Acceleration of the high speed solar wind in coronal holes

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 25-41

  Axford, W I ^a   Mckenzie, J F ^a   Sukhorukova, G V ^a   Banaszkiewicz, M ^b   Czechowski, A ^b   Ratkiewicz, R ^b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b Polish Academy of Sciences   (Poland)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001913561     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005197529250     Document Type: Article

References (38)

1. Alazraki, G., and Couturier, P.: 1971, Solar wind acceleration caused by the gradient of Alfvén wave pressure, Astron. Astrophys., 13, 380-389.
2. Axford, W. I.: 1980, Very hot plasmas in the solar system, in Highlights of Astronomy, ed. P. A. Wayman, 5, pp. 351-359.
3. Axford, W. I., and McKenzie, J. F.: 1992, The origin of high speed solar wind streams, in Solar Wind Seven, eds. E. Marsch and R. Schwenn (Oxford: Pergamon Press), pp. 1-5.
4. Axford, W. I., and McKenzie, J. F.: 1997, The solar wind, in Cosmic Winds and the Heliosphere, eds. J. R. Jokipii, C. P. Sonett, and M. S. Giampapa (Tucson: University of Arizona Press), pp. 31-36.
5. Banaszkiewicz, M., Axford, W. I., and McKenzie, J. F.: 1998, An analytic solar magnetic field model, Astron. Astrophys., 337, 940-944.
6. Belcher, J. W.: 1971, Alfvénic wave pressure in the solar wind, Astrophys. J., 168, 509-524.
7. Borrini, G., Gosling, J. T., Bame, S. J., Feldman, W. C., and Wilcox, J. M.: 1981, Solar wind helium and hydrogen structures near the heliospheric current sheet: A signal of coronal streamers at 1 AU, J. Geophys. Res., 86, 4565-4573.
8. Czechowski, A., Ratkiewicz, R., McKenzie, J. F., and Axford, W. I.: 1998, Heating and acceleration of minor ions in the solar wind, Astron. Astrophys., 335, 303-308.
9. Dowdy, J. F., Jr., Rabin, D., and Moore, R. L.: 1986, On the magnetic structure of the quiet transition region, Solar Phys., 105, 35-45.
10. Fisher, R., and Guhathakurta, M.: 1995, Physical properties of polar coronal rays and holes as observed with the Spartan 201-01 coronagraph, Astrophys. J., 447, L139-L142.
11. Gabriel, A. H.: 1976a, A magnetic model of the solar transition region, Phil. Trans. Roy. Soc., A281, 339-352.
12. Gabriel, A. H.: 1976b, Structure of the quiet chromosphere and corona, in The Energy Balance and Hydrodynamics of the Solar Chromosphere and Corona, ed. R. Bonnet and P. Delache (Clermont-Ferrand: G. de Bussal), pp. 375-418.
13. Geiss, J., Gloeckler, G., von Steiger, R., Balsiger, H., Fisk, L. A., Galvin, A. B., Ipavich, F. M., Livi, S., McKenzie, J. F., Ogilvie, K. W., and Wilken, B.: 1995, The southern high-speed stream: Results from the SWICS instrument on Ulysses, Science, 268, 1033-1036.
14. Giordano, S., Antonucci, E., and Dodero, M. A.: 1998, Velocity of the fast solar wind in coronal holes, Adv. Space Res., submitted.
15. Gold, T.: 1964, Magnetic energy shedding in the solar atmosphere, in Proc. AAS-NASA Symp. on The Physics of Solar Flares, pp. 389-395.
16. Guhathakurta, M.: 1999, these proceedings.
17. Hartle, R. E., and Sturrock, P. A.: 1968, Two-fluid model of the solar wind, Astrophys. J., 151, 1155-1170.
18. Holzer, T. E., and Axford, W. I.: 1970, The theory of stellar winds and related flows, Ann. Rev. Astron. Astrophys., 8, 31-60.
19. Hudson, H. S.: 1991, Solar flares, microflares, nanoflares, and coronal heating, Solar Phys., 133, 357-369.
20. Isenberg, P. A., and Hollweg, J. V.: 1983, On the preferential acceleration and heating of solar wind heavy ions, J. Geophys. Res., 88, 3923-3935.
21. Kopp, R. A., and Holzer, T. E.: 1976, Dynamics of coronal hole regions, 1, Steady polytropic flow with multiple critical points, Sol. Phys., 49, 43.
22. Krucker, S., and Benz, A. O.: 1998, Energy distribution of heating processes in the quiet solar corona, Astrophys. J., 501, L213-L216.
23. Leer, E., Holzer, T. E., and Flå, T.: 1982, Acceleration of the solar wind, Space Sci. Rev., 33, 161-200.
24. Li, X., Esser, R., Habbal, S. R., and Hu, Y.-Q.: 1997, Influence of heavy ions on the high-speed solar wind, J. Geophys. Res., 102, 17,419-17,432.
25. Marsch, E., and Tu, C.-Y.: 1997, Solar wind and chromospheric network, Solar Phys., 176, 87-106.
26. McKenzie, J. F., Axford, W. I., and Banaszkiewicz, M.: 1997, The fast solar wind, Geophys. Res. Lett., 24, 2877-2880.
27. McKenzie, J. F., Banaszkiewicz, M., and Axford, W. I.: 1995, Acceleration of the high speed solar wind, Astron. Astrophys., 303, L45-L48.
28. McKenzie, J. F., Sukhorukova, G. V., and Axford, W. I.: 1998a, The source region of the fast solar wind, Astron. Astrophys., 330, 1145-1148.
29. McKenzie, J. F., Sukhorukova, G. V., and Axford, W. I.: 1998b, Structure of a photoionization layer in the solar chromosphere, Astron. Astrophys., 332, 367-373.
30. Parker, E. N.: 1958, Dynamics of the interplanetary gas and magnetic fields, Astrophys. J., 128, 664-676.
31. Parker, E. N.: 1988, Nanoflares and the solar wind X-ray corona, Astrophys. J., 330, 474-479.
32. Rosner, R., Tucker, W. H., and Vaiana, G. S.: 1978, Dynamics of the quiescent solar corona, Astrophys. J., 220, 643-665.
33. 6+ ions in the solar wind, Geophys. Res. Lett., 7, 697-700.
34. Smith, E. J., et al.: 1997, Radial and azimuthal components of the heliospheric magnetic field: Ulysses observations, Adv. Space Res., 20, 47-53.
35. Tu, C.-Y.: 1987, A solar wind model with the power spectrum of Alfvénic fluctuations, Solar Phys., 109, 149-186.
36. Weber, E. J.: 1973, Multi-ion plasma in astrophysics, Astrophys. Space Sci., 20, 391-465.
37. Williams, L. L.: 1995, Heat flux and viscosity of protons in the collisionless solar wind, Astrophys. J., 453, 953-958.
38. Yeh, T.: 1970, A three-fluid model of solar winds, Planet. Space Sci., 18, 199-215.