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Submitted URL: https://dynasun.prf.jcu.cz/
Effective URL: https://www.prf.jcu.cz/en/dynasun
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Effective URL: https://www.prf.jcu.cz/en/dynasun
Submission: On July 29 via api from US — Scanned from CA
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DYNASUN
Dynamics of the Solar Corona in the Era of Data Intensive Observations
* About
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This project aims to establish a close research collaboration between several
leading European and South American research institutes specialized in solar
physics and to gain new paradigmatic insights into the dynamic processes in the
solar atmosphere, through a systematic exchange of researchers and knowledge and
joint research efforts using existing data and facilities, including innovative
data analysis techniques based on machine learning approaches. The expected
scientific impact is a significant advancement in our knowledge of key physical
processes occurring in the solar atmosphere, including breakthroughs in
unraveling the mechanism of coronal heating, transformational advances in our
understanding of impulsive energies such as solar flares and CMEs, significant
advances in MHD wave theory, and the first application of machine learning
techniques to the study of wave processes in the solar atmosphere.
The project includes four scientific work packages that address specific key
challenges in modern solar physics and heliophysics: quasi-periodic pulsations
in solar flares, wave heating and coupling to the lower atmosphere, the
development of three-dimensional CME morphology, kinematic oscillations of
coronal mass exclusion, and a work package for communication and dissemination.
Expected economic and technological impacts include gaining direct experience in
the analysis of complex oscillatory processes, experience in the design and
application of machine learning techniques for pattern recognition, new
technologies for the analysis of oscillatory processes, and input parameter
diagnostic techniques for space weather prediction models, the establishment of
facilities for knowledge exchange with foreign partners with local industries,
and the training of highly skilled professionals in numerical modeling and data
analysis. The expected societal impact is to strengthen research links between
the European and US research communities, to improve public awareness of modern
solar and heliophysics research and development issues, and to motivate school
students to pursue scientific careers.
COORDINATOR
KATHOLIEKE UNIVERSITEIT LEUVEN, Belgium
Contact: Tom Van Doorsselaere, tom.vandoorsselaere@kuleuven.be
BENEFICIARIES
JIHOCESKA UNIVERZITA V CESKYCH BUDEJOVICICH, Czechia
Contact: Petr Jelínek, pjelinek@prf.jcu.cz
UNIVERSITAET GRAZ (GRA), Austria
Contact: Astrid Veronig, astrid.veronig@uni-graz.at
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV, Germany
ASSOCIATED PARTNERS
CONSEJO NACIONAL DE INVESTIGACIONES CIENTIFICAS Y TECNICAS, Argentina
Contact: Andrea Costa, acosta@unc.edu.ar
UNIVERSIDAD NACIONAL DE COLOMBIA, Colombia
Contact: Santiago Vargaz Dominguez, svargasd@unal.edu.co
UNIVERSITY OF NORTHUMBRIA AT NEWCASTLE, United Kingdom
Contact: James McLaughlin, james.a.mclaughlin@northumbria.ac.uk
THE UNIVERSITY OF WARWICK, United Kingdom
Contact: Valery Nakariakov, V.Nakariakov@warwick.ac.uk
WP1: Quasi-periodic pulsations in solar flares
WP2: Wave heating and connection to the lower atmosphere
WP3: Evolution of three-dimensional CME morphology
WP4: Kinematic oscillations of coronal mass ejections
WP5: Communication & dissemination
1. The DynaSun kick-off meeting, KU Leuven, Belgium, 25-26 March 2024.
Programme DynaSun kick-off.PDF
2. DynaSun Network workshop: Waves, Reconnection and Particle Acceleration in
Solar Flares, Northumbria University (Newcastle upon Tyne, NE1 8ST, UK), 2-6
September 2024
https://sites.google.com/view/dynasun2024/overview
This project DynaSun has received funding under the Horizon Europe programme of
the European Union under grant agreement (no. 101131534).
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