Jasmina Magdalenic

Tenure Track Professor

KU Leuven

Belgium

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About

Jasmina Magdalenic is a Tenure Track Professor at KU Leuven in Belgium. Her research focuses on solar physics, particularly the dynamics of solar flares, coronal mass ejections, and solar radio bursts. Recent articles include studies on magnetic connectivity in solar flares and modeling the propagation of coronal mass ejections. Professor Magdalenic's work enhances the understanding of solar energetic particle events and their effects on space weather.

Articles (15)

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2025

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2024

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2020

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2020

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2020

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2020

Collaborators (11)

Andrzej Krankowski

Professor

University of Warmia and Mazury in Olsztyn

POLAND

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Manuela Temmer

Associate Professor

Graz University of Technology

AUSTRIA

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Stefan Hofmeister

Leibniz-Institut für Astrophysik Potsdam

GERMANY

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Juska Soljento

University of Helsinki

FINLAND

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Kazumasa Iwai

Associate Professor

Nagoya University

JAPAN

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Peijin Zhang

University of Helsinki

FINLAND

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Jens Pomoell

University of Helsinki

FINLAND

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Masumi Shimojo

准教授/Associate Professor

JAPAN

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Diana Morosan

University of Helsinki

FINLAND

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Dale Gary

Distinguished Professor

New Jersey Institute of Technology

UNITED STATES

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Karine Bocchialini

Université Paris-Saclay

FRANCE

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Jasmina Magdalenic

Research Interests

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Articles (15)

Magnetic connectivity of coronal loops and flare-accelerated electrons in a B-class flare

Electron Cyclotron Maser Emission and the Brightest Solar Radio Bursts

Modelling non-radially propagating coronal mass ejections and forecasting the time of their arrival at Earth

Cannibals in PARADISE: The Effect of Merging Interplanetary Shocks on Solar Energetic Particle Events

Fundamental–Harmonic Pairs of Interplanetary Type III Radio Bursts

Imaging of the Quiet Sun in the Frequency Range of 20–80 MHz

Dynamic Time Warping as a Means of Assessing Solar Wind Time Series

Generation of interplanetary type II radio emission

Coronal Conditions for the Occurrence of Type II Radio Bursts

Type III Radio Bursts Observations on 20th August 2017 and 9th September 2017 with LOFAR Bałdy Telescope

Electron acceleration and radio emission following the early interaction of two coronal mass ejections

On the Dependency between the Peak Velocity of High-speed Solar Wind Streams near Earth and the Area of Their Solar Source Coronal Holes

Fine Structure of a Solar Type II Radio Burst Observed by LOFAR

Using radio triangulation to understand the origin of two subsequent type II radio bursts

Role of the Coronal Environment in the Formation of Four Shocks Observed without Coronal Mass Ejections at Earth’s Lagrangian Point L1

Collaborators (11)

Andrzej Krankowski

Manuela Temmer

Stefan Hofmeister

Juska Soljento

Kazumasa Iwai

Peijin Zhang

Jens Pomoell

Masumi Shimojo

Diana Morosan

Dale Gary

Karine Bocchialini

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