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20212026
most citedSolar Orbiter Observations of the Kelvin-Helmholtz Instability in the Solar Wind

27 citations · 38 across the 7 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2026

Direct Measurement of Polar Coronal Hole-like Solar Wind in its Acceleration Phase

Samuel T. Badman, Yeimy J. Rivera, Michael L. Stevens +38

The early evolution of fast polar coronal hole (PCH) solar wind remains largely unconstrained by in situ measurements. In March 2025, Parker Solar Probe (Parker) at its closest app…

astro-ph.SR2026

On the Radial Evolution of the Solar Wind : The Source Alignment Method Applied to Parker Solar Probe and Solar Orbiter Observations

Jean-Baptiste Dakeyo, Tamar Ervin, Stuart Bale +10

The properties of the solar wind, as measured in situ throughout the heliosphere, depend both on the characteristics of its coronal source and on the intrinsic processes governing…

astro-ph.SR2025

Alfvénic solar wind intervals observed by Solar Orbiter: Exploiting the capability of the SWA plasma suite and source region investigation

R. D'Amicis, J. M. Raines, S. Benella +32

Fast and slow solar wind have distinct properties linked to their solar sources.Alfvénic slow wind complicates the usual speed-based classification, especially at intermediate spee…

astro-ph.SR2025★ 4 cited

A Tale of Two Shocks

Robert F. Wimmer-Schweingruber, Domenico Trotta, Rungployphan Kieokaew +23

Energetic particles in interplanetary space are normally measured at time scales that are long compared to the ion gyroperiod. Such observations by necessity average out the microp…

astro-ph.SR2024★ 7 cited

Testing the flux tube expansion factor -- solar wind speed relation with Solar Orbiter data

J-B. Dakeyo, A. P. Rouillard, V. Réville +5

The properties of the solar wind measured in-situ in the heliosphere are largely controlled by energy deposition in the solar. Previous studies have shown that long duration and la…

astro-ph.SR2021★ 27 cited

Solar Orbiter Observations of the Kelvin-Helmholtz Instability in the Solar Wind

R. Kieokaew, B. Lavraud, Y. Yang +17

The Kelvin-Helmholtz instability (KHI) is a nonlinear shear-driven instability that develops at the interface between shear flows in plasmas. KHI has been inferred in various astro…