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  1. 1
    por Démoulin, P., Dasso, S.
    Publicado 2009
    ... of this work is to find the main causes of this expansion and to derive a model to explain the plasma velocity...
    Artículo publishedVersion
  2. 2
    por Démoulin, P., Dasso, S.
    Publicado 2009
    ... of this work is to find the main causes of this expansion and to derive a model to explain the plasma velocity...
    Artículo publishedVersion
  3. 3
    por Démoulin, P., Dasso, S.
    Publicado 2009
    ... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...
    Artículo publishedVersion
  4. 4
    por Démoulin, P., Dasso, S.
    Publicado 2009
    ... dynamical laws, which are mainly dominated by magnetic forces.Aims. With in-situ observations the magnetic...
    Artículo publishedVersion
  5. 5
    por Dasso, S., Démoulin, P., Gulisano, A.M.
    Publicado 2011
    ...), they are the hugest transient object in the interplanetary medium, and the main actors for the Sun-Earth coupling...
    Artículo publishedVersion
  6. 6
    por Dasso, S., Démoulin, P., Gulisano, A.M.
    Publicado 2011
    ...), they are the hugest transient object in the interplanetary medium, and the main actors for the Sun-Earth coupling...
    Artículo publishedVersion
  7. 7
  8. 8
    ... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...
    Artículo publishedVersion
  9. 9
    .... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...
    Artículo publishedVersion
  10. 10
    por Janvier, M., Démoulin, P., Dasso, S.
    Publicado 2013
    ... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...
    Artículo publishedVersion
  11. 11
  12. 12
    ... that the decrease of the total SW pressure with distance is the main origin of the observed MC expansion rate. We...
    Artículo publishedVersion
  13. 13
    .... The timing of the first high-energy particle arrival on Earth is mainly determined by the type of IMF...
    Artículo publishedVersion
  14. 14
    por Janvier, M., Démoulin, P., Dasso, S.
    Publicado 2013
    ... and in situ data do not provide any direct estimation of the general flux rope properties. Aims. The main aim...
    Artículo publishedVersion
  15. 15
    ... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...
    Artículo publishedVersion
  16. 16
    ... and mainly determined by their own magnetic forces and the interaction with the surrounding solar wind. Aims...
    Artículo publishedVersion