Hot protons in the inner corona and their effect on the flow properties of the solar wind

Journal of Geophysical Research: Space Physics

Volumn 102, Issue A4, 1997, Pages 7063-7074

  Esser, Ruth ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37149050259     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/97JA00065     Document Type: Article

References (8)

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2. Braginski, S. I., Transport processes in plasmas, Rev. Plasma Phys., 1, 206, 1965.
3. Brickhouse, N. S., and R. Esser, Effects of high proton temperatures on diagnostics for electron density and electron temperature, Astrophys. J., in press, 1997.
4. Coles W. A., and R. Esser, An observational limit to the amplitude of Alfvén waves in the solar wind and comparison with an acceleration model, J. Geophys. Res., 97, 19139, 1992.
5. Dupree, A. K., R. T. Moore, and P. R. Shapiro, Nonequilibrium ionization in solar and stellar winds, Astrophys. J., 229, L101, 1979.
6. Dupree, A. K., M. J. Penn, and H. P. Jones, He I 10830 A wing asymmetry in polar coronal holes: Evidence for radial outflow, Astrophys. J. Lett., 467, 121L, 1996.
7. Esser, R., and S. R. Habbal, Coronal heating and plasma parameters at 1 AU, Geophys. Res. Lett., 22, 2661, 1995.
8. Esser, R., and S. R. Habbal, Modeling high flow speeds in the inner corona, in Proceedings of the Solar Wind 8 Conference, edited by D. Winterhalter, J. Gosling, S. R. Habbal, W. Kurth, and M. Neugebauer, AIP, College Park, Md., 133, 1996.