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Volumn 25, Issue 9, 1998, Pages 1529-1532

Do coronal mass ejections implode in the solar wind?

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EID: 0043176644     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/98GL01057     Document Type: Article
Times cited : (25)

References (11)
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    • Gosling, J.T.1
  • 6
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    • The acceleration of slow coronal mass ejections in the high-speed solar wind
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  • 7
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    • (1985) Collisionless Shocks in the Heliosphere: Reviews of Current Research, Geophys. Monogr. Ser. , vol.35 , pp. 51-68
    • Pizzo, V.J.1
  • 8
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    • A two-dimensional simulation of the radial and latitudinal evolution of a solar wind disturbance driven by a fast, high-pressure coronal mass ejection
    • Riley, P., et al., A two-dimensional simulation of the radial and latitudinal evolution of a solar wind disturbance driven by a fast, high-pressure coronal mass ejection, J. Geophys. Res., 102, 14,677, 1997.
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  • 9
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    • Gostekhizdat, Moscow, 4th edition, 1957, English transl. (M. Holt, ed.), Academic Press, New York
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  • 10
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    • Stone, J.M.1    Norman, M.L.2
  • 11
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    • Shock propagation in the outer heliosphere 1. Pickup ions and gasdynamics
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