Isotropization and evolution of energy-containing eddies in solar wind turbulence: Parker solar probe, helios 1, ace, wind, and voyager 1
We examine the radial evolution of correlation lengths perpendicular (${\lambda} _
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …
Isotropization and Evolution of Energy-containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager 1
ME Cuesta, R Chhiber, S Roy… - The Astrophysical …, 2022 - ui.adsabs.harvard.edu
We examine the radial evolution of correlation lengths perpendicular (${\lambda} _
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …
[PDF][PDF] Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager
ME Cuesta, R Chhiber, S Roy, J GOODWILL, F Pecora… - sun.bao.ac.cn
C≈ 1.29 at 1 au. The ratio does not appear to change significantly beyond 1 au, although
the small number of parallel intervals in the Voyager dataset precludes unambiguous …
the small number of parallel intervals in the Voyager dataset precludes unambiguous …
Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager 1
ME Cuesta, R Chhiber, S Roy, J Goodwill… - The Astrophysical …, 2022 - ntrs.nasa.gov
We examine the radial evolution of correlation lengths perpendicular (l^ C) and parallel (
lC) to the magnetic-field direction, computed from solar wind magnetic-field data measured …
lC) to the magnetic-field direction, computed from solar wind magnetic-field data measured …
[PDF][PDF] Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager
ME CUESTA, R CHHIBER, S ROY, J GOODWILL… - academia.edu
We examine the radial evolution of correlation lengths perpendicular (λ⊥ C) and parallel
(λC) to the magneticfield direction, computed from solar wind magnetic-field data measured …
(λC) to the magneticfield direction, computed from solar wind magnetic-field data measured …
[PDF][PDF] Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager
ME Cuesta, R Chhiber, S Roy, J GOODWILL, F Pecora… - sun10.bao.ac.cn
C≈ 1.29 at 1 au. The ratio does not appear to change significantly beyond 1 au, although
the small number of parallel intervals in the Voyager dataset precludes unambiguous …
the small number of parallel intervals in the Voyager dataset precludes unambiguous …
Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager 1
ME Cuesta, R Chhiber, S Roy, J Goodwill… - arXiv preprint arXiv …, 2022 - arxiv.org
We examine the radial evolution of correlation lengths perpendicular (\(\lambda_C^{\perp}\))
and parallel (\(\lambda_C^{\parallel}\)) to the magnetic-field direction, computed from solar …
and parallel (\(\lambda_C^{\parallel}\)) to the magnetic-field direction, computed from solar …
Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager 1
ME Cuesta, R Chhiber, S Roy… - SHINE 2022 …, 2022 - ui.adsabs.harvard.edu
We examine the radial evolution of correlation lengths perpendicular (λ C⊥) and parallel (λ
C‖) to the magnetic-field direction, computed from solar wind magnetic-field data measured …
C‖) to the magnetic-field direction, computed from solar wind magnetic-field data measured …