Active region evolution (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Active region evolution – Tracking active regions from the near-Earth side to the solar far side (and back) (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Atomic lines parameters inference using a global spectropolarimetric inversion (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Center-to-limb variation in Mg II intensities in quiet Sun and active regions from IRIS (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Changes in the Lower Solar Atmosphere throughout the Solar Cycle (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Chromospheric evaporation by particle beams in multi-dimensional flare models (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Chromospheric horizontal propagating waves revealed by fast cadence imaging in Ca II K with DKIST’s Visible Broadband Imager (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Classification Scheme for High-resolution Spectra Using Machine Learning Algorithms (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Comparative Study of Power Distribution in Flaring and Non-flaring Active Regions with SDO/AIA. (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Comprehensive simulation of a solar prominence with MURaM (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Coronal flux ropes over Solar Cycle 24 (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Coronal voids and their magnetic nature (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Data Analysis Tools (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Data-driven model of temporal evolution of the solar Mg II h & k profiles over the solar cycle (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Detection of the Evershed flow by the application of the SOM technique (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Differential Rotation of the Solar Chromosphere using multidecadal Ca K spectroheliograms (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
DKIST instruments and science (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
DKIST observations of small-scale, internetwork magnetism in the quiet Sun (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Do ions and neutral atoms behave differently in solar prominences? (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Evidence of external reconnection between an erupting mini-filament and ambient loops observed by Solar Orbiter/EUI (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Evolution of magnetic fields and energy release processes during homologous compact major blowout-eruption solar flares (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Examining the Closed Magnetic Field Lines Crossing the Coronal Hole Boundaries (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Exploring the inner heliosphere with combined LOFAR and Solar Orbiter / Parker Solar Probe observations (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
First GREGOR and IRIS simultaneous observations of a solar flare (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
First light and science of the UCoMP instrument of MLSO: the magnetic and thermodynamic morphology of CME precursors and eruptions (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
First results on solar flares and eruptive events from the X-ray telescope STIX on Solar Orbiter (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Flare-accelerated electrons and the evolution of the associated active region (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Formation and early evolution of coronal mass ejections (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Formation of MgII h&k spectra in an enhanced network region simulated with MURaM (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
FRANCIS: a fibre-fed prototype integral field unit for the near-UV (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Generative deep learning with high-resolution SDO EUV images of the Sun (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Identification of large scale resonant modes in sunspots in the lower solar atmosphere (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Insights Into Confined/Eruptive Stellar Flare Nature using Comprehensive Statistical Analysis of Magnetic and Thermodynamic Properties of Solar Flares Observations (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Long-term variability of solar magnetic flux and irradiance (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Machine Learning methods for solar spectroscopy and imaging (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Magnetic field changes in the photosphere during solar flares and their association with flare ribbons (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Microlensed Hyperspectral Imagers (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Modeling of the solar chromosphere (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Modelling solar eruptive events from their onset to their propagation at 1 AU (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Multiwavelength observations of small-scale eruptive phenomena in an arch filament system (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Net electric currents, flares, CMEs and the evolution of active regions (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Non-LTE formation of the widely-used Fe I 6173 Å line (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
On diversity of spectral shapes of hydrogen Lyman lines and Mg II lines in a quiescent prominences (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
On the detection of two X-class solar flares in the Sun-as-a-star with the HARPS solar telescope (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
On the origin of the Solar Mean Magnetic Field (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
On the stability of large magnetic solar structures (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Overview of SO/PHI-HRT in the Nominal Mission Phase: data and results (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Photospheric and Chromospheric Magnetic Field Evolution during the X1.6 Flare in NOAA 12192 (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Photospheric MHD simulations: From sub-granular scales to active regions (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Physics-informed neural networks for solar magnetic field simulations (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Picoflares in the Quiet Solar Corona (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Plasma thermalisation from wave damping seen in super-penumbral fibrils (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Poster popups (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Poster popups (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
poster popups (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
poster popups (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Power supply and evolution of the solar dynamo (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Quantifying Poynting Flux in the Quiet Sun Photosphere Using Observations and Simulations (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Quantifying Systematic Biases in the Measurements of the Open Magnetic Flux (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Recent Progress in Understanding Solar Flare Magnetism using Data-Driven Simulations and Statistical Analysis of Vector Magnetic Fields (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
Revisiting the long-term evolution of the Sun’s magnetic field: Solar wind sources and coronal rotation (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Role of spots in stellar Ca II H & K emissions: what can we learn from spots on the Sun? (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Sausage wave modes in small magnetic pores observed with Solar Orbiter/PHI (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Scrutinising nature of magnetic and flow fields in complex active region with HiFI+ and GRIS (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Solar Irradiance Variability - From Measurements to Modelling (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Solar-cycle variation of the quiet-sun magnetism (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
Stereoscopic disambiguation of vector magnetograms: first applications to HRT data (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Study of the evolution of magnetic energy and helicity injection in an active region with recurring eruptive events (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
SunDish Project: Single-Dish Solar Imaging and calibration in K-band with the INAF Radio Telescopes (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Sunspot penumbral evolution: a puzzle under construction (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
The effects of the surface inflows on quenching of solar cycles (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
The European Solar Telescope (EST): instruments and science (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
The magnetic complexity of solar active regions: insight on the CME-flare relationship in Solar Cycle 24 (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
The many scales observed by EUI onboard Solar Orbiter (in session "Energy and mass flow through the solar atmosphere – from solar campfires to CME (Observations and Theory)")
The relation of the Sun’s global magnetic field with the solar wind parameters on solar cycle time-scales (in session "Variations of magnetic fields with the solar cycle – synoptic observations and Theory")
The role of the chromospheric canopy in the formation of a penumbra (in session "Small and large-scale magnetic features – from bright points to sunspots (Observations and Theory)")
Time-normalized plasma flow mapping during the quadrature of SolO and SDO (in session "Innovative ways of data analysis, data handling, machine learning, and big data")
Welcome (in session "Latest facilities to observe fundamental processes - space missions, telescopes, and instrumentation")
Include materials from selected contributions
