The angular-momentum flux in the solar wind observed during Solar Orbiter's first orbit - Archive ouverte HAL Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2021

The angular-momentum flux in the solar wind observed during Solar Orbiter's first orbit

, , (1) , , , (2) , , , (3) , (3) , , , , (2) , , , , , , , ,
1
2
3
Daniel Verscharen
David Stansby
Christopher J. Owen
  • Function : Author
Timothy Horbury
Marco Velli
Stuart D. Bale
  • Function : Author
Roberto Bruno
Stefano Livi
Yuri V. Khotyaintsev
  • Function : Author
Gethyn R. Lewis
  • Function : Author
Chandrasekhar Anekallu
  • Function : Author
Christopher W. Kelly
  • Function : Author
Gillian Watson
  • Function : Author
Dhiren O. Kataria
  • Function : Author
Helen O'Brien
  • Function : Author
Vincent Evans
Virginia Angelini

Abstract


Aims: We present the first measurements of the angular-momentum flux in the solar wind recorded by the Solar Orbiter spacecraft. Our aim is to validate these measurements to support future studies of the Sun's angular-momentum loss.
Methods: We combined 60-min averages of the proton bulk moments and the magnetic field measured by the Solar Wind Analyser and the magnetometer onboard Solar Orbiter. We calculated the angular-momentum flux per solid-angle element using data from the first orbit of the mission's cruise phase in 2020. We separated the contributions from protons and from magnetic stresses to the total angular-momentum flux.
Results: The angular-momentum flux varies significantly over time. The particle contribution typically dominates over the magnetic-field contribution during our measurement interval. The total angular-momentum flux shows the largest variation and is typically anti-correlated with the radial solar-wind speed. We identify a compression region, potentially associated with a co-rotating interaction region or a coronal mass ejection, which leads to a significant localised increase in the angular-momentum flux, albeit without a significant increase in the angular momentum per unit mass. We repeated our analysis using the density estimate from the Radio and Plasma Waves instrument. Using this independent method, we find a decrease in the peaks of positive angular-momentum flux, but otherwise, our results remain consistent.
Conclusions: Our results largely agree with previous measurements of the solar wind's angular-momentum flux in terms of amplitude, variability, and dependence on radial solar-wind bulk speed. Our analysis highlights the potential for more detailed future studies of the solar wind's angular momentum and its other large-scale properties with data from Solar Orbiter. We emphasise the need for studying the radial evolution and latitudinal dependence of the angular-momentum flux in combination with data from Parker Solar Probe and other assets at heliocentric distances of 1 au and beyond.
Fichier principal
Vignette du fichier
aa40956-21.pdf (712.15 Ko) Télécharger le fichier
Origin : Publisher files allowed on an open archive

Dates and versions

insu-03672346 , version 1 (19-05-2022)

Identifiers

Cite

Daniel Verscharen, David Stansby, Adam J. Finley, Christopher J. Owen, Timothy Horbury, et al.. The angular-momentum flux in the solar wind observed during Solar Orbiter's first orbit. Astronomy and Astrophysics - A&A, 2021, 656, ⟨10.1051/0004-6361/202140956⟩. ⟨insu-03672346⟩
75 View
9 Download

Altmetric

Share

Gmail Facebook Twitter LinkedIn More