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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 | Aug. 7, 2023

NRL and NASA to Launch ComPair Instrument to Measure Gamma-Ray Emissions

By Mary Hamisevicz, U.S. Naval Research Laboratory Corporate Communications

WASHINGTON  –   The U.S. Naval Research Laboratory (NRL) and NASA Goddard Space Flight Center (GSFC) will launch ComPair aboard a high-altitude balloon from Fort. Sumner, New Mexico Aug. 10.
 
The ComPair mission instrument measures and detects gamma-ray emissions from astrophysical objects. The NRL instrument is one of the four subsystem instruments led by NASA GSFC. The mission name – ComPair – is inspired by the mechanisms by which gamma rays interact with matter.
 
“They do so via three dominant processes – photoelectric effect, Compton scattering, and pair production. These interaction mechanisms are dependent on energy, where photoelectric occurs at the lowest energies and pair production at the highest,” said NRL Space Science Division Research Physicist Richard S. Woolf, Ph.D. “The design of the ComPair instrument employs technology to measure gamma rays from both the Compton and the pair production regimes, hence Compton-Pair or ComPair.”
 
“Gamma rays allow us to study the highest-energy processes in the universe: ranging from nucleosynthesis in supernovae; jets from supermassive black holes; and gamma-ray bursts from the merger of astrophysical objects with extreme densities, like neutron stars and black holes,” Woolf said. “The atmosphere mostly blocks astrophysical sources of gamma rays from reaching the ground at sea level, to measure the rays, the instrument needs to reach above the majority of the atmosphere up to 130,000 ft.”

The goal in the development of this instrument is to increase the technical readiness level (TRL) of this gamma ray technology. One of the last steps in advancing the TRL for gamma-ray instruments is to fly on a high-altitude balloon.
 
“The hope is that what we learn during this phase will be applied to a larger, more sensitive mission that goes into orbit for a future NASA-led mission known as the All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X). AMEGO-X is a medium-class mission that will be proposed to the NASA Explorers program announcement of opportunity, expected in 2026,” Woolf said.
 
After the launch of the Fermi Gamma-ray Space Telescope in June 2008, the gamma-ray community started to consider where they should focus their attention next. The idea was to use a similar design to Fermi but with sensitivity in the much lower-energy range of the gamma ray spectrum.
 
“The ComPair instrument design is based on a previous NRL-led instrument, the Fermi Large Area Telescope (LAT) calorimeter, containing scintillation crystals, meaning they emit light or scintillates when ionizing radiation passes through it,” Woolf said. “ComPair expands on the technology of the Fermi LAT calorimeter by using a novel scintillation light readout device known as a silicon photomultiplier (SiPM) coupled to the crystals that comprise the calorimeter. These SiPMs are more sensitive for reading out scintillation light, enabling gamma-ray detection in the Compton region.”
 
Scintillation is the physical process where a material, called a scintillator, emits ultraviolet or visible light under excitation from high energy photons: such as, X-rays or gamma rays, or energetic particles.
 
The NRL Space Science Division advances technical capabilities in the orbital tracking, radio communications, and navigation realms affecting the operation of ships and aircraft, application of the near-space and space environment of the Earth, and the fundamental understanding of natural radiation and geophysical phenomena.
 
“NASA GSFC and NRL, have a history with this next-generation instrument from the start,” Woolf said. “NRL’s initial funding from NASA commenced in early 2015 and has continued with multiple rounds of funding since, allowing us to build a proof-of-concept prototype, test the prototype at several accelerator beam tests, and now fly it on a high-altitude balloon.”


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 the U.S. 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, and 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.