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A. Juhász and M. Horányi Dynamics and distribution of nano-dust particles in the inner solar system Geophysical Research Letters 40

Version of Record online: 6 JUN 2013 | DOI: 10.1002/grl.50535

Key Points

  • The acceleration of nano-dust to near solar wind speed is calculated
  • The intermittent nature of the observations can be due to the IMF configuration
  • Observations do not allow conclusions about the origin of these particles

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