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Laboratory study of avalanches in magnetized plasmas
B Van Compernolle1, G J Morales1, J E Maggs1
1Physics and Astronomy Department, University of California, Los Angeles, Los Angeles, California 90095, USA.
Controlled plasma heating reveals avalanche phenomena. Intermittent pressure collapses linked to drift-Alfvén waves show distinct power-law spectra, offering insights into plasma dynamics.
Area of Science:
- Plasma Physics
- Magnetohydrodynamics
- Wave Phenomena
Background:
- Avalanche phenomena in magnetized plasmas are complex and difficult to study under controlled conditions.
- Understanding plasma pressure profile dynamics is crucial for fusion energy and astrophysical plasmas.
- Drift-Alfvén waves are known to destabilize plasma profiles.
Purpose of the Study:
- To investigate avalanche phenomena in a large, cold magnetized plasma using a novel heating configuration.
- To characterize the power-law spectrum of plasma pressure profile collapses.
- To map the spatiotemporal evolution of individual avalanche events.
Main Methods:
- Application of a novel heating configuration to a large, cold magnetized plasma.
- Observation and analysis of intermittent plasma pressure profile collapses.
- Spectroscopic analysis of unstable drift-Alfvén waves.
- Detailed spatiotemporal mapping of avalanche events.
Main Results:
- The novel heating configuration enables controlled study of plasma avalanches.
- Intermittent pressure profile collapses exhibit a two-slope power-law spectrum.
- Spectral exponents are approximately -1 at lower frequencies and -2 to -4 at higher frequencies.
- The spatiotemporal evolution of a single avalanche event was successfully mapped.
Conclusions:
- The study successfully demonstrates controlled observation of plasma avalanche phenomena.
- The observed two-slope power-law spectrum provides new data on avalanche dynamics.
- Detailed mapping of avalanche events enhances understanding of underlying wave-particle interactions.
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