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Researcher
Jasmina Magdalenić Zhukov
- Disciplines:Radio and sub-mm astronomy, Space plasma physics and solar physics
Affiliations
- Plasma-astrophysics (Division)
Member
From1 Jan 2021 → Today
Projects
1 - 10 of 10
- Bridging the EUV and White Light observations in search of the Origins of the solar windFrom10 Jun 2025 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- Connecting large to small scales in plasma, from CME-driven shocks to radio emissionFrom26 May 2025 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- Explaining solar flare triggering mechanisms with Explainable Artificial IntelligenceFrom17 Dec 2024 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- Understanding the solar radio emission processes from the Sun to EarthAcronym: UnderRadioSunFrom1 Oct 2024 → TodayFunding: BOF - projects
- Equation Discovery and Machine Learning applications on Solar Wind and Solar Corona space-based dataFrom8 Nov 2023 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- The physics of Coronal Mass Ejections through novel Extreme Ultraviolet Imager observations and modelingFrom20 Mar 2023 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- Study of radio bursts and the novel in situ observations and modelingFrom15 Feb 2022 → TodayFunding: Own budget, for example: patrimony, inscription fees, gifts
- The solar wind and its transients through observations and modelingFrom1 Oct 2021 → 30 Sep 2023Funding: BOF - projects
- Forecasting the arrival of CMEs and CME-driven shock waves at Earth.From20 Sep 2021 → 20 Sep 2025Funding: BOF - doctoral mandates
- Deep learning prediction and hindsight of flare initiation - DELPHIFrom15 Mar 2020 → 15 Mar 2025Funding: BRAIN-be(Belgian Research Action through Interdisciplinary Networks)
Publications
1 - 10 of 49
- Magnetic connectivity of coronal loops and flare-accelerated electrons in a B-class flare Based on X-ray, EUV (DEM analysis), and type-III radio burst observations(2025)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 694
- Fine structures of a solar type III radio bursts observed with LOFAR(2025)Published in: Acta GeophysicaISSN: 1895-6572Issue: 1Volume: 73Pages: 987 - 993
- Toroidal modified Miller-Turner CME model in EUHFORIA: Validation and comparison with flux rope and spheromak(2024)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 691Pages: 1 - 27
- Modelling non-radially propagating coronal mass ejections and forecasting the time of their arrival at Earth(2024)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 690
- Validation of EUHFORIA cone and spheromak coronal mass ejection models(2024)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 689
- Calibrating the WSA model in EUHFORIA based on PSP observations(2024)Published in: Astrophysical JournalISSN: 0004-637XIssue: 1Volume: 971
- Electron Cyclotron Maser Emission and the Brightest Solar Radio Bursts(2024)Published in: Astrophysical JournalISSN: 0004-637XIssue: 1Volume: 969
- Cannibals in PARADISE: The effect of merging interplanetary shocks on solar energetic particle events(2024)Published in: Astrophysical journal lettersISSN: 2041-8205Issue: 2Volume: 967
- Polarization properties of the decameter spikes(2024)Published in: Frontiers in Astronomy and Space SciencesISSN: 2296-987XVolume: 11
- Observation of solar radio burst events from Mars orbit with the Shallow Radar instrument(2024)Published in: Astronomy & AstrophysicsISSN: 0004-6361Volume: 683