Fast Reconstruction of 3D Density Distribution around the Sun Based on the MAS by Deep Learning

Fast Reconstruction of 3D Density Distribution around the Sun Based on the MAS by Deep Learning

This study is the first attempt to generate a three-dimensional (3D) coronal electron density distribution based on the pix2pixHD model, whose computing time is much shorter than that of the magnetohydrodynamic (MHD) simulation. For this, we consider photospheric solar magnetic fields as input, and...

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Bibliographic Details
Main Authors: Sumiaya Rahman, Seungheon Shin, Hyun-Jin Jeong, Ashraf Siddique, Yong-Jae Moon, Eunsu Park, Jihye Kang, Sung-Ho Bae
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
The Sun
Solar photosphere
Astronomy data analysis
Astronomy image processing
Online Access:https://doi.org/10.3847/1538-4357/acbd3c

Internet

https://doi.org/10.3847/1538-4357/acbd3c

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