CME Observations -- from Sun to Impact on Geospace

Fuente: arXiv
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Autore principale: Temmer, Manuela
Natura: Preprint
Pubblicazione: 2025
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author Temmer, Manuela
author_facet Temmer, Manuela
contents Our Sun is an active star expelling dynamic phenomena known as coronal mass ejections (CMEs). The magnetic field configuration on the Sun and related solar wind structures affect the propagation behavior of CMEs, dominate its transit time and embedded magnetic field properties when impacting Earth. Since the conditions on the Sun constantly change, the impact of CMEs on the different regimes of geospace is quite variable and may differ significantly from event to event. This short review summarizes the different manifestations of CMEs on the Sun, their appearance in interplanetary space, and how CMEs trigger a cascade of reactions as they interact with Earth.
format Preprint
id arxiv_https___arxiv_org_abs_2501_11345
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle CME Observations -- from Sun to Impact on Geospace
Temmer, Manuela
Solar and Stellar Astrophysics
Space Physics
Our Sun is an active star expelling dynamic phenomena known as coronal mass ejections (CMEs). The magnetic field configuration on the Sun and related solar wind structures affect the propagation behavior of CMEs, dominate its transit time and embedded magnetic field properties when impacting Earth. Since the conditions on the Sun constantly change, the impact of CMEs on the different regimes of geospace is quite variable and may differ significantly from event to event. This short review summarizes the different manifestations of CMEs on the Sun, their appearance in interplanetary space, and how CMEs trigger a cascade of reactions as they interact with Earth.
title CME Observations -- from Sun to Impact on Geospace
topic Solar and Stellar Astrophysics
Space Physics
url https://arxiv.org/abs/2501.11345