DynaSun
DynaSun
Dynamics of the Solar Corona in the Era of Data Intensive Observations
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About
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.
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Consortium
COORDINATOR
KATHOLIEKE UNIVERSITEIT LEUVEN, Belgium
Contact: Tom Van Doorsselaere,
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JIHOCESKA UNIVERZITA V CESKYCH BUDEJOVICICH, Czechia
Contact: Petr Jelínek,
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Contact: Astrid Veronig,
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Contact: Pradeep Chitta,
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CONSEJO NACIONAL DE INVESTIGACIONES CIENTIFICAS Y TECNICAS, Argentina
Contact: Andrea Costa,
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Contact: Santiago Vargaz Dominguez,
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Contact: James McLaughlin,
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Contact: Valery Nakariakov,
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Work Packages
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
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Meetings
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
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Publications
The research was sponsored by the DynaSun project and has thus received funding under the Horizon Europe programme of the European Union under grant agreement (no. 101131534). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union and therefore the European Union cannot be held responsible for them."
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Communication
1. The DynaSun kick-off meeting, KU Leuven, Belgium, 25-26 March 2024.
This project DynaSun has received funding under the Horizon Europe programme of the European Union under grant agreement (no. 101131534).
- Přečteno: 4059
