articleNatureJul 1, 2011Closed access

Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind

SWScott W. McIntoshBDBart De PontieuMCM. CarlssonVHV. H. HansteenPBP. Boerner

High Altitude Observatory · NSF National Center for Atmospheric Research · +3 more institutions

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Topics & keywords

Topics
Keywords
  • Physics
  • Corona (planetary geology)
  • Solar wind
  • Chromosphere
  • Nanoflares
  • Coronal radiative losses
  • Atmosphere (unit)
  • Coronal hole
UN Sustainable Development Goals
  • Affordable and clean energy
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