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  • Determine in what conditions the radial evolution is a matter of age of turbulence or in situ heliospheric sources sources.
  •  Try to connect in situ spectrum with source spectrum at the Sun (together with sophisticated models). 
  •  Get insight into the observed correlation between speed, temperature and fluctuations amplitude (Grappin et al., 1990) by comparing in situ properties and source region properties.

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