Login

9th Metis Workshop

24–26 Jan 2024
Catania (Italy) - Museo Diocesano di Catania
UTC timezone

Local contacts

Session

Session 1

24 Jan 2024, 15:00

Conveners

Session 1

  • Daniele Spadaro (Istituto Nazionale di Astrofisica (INAF))

Presentation materials

There are no materials yet.

  1. 38. Welcome and Introduction
    Daniele Spadaro (Istituto Nazionale di Astrofisica (INAF)), Marco Romoli (INAF - Arcetri Astrophysical Observatory, Largo Enrico Fermi 5, I-50125, Florence, Italy and University of Florence – Physics and Astronomy Department, Via Sansone 1, I-50019, Sesto Fiorentino (FI), Italy)
    24/01/2024, 15:00
  2. 39. Giancarlo Noci and the Solar Wind Science
    Ester Antonucci (Istituto Nazionale di Astrofisica (INAF))
    24/01/2024, 15:10
  3. 40. ASI contributions to Heliophysics Missions
    Marco Stangalini (ASI Agenzia Spaziale Italiana)
    24/01/2024, 15:30
  4. 10. * Lyman-alpha Solar Telescope aboard the ASO-S mission
    Li Feng (Purple Mountain Observatory, CAS)
    24/01/2024, 15:40
    Oral

    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...

    Go to contribution page
  5. 6. The SOLAR-C mission
    Vincenzo Andretta (Istituto Nazionale di Astrofisica (INAF))
    24/01/2024, 16:00
    Oral

    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,...

    Go to contribution page
  6. 3. The MUSE mission and the modeling of reconnection events
    Fabio Reale (Istituto Nazionale di Astrofisica (INAF))
    24/01/2024, 16:20
    Oral

    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...

    Go to contribution page
Building timetable...