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Separating the Sound from the Noise in Hot Plasma Fusion

  • September 11, 2018
  • Physics of Plasmas
  • News
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For the first time, researchers detected the geodesic acoustic mode at two locations within an experimental fusion reactor.

From the Journal: Physics of Plasmas

EAST, the Experimental Advanced Superconducting Tokamak, located in Hefei, China, with the researcher’s new diagnostic system located in the bottom right-hand corner. Credit: Adi LiuWASHINGTON, D.C., September 11, 2018 — In the search for abundant clean energy, scientists around the globe look to fusion power, where isotopes of hydrogen combine to form a larger particle, helium, and release large amounts of energy in the process. For fusion power plants to be effective, however, scientists must find a way to trigger the low-to-high confinement transition, or “L-H transition” for short. After a L-H transition, the plasma temperature and density increase, producing more power.

Scientists observe the L-H transition is always associated with zonal flows of plasma. Theoretically, zonal flows in a plasma consist of both a stationary flow with a near-zero frequency and one that oscillates at a higher frequency called the geodesic acoustic mode (GAM), which is a global sound wave of the plasma. For the first time, researchers at Hefei University of Technology have detected GAM at two different points simultaneously within the reactor. This new experimental setup will be a useful diagnostic tool for investigating the physics of zonal flows, and their role in the L-H transition. The researchers report these findings in a new paper published in Physics of Plasmas, from AIP Publishing.

Zonal flows occur anywhere there is turbulence, such as inside a fusion device or in a planet’s atmosphere. “The most famous zonal flows in nature may be the well-known Jovian belts and zones, which make Jupiter look like a colorful, multilayered cake,” said Ahdi Liu, an author on the paper. In fusion plasmas, zonal flows are crucial for regulating turbulence and particle transport within the reactor. “With the gradual improvement of diagnostic technology, zonal flows in fusion plasma has become a research hot spot in the past two decades,” Liu said.

In these experiments, researchers used the Experimental Advanced Superconducting Tokamak (EAST), a magnetic fusion energy reactor in Hefei, China. They installed two Doppler reflectometers on different sides of EAST, which can detect fluctuations in turbulence and plasma density with high precision. The detected GAM had a pitch of F, five octaves above middle C.

Previously, researchers at ASDEX-U, the fusion research device at the Max Plank Institute of Plasma Physics, used a similar system to detect GAM, but they measured the plasma at a single location, which makes the setup prone to interference. “This disadvantage is the main motivation for using two sets of Doppler reflectometers,” Liu said. “We could ‘purify’ the GAM information by comparing the two location’s measurements.”

The measurements taken at the two points did not entirely agree, showing that each reflectometer also picked up information from nonzonal flows. “It is completely necessary to extract accurate zonal flows information from multipoint measurement,” Liu said. Using both measurements, they could clearly show that GAM interacted with the ambient turbulence. Going forward, the researchers will further investigate the role of zonal flows in turbulence and turbulent transport within EAST.

###

For More Information:
Rhys Leahy
media@aip.org
301-209-3090
@AIPPhysicsNews

Article Title

Observation of geodesic acoustic mode in EAST using Doppler backscattering system

Authors

Xiaohui Zhang, Ahdi Liu, Chu Zhou, Jianqiang Hu, Mingyuan Wang, Xi Feng, Chunhua Li, Xingming Yang, Lei Sang and Jiaqiu Ai

Author Affiliations

Hefei University of Technology and the University of Science and Technology of China


Physics of Plasmas

Physics of Plasmas is devoted to the publication of original experimental and theoretical work in plasma physics, from basic plasma phenomena to astrophysical and dusty plasmas.

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