Large-Scale Solar Wind Phenomena Affecting the Turbulent Cascade Evolution behind the Quasi-Perpendicular Bow Shock

Large-Scale Solar Wind Phenomena Affecting the Turbulent Cascade Evolution behind the Quasi-Perpendicular Bow Shock

The Earth’s magnetosphere is permanently influenced by the solar wind. When supersonic and superalfvenic plasma flow interacts with the magnetosphere, the magnetosheath region is formed, which is filled with shocked turbulent plasma. Varying SW parameters influence the mechanisms of formation of thi...

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Bibliographic Details
Main Authors: Liudmila S. Rakhmanova, Maria O. Riazantseva, Georgy N. Zastenker, Yuri I. Yermolaev
Format: Article
Language:English
Published: MDPI AG 2022-11-01
Series:Universe
Subjects:
solar-terrestrial relations
space plasma
turbulence
solar wind
magnetosheath
Online Access:https://www.mdpi.com/2218-1997/8/12/611

Internet

https://www.mdpi.com/2218-1997/8/12/611

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