Participants

Säm KruckerFHNW/UCB
PSP/FIELDS radio events and their association with STIX flares
Anna KępaSpace Research Centre Polish Academy of Sciences
A multi-thermal analysis of M-class flare observed in common by STIX and XSM
Gelu M. NitaNew Jersey Institute of Technology
GX Simulator in the era of stereoscopic Hard X-ray observations
Laura HayesESA
Flare list fun
Olivier LimousinCEA/DRF/Irfu/Astrophysics division
Galina G. MotorinaAstronomical Institute of the CAS
Frederic SchullerLeibniz Institut für Astrophysik Potsdam
Updates on STIX and Solar Orbiter poiting
Alexander WarmuthLeibniz-Institute for Astrophysics Potsdam (AIP)
Update on solar electron events observed with remote-sensing and in-situ instruments on Solar Orbiter
Muriel Zoë StiefelFHNW & ETH Zürich
STIX hard X-ray signatures from erupting filaments
Dr Nicole VilmerLESIA-Paris Observatory-PSL
A multi wavelenght study of the long duration May 9 2021 event: combined X-ray, radio and EUV observations
Debesh BhattacharjeeUniversity of Glasgow, Glasgow, UK
On the Modelling of Solar Flare Hard X-Ray Spectra using STIX Data
Antoine StrugarekCEA Paris-Saclay
Natalia BajnokovaUniversity of Glasgow
First joint NuSTAR and Solar Orbiter/STIX X-ray observations of solar microflares
Hannah CollierFHNW, ETHZ
EUI/FSI short exposure observations of STIX flares
Andrea Francesco BattagliaFHNW
Hot X-ray onsets: Tracing flare precursors in Mg II for predictive insights
Arun Kumar AwasthiSpace Research Centre, Polish Academy of Sciences, Wroclaw, Poland
Hard X-ray richness in weak flares observed by STIX, AIA, and STEREO-A
BRUN Allan SachaDept. of Astrophysics, CEA Paris-Saclay
Alexandra LysenkoIoffe Institute
Joint Observations of Solar Flares by Konus-Wind and SolO/STIX
Hanya PanUniversity of Graz, University of Science and Technology of China
The height evolution and distribution of double-source X-ray emission during a flare
Michalina LitwickaUniversity of Wrocław, Centre of Scientific Excellence – Solar and Stellar Activity, Kopernika 11, PL-51622 Wrocław, Poland / and / Space Research Centre PAS
Statistical analysis of compact flares observed by STIX
Daniel RyanFHNW
3D evolution of a solar flare thermal X-ray loop-top source
František FárníkAstronomical Institute Ondřejov
Rohit SharmaFHNW, Windisch
Simultaneous solar flares observations in X-rays and meterwavelengths using STIX and MWA
Jana KašparováAstronomical Institute of the CAS
STIX HXR sources of the Apr 2, 2022 eruptive flare
Sophie MussetEuropean Space Agency
Marek StęślickiCentrum Badań Kosmicznych PAN
Karol J. KułagaAstronomical Institute, University of Wroclaw, Kopernika 11, 51-622 Wroclaw, Poland
Elementary flare profile fit to X-ray light curves registered by STIX - Continuation
Paolo MassaWestern Kentucky University
Yingjie LuoUniversity of Glasgow
Ivan ZimovetsSpace Research Institute of the Russian Academy of Sciences
Janusz SylwesterSpace Research Centre, PAS, Solar Physics Division Wrocław
TEMIRA – a new approach for determining flare plasma parameters from X-ray spectrum below 10 keV
Shilpi BhuniaDublin Institute for Advanced Studies, Trinity College Dublin
Localising Signatures of Particles Acceleration in Low Solar Atmosphere
Shilpi BhuniaDublin Institute for Advanced Studies, Trinity College Dublin
Localising Signatures of Particles Acceleration in Low Solar Atmosphere
Barbara SylwesterSpace Research Centre, PAS Warsaw, Solar Physics Division Wrocław
An Atlas of archived Flat Crystal Spectrometer (SMM) spectra
Michal VaradyFaculty od Science, UJEP
Emma PerracchionePolitecnico di Torino
michele pianaMIDA, dipartimento di matematica, università di genova
Automated and multi-scale CLEAN methods for STIX visibilities
Anna VolparaMIDA, dipartimento di matematica, Università degli Studi di Genova
Update on electron maps for STIX
Tomasz MrozekCentrum Badań Kosmicznych PAN
Update on coronal HXR sources produced during a failed eruption.
Katarzyna MikułaSpace Research Centre, PAS
The energy-altitude relation in the solar flare footpoints observed by STIX
Ewan DicksonUniversity of Graz
STIX IDL GSW update
Kenneth PhillipsNatural History Museum, London
Getting the flare iron abundance from RHESSI observations of the Fe line feature in solar flares.
Gregory FleishmanCSTR
Petr HeinzelCzech Academy of Sciences/Wroclaw University
Shane MaloneyDublin Institute of Advanced Studies
Mateusz TykierkoWroclaw Centre for Networking and Supercomputing
Data processing services for scientific community
Sylwester KołomańskiAstronomical Institute, University of Wrocław
Jana KasperováJ. E. Purkyně University in Ústí nad Labem
Dale GaryNew Jersey Institute of Technology
EOVSA Update
Arkadiusz BerlickiCentre of Excellence - Solar and Stellar Activity, University of Wrocław, Poland
Małgorzata PietrasUniversity of Wrocław
Kamil BiczAstronomical Institute of the University of Wrocław
Paweł PreśInstytut Astronomiczny, University of Wrocław
Gordon HurfordFHNW / HMS
Yang SuPurple Mountain Observatory, Chinese Academy of Sciences
The status and early results of ASO-S/HXI
Qiao LiPurple Mountain Observatory
Changxue ChenPurple Mountain Observatory, CAS
Hard X-ray imaging of quasi periodic pulsations at the footpoints of a solar flare
Zhentong LiPurple Mountain Observatory