Name: SOLARNET Conference: The Many Scales of the Magnetic Sun
Start: 2023-05-08T00:00:00+02:00
End: 2023-05-12T14:20:00+02:00
Location: Haus H, Telegrafenberg

Monday, 8 May 2023

10:00 Resgistration desk open
Resgistration desk open
10:00 - 14:00
14:00
14:00 - 15:05
Contributions

14:00 Welcome

14:10 The European Solar Telescope (EST): instruments and science - Rolf Schlichenmaier (Leibniz-Institut für Sonnenphysik (KIS))

14:35 Exploring the inner heliosphere with combined LOFAR and Solar Orbiter / Parker Solar Probe observations - Christian Vocks (Leibniz-Institut für Astrophysik Potsdam (AIP))

14:50 Overview of SO/PHI-HRT in the Nominal Mission Phase: data and results - Daniele Calchetti (Max Planck Insitute for Solar System Reaserch (MPS))
15:05
15:05 - 15:30
Contributions

15:05 Coronal flux ropes over Solar Cycle 24 - Anthony Yeates (Durham University)
15:30
15:30 - 16:30
Contributions

15:30 poster popups - Bartosz Dabrowski (Space Radio-Diagnostics Research Centre, University of Warmia and Mazury) Fabio Duvan Lora Clavijo (Universidad Industrial de Santander) Frederic Schuller (AIP) Markus Roth (Thüringer Landessternwarte) Merlin Mendoza (Department of Space Science and Engineering, National Central University, Taiwan) Robbe Vansintjan (Royal Observatory of Belgium) Ziwen Huang (Max-planck Institute for Solar System Research)
16:30
16:30 - 20:30
Contributions

16:30 FRANCIS: a fibre-fed prototype integral field unit for the near-UV - David Jess (Queen's University Belfast)

16:55 SunDish Project: Single-Dish Solar Imaging and calibration in K-band with the INAF Radio Telescopes - Sara Mulas (INAF-OAC)

17:10 First light and science of the UCoMP instrument of MLSO: the magnetic and thermodynamic morphology of CME precursors and eruptions - Maurice Wilson (NCAR High Altitude Observatory)

17:25 DKIST observations of small-scale, internetwork magnetism in the quiet Sun - ryan campbell (queen's university belfast)

17:40 Microlensed Hyperspectral Imagers - Michiel van Noort (MPS)
Tuesday, 9 May 2023
09:00
09:00 - 11:15
Contributions

09:00 Photospheric MHD simulations: From sub-granular scales to active regions - Matthias Rempel (High Altitude Observatory, National Center for Atmospheric Research)

09:30 Chromospheric horizontal propagating waves revealed by fast cadence imaging in Ca II K with DKIST’s Visible Broadband Imager - Catherine Fischer (National Solar Observatory)

09:45 Non-LTE formation of the widely-used Fe I 6173 Å line - Smitha Narayanamurthy (Max Planck Institute for Solar System Research)

10:00 Coronal voids and their magnetic nature - Jonathan David Nölke (Max Planck Institute for Solar System Research)

10:15 Study of the evolution of magnetic energy and helicity injection in an active region with recurring eruptive events - Marcelo López Fuentes (Instituto de Astronomía y Física del Espacio (CONICET-UBA))
11:15
11:15 - 14:00
Contributions

11:15 Active region evolution - Lucie Green (MSSL)

11:45 Scrutinising nature of magnetic and flow fields in complex active region with HiFI+ and GRIS - Robert Kamlah (Leibniz-Institut fuer Astrophysik Potsdam (AIP))

12:00 Sausage wave modes in small magnetic pores observed with Solar Orbiter/PHI - Shahin Jafarzadeh (Max Planck Institute for Solar System Research, Germany))

12:15 Detection of the Evershed flow by the application of the SOM technique - Paolo Romano (INAF - Catania Astrophysical Observatory)

12:30 Insights Into Confined/Eruptive Stellar Flare Nature using Comprehensive Statistical Analysis of Magnetic and Thermodynamic Properties of Solar Flares Observations - Maria Kazachenko (University of Colorado - Boulder / National Solar Observatory)
14:00 Session 2-b
Session 2-b
14:00 - 15:25
Contributions

14:00 Modeling of the solar chromosphere - Sanja Danilovic (Sanja)

14:25 Stereoscopic disambiguation of vector magnetograms: first applications to HRT data - Gherardo Valori (MPS - Max Planck Institute for Solar System Research)

14:40 Quantifying Systematic Biases in the Measurements of the Open Magnetic Flux - Ivan Milic (Leibniz Institute for Solar Physics (KIS))

14:55 Active region evolution – Tracking active regions from the near-Earth side to the solar far side (and back) - Hanna Strecker (Instituto de Astrofísica de Andalucía ((IAA-CSIC) & Spanish Space Solar Physics Consortium)

15:10 The role of the chromospheric canopy in the formation of a penumbra - Philip Lindner (Leibniz-Institut fuer Sonnenphysik (KIS))
15:25
15:25 - 16:30
Contributions

15:25 poster popups - Arooj Faryad Fallon Konow (Georgia State University / University of Rome Sapienza / University of Rome Tor Vergata / National Institute of Astrophysics (INAF)) José Roberto Canivete Cuissa (IRSOL) Matteo Cantoresi (University of Rome Tor Vergata) Meetu Verma ( Leibniz-Institut für Astrophysik Potsdam (AIP)) Nikolina Milanović (Max Planck Institute for Solar System Research) Philip Lindner (Leibniz-Institut fuer Sonnenphysik (KIS))
16:30
16:30 - 18:10
Contributions

16:30 Sunspot penumbral evolution: a puzzle under construction - Mariarita Murabito (INAF OACN)

16:55 On the stability of large magnetic solar structures - Jan Jurcak (Astronomical Institute of the CAS)

17:10 Evidence of external reconnection between an erupting mini-filament and ambient loops observed by Solar Orbiter/EUI - Zhuofei Li (MPS)

17:25 Plasma thermalisation from wave damping seen in super-penumbral fibrils - William Bate (Queen's University Belfast)

17:40 On diversity of spectral shapes of hydrogen Lyman lines and Mg II lines in a quiescent prominences - Pavol Schwartz (Astronomical Institute, Slovak Academy of Sciences)

17:55 Magnetic field changes in the photosphere during solar flares and their association with flare ribbons - Rahul Yadav (University of Colorado, Boulder)
Wednesday, 10 May 2023
09:00
09:00 - 09:30
Contributions

09:00 Center-to-limb variation in Mg II intensities in quiet Sun and active regions from IRIS - Megha Anand (nter University Centre for Astronomy and Astrophysics, Post Bag-4, Ganeshkhind, Pune 411007, India)

09:15 Quantifying Poynting Flux in the Quiet Sun Photosphere Using Observations and Simulations - Denis Tilipman (University of Colorado, Boulder; National Solar Observatory (NSO))
09:30
09:30 - 11:10
Contributions

09:30 Recent Progress in Understanding Solar Flare Magnetism using Data-Driven Simulations and Statistical Analysis of Vector Magnetic Fields - Maria Kazachenko (University of Colorado - Boulder / National Solar Observatory)

09:55 The magnetic complexity of solar active regions: insight on the CME-flare relationship in Solar Cycle 24 - Luca Giovannelli (University of Rome Tor Vergata)

10:10 Evolution of magnetic fields and energy release processes during homologous compact major blowout-eruption solar flares - Suraj Sahu (Physical Research Laboratory)
11:10
11:10 - 14:10
Contributions

11:10 Formation and early evolution of coronal mass ejections - Emilia Kilpua (University of Helsinki)

11:40 First results on solar flares and eruptive events from the X-ray telescope STIX on Solar Orbiter - Alexander Warmuth (Leibniz Institute for Astrophysics Potsdam (AIP))

11:55 First GREGOR and IRIS simultaneous observations of a solar flare - Marta Garcia-Rivas ((1)Astronomical Institute of the CAS (2)Astronomical Institute, Faculty of Mathematics and Physics, Charles University)

12:10 Modelling solar eruptive events from their onset to their propagation at 1 AU - Antoine Strugarek

12:25 Flare-accelerated electrons and the evolution of the associated active region - Malte Bröse (AIP)

12:40 Do ions and neutral atoms behave differently in solar prominences? - Horst Balthasar (Leibniz-Institute for Astrophysics Potsdam)
14:10 Session 3B
Session 3B
14:10 - 16:20
Contributions

14:10 The many scales observed by EUI onboard Solar Orbiter - David Berghmans (Royal Observatory of Belgium)

14:35 Photospheric and Chromospheric Magnetic Field Evolution during the X1.6 Flare in NOAA 12192 - Fabiana Ferrente (University of Catania)

14:50 On the detection of two X-class solar flares in the Sun-as-a-star with the HARPS solar telescope - Alex Pietrow (AIP)

15:05 Comprehensive simulation of a solar prominence with MURaM - Lisa-Marie Zessner (Max Planck Institute for Solar System Research)

15:20 Multiwavelength observations of small-scale eruptive phenomena in an arch filament system - Salvo Guglielmino (Istituto Nazionale di Astrofisica (INAF))

15:35 Picoflares in the Quiet Solar Corona - Olena Podladchikova (The Leibniz Institute for Astrophysics Potsdam (AIP))

15:50 Chromospheric evaporation by particle beams in multi-dimensional flare models - Malcolm Druett (KU Leuven)

16:05 Net electric currents, flares, CMEs and the evolution of active regions - Ioannis Kontogiannis (Leibniz Institute for Astrophysics Potsdam (AIP) Germant)
16:20
16:20 - 19:10
Contributions

16:20 Poster popups - Salvo Guglielmino (Istituto Nazionale di Astrofisica (INAF)) Sibaek Yi (Kyung Hee University) Sofya Belov (Branišovská 1760, 37005 České Budějovice) Tino L. Riethmüller (Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany) Xiang Li Xudong Sun (University of Hawaii)
Thursday, 11 May 2023
09:00
09:00 - 09:30
Contributions

09:00 Comparative Study of Power Distribution in Flaring and Non-flaring Active Regions with SDO/AIA. - Aneta Wisniewska (Leibniz Institute for Astrophysics Potsdam (AIP))

09:15 Formation of MgII h&k spectra in an enhanced network region simulated with MURaM - Patrick Ondratschek (Max Planck Institute for Solar System Research)
09:30
09:30 - 11:10
Contributions

09:30 Long-term variability of solar magnetic flux and irradiance - Natalie Krivova (Max Planck Institute for Solar System Research)

09:55 Examining the Closed Magnetic Field Lines Crossing the Coronal Hole Boundaries - Chia-Hsien Lin (Department of Space Science and Engineering, National Central University)

10:10 The relation of the Sun’s global magnetic field with the solar wind parameters on solar cycle time-scales - Raffaele Reda (University of Rome Tor Vergata)
11:10
11:10 - 11:35
Contributions

11:10 DKIST instruments and science - Thomas Rimmele (National Solar Observatory)
11:35
11:35 - 13:50
Contributions

11:35 Power supply and evolution of the solar dynamo - Quentin Noraz (Rosseland Centre for Solar Physics, University of Oslo, P.O. Box 1029 Blindern, Oslo, NO-0315, Norway)

11:50 Role of spots in stellar Ca II H & K emissions: what can we learn from spots on the Sun? - Sowmya Krishnamurthy (Max Planck Institute for Solar System Research)

12:05 Data-driven model of temporal evolution of the solar Mg II h & k profiles over the solar cycle - Julius Koza (Astronomical Institute, Slovak Academy of Sciences)

12:20 Solar-cycle variation of the quiet-sun magnetism - Andreas Korpi-Lagg (Max Planck Institute for Solar System Research / Aalto University)
13:50 Session 4B
Session 4B
13:50 - 15:15
Contributions

13:50 Solar Irradiance Variability - From Measurements to Modelling - Margit Haberreiter (PMOD/WRC)

14:15 Revisiting the long-term evolution of the Sun’s magnetic field: Solar wind sources and coronal rotation - Adam Finley (CEA Paris-Saclay)

14:30 Differential Rotation of the Solar Chromosphere using multidecadal Ca K spectroheliograms - Dibya Kirti Mishra (ARIES, India)

14:45 The effects of the surface inflows on quenching of solar cycles - MOHAMMED TALAFHA (Dept. of Space Physics and Technology, Wigner Research Centre for Physics)

15:00 On the origin of the Solar Mean Magnetic Field - Vishnu M (Indian Institute of Astrophysics)
15:15
15:15 - 17:30
Contributions

15:15 Poster popups - Andrei Gorobets (Leibniz-KIS) Carsten Denker (Leibniz Institute for Astrophysics Potsdam (AIP)) Francesco Berrilli (University of Rome Tor Vergata) Malcolm Druett (KU Leuven) Meetu Verma (Leibniz-Institut für Astrophysik Potsdam (AIP)) Saida Milena Diaz Castillo (Leibniz Institute for Solar Physics - KIS) Sanghita Chandra (Max Planck Institute for Solar System Research)
Friday, 12 May 2023
09:00
09:00 - 09:15
Contributions

09:00 Changes in the Lower Solar Atmosphere throughout the Solar Cycle - James Crowley (National Solar Observatory; University of Colorado, Boulder)
09:15
09:15 - 11:20
Contributions

09:15 Data Analysis Tools - Nazaret Bello Gonzalez (Leibniz-Institut für Sonnenphysik (KIS))

09:40 Classification Scheme for High-resolution Spectra Using Machine Learning Algorithms - Ekaterina Dineva (Katholieke Universiteit Leuven)

09:55 Atomic lines parameters inference using a global spectropolarimetric inversion - Dušan Vukadinović (Max Planck Institute for Solar System Research)

10:10 Machine Learning methods for solar spectroscopy and imaging - Andrés Asensio Ramos (Instituto de Astrofísica de Canarias)
11:20
11:20 - 14:20
Contributions

11:20 Identification of large scale resonant modes in sunspots in the lower solar atmosphere - Marco Stangalini (ASI Italian Space Agency)

11:45 Physics-informed neural networks for solar magnetic field simulations - Robert Jarolim

12:00 Generative deep learning with high-resolution SDO EUV images of the Sun - Frederic Effenberger (Ruhr-University Bochum)

12:15 Time-normalized plasma flow mapping during the quadrature of SolO and SDO - Gabriel Muro (Aberystwyth University)