Nature of the MHD and Kinetic Scale Turbulence in the Magnetosheath of Saturn: Cassini Observations - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles The Astrophysical journal letters Year : 2015

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

Abstract

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.
Fichier principal
Vignette du fichier
Hadid_2015_ApJL_813_L29.pdf (994.49 Ko) Télécharger le fichier
Origin : Publisher files allowed on an open archive
Loading...

Dates and versions

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

Identifiers

Cite

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⟩
211 View
57 Download

Altmetric

Share

Gmail Facebook X LinkedIn More