Using HERCULES to probe the interior of dense plasmas
Thanks to HERCULES, scientists are now able to study very dense plasmas — a crucial step in nuclear fusion and astrophysical research.
For the first time, researchers probed the interior of highly dense plasmas using the world’s most intense tabletop laser called HERCULES, located in the Center for Ultrafast Optical Science (CUOS). Scientists are now able to study very dense plasmas, which has important implications for nuclear fusion energy and astrophysical research.
“No one has been able to do this before,” said Dr. Anatoly Maksimchuk, who specializes in high-intensity laser research and laser-plasma interaction at CUOS along with Dr. Vladimir Chyvkov, Dr. Victor Yanovsky, director of the HERCULES laser, Prof. Alec Thomas, and Prof. Karl Krushelnik, director of CUOS. “It took the capability of HERCULES to generate directional electron beams of sufficient quality and strength to accomplish this breakthrough.”
Exploiting this capability, graduate student Will Schumaker and a team of researchers were able to image extremely strong magnetic fields (10,000 times that of the strongest bar magnet) in a surface plasma of only 10s of microns in size that was expanding at close to the speed of light. The research was published in the January edition of Physical Review Letters.
Explains Dr. Maksimchuk, “Intense laser pulses interacting with solid surfaces can create very energetic and dense plasmas. These plasmas are highly complex and often evolve on very short time scales, so that measurement of plasma parameters such as density and magnetic field strength requires very short bursts of probing radiation which can penetrate through the plasma.
Using the 30 femtosecond (30×10-15 seconds) duration laser pulse from the HERCULES laser, intense light was focused onto a thin metal foil to generate a rapidly expanding surface plasma. To “probe” the magnetic fields generated within this plasma, a second short laser pulse was focused into atmospheric density gas. This generated a burst of relativistic electrons by “surfing” them on the electric plasma wave generated behind the pulse; the temporal duration of the resulting electrons was comparable to that of the laser pulse.
Having propagated through the magnetic fields generated in the laser-solid interaction, the spatial distribution of electrons reflects the magnetic field structure at the time when they were deflected. By adjusting the delay between the pulse hitting the solid target and the probe electron pulse, it is now possible to make a “movie” of plasma evolution.”
This will facilitate research into numerous areas, including: inertial confinement fusion; compact particle accelerators; radiation sources; and scaled astrophysical experiments.
The research was highlighted on the American Physics Society website, Physics, which spotlights exceptional research of the selected papers published in the Physical Review Letters journal. The original paper, Ultrafast Electron Radiography of Magnetic Fields in High-Intensity Laser-Solid Interactions, by William Schumaker, N. Nakanii, C. McGuffey, C. Zulick, Vladimir Chyvkov, F. Dollar, H. Habara, Galina Kalintchenko, Anatoly Maksimchuk, K. A. Tanaka, A. G. R. Thomas, Victor Yanovsky, and Karl Krushelnick. Phys. Rev. Lett. 110, 015003 (2013), was published Jan. 2, 2013.
Slashing exposure time for plasma imaging (by Kate McAlpine, College of Engineering Press Release, Jan. 11, 2013)
A stellar achievement: Magnetized space winds in the laboratory
The international team that includes Prof. Louise Willingale is investigating the role of intense magnetic fields dragged by high-speed plasmas through astrophysical environments. HERCULES was used in the experiments.
Why space weather is being made in the lab
Lousie Willingale, assistant professor ECE, discusses her research using HERCULES to study magnetized space winds in a lab.