Name: 17th European Solar Physics Meeting ESPM-17
Start: 2024-09-09T08:00:00+02:00
End: 2024-09-13T18:00:00+02:00
Location: Turin, Italy

17th European Solar Physics Meeting ESPM-17

from Monday, 9 September 2024 (08:00) to Friday, 13 September 2024 (18:00)

Monday, 9 September 2024

08:55 Welcome and opening

08:55 - 09:10
09:10 Solar interior, sub-surface flows and long-term variability
09:10 - 10:30
Contributions

09:10 Dynamo of the solar interior: Powering the decadal cycle and Its comparison to stellar magnetic cycles - Quentin Noraz (Rosseland Centre for Solar Physics, University of Oslo, Norway)

09:35 The Sun’s differential rotation is controlled by baroclinically-unstable high-latitude inertial modes - Yuto Bekki (Max Planck Institute for Solar System Research)

09:50 EPS Invited Speaker - The role of convection during active region emergence - Hannah Schunker (University of Newcastle)

10:15 Modelling solar irradiances with proxies of activity along a cycle - Evangelia Deliporanidou (University of Cambridge)
10:30 Coffee break and poster session 1

10:30 - 11:30
11:30 Fundamental mechanisms of solar plasmas: magnetic reconnection, waves, radiation and particle acceleration
11:30 - 12:50
Contributions

11:30 Disentangling magnetic reconnection in the solar atmosphere. - Daniel Nóbrega-Siverio (Instituto de Astrofísica de Canarias (IAC) | Rosseland Centre for Solar Physics (RoCS))

11:55 Flux-rope mediated turbulent reconnection - Alexander Russell (University of St Andrews)

12:10 State-of-the-art observational aspects of MHD waves in the lower atmosphere - Marco Stangalini (ASI Italian Space Agency)

12:35 Simulating Energetic Particle Transport in the Solar Corona with COCONUT+PARADISE - Edin Husidic (KU Leuven, Belgium/University of Turku, Finland)
12:50 Lunch break

12:50 - 14:35
14:35 Fundamental mechanisms of solar plasmas: magnetic reconnection, waves, radiation and particle acceleration
14:35 - 16:00
Contributions

14:35 Radiation Properties of Cool Coronal Condensations - Petr Heinzel (Czech Academy of Sciences)

15:00 Nanoflare and nanojets in MHD simulations of magnetic reconnection in coronal loops. - Paolo Pagano (Università degli Studi di Palermo)

15:15 Estimating the total energy content in escaping accelerated solar electron beams - Alexander James (University College London)

15:30 The angular dependence of rise and decay times of solar radio bursts using multi-spacecraft observations - Nicolina Chrysaphi (LPP, Sorbonne University, France)

15:45 Simulation of particle acceleration and transport in 3D turbulent reconnection regions - Xin Cheng (Nanjing University)
16:00 Coffee break and poster session 1

16:00 - 17:00
17:00 Energy and mass transfer throughout the solar atmosphere and structures within
17:00 - 18:15
Contributions

17:00 Restructuring of magnetic fields at the periphery of granules - G. Vigeesh

17:15 Vortex Flows in the Solar Atmosphere: Detection and Heating Mechanisms in 3D MHD Numerical Simulations - Matias Koll Pistarini (Instituto de Astrofísica de Canarias)

17:30 High flow speeds and transition-region like temperatures in the chromosphere caused by reconnection - Jorrit Leenaarts

17:45 On the sunspot penumbra formation with nonlinear force-free field extrapolations - Jan Jurcak (Astronomical Institute of the Czech Academy of Sciences)

18:00 Impact of small-scale photospheric magnetic reconnection events on the upper atmosphere - Luc Rouppe van der Voort (Rosseland Centre for Solar Physics, University of Oslo)
Tuesday, 10 September 2024
09:00 Energy and mass transfer throughout the solar atmosphere and structures within
09:00 - 10:25
Contributions

09:00 Small EUV brightenings in the quiet solar atmosphere: new insights from the Solar Orbiter mission - Susanna Parenti (Institut d'Astrophysique Spatiale, CNRS/Université Paris-Saclay)

09:25 First Solar Orbiter observation of a Dark Halo in the solar atmosphere - Serena Maria Lezzi (Istituto Nazionale di Astrofisica (INAF))

09:40 Stereoscopic study of energy and mass transfer in the solar atmosphere - Sanja Danilovic (Stockholm University)

09:55 Waves in coronal structures up to 1 Rsun? - David Berghmans (Royal Observatory of Belgium)

10:10 Probing the physical parameters of the solar chromosphere and the corona through radio observations in the 18-26 GHz frequency range - Marco Marongiu (Istituto Nazionale di Astrofisica (INAF))
10:25 Coffee break and poster session 1

10:25 - 11:25
11:25 Energy and mass transfer throughout the solar atmosphere and structures within
11:25 - 13:00
Contributions

11:25 Thermal non-equilibrium : its importance for the energy and mass cycles in the atmosphere and its possible solar wind implications - Clara Froment (CNRS/LPC2E)

11:50 Numerical Modeling of Prominence Dynamics, Eruption and Coronal Waves Propagation Using MPI-AMRVAC - Valeriia Liakh (Centre for mathematical Plasma Astrophysics KU Leuven)

12:15 On the magnetic source of chromospheric heating - Oskar Steiner (Leibniz-Institut für Sonnenphysik)

12:30 Plasma Motions and Compressive Wave Energetics in the Solar Corona and Solar Wind from Radio Wave Scattering Observations - Francesco Azzollini (University of Glasgow)

12:45 Global coronal models driven with Alfven and kink waves - Tom Van Doorsselaere (KU Leuven)
13:00 Lunch break

13:00 - 14:30

13:30 ESPD Business Meeting

13:30 - 14:30
14:30 Energy and mass transfer throughout the solar atmosphere and structures within
14:30 - 15:30
Contributions

14:30 Are Switchbacks the Magnetohydrodynamic Equivalent of Smoke Rings? - Peter Wyper

14:45 Photospheric driving of sustained kink oscillations in coronal loops - Nicolas Poirier (IRAP)

15:00 Mass Cycle and Dynamics of a Virtual Quiescent Prominence - Dion Donné (KU Leuven)

15:15 Simulation of a solar prominence with MURaM - Lisa-Marie Zessner (Max Planck Institute for Solar System Research)
15:30 Multi-scale energy release, flares and coronal mass ejections
15:30 - 15:55
Contributions

15:30 Exploring Coronal Mass Ejections: An Overview - Marilena Mierla
15:55 Coffee break and poster session 1

15:55 - 16:55
16:55 Multi-scale energy release, flares and coronal mass ejections
16:55 - 18:25
Contributions

16:55 Refining Coronal Mass Ejection Dynamics: A Semi-Analytical Flux-Rope Model Incorporating Magnetic Erosion - Sotiris Stamkos (University of Ioannina)

17:10 What can we learn about coronal mass ejections from their associated coronal dimmings? - Astrid Veronig (Institute of Physics & Kanzelhöhe Observatory, University of Graz, Austria)

17:25 Rare case of the three-part structure of coronal mass ejection observed in low coronal signatures - Tatiana Podladchikova (Skolkovo Institute of Science and Technology)

17:40 CME small-scale structures: new insights from white light observations taken between 0.06 -- 1 AU - Greta Cappello (University of Graz)

17:55 Synthetic Parker Solar Probe Observables of an Idealized Pseudostreamer CME Eruption - Benjamin Lynch (Space Sciences Laboratory, University of California--Berkeley)

18:10 Helical Structures Captured by Metis During a Polar Crown Prominence Eruption - Paolo Romano (Istituto Nazionale di Astrofisica (INAF))
Wednesday, 11 September 2024
09:00 Multi-scale energy release, flares and coronal mass ejections
09:00 - 10:30
Contributions

09:00 Solar Eruptions Triggered by Flux Emergence Below or Near a Coronal Flux Rope - Tibor Torok

09:15 The Role of Magnetic Reconnection in the Formation and Evolution of Eruptive Magnetic Flux Ropes - Rui Liu

09:30 Identifying and Tracking CME Flux Ropes On The Example of AR12473 - Andreas Wagner (University of Helsinki)

09:45 Sunspot Scars: New Features of Solar Flux Rope Footpoints - Chen Xing (Nanjing University)

10:00 Unveiling the Global Magnetic Topology with Physics-Informed Neural Networks - Robert Jarolim (University of Graz)

10:15 Can we find distinct flare precursors observed with the IRIS spectrograph? - Jonas Zbinden (Astronomical institute University of Bern)
10:30 Coffee break and poster session 2

10:30 - 11:30
11:30 Multi-scale energy release, flares and coronal mass ejections
11:30 - 13:10
Contributions

11:30 3D Magnetic reconnection and energy release in solar flares and eruptions - Jaroslav Dudík (Astronomical Institute of the Czech Academy of Sciences)

11:55 X-ray observations of small-scale flaring energy releases - Iain Hannah (University of Glasgow)

12:10 Analysis of flare ribbon fine structures using high-resolution observations - Jonas Thoen Faber (Rosseland Centre for Solar Physics, University of Oslo)

12:25 Turbulent Dynamics in Gradual-Phase Flare Loops: Insights from 3D MHD Simulations - Wenzhi Ruan (Max Planck Institute for Solar System Research)

12:40 Understanding the thermal and magnetic properties of an X-class flare in the low solar atmosphere - Fabiana Ferrente (Università Degli Studi di Catania)

12:55 Chromospheric evaporation as observed by STIX from the perihelion of Solar Orbiter - Katarzyna Mikuła (Space Research Centre, Polish Academy of Sciences)
13:10 Lunch break

13:10 - 14:30

14:30 Social excursions

14:30 - 19:30
Thursday, 12 September 2024
09:00 Multi-scale energy release, flares and coronal mass ejections
09:00 - 10:25
Contributions

09:00 The fine scales of solar flares - Lyndsay Fletcher (University of Glasgow)

09:25 Probing particle acceleration and transport through behind-the-limb gamma-ray Solar flare observations - Melissa Pesce-Rollins (INFN-Pisa)

09:40 High-Resolution Observations from the Solar Orbiter Major Flare SOOP Campaign: Insights from X-ray and Fast Cadence EUV Observations of Solar Flares - Laura Hayes (European Space Agency)

09:55 The May 2024 flare sequence: a rich opportunity for QPP analysis - Marie Dominique (Royal Observatory of Belgium)

10:10 First comparison of MSDP spectroscopic observation of the C1.6 solar flare with FLARIX NLTE simulations - Arkadiusz Berlicki (Centre of Scientific Excellence - Solar and Stellar Activity, University of Wroclaw, Poland)
10:25 ESPM-17 group picture

10:25 - 10:30

10:30 Coffee break and poster session 2

10:30 - 11:25
11:25 Diagnostic tools and numerical methods in solar physics
11:25 - 12:50
Contributions

11:25 The inversion of spectropolarimetric data and machine learning: a story about old friends and their adventures - Alberto Sainz Dalda (Bay Area Environmental Research Institute/Lockheed Martin Solar and Astrophysics Laboratory)

11:50 Improved reconstruction of solar magnetic fields from imaging spectropolarimetry through spatio-temporal regularisation - Jaime de la Cruz Rodriguez (Institute for Solar Physics, Stockholm University)

12:05 Modeling the polarization of strong chromospheric lines and its magnetic sensitivity - Luca Belluzzi (Istituto ricerche solari Aldo e Cele Daccò (IRSOL))

12:20 Parametrization of SHARP Vector Magnetic Field Using Disentangled Representation Learning - Ekaterina Dineva (Centre for mathematical Plasma-Astrophysics)

12:35 Implementation of thermal conduction energy transfer codes in the Bifrost Solar atmosphere MHD solver - George Cherry (Rosseland Centre for Solar physics, universitetet i oslo)
12:50 Lunch break

12:50 - 14:25
13:25 Outreach in Solar Physics: Outreach in Solar Physics
Outreach in Solar Physics
13:25 - 14:25
Contributions

13:25 Outreach in Solar Physics - Helen Mason (University of Cambridge) Hugh Hudson (UC Berkeley / U of Glasgow)
14:25 Diagnostic tools and numerical methods in solar physics
14:25 - 15:50
Contributions

14:25 Chromospheric Magnetic Field Reconstruction through Neural Field Assisted Spectropolarimetric Inversions - Carlos Jose Diaz Baso (Oslo University)

14:40 Spectroscopic measurements from Solar Orbiter Full Disk Mosaic - Alessandra Giunta (STFC RAL Space)

14:55 Bayes in Space: A Bayesian Deep Learning approach for Coronal Temperature estimation - Nikita Balodhi (Northumbria University, Newcastle)

15:10 The Tunable-Imaging Spectropolarimeters/Fixed-Band Imagers for the European Solar Telescope - Luis Bellot Rubio (Instituto de Astrofisica de Andalucia (IAA-CSIC))

15:25 Challenges in forecasting space weather consequences of coronal mass ejections - Emilia Kilpua (University of Helsinki)
15:50 Coffee break and poster session 2

15:50 - 16:50
16:50 Senior Prize Lecture
16:50 - 17:20
Contributions

16:50 The never-ending attraction of the Sun’s magnetic personality - Sami K. Solanki (Max-Planck-Institut für Sonnensystemforschung (MPS), Göttingen, Germany) and School of Space Research, Kyung Hee University, Yongin, Republic of Korea)
19:00 Conference dinner

19:00 - 23:00
Friday, 13 September 2024
09:00 Diagnostic tools and numerical methods in solar physics
09:00 - 09:25
Contributions

09:00 Why use real-time operational data in Solar Physics and Space Weather research? - Judith de Patoul (Solar-Terrestrial Centre of Excellence - SIDC, Royal Observatory of Belgium)
09:25 Space weather and the solar-heliospheric connections
09:25 - 10:35
Contributions

09:25 Solar wind, space weather and solar-terrestrial connection - Michaela Brchnelova (KU Leuven)

09:50 Predicting geo-effectiveness two days prior to CME impact with EUHFORIA - Anwesha Maharana (KU Leuven)

10:05 Comparison of "homologous" solar eruptive events from two different solar rotations - Manuela Temmer (Institute of Physics)

10:20 The Open Flux Problem: First steps with Solar Orbiter to investigate the underestimation of magnetic flux - Jonas Sinjan (Max Planck Institute for Solar System Research)
10:35 Coffee break and poster session 2

10:35 - 11:35
11:35 Space weather and the solar-heliospheric connections
11:35 - 13:10
Contributions

11:35 Exploring the connection between the Sun and the Heliosphere - Stephanie Yardley (Northumbria University)

12:00 From multi-decadal to real-time solar wind modelling, connectivity and plasma signatures on and off the ecliptic plane - Rui Pinto (IRAP & InforMarty)

12:25 Reconstruction of CME-driven shocks detected by multi-spacecraft observations - Federica Chiappetta (Department of Physics, Università della Calabria)

12:40 How changing of source surface height parameter in EUHFORIA affect solar wind simulations - Senthamizh Pavai Valliappan (Royal Observatory of Belgium)

12:55 Coronal magnetic field modeling using a non-spherical source surface: implications for the global structuring of the corona - Jens Pomoell (University of Helsinki)
13:10 Closing and final remarks

13:10 - 13:15

Choose timezone