Nanodust Measured with LF Radio Antennas
Observatoire de Paris
Observatoire de Paris
Batiment 16
5, Place Jules Janssen
92195 Meudon Cedex France
Dr. Maksimovic’s research interests include the study and modeling of the radio emissions associated with the coronal mass ejections (Type IIs) and heliospheric energetic particles (Type IIIs), in-situ measurements in the solar wind and modeling of the particle velocity distribution functions, and models of solar wind formation and acceleration. Additionally, he's the PI of the Radio & Plasma Waves instrument on the Solar Orbiter missions and co-PI of the SWAVES instrument on STEREO, CoI on FIELDS / Parker SOalr Probe, Bepi Colombo, and CLUSTER.