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Prasad Subramanian, Alejandro Lara and Andrea Borgazzi Can solar wind viscous drag account for coronal mass ejection deceleration? Geophysical Research Letters 39

Version of Record online: 13 OCT 2012 | DOI: 10.1029/2012GL053625

Key Points

  • Understanding the origin of CME drag is essential for arrival time predictions
  • This is the first physical characterization of CME aerodynamic drag
  • Our results elucidate the essential physics involved in CME deceleration

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