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Detailed Reference Information |
Hellinger, P., Velli, M., Trávnícek, P., Gary, S.P., Goldstein, B.E. and Liewer, P.C. (2005). Alfvén wave heating of heavy ions in the expanding solar wind: Hybrid simulations. Journal of Geophysical Research 110: doi: 10.1029/2005JA011244. issn: 0148-0227. |
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We present hybrid expanding box simulations of the interaction of left-handed Alfv¿n waves with protons, alpha particles, and a tenuous population of oxygen O5+. The Alfv¿n waves are initially nonresonant with the ions, and the expansion brings them to the cyclotron resonance with O5+ ions, then with alpha particles, and finally with protons. The simulations show that O5+ ions are efficiently heated in the directions perpendicular to the background magnetic field but are only slightly accelerated. Oxygen scattering has a finite time span and saturates mainly due to the marginal stabilization with respect to the oxygen cyclotron instability generated by the temperature anisotropy. During the scattering, oxygen ions are able to absorb only a limited amount of available fluctuating energy and, for the parameters used in the simulations, their presence has a minimum influence on alpha particles and protons. |
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Abstract |
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Keywords
Interplanetary Physics, Solar wind plasma, Interplanetary Physics, Plasma waves and turbulence, Space Plasma Physics, Wave/particle interactions (2483, 6984), Space Plasma Physics, Kinetic and MHD theory, Space Plasma Physics, Plasma energization, Alfvén waves, solar wind heating, microinstabilities |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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