The kinetic shell model of coronal heating and acceleration by ion cyclotron waves 1. Outward propagating waves

Journal of Geophysical Research: Space Physics

Volumn 106, Issue 4, 2001, Pages 5649-5660

  Isenberg, Philip A ^a,b   Lee, Martin A ^a,b   Hollweg, Joseph V ^a,b  

^a Univ of New Hampshire   (United States)

^b UNIVERSITY OF NEW HAMPSHIRE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000992233     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2000ja000099     Document Type: Article

References (64)

1. Abraham-Shrauner, B., and W. C. Feldman, Nonlinear Alfvén waves in high-speed solar wind streams, J. Geophys. Res., 82, 618,1977.
2. Axford, W. I., and J. F. McKenzie, The origin of high speed solar wind streams, in Solar Wind Seven, edited by E. Marsch, and R. Schwenn, p. 1, Pergamon, Tarrytown, N. Y., 1992.
3. Axford, W. I., and J. F. McKenzie, The acceleration of the solar wind, in Solar Wind Eight, edited by D. Winterhalter, J. T. Gosling, S. R. Habbal, W. S Kurth, and M. Neugebauer, p. 72, Am. Inst, of Phys., College Park, Md., 1996.
4. Cranmer, S. R., Ion cyclotron wave dissipation in the solar corona: The summed effect of more than 2000 ion species, Astrophys. J., 532, 1197,2000.
5. Cranmer, S. R., G. B. Field, G. Noci, and J. L. Kohl, The impact of UVCS/SOHO observations on models of ion-cyclotron resonance heating of the solar corona, in Correlated Phenomena at the Sun, in the Heliosphere, and in Geospace, edited by A. Wilson, p 89, Eur. Space Agency. Noordwijk, Netherlands, 1997.
6. Cranmer, S. R., G. B. Field, and J. L Kohl, Spectroscopic constraints on models of ion cyclotron resonance heating in the polar solar corona and high-speed solar wind, Astrophys J., 518, 937, 1999.
7. Dodero, M. A., E. Aiitonucci, S. Giordano, and R. Martin, Solar wind velocity and anisotropic coronal kinetic temperature measured with the O VI doublet ratio, Sol. Phys., 183, 77, 1998.
8. Dusenbery, P. B., and J. V. Hollweg, Ion-cyclotron heating and acceleration of solar wind minor ions, J Geophys. Res., 86, 153, 1981.
9. Esser, R., and S. R. Habbal, Coronal heating and plasma parameters at 1 AU, Geophys. Res. Lett., 22, 2661, 1995.
10. Esser, R., S. R. Habbal, W. A. Coles, and J. V Hollweg, Hot protons in the inner corona and their effect on the flow properties of the solar wind, J. Geophys. Res., 102, 7063, 1997.
11. Esser, R., S. Fineschi, D. Dobrzycka, S. R. Habbal, R. J. Edgar, J. C. Raymond, J. L. Kohl, and M. Guhathakurta, Plasma properties in coronal holes derived from measurements of minor ion spectral lines and polarized white light intensity, Astrophys. J., 510, L63, 1999.
12. Feldman, W. C, Unresolved questions about the structure and dynamics of the extended solar corona, in Sun-Earth Plasma Connections, Geophys. Monogr. Ser., vol.109, edited by J. L. Burch, R. L. Carovillano, and S. K. Antiochos, p. 121, AGU, Washington, D.C., 1999.
13. Fisher, R., and M. Guhathakurta, Physical properties of polar coronal rays and holes as observed with the Spartan 201-01 coronagraph, Astrophys. J., 447, L139, 1995.
14. Galinsky, V. L., and V. I. Shevchenko, Nonlinear cyclotron resonant wave-particle interaction in a nonuniform magnetic field, Phys. Rev. Lett., 85,90,2000.
15. Habbal, S. R., R. Esser, M. Guhathakurta, and R. R. Fisher, Flow properties of the solar wind derived from a two-fluid model with constraints from white light and in situ interplanetary observations, Geophys. Res. Lett., 22, 1465, 1995
16. Hammer, R., Energy balance of stellar coronae, I, Methods and examples, Astrophys J., 259,767, 1982a.
17. Hammer, R., Energy balance of stellar coronae, II, Effect of coronal heating, Astrophys. J., 259,119, 1982b.
18. Hansteen, V. H., and E. Leer, Coronal heating, densities, and temperatures and solar wind acceleration, J. Geophys. Res., 100,21,593, 1995.
19. Hollweg, J. V., Alfvénic acceleration of solar wind helium and related phenomena, 1., Theory, J. Geophys. Res., 79, 1357, 1974.
20. Hollweg, J. V., Transition region, corona, and solar wind in coronal holes, J. Geophys. Res., 91, 4111, 1986.
21. Hollweg, J. V., Potential wells, the cyclotron resonance, and ion heating in coronal holes, J. Geophys. Res., 104, 505, 1999a.
22. +9 , J. Geophys. Res., 104, 24,781, 1999b.
23. Hollweg, J. V., Cyclotron resonance in coronal holes, 2, A two-proton description, J. Geophys. Res., 104,24,793, 1999c.
24. Hollweg, J. V., Cyclotron resonance in coronal holes, 3, A five-beam turbulence-driven model, J. Geophys. Res., 105, 15,699, 2000a.
25. Hollweg, J V., Compressibility of ion cyclotron and whistler waves: Can radio measurements detect high-frequency waves of solar origin in the corona?, J. Geophys. Res., 105, 7573,2000b.
26. Hollweg, J. V., and W. Johnson, Transition region, corona, and solar wind in coronal holes: Some two-fluid models, J. Geophys. Res., 93, 9547, 1988.
27. ++, 3, Effects of resonant and nonresonant interactions with transverse waves, J. Geophys. Res., 83, 97, 1978.
28. Holzer, T. E., and E. Leer, Conductive solar wind models in rapidly diverging flow geometries, J. Geophys. Res., 85,4665, 1980.
29. Hu, Y. Q., and S. R. Habbal, Resonant acceleration and heating of solar wind ions by dispersive ion cyclotron waves, J. Geophys. Res., 104, 17,045,1999.
30. Hu, Y. Q., R Esser, and S. R. Habbal, A fast solar wind model with anisotropic proton temperature, J. Geophys. Res., 102, 14,661, 1997.
31. Hu, Y. Q., S. R. Habbal, and X. Li, On the cascade processes of Alfvén waves in the fast solar wind, J. Geophys. Res., 104, 24,819, 1999.
32. Hu, Y. Q., R. Esser, and S. R. Habbal, A four-fluid turbulence-driven solar wind model for preferential acceleration and heating of heavy ions, J. Geophys. Res., 105, 5093,2000.
33. Isenberg, P. A., Acceleration of heavy ions in the solar wind, in Solar Wind Five, edited by M. Neugebauer, NASA Conf. Proc-2280, 655, 1983.
34. Isenberg, P. A., Resonant acceleration and heating of solar wind ions: Anisotropy and dispersion, J. Geophys. Res., 89, 6613, 1984.
35. Isenberg, P. A., Investigations of a turbulence-driven solar wind, J. Geophys. Res., 95, 6431, 1990.
36. Isenberg, P. A., A hemispherical model of anisotropic interstellar pickup ions, J. Geophys. Res., 102,4719, 1997.
37. Isenberg, P. A., Heating of coronal holes and generation of the solar wind by ion-cyclotron resonance, Space Set. Rev., in press, 2001.
38. Isenberg, P. A., and J. V. Hollweg, On the preferential acceleration and heating of solar wind heavy ions,J. Geophys Res., 88, 3923, 1983.
39. Isenberg, P. A., and M. A. Lee, A dispersive analysis of bispherical pickup ion distributions, J. Geophys. Res., 101, 11,055, 1996.
40. Isenberg, P. A., M. A. Lee, and J. V. Hollweg, A kinetic model of coronal heating and acceleration by ion-cyclotron waves: Preliminary results, Sol. Phys., 193, 247,2000.
41. Kennel, C. F., and F Engelmann, Velocity space diffusion from weak plasma turbulence in a magnetic field, Phys. Fluids, 9, 2311, 1966.
42. Kohl, J. L., et al., UVCS/SOHO empirical determinations of anisotropic velocity distributions in the solar corona, Astrophys. J., 501, L127 1998.
43. Kohl, J. L., R. Esser, S. R. Cranmer, S. Fineschi, L. D. Gardner, A. V. Panasyuk, L. Strachen, R. M. Suleiman, R. A. Frazin, and G. Noci, EUV spectral line profiles in polar coronal holes from 1.3 to 3.0 R , Astrophys. J., 510, L59, 1999.
44. Kulsrud, R. M., MHD description of plasma, in Basic Plasma Physics I, edited by A. A. Galeev and R. N. Sudan, p. 115-145, North-Holland, New York, 1983.
45. Leer, E., and T. E. Holzer, Energy addition in the solar wind, J. Geophys. Res., 85, 4681, 1980.
46. Li, X., Proton temperature anisotropy in the fast solar wind: A 16-moment bi-Maxwellian model, J. Geophys. Res., 104, 19,773, 1999.
47. Li, X., S. R. Habbal, J. V. Hollweg, and R. Esser, Heating and cooling of protons by turbulence-driven ion cyclotron waves in the fast solar wind, J. Geophys. Res., 104, 2521, 1999a.
48. Li, X., S. R. Habbal, J. V. Hollweg, and R. Esser, Proton temperature anisotropy in the fast solar wind: Turbulence-driven dispersive ion-cyclotron waves, in Solar Wind Nine, edited by S. R. Habbal, R. Esser, J. V. Hollweg, and P. A. Isenberg, p. 531, Am. Inst, of Phys., College Park, Md., 1999b.
49. Marsch, E., Kinetic physics of the solar wind plasma, in Physics of the Inner Heliosphere. vol.2. Particles, Waves and Turbulence, edited by R. Schwenn and E. Marsch, p. 45, Springer-Verlag, New York, 1991.
50. Marsch, E., and C.-Y. Tu, The effects of high-frequency Alfvén waves on coronal heating and solar wind acceleration, Astron. Astrophys., 319, L17, 1997.
51. Marsch, E., C. K. Goertz, and A. K. Richter, Wave heating and acceleration of solar wind ions by cyclotron resonance, J. Geophys. Res., 87, 5030,1982.
52. Matthaeus, W. H., G. P. Zank, S. Oughton, D. J. Mullan, and P. Dmitruk, Coronal heating by magnetohydrodynamic turbulence driven by reflected low-frequency waves, Astrophys. J., 523, L93, 1999.
53. McKenzie, J. F., W.-H. Ip, and W. I. Axford, The acceleration of minor ion species in the solar wind, Astrophys. Space Sci., 64, 183, 1979.
54. McKenzie, J. F., M. Banaszkiewicz, and W. I. Axford, Acceleration of the high speed solar wind, Astron. Astrophys., 303, 45, 1995.
55. McKenzie, J. F., W. I. Axford, and M. Banaszkiewicz, The fast solar wind, Geophys. Res. Lett., 24, 2877, 1997.
56. Munro, R. H., and B. V. Jackson, Physical properties of a polar coronal hole from 2 to 5 R Astrophys. J., 213, 874, 1977.
57. Olsen, E. L., and E Leer, A study of solar wind acceleration based on gyrotropic transport equations, J. Geophys. Res., 104, 9963, 1999.
58. Rowlands, J., V. D Shapiro, and V. I. Shevchenko, Quasilinear theory of plasma cyclotron instability, Sov. Phys. JETP, Engl. Transl., 23, 651, 1966.
59. Ruzmaikin, A., and M. A. Berger, On a source of Alfvén waves heating the solar corona, Astron. Astrophys., 337, L9, 1998.
60. Shevchenko, V I., V. L. Galinsky, M. Medvedev, P. H. Diamond, S. K. Ride, and R. Z Sagdeev, Acceleration of the solar wind ions, Eos Trans. AGU, 80(46), Fall Meet. Suppl., F800, 1999.
61. Skilling, J., Cosmic rays in the galaxy: Convection or diffusion?, Astrophys. J., 170, 265, 1971.
62. Tarn, S. W. Y., and T. Chang, Kinetic evolution and acceleration of the solar wind, Geophys. Res. Lett., 26, 3189, 1999.
63. Tu, C.-Y., and E. Marsch, Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfv6n waves, Sol. Phys., 171, 363, 1997.
64. Withbroe, G. L., The temperature structure, mass, and energy flow in the corona and inner solar wind, Astrophys. J., 325,442, 1988.