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EGU2015-2941.pdf

EGU2015-2941.pdf
Preview of EGU2015-2941
🔗 Source: meetingorganizer.copernicus.org
📊 Size: 34 KB
📄 Pages: 1 page
⬇️ Downloads: 51

Summary

Magnetic flux tubes in the solar wind can become unstable due to Kelvin-Helmholtz and kink instabilities, generating turbulence, reconnection, and dissipation, and potentially changing local field and plasma conditions, according to recent analytical and numerical calculations.

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Description

Magnetic flux tubes in the solar wind can become unstable due to Kelvin-Helmholtz and kink instabilities, generating turbulence, reconnection, and dissipation,...

Technical Information

  • File Format: PDF
  • File Size: 34 KB
  • Pages: 1
  • Language: EN
  • Total Downloads: 51
  • Last Updated: 1 week ago

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