Solar wind electron characteristics inside and outside coronal mass ejections

Journal of Geophysical Research: Space Physics

Volumn 105, Issue A10, 2000, Pages 23069-23084

  Skoug, R M ^a   Feldman, W C ^a   Gosling, J T ^a   McComas, D J ^a   Smith, C W ^a  

^a LOS ALAMOS NATIONAL LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 39449129622     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (8)

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4. Burlaga, L. F., and K. W. Ogilvie, Magnetic and thermal pressures in the solar wind, Sol. Phys., 15, 61, 1970.
5. Burlaga, L., E. Sittler, F. Mariani, and R. Schwenn, Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations, J. Geophys. Res., 86, 6673, 1981.
6. Cane, H. V., I. G. Richardson, and G. Wibberenz, Helios 1 and 2 observations of particle decreases, ejecta, and magnetic clouds, J. Geophys. Res., 102, 7075, 1997.
7. Chen, J., Theory of prominence eruption and propagation: Interplanetary consequences, J. Geophys. Res., 101, 27,499, 1996.
8. Fainberg, J., V. A. Osherovich, R. G. Stone, R. J. MacDowall, and A. Balogh, Ulysses observations of electron and proton components in a magnetic cloud and related wave activity, in Solar Wind Eight, edited by D. Winterhalter et al., AIP Conf. Proc., 382, pp. 554-557, 1996.