Join us through Marie Skłodowska-Curie Fellowships

MSCA Postdoctoral Fellowships fund researchers looking to enhance their career development by working abroad. These grants are provided for experienced researchers to support their mobility, research project and training both within and outside of Europe.

If you are

then we can help you with your funding application to start your CHAMOS career!

Please see detailed, general information on the MSCA Postoctoral Fellowship web pages. The deadline for the fellowship applications is in 9th of September, 2026, a fellowship would then start in 2027. Mobility is a must: you have to move from your residence to another country for the fellowship. And the move has to be within, to, or from Europe. In the CHAMOS context, the most important points are:

Possible CHAMOS host institutes are:

Sodankylä Geophysical Observatory (SGO), Finland
(https://www.sgo.fi)

Possible topics include: Energetic particle precipitation, ionosphere-neutral atmosphere coupling and composition; Ground-based and satellite-based observations (EISCAT, riometers, VLF); Simulations (SIC and WACCM models). Contact person: Antti Kero

Finnish Meteorological Institute (FMI), Finland
(https://space.fmi.fi)

Possible topics include: Atmospheric chemistry response to energetic particle precipitation, dynamical coupling to troposphere, regional climate variability; Satellite-based atmospheric observations; Atmosphere and climate simulations (WACCM model). Contact person: Pekka Verronen

University of Otago, New Zealand
(https://blogs.otago.ac.nz/atmosphere/)

Possible topics include: Atmospheric impacts of energetic particle precipitation, dynamical coupling to troposphere, regional climate variability; Satellite-based atmospheric observations; Atmosphere and climate simulations (WACCM model). Contact person: Annika Seppälä

Institute for Space and Earth Environmental Research (ISEE), Nagoya University, Japan
(https://www.isee.nagoya-u.ac.jp)

Possible topics include: Magnetosphere-Ionosphere-Atmosphere coupling; Observation (Arase, EISCAT, riometer, camera, VLF, radiometer, LIDAR, optical interferometer); Simulations (wave-particle interaction, energetic particle precipitation, aurora emisions). Contact person: Shin-ichiro Oyama