A 2.5-dimensional MHD Alfvén-wave-driven solar wind model

Journal of Geophysical Research: Space Physics

Volumn 108, Issue A10, 2003, Pages

  Hu, Y Q ^a,b   Li, X ^b   Habbal, S R ^b,c  

^a UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^b ABERYSTWYTH UNIVERSITY   (United Kingdom)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

2.5 D MHD model; Alfv n wave driven solar wind; Azimuthal components of solar wind; Differential rotation; Solar wind

Indexed keywords

EID: 8644237562     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2003JA009889     Document Type: Article

References (17)

1. Braginskii, S. I., Transport phenomena in a plasma, in Reviews of Plasma Physics, vol. 1, p. 205, Consult. Bur., New York, 1965.
2. Forsyth, R. J., et al., The underlying magnetic field direction in Ulysses observations, Geophys. Res. Lett., 22, 3321-3324, 1995.
3. Forsyth, R. J., et al., The underlying Parker spiral structure in the Ulysses magnetic field observations 1990-1994, J. Geophys. Res., 101, 395-403, 1996.
4. Hollweg, J. V., Transition region, corona, and solar wind in coronal holes, J. Geophys. Res., 91, 4111-4125, 1986.
5. Howard, R., and J. Harvey, Spectroscopic determinations of solar rotation, Solar Phys., 12, 23-51, 1970.
6. Hu, Y. Q., A multistep implicit scheme for time-dependent, two-dimensional magnetohydrodynamic flows, J. Comput. Phys., 84, 441-460, 1989.
7. Hu, Y. Q., and B. C. Low, Steady hydromagnetic flows in open magnetic fields. III. Allowing for variations of density with latitude and nonalignment of velocity with magnetic field, Astrophys. J., 342, 1049-1060, 1989.
8. Hu, Y. Q., and S. T. Wu, A full-implicit-continuous-Eulerian (FICE) scheme for multi-dimensional, transient magnetohydrodynamic (MHD) flows, J. Comput. Phys., 55, 33-64, 1984.
9. Hu, Y. Q., S. R. Habbal, Y. Chen, and X. Li, Are coronal holes unique source of fast solar wind?, J. Geophys. Res., 108, doi:10.1029/ 2002JA009776, in press, 2003.
10. Hundhausen, A. J., Coronal Expansion and Solar Wind, Springer-Verlag, New York, 1972.
11. Low, B. C., and K. Tsinganos, Steady hydromagnetic flows in open magnetic fields. I. A class of analytical solutions, Astrophys. J., 302, 163-187, 1986.
12. McComas, D. J., et al., Solar wind observations over Ulysses' first full polar orbit, J. Geophys. Res., 105, 10,419-10,433, 2000.
13. Parker, E. N., Dynamics of the interplanetary gas and magnetic field, Astrophys. J., 128, 664-676, 1958.
14. Smith, C. W., and J. W. Bieber, Solar cycle variation of the interplanetary magnetic field spiral, Astrophys. J., 370, 435-441, 1991.
15. Spitzer, L., Jr., Physics of Fully Ionized Gases, Wiley-Interscience, Hoboken, N. J., 1962.
16. Tsinganos, K., and B. C. Low, Steady hydromagnetic flows in open magnetic fields. II. Global flows with static zones, Astrophys. J., 342, 1028-1048, 1989.
17. Weber, E. J., and L. D. Davis Jr., The angular momentum of the solar wind, Astrophys. J., 148, 217-227, 1967.