Near-real-time 3D Reconstruction of the Solar Coronal Parameters Based on the Magnetohydrodynamic Algorithm outside a Sphere Using Deep Learning

For the first time, we generate solar coronal parameters (density, magnetic field, radial velocity, and temperature) on a near-real-time basis by deep learning. For this, we apply the Pix2PixCC deep-learning model to three-dimensional (3D) distributions of these parameters: synoptic maps of the phot...

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Bibliographic Details

Published in:	The Astrophysical Journal Supplement Series
Main Authors:	Sumiaya Rahman, Hyun-Jin Jeong, Ashraf Siddique, Yong-Jae Moon, Bendict Lawrance
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Active solar corona Astronomy data analysis Astronomy image processing The Sun
Online Access:	https://doi.org/10.3847/1538-4365/ad1877