Coherence of Elsässer Variables in the slow solar wind from 0.1 au to 0.3 au

Coherence of Elsässer Variables in the slow solar wind from 0.1 au to 0.3 au

The highly Alfvénic fluctuations (AF) and magnetic-velocity alignment structures (MVAS) are two distinguished components in the near-Sun slow solar wind observed by Parker Solar Probe. The amplitudes of the Elsässer Variables z± of AF and MVAS show distinct features. However, how these fluctuations...

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Bibliographic Details
Main Authors: Honghong Wu, Liping Yang, Shiyong Huang
Format: Article
Language:English
Published: Frontiers Media S.A. 2024-01-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
solar wind
turbulence
magnetic field
interplanetary medium
in situ observation
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2023.1329284/full

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