms. CMEs can have severe consequences, including damage to satellites, disruptions to radio communications, and power grid failures.
 
NRL’s CCOR is the nation’s first operational coronagraph. Operational means that the instrument is tailored to provide low-latency observations of the corona and has some resilience to radiation-induced space weather effects.
 
CCOR is just the beginning of a series of operational coronagraphs that NRL is developing for NOAA. A second instrument, CCOR-2, is scheduled for launch in mid-2025. Additionally, NRL is working on a compact coronagraph for the European Space Agency's Vigil mission, which is scheduled for launch in 2031.
 
"The NRL team, in collaboration with the NOAA-NASA GOES Team, will continue testing the capabilities of CCOR-1 in space up until the end of January 2025 when it will be handed over to NOAA,” Thernisien said. “NRL would like to thank NOAA-NASA's Office of Space Weather Observations and the Office of Naval Research for their support.”
 
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 is 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.
 
For more information, contact NRL Corporate Communications at (202) 480-3746 or nrlpao@nrl.navy.mil. Please reference package number at top of press release.
 
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