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SCIENTIFIC
RATIONALE
Spectroscopy
is a power tool for the analysis of radiation from different plasmas in
astronomy, laboratory, fusion research, atmospheric research and industry.
Efficacy of theoretical analysis, synthesis and modelling of stellar spectra
as well as the spectra from other plasma sources, depends on atomic data and
their sources. In particular for the modelling 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.
Consequently, the development of databases with atomic data and
astroinformatics is important for stellar spectroscopy.
The
Conference is planned as an opportunity to consider above mentioned aspects
of spectroscopic research on plenary sessions and than to work on the
special mini-projects, which will result in common papers to be published in
international astronomical journals after the Conference.
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