EGU24-16590, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-16590
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Automated detection and tracking of CMEs using HI instruments

Maike Bauer1,2, Justin LeLouedec1, Tanja Amerstorfer1, and Jackie Davies3
Maike Bauer et al.
  • 1Austrian Space Weather Office, GeoSphere Austria, Graz, Austria
  • 2Institute of Physics, University of Graz, Graz, Austria
  • 3RAL Space, Science and Technology Facilities Council, Didcot, UK

Timely and accurate prediction of coronal mass ejections (CMEs) is vital for mitigating the potential impact of severe space weather events on critical infrastructures. Currently, manual detection and tracking of CMEs as they traverse the heliosphere are the norm. This presentation introduces an innovative approach: the development and implementation of a machine learning algorithm for automatic detection and tracking of CMEs, leveraging data from various heliospheric imager (HI) instruments. The wealth of active spacecraft equipped with HI instruments provides a unique opportunity to train the algorithm using diverse datasets.

This work gains significance in light of the upcoming launch of Vigil, a space weather monitor scheduled for deployment in the early 2030s at the L5 point. Vigil will continuously observe and provide real-time HI observations along the Sun-Earth line. Our presentation showcases preliminary outcomes from an automated CME detection and tracking algorithm, demonstrating its effectiveness with training on STEREO-HI data. We also discuss potential future steps and challenges in the development and testing of this algorithm, emphasizing its role in advancing operational space weather prediction capabilities, especially in anticipation of the Vigil mission.

How to cite: Bauer, M., LeLouedec, J., Amerstorfer, T., and Davies, J.: Automated detection and tracking of CMEs using HI instruments, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16590, https://doi.org/10.5194/egusphere-egu24-16590, 2024.

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