Name: RoCMI 2023 Svalbard
Start: 2023-02-27T08:30:00+01:00
End: 2023-03-02T21:30:00+01:00
Location: No location set

Monday, 27 February 2023

08:30

08:30 - 09:00
09:00
09:00 - 10:55
Contributions

09:00 Modeling the Solar Atmosphere: Current challenges and future directions - Matthias Rempel (High Altitude Observatory, National Center for Atmospheric Research)

09:24 Current numerical approaches and how to expand them - Åke Nordlund (University of Copenhagen)

09:48 Future high-resolution observation capabilities of the chromosphere and corona from Earth - Jorrit Leenaarts (Stockholm University)

10:12 Future high-resolution observations of the low solar atmosphere from space - Bart De Pontieu (Lockheed Martin Solar & Astrophysics Laboratory)
10:55 Morning break
Morning break
10:55 - 11:40
11:40
11:40 - 12:30
Contributions

11:40 What do we know about the photospheric and chromospheric magnetic field? - Luis Bellot Rubio (Instituto de Astrofísica de Andalucía (IAA-CSIC))

12:05 Driving of atmospheric heating from the convection zone - Robert Cameron (Max Planck Institute for Solar System Research)
12:30 Lunch
Lunch
12:30 - 13:30
13:30
13:30 - 15:00
Contributions

13:30 Advances on multi-fluid modeling of the solar atmosphere - Juan Martinez Sykora (BAERI/LMSAL/UiO)

13:55 Towards multi-fluid simulations of the solar chromosphere - Elena Khomenko (Instituto de Astrofisica de Canarias)

14:10 Ebysus, a multi-fluid multi-species code: application to upper chromospheric magnetic reconnection with Helium-Hydrogen mixture - Q. M. Wargnier (LMSAL)

14:25 Role of chromospheric partial ionization on the dynamics of kink unstable flux ropes - Giulia Murtas (Los Alamos National Laboratory)
15:00

15:00 - 16:45
16:45
16:45 - 18:00
Contributions

16:45 Setting observational constraints on the chromospheric heating problem - Jaime de la Cruz Rodriguez (Stockholm University)

17:10 First Results of the MURaM Chromospheric Extension - Damien Przybylski (Max Planck Institute for Solar System Research)

17:25 Constraining the acoustic wave flux in the solar chromosphere with observations and simulations - Momchil Molnar (High Altitude Observatory, National Center for Atmospheric Research)
Tuesday, 28 February 2023
09:00
09:00 - 10:30
Contributions

09:00 High-resolution observations of chromospheric dynamics - Luc Rouppe van der Voort (Rosseland Centre for Solar Physics)

09:25 Understanding chromospheric dynamics - Sanja Danilovic (Stockholm University)

09:40 Differentiable programming for spectra modeling and inference - Carlos Jose Diaz Baso (Rosseland Centre for Solar Physics, University of Oslo, Oslo)

09:55 Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere - Moa Skan (Institute for Solar Physics, Stockholm University)
10:30 Morning break
Morning break
10:30 - 11:15
11:15
11:15 - 12:30
Contributions

11:15 Interplay between modelling and observations of the upper solar atmosphere - Hardi Peter (Max Planck Institute for Solar System Research)

11:40 Recent advances in Coronal Heating due to High Resolution Imaging: Results from the High-Resolution Coronal Imager - Amy Winebarger (NASA MSFC)

11:55 MUSE diagnostics of coronal heating from MHD modeling of magnetically stressed coronal loops - Fabio Reale (University of Palermo)
12:30 Lunch
Lunch
12:30 - 13:30
13:30
13:30 - 15:00
Contributions

13:30 Flux emergence and the state of the outer solar atmosphere - Viggo Hansteen (RoCS/BAERI/LMSAL)

13:55 MUSE ‘observations’ of coronal heating simulations. - Thomas Howson (University of St Andrews)

14:10 Toward resolving the nonthermal motions in the solar corona - Cosima Alexandra Breu (School of Mathematics and Statistics, University of St. Andrews)

14:25 Modeling Coronal Bright Points - Daniel Nóbrega-Siverio (Instituto de Astrofísica de Canarias (IAC))
15:00

15:00 - 16:45
16:45
16:45 - 18:00
Contributions

16:45 The current state of wave-based heating mechanisms - Tom Van Doorsselaere (KU Leuven)

17:10 Deciphering the Nanojet Phenomenon - Patrick Antolin (Northumbria University)

17:25 Decay-less oscillations of turbulent loops - Konstantinos Karampelas (KU Leuven)
Wednesday, 1 March 2023
09:00
09:00 - 10:30
Contributions

09:00 Coronal heating diagnostics from high spatial and temporal resolution spectroscopic observations - Paola Testa (Harvard Smithsonian Center for Astrophysics)

09:25 Solar coronal heating from small-scale magnetic braids - Lakshmi Pradeep Chitta (Max Planck Institute for Solar System Research)

09:40 Chromospheric and Coronal heating in active region plage by dissipation of currents - Souvik Bose (Lockheed Martin Solar & Astrophysics Laboratory, Palo Alto, CA, USA)

09:55 Signatures of drama in the not-so-Quiet Sun - Rebecca Robinson (Rosseland Centre for Solar Physics)
10:30 Morning break
Morning break
10:30 - 11:15
11:15
11:15 - 12:30
Contributions

11:15 Study Solar Eruptions from a Global Perspective: Current Status and Future Improvements on the Global MHD Models - Meng Jin (Lockheed Martin Solar & Astrophysics Lab)

11:40 Recent and future observations connecting the solar wind to sources in the Sun's atmosphere - David Brooks (George Mason University @ ISAS/JAXA)

11:55 Predicted appearance of Magnetic Flux Rope and Sheared Magnetic Arcade Structures before a Coronal Mass Ejection via three-dimensional radiative Magnetohydrodynamic Modeling - Georgios Chintzoglou (Lockheed Martin Advanced Technology Center)
12:30 Lunch
Lunch
12:30 - 14:00

14:00 Excursion
Excursion
14:00 - 16:00

16:00 Free time
Free time
16:00 - 16:45
16:45
16:45 - 18:00
Contributions

16:45 MPI-AMRVAC: open-source grid-adaptive simulations for solar physics and applications to prominences - Rony Keppens (CmPA, KU Leuven)

17:00 Transverse MHD waves as signatures of braiding-induced magnetic reconnection in coronal loops - Ramada Sukarmadji (Northumbria University)

17:15 Data-constrained magnetohydrodynamics simulations of the solar atmosphere using the Bifrost code - Avijeet Prasad (Rosseland Center for Solar Physics, University of Oslo)
18:30 Workshop Dinner
Workshop Dinner
18:30 - 21:15
Thursday, 2 March 2023
09:00
09:00 - 10:30
Contributions

09:00 SOLAR-C Mission and Numerical Modeling of Flaring Plasma - Shinsuke Imada (The University of Tokyo)

09:25 3D reconnection in solar flares and the hot flare emission - Jaroslav Dudík (Astronomical Institute of the Czech Academy of Sciences)

09:40 Modeling flare heating with turbulent thermal conduction - Joel Allred (NASA/GSFC)

09:55 Modelling of pre-eruptive magnetic structure: the need to get the electric currents right! - Etienne Pariat (Laboratoire de Physique des Plasmas, CNRS)
10:30 Morning break
Morning break
10:30 - 11:15
11:15
11:15 - 12:30
Contributions

11:15 Interrogating Solar Flare Models with IRIS Observations and Looking to the Future - Graham Kerr (The Catholic Univeristy of America)

11:40 Modelling and observations: what is (still) needed to understand the role of magnetic fields in flares and eruptions? - Miho Janvier (European Space Agency)

11:55 Understanding the Physics of solar coronal jets and surges: Unified approach with high resolution observations and numerical modelling - Reetika Joshi (RoCS, University of Oslo)
12:30 Lunch
Lunch
12:30 - 13:30
13:30
13:30 - 15:00
Contributions

13:30 The gaps in our understanding of flare energy release: prospects with MUSE and other observatories - Lyndsay Fletcher (School of Physics and Astronomy, University of Glasgow and Rosseland Centre for Solar Physics, University of Oslo)

13:55 Diagnosing Magnetic Reconnection and Energy Release from High-resolution Observations of Flare Ribbons - Jiong Qiu (Montana State University)

14:10 Insights into Solar Flare Reconnection and Energetics from Novel Forms of High-resolution Observation and Modeling - Dana Longcope (Montana State University)

14:25 Deciphering the evolution of pre-eruptive CMEs - Chen Xing ([1] School of Astronomy and Space Science, Nanjing University, Nanjing, China [2] Sorbonne Université, Observatoire de Paris-PSL, École Polytechnique, IP Paris, CNRS, Laboratoire de Physique des Plasmas, Paris, France)
15:00

15:00 - 16:45
16:45
16:45 - 18:00
Contributions

16:45 3D MHD of Flares & Eruptions - Mark Cheung (CSIRO)

17:10 Understanding the formation of flare-productive active regions using realistic flux emergence simulations - Shin Toriumi (Japan Aerospace Exploration Agency)

17:25 MHD turbulence formation in solar flares: 3D simulation and synthetic observations - Wenzhi Ruan (KU Leuven)
18:00

18:00 - 18:10