EGU22-5000
https://doi.org/10.5194/egusphere-egu22-5000
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Disturbance Storm Time (Dst) index estimation using deep learning applied to Swarm satellite data

Gianfranco Cianchini1, Alessandro Piscini2, Angelo De Santis1, and Saioa Arquero Campuzano3
Gianfranco Cianchini et al.
  • 1Istituto Nazionale di Geofisica e Vulcanologia, Roma 2, 00143 Roma, Italy
  • 2Istituto Nazionale di Geofisica e Vulcanologia, Osservatorio Nazionale Terremoti (ONT), 00143 Roma, Italy
  • 3Instituto de Geociencias IGEO (CSIC-UCM), 28040 Madrid, Spain

Computed from the intensity of the globally symmetrical equatorial electrojet (Ring Current) measured by a series of near-equatorial geomagnetic observatories, the Dst (Disturbance Storm Time) is an hourly index of magnetic activity. To give the estimation of the Dst index through the magnetic data measured by the Swarm three-satellite mission, we selected and trained an Artificial Neural Network (ANN). From November 2014 to December 2019, we collected a big Swarm magnetic dataset, confined in space to three very narrow belts of low-to-mid latitude, to better resemble the geographic distribution of the four geomagnetic observatories used to estimate at ground Dst. We also extended the analysis to mid latitude locations to increase the number of satellite samples. By using a Deep Learning architecture and based on its performance, we selected the best topology and trained the network testing its modelling capabilities. The outcomes show that the ANN is able to give a reliable fast estimation of the Dst index directly from Swarm satellite magnetic data, especially during magnetically disturbed periods.

How to cite: Cianchini, G., Piscini, A., De Santis, A., and Arquero Campuzano, S.: Disturbance Storm Time (Dst) index estimation using deep learning applied to Swarm satellite data, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-5000, https://doi.org/10.5194/egusphere-egu22-5000, 2022.