| Presentation Title: | What are the properties of energetic electrons associated with solar jets? |
| Author(s): | Sophie Musset and the Solar Jet Hunter team |
Abstract:
Solar flares are one of the sources of energetic particles that fill the heliosphere. With the launch of recent missions such as Parker Solar Probe and Solar Orbiter, we aim to understand both how particles get accelerated during flares, and how they escape the flare site in the solar corona, to reach the interplanetary medium and fill the heliosphere. Coronal jets are one of the features often observed when flare-accelerated particles escape the solar atmosphere. I will present a statistical approach to the study of this phenomena using the new catalogue of solar jets resulting from the citizen science Solar Jet Hunter, in which hundreds of jets have been reported in the 304 A AIA observations. A description of the jets in this catalogue will be followed by a focus on the properties of the accelerated particles in flare-associated jets. I will also present preliminary results on the detection of solar jets using machine learning, which will be used to enhance our data sets in combination with citizen science.