How does “the Saône-Rhône” (Sun run) the heliosphere?

9:00 - 9:30 (30min)

Coffee break

9:30 - 10:00 (30min)

Solar Radio Burst Tracker – A Citizen Science Campaign for Identifying Type III Solar Radio Bursts

Katerina Pesini

10:00 - 10:30 (30min)

Using Type III radio bursts as evidence of particle escape from the Sun for enhancing solar proton forecasting capabilities

Olga Malandraki

10:30 - 11:00 (30min)

Origin of the Unusual Composition of 3He-rich Solar Energetic Particles

Radoslav Bucik

11:00 - 11:30 (30min)

Coffee break

11:00 - 11:30 (30min)

Posters Session

› Assessment and optimisation of Solar Orbiter communication rolls strategy to minimise impact on SWA-PAS science return - Denis Kupriianov, Mullard Space Science Laboratory - Gethyn Lewis, Mullard Space Science Laboratory 11:00-11:30 (30min)

› Magnetic signatures of dust impacts - Kristina Rackovic Babic, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace 11:00-11:30 (30min)

› Wave processes in the solar wind during type III radio bursts : 2D/3V PIC simulations - Francisco Javier Polanco Rodríguez, Laboratoire de Physique des Plasmas 11:00-11:30 (30min)

› Simulation of weak electron beam relaxation into plasma with open boundary conditions - Vladimir Annenkov, Laboratoire de Physique des Plasmas 11:00-11:30 (30min)

› Dynamic behavior of almost monoenergetic ions near Earth's bow shock - Liu Yang, Institut für Experimentelle und Angewandte Physik [Kiel] 11:00-11:30 (30min)

› Modelling spacecraft-emitted electrons measured by EAS experiment on board Solar Orbiter mission - Štěpán Štverák, Institute of Atmospheric Physics CAS, Astronomical Institute, CAS 11:00-11:30 (30min)

› Interplay Between Kinetic Instabilities and Coulomb Collisions in the Radial Evolution of the Solar Wind - Hao Ran, Mullard Space Science Laboratory 11:00-11:30 (30min)

› Electron density at different spacecraft potential regimes - Jordi Boldu, Swedish Institute of Space Physics [Uppsala] 11:00-11:30 (30min)

› magneto-gravity-precessional instability - Abdelaziz Salhi, Faculté des Sciences de Tunis, Université Tunis El Manar, 2092 El Manar, Tunisia 11:00-11:30 (30min)

› A comparative study of coronal microjet numerical modelling under the influence of p-modes. - Ayu Ramada Sukarmadji, Institut de recherche en astrophysique et planétologie 11:00-11:30 (30min)

› Langmuir Wave Excitation in Solar-wind Magnetic Holes - Jingting Liu, Mullard Space Science Laboratory 11:00-11:30 (30min)

› Comparative Study of Alfvénic characteristics Across Diverse Solar Wind Regimes - Omkar Dhamane, INAF-IAPS, Rome 11:00-11:30 (30min)

› Refining PAS Proton and Alpha Particle Moments for Solar Wind and Magnetic Reconnection Studies - Tristan Vergé, Institut de recherche en astrophysique et planétologie 11:00-11:30 (30min)

11:30 - 12:00 (30min)

Farside Transient Activity Triggering Nearside Recurrent 3He-rich SEP Events

Samuel Hart

12:00 - 12:30 (30min)

The 23 July 2024 Fe-rich SEP event as Observed by Multiple Spacecraft

Christina Cohen

12:30 - 14:00 (1h30)

Lunch break

14:00 - 14:30 (30min)

Using the Field-Particle Correlation Technique to Identify Particle Energization using Single-Point Spacecraft Observations

Gregory Howes

14:30 - 15:00 (30min)

Investigating heliospheric current sheet with Heavy Ion Sensor

Keiichi Ogasawara

15:00 - 15:30 (30min)

Differences in heavy ion streaming in the inner heliosphere

Ryan Dewey

15:30 - 16:00 (30min)

Coffee break

15:30 - 16:00 (30min)

Discussions

16:00 - 16:30 (30min)

Observations by Solar Orbiter’s Solar Wind Analyser - Heavy Ion Sensor: Properties of Magnetic Switchbacks and Kinetic Physics

Jesse Coburn

16:30 - 17:00 (30min)

Polytropic analysis of large-scale compressive fluctuations in the solar wind using Solar Orbiter data

Charalambos Ioannou

17:00 - 17:30 (30min)

Discussions