Nature of the MHD and Kinetic Scale Turbulence in the Magnetosheath of Saturn: Cassini Observations - INSU - Institut national des sciences de l'Univers
Article Dans Une Revue The Astrophysical journal letters Année : 2015

Nature of the MHD and Kinetic Scale Turbulence in the Magnetosheath of Saturn: Cassini Observations

Résumé

Low-frequency turbulence in Saturn's magnetosheath is investigated using in situ measurements of the Cassini spacecraft. Focus is put on the magnetic energy spectra. A set of 42 time intervals in the magnetosheath were analyzed, and three main results that contrast with known features of solar wind turbulence are reported.
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Dates et versions

insu-01225064 , version 1 (28-05-2020)

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Lina Hadid, Fouad Sahraoui, K. H. Kiyani, Alessandro Retinò, Ronan Modolo, et al.. Nature of the MHD and Kinetic Scale Turbulence in the Magnetosheath of Saturn: Cassini Observations. The Astrophysical journal letters, 2015, 813 (2), pp.L29. ⟨10.1088/2041-8205/813/2/L29⟩. ⟨insu-01225064⟩
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