SuNeRF: 3D Reconstruction of the Solar EUV Corona Using Neural Radiance Fields

SuNeRF: 3D Reconstruction of the Solar EUV Corona Using Neural Radiance Fields

To understand its evolution and the effects of its eruptive events, the Sun is permanently monitored by multiple satellite missions. The optically thin emission of the solar plasma and the limited number of viewpoints make it challenging to reconstruct the geometry and structure of the solar atmosph...

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Bibliografski detalji
Glavni autori: Robert Jarolim, Benoit Tremblay, Andrés Muñoz-Jaramillo, Kyriaki-Margarita Bintsi, Anna Jungbluth, Miraflor Santos, Angelos Vourlidas, James P. Mason, Sairam Sundaresan, Cooper Downs, Ronald M. Caplan
Format: Članak
Jezik:English
Izdano: IOP Publishing 2024-01-01
Serija:The Astrophysical Journal Letters
Teme:
Solar corona
Active solar corona
Neural networks
Solar filament eruptions
Solar coronal holes
Online pristup:https://doi.org/10.3847/2041-8213/ad12d2

Internet

https://doi.org/10.3847/2041-8213/ad12d2

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