Conveners
Session 1
- Daniele Spadaro (Istituto Nazionale di Astrofisica (INAF))
The ASO-S mission has three payloads, a Full-disk vector MagnetoGraph (FMG) to measure photospheric magnetic Fields, a Hard X-ray Imager (HXI) to observe non-thermal signals from 30 to 200 keV, and Lyman-alpha Solar Telescope (LST) to take images of the Sun in Lyman-alpha and white light. In this presentation, we focus in the LST payload including the introduction to its three instruments, the...
SOLAR-C is the next JAXA-led solar physics mission, scheduled to be launched in mid 2028. The main mission payload is EUVST (EUV High-Throughput Spectroscopic Telescope), an EUV imaging spectrometer with slit-jaw imaging system whose science goal is to understand how underlying physical processes, acting on small scales, lead to the formation of the outer solar atmosphere and the solar wind,...
The MUSE NASA mission, with significant ASI-INAF contribution, will use EUV spectroscopy in 3 single-line bands to probe basic magnetic and heating processes in the solar corona. The lines are sensitive to plasma emission at about 1, 2.5 and >8 MK and can therefore track the evolution of plasma when it is heated up and then cools down. Resolving the lines will allow to obtain information about...
