Solar wind models from the sun to 1 au: Constraints by in situ and remote sensing measurements

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 1-24

  Marsch, E ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Boundary conditions; Future research topics; Kinetic and multifluid characteristics; Radial profiles; Solar corona and wind

Indexed keywords

EID: 0002688265     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1007/978-94-015-9167-6_1     Document Type: Article

References (95)

1. Alazraki, G., and Couturier, P.: 1971, Solar wind acceleration caused by the gradient of Alfvén wave pressure, Astron. Astrophys., 13, 380.
2. Axford, W. I., and McKenzie, J. F.: 1992, The origin of high speed solar wind streams, in Solar Wind Seven, ed. E. Marsch and R. Schwenn, (Pergamon Press: Oxford, England), pp. 1-4.
3. Axford, W. I., and McKenzie, J. F.: 1997, The solar wind, in Cosmic Winds and the Heliosphere, ed. J. R. Jokipii, C. P. Sonett, and M. S. Giampapa, (University of Arizona Press: Tucson, USA), pp. 31-66.
4. Banaszkiewicz, M., Axford, W. I., and McKenzie, J. F.: 1998, An analytic solar magnetic field model, Astron. Astrophys., 337, 940-944.
5. Barnes, A., Gazis, P. R., and Phillips, J. L.: 1995, Constraints on solar wind acceleration mechanisms from Ulysses plasma observations: The first polar pass, Geophys. Res. Lett., 22, 3309-3311.
6. Belcher, J.: 1971, Alfvénic wave pressure and the solar wind, (Astrophys. J., 168, 509.
7. Bertaux, J.-L., Quemerais, E., and Lallement, R.: 1996, Observations of a sky Lyman α groove related to enhanced solar wind mass flux in the neutral sheet, Geophys. Res. Lett., 23, 3675-3678.
8. Bravo, S., Stewart, G. A., and Blanco-Cano, X.: 1998, The varying multipolar structure of the Sun's magnetic field and the evolution of the solar magnetosphere through the solar cycle, Solar Phys., 179, 223-235.
9. Brekke, P., Hassler, D. M., and Wilhelm, K.: 1997, Doppler shifts in the quiet-Sun transition region and corona observed with SUMER on SOHO, Solar Phys., 175, 349-374.
10. Chae, J., Yun, H. S., and Poland, A. I.: 1998, Temperature dependence of UV line average Doppler shifts in the quiet Sun, Astrophys. J. Supp., 114, 151.
11. Corti, G., Poletto, G., Romoli, M., Michels, J., Kohl, J., and Noci, G.: 1997, Physical parameters in plume and interplume regions from UVCS observations, in Proceedings of the Fifth SOHO Workshop, ESA-SP-404, pp. 289-294.
12. Cranmer, S. R., Kohl, J. L., Noci, G., et al.: 1999, An empirical model of a polar coronal hole at solar minimum, Astrophys. J., 511, 481.
13. David, C., Gabriel, A. H., Bely-Dubau, F., Fludra, A., Lemaire, P., and Wilhelm, K.: 1998, Measurement of the electron temperature gradient in solar coronal holes, Astron. Astrophys., 336, L90.
14. Dusenbery, P. B., and Hollweg, J. V.: 1981, Ion-cyclotron heating and acceleration of solar wind minor ions, J. Geophys. Res., 86, 153-164.
15. Esser, R., Habbal, S. R., Coles, W. A., and Hollweg, J. V.: 1997, Hot protons in the inner corona and their effect on the flow properties of the solar wind, J. Geophys. Res., 102, 7063-7074.
16. Feldman, W. C., Asbridge, J. R., Bame, S. J., Gary, S. P., and Montgomery, M. D.: 1976a, Electron parameter correlations in high-speed streams and heat flux instabilities, J. Geophys. Res., 81, 2377-2382.
17. Feldman, W. C., Asbridge, J. R., Bame, S. J., Gary, S. P., Montgomery, M. D., and Zink, S. M.: 1976b, Evidence for the regulation of solar wind heat flux at 1 AU, J. Geophys. Res., 81, 5207-5211.
18. 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.
19. Geiss, J., Gloeckler, G., and von Steiger, R.: 1995, Origin of the solar wind from composition data, Space Science Reviews, 72, 49-60.
20. Grall, R. R., Coles, W. A., Klinglesmith, M. T., Breen, A. R., Williams, P. J. S., Markkanen, J., and Esser, R.: 1996, Rapid acceleration of the polar solar wind, Letters of Nature, 379, 429-432.
21. Habbal, S. R., Woo, R., Fineschi, S., O'Neal, R., Kohl, J., Noci, G., and Korendyke, C.: 1997, Origins of the slow and the ubiquitous fast solar wind, Astrophys. J., 489, L103.
22. Hammer, R.: 1982a, Energy balance of stellar corona: I. Methods and examples, Astrophys. J., 259, 767-778.
23. Hammer, R.: 1982b, Energy balance of stellar corona: II. Effect of coronal heating, Astrophys. J., 259, 779-791.
24. Hansteen, V., and Leer, E.: 1995, Coronal heating, densities, and temperatures and solar wind acceleration, Journal of Geophys. Res., 100, 21577-21593.
25. Hansteen, V., Leer, E., and Holzer, T.: 1997, The role of helium in the outer solar atmosphere, Astrophys. J., 482, 498.
26. Hassler, D. M., Dammasch, I. E., Lemaire, P., Brekke, P., Curdt, W., Mason, H. E., Vial, J.-C., and Wilhelm, K.: 1999, Solar coronal hole outflow velocities and the chromospheric network, Science, 283, 5040, 810-813.
27. Hartle, R. E., and Sturrock, P. A.: 1968, Two-fluid model of the solar wind, Astrophys. J., 151, 1155-1170.
28. Hefti, S., Grünwaldt, H., Ipavich, F. M., et al.: 1998, Kinetic properties of solar wind minor ions and protons measured with SOHO/CELIAS, J. Geophys. Res., in press.
29. Hoeksema, J. T.: 1995, The large-scale structure of the heliospheric current sheet during the Ulysses epoch, Space Science Reviews, 72, 137-148.
30. Hollweg, J. V.: 1978, Some physical processes in the solar wind, Rev. Geophys. Space Phys., 16, 689-720.
31. Hollweg, J. V.: 1986, Transition region, corona, and solar wind in coronal holes, J. Geophys. Res., 91, 4111-4125.
32. ++, 3, Effects of resonant and nonresonant intercations with transverse waves, J. Geophys. Res., 83, 97-113.
33. Hollweg, J. V., and Johnson, W.: 1986, Transition region, corona, and solar wind in coronal holes: Some two-fluid models, J. Geophys. Res., 93, 9547-9554.
34. Holzer, T. E., and Axford, W. I.: 1970, The theory of stellar winds and related flows, Ann. Rev. Astron. Astrophys., 8, 31-61.
35. Hu, Y. Q., Esser, R., and Habbal, S. R.: 1997, A fast solar wind model with anisotropic proton temperature, J. Geophys. Res., 102, 14661-14676.
36. 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.
37. Isenberg, P. A.: 1990, Investigations of a turbulence driven wave model, J. Geophys. Res., 95, 6437.
38. Jacques, S. A.: 1978, Solar wind models with Alfvén waves, Astrophys. J., 226, 632-649.
39. Ko, Y.-K., Fisk, L., Geiss, J., Gloeckler, G., and Guhathakurta, M.: 1997, An empirical study of the electron temperature and heavy ion velocities in the south polar coronal hole, Solar Phys., 171, 345-361.
40. Kohl, J. L., Noci, G., Anonucci, E., Tondello, G., Huber, M. C. E., Gardner, L. D., Nicolosi, P., Strachan, L., Fineschi, S., Raymond, J. C., Romoli, M., Spadaro, D., Panasyuk, A., Siegmund, O. H. W., Benna, C., Ciaravella, A., Cranmer, S. R., Giordano, S., Karovska, M., Martin, R., Michels, J., Modigliani, A., Naletto, G., Pernechele, C., Poletto, G., and Smith, P. L.: 1997, First results from the SOHO Ultraviolet Coronagraph Spectrometer, Solar Phys., 175, 613-644.
41. Kopp, R. A., and Holzer, T. E.: 1976, Dynamics of coronal hole regions, I. Steady polytropic flows with multiple critical points, Solar Phys., 49, 43-56.
42. Leer, E., and Axford, W. I.: 1972, A two fluid model with anisotropic proton temperature, Solar Phys., 23, 238-250.
43. Leer, E., Holzer, T. E., and Flå, T.: 1982, Acceleration of the solar wind, Space Sci. Rev., 33, 161-200.
44. Lemaire, P., Wilhelm, K., Curdt, W., Schühle, U., Marsch, E., Poland, A. I., Jordan, S. D., Thomas, R. J., Hassler, D. M., Vial, J. C., Kühne, M., Huber, M. C. E., Siegmund, O. H. W., Gabriel, A., Timothy, J. G., and Grewing, M.: 1997, First results of the SUMER telescope and spectrometer on SOHO, II. Imagery and data management, Solar Phys., 170, 105-122.
45. Li, X., Esser, R., and Habbal, S. R.: 1997, Influence of heavy ions on the high-speed solar wind, J. Geophys. Res., 102, 17419-17432.
46. Lie-Svendsen, O., Hansteen, V. H., and Leer, E.: 1997, Kinetic electrons in high-speed solar wind streams: Formation of high-energy tails, J. Geophys. Res., 102, 4701-4718.
47. Mariska, J. T.: 1992, The Solar Transition Region (Cambridge Astrophysics Series 23, Cambridge, University Press).
48. Marsch, E., Goertz, C. K., and Richter, K.: 1982, Wave heating and acceleration of solar wind ions by cyclotron resonance, J. Geophys. Res., 87, 5030-5044.
49. Marsch, E., and Richter, A. K.: 1984, Helios observational constraints on solar wind expansion, J. Geophys. Res., 89, 6599-6612.
50. Marsch, E.: 1991a, Kinetic physics of the solar wind plasma, in Physics of the Inner Heliosphere, Vol. II, eds. R. Schwenn and E. Marsch, (Springer-Verlag: Heidelberg), pp. 45-133.
51. Marsch, E.: 1991b, MHD Turbulence in the Solar Wind, in Physics of the Inner Heliosphere, Vol. II, eds. R. Schwenn and E. Marsch, (Springer Verlag: Heidelberg), pp. 159-241.
52. Marsch, E.: 1992, On the possible role of plasma waves in the heating of chromosphere and corona, in Solar Wind Seven, ed. E. Marsch and R. Schwenn, (Pergamon Press: Oxford, England), pp. 65-68.
53. Marsch, E., and Tu, C.-Y.: 1997a, Solar wind and chromospheric network, Solar Physics, 176, 87-106.
54. Marsch, E., and Tu, C.-Y.: 1997b, The effects of high-frequency Alfvén waves on coronal heating and solar wind acceleration, Astron. Astrophys., 319, L17-L20.
55. Marsden, R. G.: 1995, The High Latitude Heliosphere, (vol. 72 of Space Science Reviews, Kluwer Academic Publishers, Dordrecht, The Netherlands).
56. Maksimovic, M., Pierrard, V., and Lemaire, J. F.: 1997, A kinetic model of the solar wind with Kappa distribution functions in the corona, Astron. Astrophys., 324, 725-734.
57. McComas, D. J., Bame, S. J., Feldman, W. C., Gosling, J. T., and Phillips, J. L.: 1992, Solar wind halo electrons from 1-4 AU, Geophys. Res. Lett., 19, 1291-1294.
58. McKenzie, J. F., Banaszkiewicz, M., and Axford, W. I.: 1995, Acceleration of the high speed solar wind, Astron. Astrophys., 303, L45-L48.
59. McKenzie, J. F., Axford, W. I., and Banaszkiewicz, M.: 1997, The fast solar wind, Geophys. Res. Lett., 24, 2877-2880.
60. Neugebauer, M.: 1981, Observations of solar wind helium, Fundam. Cosmic Phys., 7, 131-199.
61. Neugebauer, M., Goldstein, B. E., Bame, S. J, and Feldman, W. C.: 1994, Ulysses near-ecliptic observations of differential flow between protons and alphas in the solar wind, J. Geophys. Res., 99, 2505-2511.
62. Neugebauer, M., Goldstein, B. E., Bame, S. J, and Feldman, W. C.: 1996, Ulysses observations of differential alpha-proton streaming in the solar wind, J. Geophys. Res., 101, 17047-17055.
63. Olsen, E. L., and Leer, E.: 1996, Thermally-driven one-fluid electron-proton solar wind; 8-moment approximation, Astrophys. J., 462, 982-996.
64. Parker, E. N.: 1958, Dynamics of the interplanetary gas and magnetic fields, Astrophys. J., 128, 664-684.
65. Peter, H., and Marsch, E.: 1997, Ionization layer of hydrogen in the solar chromosphere and the solar wind mass flux, in Proceedings of the Fifth SOHO Workshop, ESA-SP-404, pp. 591-594.
66. Pilipp, W. G., Miggenrieder, H., Montgomery, M. D., Mühlhäuser, K.-H., Rosenbauer, H., and Schwenn, R.: 1987, Characteristics of electron velocity distribution functions in the solar wind derived from the Helios plasma experiment, J. Geophys. Res., 92, 1075-1092.
67. Phillips, J. L., Feldman, W. C., Gosling, J. T., and Scime, E. E.: 1995, Solar wind plasma electron parameters based on aligned observations by ICE and Ulysses, Adv. Space Res., 16 (9), 95-100.
68. Riley, P., Sonett, C. P., Balogh, A., Forsyth, R. J., Scime, E. E., and Feldman, W. C.: 1995, Alfvénic fluctuations in the solar wind: A case study using Ulysses measurements, Space Sci. Rev., 72, 197-200.
69. Schwenn, R.: 1990, Large scale structure of the interplanetary medium, in Physics of the Inner Heliosphere, Vol. 1, ed. R. Schwenn and E. Marsch, (Springer Verlag: Berlin, Heidelberg, New York), pp. 99-181.
70. Schwenn, R., Inhester, B., Plunkett, S. P., Epple, A., Podlipnik, B., Bedford, D. K., Bout, M. V., Brueckner, G. E., Dere, K. P., Eyles, C. J., Howard, R. A., Koomen, M. J., Korendyke, C. M., Lamy, P. L., Llebaria, A., Michels, D. J., Moses, J. D., Moulton, N. E., Paswaters, S. E., Simnett, G. M., Socker, D. G., St. Cyr, O. C., Tappin, S. J., and Wang, D.: 1997, First view of the extended green line emission corona at solar activity minimum using the LASCO-C1 coronagraph on SOHO, Solar Phys., 175, 667-684.
71. Scime, E. E., Bame, S. J., Feldman, W. C., Gary, S. P., and Phillips, J. L.: 1994, Regulation of the solar wind electron heat flux from 1 to 5 AU: Ulysses observations, J. Geophys. Res., 99, 23401-23410.
72. Scudder, J. D., and Olbert, S.: 1979a, A theory of local and global processes which affect solar wind electrons, 1. The origin of typical 1 AU velocity distribution functions - Steady state theory, J. Geophys. Res., 84, 2755-2772.
73. Scudder, J. D., and Olbert, S.: 1979b, A theory of local and global processes which affect solar wind electrons, 2. Experimental support, J. Geophys. Res., 84, 6603-6620.
74. Seely, J. F., Feldman, U., Schühle, U., Wilhelm, K., Curdt, W., and Lemaire, P.: 1997, Turbulent velocities and ion temperatures in the solar corona obtained from SUMER line widths, Astrophys. J., 484, L87-L90.
75. Sheeley, N. R., Jr., Wang, Y.-M., Hawley, S. H., Brueckner, G. E., Dere, K. P., Howard, R. A., Koomen, M. J., Korendyke, C. M., Michels, D. J., Paswaters, S. E., Socker, D. G., St. Cyr, O. C., Wang, D., Lamy, P. L., Llebaria, A., Schwenn, R., Simnett, G. M., Plunkett, S., and Biesecker, D. A.: 1997, Measurements of flow speeds in the corona between 2 and 30 R⊙, Astrophys. J., 484, 472-478.
76. Smith, E. J., Neugebauer, M., Balogh, A., Bame, S. J., Lepping, R. P., and Tsurutani, B. T.: 1995, Ulysses observations of latitude gradients in the heliospheric magnetic field: Radial component and variances, Space Science Reviews, 72, 165-170.
77. Thieme, K. M., Marsch, E., and Schwenn, R.: 1990, Spatial structures in high-speed streams as signatures of fine structures in coronal holes, Annales Geophysicae, 8 (11), 713-724.
78. Tsurutani, B. T., Ho, C. M., Arballo, J. K., Lakhina, G. S., Glassmeier, K.-H., and Neubauer, F. M.: 1997, Nonlinear electromagnetic waves and spherical arc-polarized waves in space plasmas, Plasma Phys. Control Fusion, 39, A237-A250.
79. Tu, C.-Y., Pu, Z.-Y., and Wei, F.-S.: 1984, The power spectrum of interplanetary Alfvénic fluctuations: Derivation of the governing equations and its solution, J. Geophys. Res., 89, 9695-9702.
80. Tu, C.-Y.: 1987, A solar wind model with the power spectrum of Alfvénic fluctuations, Solar Phys., 109, 149-186.
81. Tu, C.-Y.: 1988, The damping of interplanetary Alfvénic fluctuations and the heating of the solar wind, J. Geophys. Res., 93, 7-20.
82. Tu, C.-Y., and Marsch, E.: 1995a, MHD structures, waves and turbulence in the solar wind: Observations and theories, Space Science Reviews, 73, 1-210.
83. Tu, C.-Y., and Marsch, E.: 1995b, Comment on "Evolution of energy-containing turbulent eddies in the solar wind" by W. H. Matthaeus, S. Oughton, D. H. Pontius Jr., and Y. Zhou, J. Geophys. Res., 100, 12323-12328.
84. Tu, C.-Y., and Marsch, E. (1997): Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfvén waves, Solar Physics, 171, 363-391.
85. Tu, C.-Y., Marsch, E., Wilhelm, K., and Curdt, W.: 1998, Ion temperatures in a solar polar coronal hole observed by SUMER on SOHO, Astrophys. J., 503, 475-482.
86. von Steiger, R., Geiss, J., Gloeckler, G., and Galvin, A. B.: 1995, Kinetic properties of heavy ions in the solar wind from SWICS/Ulysses, Space Science Reviews, 72, 71-76.
87. Vasquez, B. J., and Hollweg, J.: 1998a, Formation of spherically polarized Alfvén waves and imbedded rotational discontinuities from a small number of entirely oblique waves, J. Geophys. Res., 103, 335.
88. Vasquez, B. J., and Hollweg, J.: 1998b, Formation of imbedded rotational discontinuities with nearly field aligned normals, J. Geophys. Res., 103, 349.
89. Wang, Y. M., and Sheeley, N. R., Jr.: 1990, Solar wind speed and coronal flux-tube expansion, Astrophys. J., 355, 726.
90. Wang, Y. M., Sheeley, N. R., Jr., Walters, J. H., Brueckner, G. E., Howard, R. A., Michels, D. J., Lamy, P. L., Schwenn, R., and Simnett, G. M.: 1998, Origin of streamer material in the outer corona, Astrophys. J., 498, L165.
91. Wilhelm, K., Curdt, W., Marsch, E., Schühle, U., Lemaire, P., Gabriel, A., Vial, J. C., Grewing, M., Huber, M. C. E., Jordan, S. D., Poland, A. I., Thomas, R. J., Kühne, M., Timothy, J. G., Hassler, D. M., and Siegmund, O. H. W.: 1995, SUMER - Solar Ultraviolet Measurements of Emitted Radiation, Solar Phys., 162, 189-231.
92. Wilhelm, K., Lemaire, P., Curdt, W., Schühle, U., Marsch, E., Poland, A. I., Jordan, S. D., Thomas, R. J., Hassler, D. M., Huber, M. C. E., Vial, J.-C., Kühne, M., Siegmund, O. H. W., Gabriel, A., Timothy, J. G., Grewing, M., Feldman, U., Hollandt, J., and Brekke, P.: 1997a, First results of the SUMER telescope and spectrometer on SOHO, Solar Phys., 170, 75-104.
93. Wilhelm, K., Marsch, E., Dwivedi, B. N., Hassler, D. M., Lemaire, P., Gabriel, A. H., and Huber, M. C. E.: 1998, The solar corona above polar coronal holes as seen by SUMER on SOHO, Astrophys. J., 500, 1023-1038.
94. Withbroe, G. L.: 1988, The temperature structure, mass and energy flow in the corona and inner solar wind, Astrophys. J., 325, 442-467.
95. Woch, J., Axford, W. I., Mall, U., Wilken, B., Livi, S., Geiss, J., Gloeckler, G., and Forsyth, R. J.: 1997, SWICS/Ulysses observations: The three-dimensional structure of the heliosphere during solar minimum, Geophys. Res. Lett., 24, 2885-2888.