Program

Cool material in the solar corona
Welcome
A Quick Look at the History of Solar Physics in Space and A brief Glance Forward
Forty-Year China-France Collaboration in Solar Physics
SMESE ou les prémices d'une coopération franco-chinoise
From SMESE to ASO-S
Effects of Solar and Galactic Cosmic Rays observed by SoHO
Spicule observations with ALMA
Coffee break
La création d'un Centre d'opération Européen pour le projet SOHO (MEDOC); une aventure avec JCV.
Formation and continued presence of cool material in solar prominences
Rapports sciences - société : l'impératif d'une réflexion collective
Radiative transfer : JCV and the National Committee of CNRS
Fifty years to unravel the Sun’s great enigmas

Cool material in the solar corona
2D stellar-rotation evolution models in the light of 2D asteroseismology
The matter cycle in the solar atmosphere: periodic evaporation and condensation in coronal loops
Structure and dynamics of prominence magnetic configurations
Cool material in the solar corona: eruption of mini-filaments
Coffee break
CMEs, from the corona to the interplanetary medium
The corona transition region of solar prominences : from SUMER/SOHO to SPICE/Solar Orbiter
The cold corona and Hα emission
RAMSES: The CNES Solar Probe Proposal
"La matrice densité atomique pour la théorie de l'effet Hanle et de la dépolarisation collisionnelle"
Lunch
Monsieur Protu
UV spectroscopy and non-LTE modeling of the solar atmosphere, including the chromosphere, flares, plages etc. and prominences.
Studying solar transition region spectra: scientific journeys with Jean-Claude
R&D for Solar Instrumentation
JC Superstar