Publication | Open Access
Spectral gap of shear Alfvén waves in a periodic array of magnetic mirrors
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Citations
38
References
2008
Year
Electromagnetic WaveEngineeringMagnetic MirrorsPhysicsWave PropagationApplied PhysicsPlasma TheoryShear Alfvén WavesPlasma InstabilityApplied Plasma PhysicPlasma PhysicsLapd PlasmaSpace Plasma PhysicInstrumentationSpectral GapLarge Plasma DevicePlasma DiagnosticsMirror Array Configuration
A multiple magnetic mirror array is formed at the Large Plasma Device (LAPD) [W. Gekelman, H. Pfister, Z. Lucky, J. Bamber, D. Leneman, and J. Maggs, Rev. Sci. Instrum. 62, 2875 (1991)] to study axial periodicity-influenced Alfvén spectra. Shear Alfvén waves (SAW) are launched by antennas inserted in the LAPD plasma and diagnosed by B-dot probes at many axial locations. Alfvén wave spectral gaps and continua are formed similar to wave propagation in other periodic media due to the Bragg effect. The measured width of the propagation gap increases with the modulation amplitude as predicted by the solutions to Mathieu’s equation. A two-dimensional finite-difference code modeling SAW in a mirror array configuration shows similar spectral features. Machine end-reflection conditions and damping mechanisms including electron-ion Coulomb collision and electron Landau damping are important for simulation.
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