A Coronal Mass Ejection Impacting Parker Solar Probe at 14 Solar Radii

A Coronal Mass Ejection Impacting Parker Solar Probe at 14 Solar Radii

The relationship between CME properties in the corona and their interplanetary counterparts is not well understood. Until recently, a wide spatial gap existed between the two regions, which prevented us from disentangling the spatial and temporal evolution of CMEs. NASA’s Parker Solar Probe (PSP) ha...

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Bibliographic Details
Main Authors: Carlos R. Braga, Vamsee Krishna Jagarlamudi, Angelos Vourlidas, Guillermo Stenborg, Teresa Nieves-Chinchilla
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar corona
Solar coronal transients
Solar wind
Interplanetary magnetic fields
Space plasmas
Solar coronal mass ejections
Online Access:https://doi.org/10.3847/1538-4357/ad2b4e

Internet

https://doi.org/10.3847/1538-4357/ad2b4e

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