Speaker
Description
First Name: David
Last Name: Arroyo Caballero
Affiliation: IAA-CSIC
All Authors: David Arroyo Caballero, David Orozco Suarez
Abstract: Understanding the formation, evolution, and eruption mechanisms of solar filaments is essential both for improving our physical comprehension of solar activity and for enhancing space weather forecasting capabilities. The unique vantage points of Solar Orbiter and other spacecraft enable the use of stereoscopy to better constrain the three-dimensional dynamics of filament eruptions. In this work, I present the first steps toward analyzing solar filament ejections through stereoscopic techniques. By combining multi-viewpoint observations we aim to determine filament velocities, accelerations, and ultimately their masses. These preliminary results open the path to future automatic detection using neural networks and to the inclusion of Solar Orbiter/PHI observations to investigate the magnetic mechanisms driving filament eruptions.