Constraining Ion-Scale Heating and Spectral Energy Transfer in Observations of Plasma Turbulence.
Journal
Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141
Informations de publication
Date de publication:
10 Jul 2020
10 Jul 2020
Historique:
revised:
11
05
2020
received:
14
01
2020
accepted:
22
05
2020
entrez:
24
7
2020
pubmed:
24
7
2020
medline:
24
7
2020
Statut:
ppublish
Résumé
We perform a statistical study of the turbulent power spectrum at inertial and kinetic scales observed during the first perihelion encounter of the Parker Solar Probe. We find that often there is an extremely steep scaling range of the power spectrum just above the ion-kinetic scales, similar to prior observations at 1 A.U., with a power-law index of around -4. Based on our measurements, we demonstrate that either a significant (>50%) fraction of the total turbulent energy flux is dissipated in this range of scales, or the characteristic nonlinear interaction time of the turbulence decreases dramatically from the expectation based solely on the dispersive nature of nonlinearly interacting kinetic Alfvén waves.
Identifiants
pubmed: 32701332
doi: 10.1103/PhysRevLett.125.025102
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM