1st Meeting

The first meeting took place from 2 to 4 December 2013. Here is the list of the contributions:

NON-THERMAL PARTICLES IN THE SOLAR ATMOSPHERE AND WIND
Cristian Vock
Suprathermal electron production in the quiet solar corona
Lorenzo Matteini
Solar wind ions, their non-thermal properties and the state of art of the theoretical modelling
Giulio Del Zanna
Possible contributions of active regions to the solar wind. Evidence and hydrodynamical modelling

ATOMIC PROCESSES, DATA & CHIANTI
Helen Mason
CHIANTI
Giulio Del Zanna
Updates on atomic data calculations potentially relevant for diagnostics of non-thermal effects + CHIANTI v.8
Peter Young
Develop a framework for incorporating non-equilibrium processes into the CHIANTI database

NON-MAXWELLIAN DISTRIBUTIONS – THEORY AND OBSERVATIONS
Elena Dzifcakova
Ionization equilibrium (elements H to Zn) for the kappa-distributions
CHIANTI modification for the kappa-distributions
Jaroslav Dudik
The influence of non-Maxwellian distributions on interpretation of observations
and some consequences for numerical modeling
Simon Mackovjak
DEM analysis and the non-Maxwellian kappa-distributions

David Williams
Signatures of non-thermal distributions of ions in the solar corona
Alessandra Giunta
Multi-thermal analysis of the solar upper atmosphere: towards the inclusion of transient behaviour
Jaroslav Dudik
Transition Region lines observed by IRIS

X-RAY EMISSION
Sam Krucker
Hard X-ray Observations as Diagnostics of Non-thermal Electron Distributions
in Solar Flares + movie
Barbara Sylwester
RESIK soft X-ray spectra- status of database
Janusz Sylwester
ChemiX- the Bragg crystal spectrometer for the Interhelioprobe mission to the Sun

Peter Young
Search for and identify examples of non-equilibrium processes occurring in Hinode/EIS data in coordination with other instruments (particularly RHESSI)
Giulio Del Zanna
Possible diagnostics in the X-rays from the iron satellite lines during flares
Jaroslav Dudik
Non-Maxwellian distributions with strong peaks: The story of Si dielectronic lines observed by RESIK