The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - INSU - Institut national des sciences de l'Univers Accéder directement au contenu
Article Dans Une Revue The Astrophysical Journal Supplement Année : 2020

The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere

J. Bonnell
D. Borovikov
  • Fonction : Auteur
T. Bowen
A. Case
B. Chandran
K. Goetz
P. Harvey
J. Kasper
K. Klein
K. Korreck
D. Larson
R. Livi
R. Macdowall
D. Malaspina
M. Mcmanus
M. Pulupa
M. Stevens
P. Whittlesey

Résumé

The first two orbits of the Parker Solar Probe spacecraft have enabled the first in situ measurements of the solar wind down to a heliocentric distance of 0.17 au (or 36 ${R}_{\odot }$). Here, we present an analysis of this data to study solar wind turbulence at 0.17 au and its evolution out to 1 au. While many features remain similar, key differences at 0.17 au include increased turbulence energy levels by more than an order of magnitude, a magnetic field spectral index of −3/2 matching that of the velocity and both Elsasser fields, a lower magnetic compressibility consistent with a smaller slow-mode kinetic energy fraction, and a much smaller outer scale that has had time for substantial nonlinear processing. There is also an overall increase in the dominance of outward-propagating Alfvénic fluctuations compared to inward-propagating ones, and the radial variation of the inward component is consistent with its generation by reflection from the large-scale gradient in Alfvén speed. The energy flux in this turbulence at 0.17 au was found to be ~10% of that in the bulk solar wind kinetic energy, becoming ~40% when extrapolated to the Alfvén point, and both the fraction and rate of increase of this flux toward the Sun are consistent with turbulence-driven models in which the solar wind is powered by this flux.
Fichier principal
Vignette du fichier
Chen_2020_ApJS_246_53.pdf (1004.59 Ko) Télécharger le fichier
Origine : Fichiers éditeurs autorisés sur une archive ouverte
Loading...

Dates et versions

insu-02937674 , version 1 (17-09-2020)

Licence

Paternité - Pas de modifications

Identifiants

Citer

C. Chen, S. Bale, J. Bonnell, D. Borovikov, T. Bowen, et al.. The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere. The Astrophysical Journal Supplement, 2020, Early Results from Parker Solar Probe: Ushering a New Frontier in Space Exploration, 246 (2), pp.53. ⟨10.3847/1538-4365/ab60a3⟩. ⟨insu-02937674⟩
52 Consultations
152 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More