A two-fluid, MHD coronal model

Journal of Geophysical Research: Space Physics

Volumn 104, Issue A3, 1999, Pages 4697-4708

  Suess, S T ^a  

^a NASA MARSHALL SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001070731     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (5)

1. Braginskii, S. I., Transport processes in a plasma, in Reviews of Plasma Physics, edited by M. A. Leontovich, vol. 1, pp. 205-311, Consultants Bureau, New York, 1965.
2. Burlaga, L. F., and K. W. Ogilvie, Heating of the solar wind, Astrophys. J., 159, 659, 1970.
3. Burlaga, L. F., and K. W. Ogilvie, Solar wind temperature and speed, J. Geophys. Res., 78, 2028, 1973.
4. Corti, G., G. Poletto, M. Romoli, J. Michels, J. Kohl, and G. Noci, Physical parameters in plume and interplume regions from UVCS observations, in The Corona and Solar Wind Near Minimum Activity, Eur. Space Agency Spec. Publ., ESA SP-404, 289, 1997.
5. Esser, R., E. Leer, S. R. Habbal and G. L. Withbroe, A two-fluid solar wind model with Alfvén waves: Parameter study and application to observations, J. Geophys. Res., 91, 2950, 1986.