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Oral contributions

Session 5

Review	C. J. Diaz Baso	Application of machine learning and neural networks to data processing in solar physics
Invited	R. Ishikawa	Solar magnetic fields from the photosphere to the top chromosphere revealed by CLASP2 and Hinode
Invited	J. Stepan	Novel framework for the three-dimensional NLTE inverse problem
Contributed	N. Zambrana Prado	Elemental composition diagnostics for Hinode/EIS
Contributed	B. Panos	Explainable solar flare prediction using IRIS Mg II spectra
Contributed	K. Fukumitsu	Image Restoration based on Deep Learning for High-Resolution Solar Images
Contributed	T. Pereira	SunnyNet: Speeding up 3D non-LTE spectral synthesis with neural networks
Contributed	D. Nobrega-Siverio	Solar surges related to UV bursts: Characterization through k-means, inversions, and density diagnostics
Contributed	N. Karna	The study of polar coronal holes since the launch of Hinode
Contributed	J. M. Jenkins	The Lightweaver 1.5D Spectral Synthesis of an MPI-AMRVAC Solar Prominence/Filament
Contributed	D.F. Ryan	Deriving and Visualizing X-ray Source Properties in 3-D Using Hinode/XRT and SolO/STIX

Session 1

Review	N. Bello Gonzalez	Convective cells and magnetic fields
Invited	K. Cho	Generation of umbral oscillations and subsurface structure of sunspots
Invited	R.T. Ishikawa	Multi-scale deep learning for estimating horizontal velocity fields on the solar surface
Invited	S. S. A. Silva	Formation of vortex tubes
Contributed	N. Nitta	How much do we know about the polar field?
Contributed	A. Popovas	First results from global MHD simulations of Solar convective zone
Contributed	T. Oba	Study of the relation between the reversed granulation and the gas compression/expansion
Contributed	L. Bellot Rubio	Unipolar and bipolar magnetic flux appearance in the solar internetwork

Session 2

Review	K. Reeves	A Review of the Hinode and IRIS Contributions to Understanding Magnetic Reconnection and Prospects for the Future
Invited	W. Ashfield	Condensation in flares, observation and modeling
Invited	R.J. French	Probing Current Sheet Instabilities from Flare Ribbon Dynamics
Contributed	Ying Li	Spectroscopic observations of a solar flare from IRIS and CHASE
Contributed	S. Jejcic	Non-LTE Inversion of Prominence Spectroscopic Observations in H-alpha and MgII lines
Contributed	I. Cabello	A textbook example of magnetic flux emergence leading to EBs, UV bursts, surges and EUV signatures
Contributed	S.L. Guglielmino	Small-scale reconnection events observed by IRIS: microflares, UV bursts and their complex configurations
Contributed	M. Garcia-Rivas	First co-temporal GREGOR and IRIS observations of a solar flare
Contributed	J. Zbinden	How well can we predict flares based on IRIS Mg II, Si IV, and C II spectra?
Contributed	G. Chintzoglou	Revealing Strong Photospheric Downflows in Collisional Polarity Inversion Lines of Flare- and CME-Productive Active Regions
Contributed	S. Roy	Thermal and Non-thermal Energy Evolution in Solar Flares
Contributed	J. Dudik	Filament self-reconnection as a possible source of SADs

Session 3

Review	D. Baker	Upflows in active regions and their composition
Invited	J. M. da Silva Santos	Heating of the solar chromosphere
Invited	Leping Li	Coronal condensations in hybrid prominence/coronal rain structures
Contributed	M. Gosic	Emergence of internetwork magnetic fields into the chromosphere and transition region
Contributed	Yajie Chen	Doppler shifts of spectral lines formed in the solar transition region and corona
Contributed	J. de la Cruz Rodriguez	Spatially-resolved radiative losses in the chromosphere
Contributed	S. Bose	On the correlation between chromospheric and coronal heating in an active region moss
Contributed	C.M.J. Osborne	Considering the Radiative Interaction between Flares and Neighbouring Chromosphere
Contributed	M. Barta	What is the temperature of solar prominences? First independent determination using ALMA, H-alpha, and IRIS
Contributed	V. Hansteen	Mg II formation in the Solar Chromosphere
Contributed	S. Sahin Metcalf lecture	Prevalence of Thermal Non-Equilibrium over an Active Region
Contributed	P. Testa	Evolution of coronal abundances in active regions
Contributed	T.A. Howson	The atmospheric response to heating driven by random foot point driving
Contributed	R. Morosin	Spatio-temporal analysis of chromospheric heating in a plage region
Contributed	T. Mihailescu	What determines active region coronal plasma composition?
Contributed	S. Mulay	A detailed investigation of molecular hydrogen at three flare ribbons

Session 4

Review	K. Karampelas	MHD waves and instabilities in relation to oscillatory reconnection
Invited	Wenxian Li	Coronal magnetic fields measurement using MIT method
Invited	B. Popescu Braileanu	Ion-neutral interactions, MHD instabilities
Contributed	A. Sainz Dalda	Turbulence in the chromosphere during flares: taking on the challenge
Contributed	M. Murabito	Relationship between high FIP bias and magnetic wave power
Contributed	J. Lorincik	Rapid variations of Si IV line properties in an M-class flare observed by IRIS at very high cadence
Contributed	J. Joshi	Properties of ubiquitous magnetic reconnection events in the lower solar atmosphere
Contributed	P. Kohutova	Coronal oscillations in the self-consistent 3D MHD simulations of the solar atmosphere
Contributed	Y. Kotani	Universal Correlation between the Ejected Mass and Total Flare Energy for Solar and Stellar Cold Plasma Ejection
Contributed	V. Polito	IRIS and NuSTAR observations of a small B-class flare
Contributed	P. Ondratschek	MgII spectra of an enhanced network region simulated with the MURaM code
Contributed	A.R.C. Sukarmadji	Nanojets as pointers to the flare initiation process

New missions

Invited	B. De Pontieu	The MUlti-slit Solar Explorer mission
Invited	T. Shimizu	Solar-C EUVST