Other
Scientific paper
Mar 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phrvl..96l5001w&link_type=abstract
Physical Review Letters, vol. 96, Issue 12, id. 125001
Other
27
Plasma Production And Heating, Nonlinear Phenomena: Waves, Wave Propagation, And Other Interactions, Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
Finite-amplitude intrinsic Alfvén waves exist pervasively in astrophysical and solar-terrestrial environment. It is generally believed that linear wave-particle resonant interaction between thermal protons and Alfvén waves is ineffective when the proton beta is low. However, this Letter demonstrates that the ions can be heated by Alfvén waves via nonresonant nonlinear interaction. Contrary to the customary expectation, it is found that the lower the plasma beta value, the more effective is the heating process. It is also shown that the ion temperature increase is more prominent along perpendicular direction.
Wang Chang-Bin
Wu Shang-Chen
Yoon Peter H.
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