- 1LPC2E, OSUC, CNRS, University of Orléans, CNES, 3A avenue de la Recherche Scientifique, 45071 Orléans, France (panisara.thepthong@cnrs-orleans.fr)
- 2LIRA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France
- 3Radboud Radio Lab, Department of Astrophysics, Radboud University Nijmegen, Nijmegen, The Netherlands
Solar type III radio bursts are common radio emissions generated by energetic electron beams traveling through the solar corona. These serve as important remote sensing tools for studying plasma and electron beams in the solar wind. In this work, we aim to combine observations from both the Parker Solar Probe (PSP) and Solar Orbiter (SolO) spacecrafts in order to study solar type III radio bursts from different point of view and distances. In particular, we investigate observed differences in the fine structures, such as striae, as well as in the radio spectrum fluctuations to gain a deeper understanding of the physical mechanisms influencing the propagation of electrons beams.
How to cite: Thepthong, P., Kretzschmar, M., Maksimovic, M., and Pesini, A.: Joint Analysis of Solar Type III Radio bursts with Parker Solar Probe and Solar Orbiter, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10692, https://doi.org/10.5194/egusphere-egu25-10692, 2025.
