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

  • Authors: Robert Jarolim, Martin Sanner, Chia-Man Hung, Emma Stevenson, Hala Lamdouar, Josh Veitch-Michaelis, Ioanna Bouri, Anna Malanushenko, Elena Provornikova, Vít Růžička, Carlos Urbina-Ortega

Robert Jarolim et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 2.

Synthetic observations and corresponding tomographic reconstructions of a CME event, shown 12.5 hr after launch. (a) Synthetic white-light images from two ecliptic viewpoints located at 175° and 235° longitude. (b), (c) Slices of the reconstructed electron density and plasma velocity obtained using our tomographic reconstruction method, illustrating the 3D CME structure. Note that panel (b) shows ecliptic slices at 0° latitude and panel (c) shows slices at 135° longitude. White arrows indicate velocity vectors > 300 km s−1. The white dashed lines mark the main propagation direction of the CME at 0° latitude and 135° longitude in heliocentric coordinates.

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