Abstract: Global solar magetic field organization in the extended corona: influence on the solar wind speed and density over the cycle. (2017 AGU Fall Meeting)

Global solar magetic field organization in the extended corona: influence on the solar wind speed and density over the cycle.

Victor Réville¹, Marco C M Velli¹ and Sacha Brun², (1)University of California Los Angeles, Los Angeles, CA, United States, (2)AIM, CEA, SACLAY, France

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