Three-dimensional inversion of corona structure and simulation of solar wind parameters based on the photospheric magnetic field deduced from the Global Oscillation Network Group

Three-dimensional inversion of corona structure and simulation of solar wind parameters based on the photospheric magnetic field deduced from the Global Oscillation Network Group

In this research, the Potential Field Source Surface–Wang–Sheeley–Arge (PFSS–WSA) solar wind model is used. This model consists of the Potential Field Source Surface (PFSS) coronal magnetic field extrapolation module and the Wang–Sheeley–Arge (WSA) solar wind velocity module. PFSS is implemented by...

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Bibliographic Details
Main Authors: Xiao Zhang, Shican Qiu, Willie Soon, Hamad Yousof
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-08-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
solar wind
coronal magnetic field
numerical simulation
WSA solar wind model
PFSS model
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2023.1234391/full

Internet

https://www.frontiersin.org/articles/10.3389/fspas.2023.1234391/full

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