| 1. Fundamental physical processes and modeling |
| Lei Ni: |
Connecting reconnection models to IRIS observations |
| Tom van Doorsselaere: |
Alfvén wave turbulence in coronal loops |
| Juan Martinez-Sykora: |
What does modeling the non-equilibrium chromosphere tell us about the reliability of IRIS diagnostics? |
| 2. Chromospheric heating and dynamics |
| Sanja Danilovic: |
A modeler's perspective on UV bursts |
| Andreas Lagg: |
Magnetic field in the chromosphere |
| 3. Magnetic coupling and mass flux through the atmosphere |
| Pradeep Chitta: |
Magnetic coupling through the atmosphere |
| Tiago Pereira:: |
Thermal coupling through the atmosphere |
| Shin Toriumi: |
Flux emergence and related IRIS observations |
| 4. Eruptions in the solar atmosphere |
| Vanessa Polito: |
Connecting flares to the low atmosphere |
| Alphonse Sterling: |
What are the outstanding issues with jets? |
| Miho Janvier: |
What can IRIS observation tell us about modeling of eruptions? |
| 5. Opportunities and challenges |
| Andres Asensio-Ramos: |
Machine learning to investigate magnetic field and other complex data sets |
| Alberto Sainz-Dalda: |
Machine learning and inversions of Mg II h/k spectra |
| Steven White: |
What can we really get from ALMA? |
| 6. Science together with future facilities |
| Gianna Cauzzi:: |
New science windows with future ground-based observations |
| Nour-Eddine Raouafi: |
The Parker Solar Probe (PSP) and IRIS |
| Javier Trujillo-Bueno: |
Rocket science with IRIS: CLASP-1 and 2 |