Physics
Scientific paper
Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216...64i&link_type=abstract
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 64-67 (2010).
Physics
1
Solar Wind, Magnetohydrodynamics, Cyclotron Resonance, Plasma Waves, Particle Emission, Solar Wind, Magnetohydrodynamics And Plasmas, Ion Cyclotron Resonance Mass Spectrometry, Plasma Interactions With Antennas, Plasma-Filled Waveguides
Scientific paper
We investigate the quasilinear effects of the resonant wave-particle interaction under conditions of imbalanced turbulent heating in the collisionless coronal hole. We find that velocity-space transport of protons from the heated part of the distribution leads to strong wave growth in the minority (sunward) direction. In the present quasilinear analysis, the ``reflected'' waves grow to unphysical levels, indicating the necessity of including nonlinear processes. This mechanism is likely to be important in development of the fast solar wind, and may explain the puzzling minor ion observations of Landi & Cranmer (2009).
Chandran Benjamin D. G.
Isenberg Philip A.
Pongkitiwanichakul Peera
Vasquez Bernard J.
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