Two-dimensional hybrid model of wave and beam heating of multi-ion solar wind plasma

Journal of Geophysical Research: Space Physics

Volumn 112, Issue 6, 2007, Pages

  Ofman, L ^a,b   Vinas A F ^b  

^a CATHOLIC UNIVERSITY OF AMERICA   (United States)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 34548346894     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2006JA012187     Document Type: Article

References (33)

1. Araneda, J. A., A. F. Viñas, and H. F. Astudillo (2002), Proton core temperature effects on the relative drift and anisotropy evolution of the ion beam instability in the fast solar wind, J. Geophys. Res., 107(A12), 1453, doi: 10.1029/2002JA009337.
2. Cranmer, S. R. (2000), Ion cyclotron wave dissipation in the solar corona: The summed effect of more than 2000 ion species, Astrophys. J., 532, 1197-1208.
3. Cranmer, S. R., G. B. Field, and J. L. Kohl (1999a), Spectroscopic constraints on models of ion cyclotron resonance heating in the polar solar corona and high-speed solar wind, Astrophys. J., 518, 937-947.
4. Cranmer, S. R., et al. (1999b), An empirical model of a polar coronal hole at solar minimum, Astrophys. J., 511, 481-501, doi:10.1086/306675.
5. Daughton, W., and S. P. Gary (1998), Electromagnetic proton/proton instabilities in the solar wind, J. Geophys. Res., 103, 20,613-20,620.
6. Daughton, W., S. P. Gary, and D. Winske (1999), Electromagnetic proton/ proton instabilities in the solar wind: Simulations, J. Geophys. Res., 104, 4657-4668.
7. Davidson, R. C., and J. M. Ogden (1975), Electromagnetic ion cyclotron instability driven by ion energy anisotropy in high-beta plasmas, Phys. Fluids, 18, 1045-1050.
8. Dusenbery, P. B., and J. V. Hollweg (1981), Ion-cyclotron heating and acceleration of solar wind minor ions, J. Geophys. Res., 86, 153-164.
9. Fried, B. D., and S. D. Conte (1961), The Plasma Dispersion Function, Academic, San Diego, Calif.
10. Gary, S. P. (1993), Theory of Space Plasma Microinstabilities, Cambridge Univ. Press, New York.
11. Gary, S. P., L. Yin, D. Winske, and L. Ofman (2001), Electromagnetic heavy ion cyclotron instability: Anisotropy constraint in the solar corona, J. Geophys. Res., 106, 10,715-10,722.
12. Gary, S. P., L. Yin, D. Winske, L. Ofman, B. E. Goldstein, and M. Neugebauer (2003), Consequences of proton and alpha anisotropics in the solar wind: Hybrid simulations, J. Geophys. Res., 108(A2), 1068, doi:10.1029/2002JA009654.
13. Gomberoff, L., and R. Elgueta (1991), Resonant acceleration of alpha particles by ion cyclotron waves in the solar wind, J. Geophys. Res., 96, 9801-9804.
14. + plasma, J. Geophys. Res., 88, 2170-2174.
15. Gomberoff, L., F. T. Gratton, and G. Gnavi (1996), Acceleration and heating of heavy ions by circularly polarized Alfvén waves, J. Geophys. Res., 101, 15,661-15,666.
16. Hollweg, J. V. (2006), Drivers of the solar wind: then and now, R. Soc. Phil. Trans. London, Ser. A, 364, 505-527.
17. Hollweg, J. V., and P. A. Isenberg (2002), Generation of the fast solar wind: A review with emphasis on the resonant cyclotron interaction, J. Geophys. Res., 107(A7), 1147, doi:10.1029/2001JA000270.
18. Isenberg, P. A. (2004), The kinetic shell model of coronal heating and acceleration by ion cyclotron waves: 3. The proton halo and dispersive waves, J. Geophys. Res., 109, A03101, doi:10.1029/2002JA009449.
19. Isenberg, P. A., and J. V. Hollweg (1982), Finite amplitude Alfven waves in a multi-ion plasma: Propagation, acceleration, and heating, J. Geophys. Res., 87, 5023-5029.
20. Isenberg, P. A., and J. V. Hollweg (1983), On the preferential acceleration and heating of solar wind heavy ions, J. Geophys. Res., 88, 3923-3935.
21. Kohl, J. L., et al. (1997), First results from the SOHO ultraviolet coronagraph spectrometer, Sol. Phys., 175, 613-644.
22. Leubner, M. P., and A. F. Viñas (1986), Stability analysis of double-peaked proton distribution functions in the solar wind, J. Geophys. Res., 91, 13,366-13,372.
23. Li, X., S. R. Habbal, J. Kohl, and G. Noci (1998), The effect of temperature anisotropy on observations of Doppler dimming and pumping in the inner corona, Astrophys. J., 501, L133-L137.
24. Liewer, P. C., M. Velli, and B. E. Goldstein (2001), Alfvén wave propagation and ion cyclotron interactions in the expanding solar wind: One-dimensional hybrid simulations, J. Geophys. Res., 106, 29,261-29,282.
25. Lu, Q. M., L. D. Xia, and S. Wang (2006), Hybrid simulations of parallel and oblique electromagnetic alpha/proton instabilities in the solar wind, J. Geophys. Res., 111, A09101, doi:10.1029/2006JA011752.
26. Ofman, L. (2005), MHD Waves and Heating in Coronal Holes, Space Sci. Rev., 120, 67-94, doi: 10.1007/s11214-005-5098-1.
27. +5 anisotropy in the solar corona, Astrophys. J., 547, L175-L178, doi:10.1086/ 318900.
28. Ofman, L., S. P. Gary, and A. Viñas (2002), Resonant heating and acceeration of ions in coronal holes driven by cyclotron resonant spectra, J. Geophys. Res., 107(A12), 1461, doi:10.1029/2002JA009432.
29. Ofman, L., J. M. Dávila, V. M. Nakariakov, and A.-F. Viñas (2005), High-frequency Alfvén waves in multi-ion coronal plasma: Observational implications, J. Geophys. Res., 110, A09102, doi: 10.1029/ 2004JA010969.
30. Vasquez, B. J. (2005), Resonant absorption of an Alfvén wave: Hybrid simulations, J. Geophys. Res., 110, A10S02, doi:10.1029/ 2004JA010872.
31. Wimmer-Schweingruber, R. F., R. von Steiger, J. Geiss, G. Gloeckler, F. M. Ipavich, and B. Wilken (1998), O5+ in high speed solar wind streams: SWICS/Ulysses results, Space Sci. Rev., 85, 387-396.
32. Winske, D., and N. Omidi (1993), Computer Space Plasma Physics: Simulation Techniques and Sowftware, edited by H. Matsumoto and Y. Omura, pp. 103-160, Terra Sci., Tokyo.
33. Xie, H., L. Ofman, and A. Viñas (2004), Multiple ions resonant heating and acceleration by Alfvén/cyclotron fluctuations in the corona and the solar wind, J. Geophys. Res., 109, A08103, doi: 10.1029/2004JA010501.