Organisation/Company CNRS Department Laboratoire d'Instrumentation et de Recherche en Astrophysique Research Field Astronomy Researcher Profile First Stage Researcher (R1) Application Deadline 4 Nov 2026 - 23:59 (UTC) Country France Type of Contract Temporary Job Status Full-time Hours Per Week 35 Offer Starting Date 1 Dec 2026 Is the job funded through the EU Research Framework Programme? Not funded by a EU programme Is the Job related to staff position within a Research Infrastructure? No
Offer Description
The mission of the post-doc researcher will be to investigate the acceleration and propagation of energetic electrons during solar flares using data from the Solar Orbiter mission.
Understanding how energetic electrons produced in solar flares fill the heliosphere is one of the key questions of Solar Orbiter. The post-doc will directly contribute to this topic by analysing the radio diagnostics of the energetic electrons escaping from the solar surface to the interplanetary medium. These energetic electrons produce Langmuir waves while propagating along the interplanetary magnetic field lines which are converted via non-linear processes to radio electromagnetic radiation.
The analysis of these emissions provide information on the characteristics of the electron beams in the interplanetary medium (velocity, number) but also on the conditions of propagation of the radio electromagnetic radiation itself, since the radio emission can be scattered in the turbulent interplanetary medium.
The post-doc researcher will work on the catalog of « type III » radio emissions produced by electron beams and observed by the RPW instrument (more than 15000 bursts). He/she will develop a method to automatically analyse the detailed time evolution of the radio emission at different frequencies so as derive distributions of electron beam velocities at the start, peak and in the decacy of the emissions. These distributions will be compared with the results of simulations of radio emissions and will also be used to estimate the effect of wave scattering in the interplanetary medium.
The post-doc researcher will work in the team « Helioshhere and Astrophysical Plasmas) at LIRA. The work will take place in the Meudon site of the Paris Observatory.
The researcher will report directly to Milan Maksimovic.
The team has a long experience in the study of heliospheric plasmas and in the field of radio-instrumentation. Members of the team are strongly involved in the scientific analysis of Solar Orbiter and in particular of the RPW instrument (plasma and radio wave experiment).
- To have a Phd in astrophysics or equivalent
- To have a good knowledge in radio instrumentation
- To have a good knowledge in python
- To have good capacities in communication and work in teams, to have motivation to contribute to a constructive, collaborative and positive working atmosphere.
- To be autonomous and to be willing to take initiatives.
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Post-doc researcher in heliospheric plasma physics (M/F) employeur : CNRS - National Center for Scientific Research
Le CNRS est un employeur exceptionnel qui offre un environnement de recherche collaboratif et multidisciplinaire, idéal pour les chercheurs souhaitant explorer l'impact de l'IA sur le travail. Avec un fort accent sur la science ouverte et la responsabilité sociale, les employés bénéficient d'opportunités de croissance professionnelle et d'un cadre de travail enrichissant, tout en contribuant à des projets ayant un impact sociétal significatif.
Coordonnées :
Équipe de recrutement de CNRS - National Center for Scientific Research
