Heliocentric Distance and Solar Activity Dependence of Sustained Quasi-radial Interplanetary Magnetic Field Occurrence

Heliocentric Distance and Solar Activity Dependence of Sustained Quasi-radial Interplanetary Magnetic Field Occurrence

Planets close to their stars experience an interplanetary magnetic field (IMF) that is dominantly quasi-radial. Our solar system serves as a laboratory to study how the occurrence of quasi-radial IMF varies away from the star and under different stellar activities. Furthermore, on time and spatial s...

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Bibliographic Details
Main Authors: Brandon L. Burkholder, Li-Jen Chen, Norberto Romanelli, Dave Sibeck, Jaye Verniero, Gina A. DiBraccio, Daniel Gershman, Menelaos Sarantos
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Interplanetary magnetic fields
Planetary bow shocks
Solar cycle
Online Access:https://doi.org/10.3847/1538-4357/ace328

Internet

https://doi.org/10.3847/1538-4357/ace328

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