Acceleration of the fast solar wind by the emergence of new magnetic flux

Journal of Geophysical Research: Space Physics

Volumn 104, Issue A9, 1999, Pages 19765-19772

  Fisk, L A ^a  

^a UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001753140     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (5)

1. Axford, W. I., The three-dimensional structure of the interplanetary medium, in Study of Traveling Interplanetary Phenomena, edited by M. A. Shea, D. F. Smart, and S.-T. Wu, p. 145, D. Reidel, Norwell, Mass., 1977.
2. Axford, W. I., and J. F. McKenzie, The solar wind, in Cosmic Winds in the Heliosphere, edited by J. R. Jokipii, C. P. Sonett, and M. S. Giampapa, p. 31, Univ. of Ariz. Press, Tucson, 1997.
3. Balogh, A., E. J. Smith, B. T. Tsurutani, D. J. Southwood, R. J. Forsyth, and T. S. Horbury, The heliospheric magnetic field over the south polar region of the Sun, Science, 268, 1007, 1995.
4. Fisk, L. A., T. H. Zurbuchen, and N. A. Schwadron, On the coronal magnetic field: Consequences of large-scale motions, Astrophys. J., in press, 1999.
5. Habbal, S. R., R. Esser, M. Guhathakurta, and R. R. Fisher, Flow properties of the solar wind from a two-fluid model with constraints from white light and in situ interplanetary observations, Geophys. Res. Lett., 22, 1465, 1995.