Frequency Transition From Weak to Strong Turbulence in the Solar Wind

During a specific time window while approaching the Sun, the longitudinal speed of Parker Solar Probe matches that of the Sun’s rotation. The spacecraft therefore co-rotates with the Sun, and as long as it does so, it is immersed in the solar-wind plasma of the same flow tube. This unique feature of...

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Bibliographic Details
Main Author: Daniele Telloni
Format: Article
Language:English
Published: Frontiers Media S.A. 2022-05-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2022.917393/full