Automatic Detection of CMEs Using Synthetically-Trained Mask R-CNN
Coronal mass ejections (CMEs) are a major driver of space weather. To assess CME geoeffectiveness, among other scientific goals, it is necessary to reliably identify and characterize their morphology and kinematics in coronagraph images. Current methods of CME identification are either subjected to human biases or perform a poor identification due to deficiencies in the automatic detection. In this approach, we have trained the deep convolutional neural model Mask R-CNN to automatically segment the outer envelope of one or multiple CMEs present in a single difference coronagraph image. The empirical training dataset is composed of $1.13\times 10^{5}$ synthetic coronagraph images with known pixel-level CME segmentation masks. It is obtained by combining quiet (no CME) coronagraph observations, with synthetic white-light CMEs produced using the Graduated Cylindrical Shell geometric model and ray-tracing technique. To filter the different instances found by Mask R-CNN, we use the temporal consistency of mask properties such as the intersection over union ( $IoU$ ). We found that our model-based trained Mask R-CNN infers segmentation masks that are smooth and topologically connected (without holes or isolated patches). While the inferred masks are not representative of the detailed outer envelope of complex CMEs, the neural model can better differentiate a CME from other radially moving background/foreground features, segment multiple simultaneous CMEs that are close to each other, and work with images from different instruments. This is accomplished without relying on kinematic information, i.e. only the included in the single input difference image. We obtain a median $IoU=0.98$ for $1.6\times 10^{4}$ synthetic validation images, and $IoU=0.77$ when compared with two independent manual segmentations of 115 observations acquired by the COR2-A, COR2-B, and LASCO C2 coronagraphs. The methodology presented in this work can be used with other CME models to produce more realistic synthetic brightness images while preserving desired morphological features, and obtain more robust and/or tailored segmentations.
Authors
- Franco Manini (ORCID: https://orcid.org/0000-0002-8455-2632)
- D. G. Lloveras (ORCID: https://orcid.org/0000-0003-1402-0398)
- Andrés Asensio Ramos
- Yasmin Machuca
- Fernando Vázquez López
- Mariano Sanchez Toledo
- Hebe Cremades
- Francisco A. Iglesias
- Florencia L. Cisterna
Institutions
- University of Mendoza (AR)
- Goddard Space Flight Center (US)
- George Mason University (US)
- Heliophysics (US)
- Centro Científico Tecnológico - San Juan (AR)
- Instituto de Astrofísica de Canarias (ES)
- Heliophysics Science Division (US)
Publication Details
- Journal
- Solar Physics
- Published
- 2026-02-01
- DOI
- https://doi.org/10.1007/s11207-026-02613-5
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Aeronautics and Space Administration
- UK Space Agency
- Belgian Federal Science Policy Office
- Centre National d’Etudes Spatiales
- Bundesministerium für Wirtschaft und Energie
- National Oceanic and Atmospheric Administration
- Office of Naval Research
- U.S. Naval Research Laboratory