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astro-ph.SR2026

SuNeRF-CME: Physics-Informed Neural Radiance Fields for Tomographic Reconstruction of Coronal Mass Ejections

Robert Jarolim, Martin Sanner, Chia-Man Hung +8

Coronagraphic observations enable direct monitoring of coronal mass ejections (CMEs) through scattered light from free electrons, but determining the 3D plasma distribution from 2D…

astro-ph.SR2026

Deep Generative model that uses physical quantities to generate and retrieve solar magnetic active regions

Subhamoy Chatterjee, Andres Munoz-Jaramillo, Anna Malanushenko

Deep generative models have shown immense potential in generating unseen data that has properties of real data. These models learn complex data-generating distributions starting fr…

astro-ph.SR2026

Polarimeter to Unify the Corona and Heliosphere (PUNCH)

Craig E. DeForest, Sarah E. Gibson, Ronnie Killough +74

The Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a NASA Small Explorer to determine the cross-scale processes that unify the solar corona and heliosphere. PUN…

astro-ph.SR2026

Polarization Diagnostics Applied to Coronal Mass Ejections and the Background Solar Wind

Sarah E Gibson, Craig E. DeForest, Curt A. de Koning +6

The ratio of radially to tangentially polarized Thomson-scattered white light provides a powerful tool for locating the 3D position of compact structures in the solar corona and in…

astro-ph.SR2024

MHD modeling of a geoeffective interplanetary CME with the magnetic topology informed by in-situ observations

E. Provornikova, V. G. Merkin, A. Vourlidas +4

Variations of the magnetic field within solar coronal mass ejections (CMEs) in the heliosphere depend on the CME`s magnetic structure as it leaves the solar corona and its subseque…