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1.2.1.2 Energy and mass flux in the corona. Loss in form of conduction, radiation, gravitational enthalpy, and kinetic energy fluxes into the accelerating solar wind plasma.

 


Required observations:

  • SWASWA Normal Mode, A few hours of connected observations, other instruments: ALL.
  • All instruments.

Duration:

  • A few hours of connected observations.

Other constraints:

  • Connected observations.

 

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