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Institute of Physics Belgrade

Efficiency of theoretical analysis, synthesis and modeling of various environments, depends on atomic data and their sources. In particular, for the modeling of stellar atmospheres and opacity calculations a large number of atomic data is needed, since we do not know a priori the chemical composition of a stellar atmosphere. The same holds for Earth observations. Consequently, the development of databases with atomic data as well as astro-geoinformatics is important. This meeting will bring together physicists, astro & geophysicists from Serbia and elsewhere to review the present stage of research in this field.

Local Organizing Committee;     Email: asspectro.conf@gmail.com

Modeling the Atmosphere of planets and stars, Big data in Astronomy and Earth Observations, Radiative & Collisional Processes, Stellar and laboratory plasmas.

Astronomie, Astrophysik und Kosmologie,    Plasmaphysik, Kernfusion