PZ
Pietro Zucca
Netherlands Institute for Radio Astronomy, Trinity College Dublin, University of Bologna, University of Padua
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Radio Astronomy Observations and Technology
0000-0002-6760-797X
Employment
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Netherlands Institute for Radio Astronomy Associate Scientist2017 - Present
Education
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Trinity College Dublin PhD Physics? - 2014
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Università degli Studi di Bologna M.Sc. Astrophysics and Cosmology? - 2010
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Università degli Studi di Padova B.sc. Astronomy? - 2008
Projects & Funding
Projects & funding information is unavailable.
Publications (27)
- An AI-Driven Framework for Automated Identification and Classification of Multi-Label Solar Radio Bursts Save
- Catalog of Solar Radio Bursts Detected by the LOFAR LV614 Station at the Irbene Observatory during Solar Cycle 25 Save
- solar bursts detected by LV614 LOFAR station Save
- Multiple shocks generated by the 2024 May 14 coronal mass ejection Save
- Driving the mid-latitude ionosphere from below: A statistical study using LOFAR Save
- An automated, self-calibration-based pipeline for high-fidelity solar imaging with LOFAR: SIMPL Save
- Three-Dimensional Characterization of Coronal Loops Using Combined Radio and EUV Observations Save
- Source location and evolution of a multilane type II radio burst Save
- The source sizes of type II radio bursts with LOFAR Save
- In-depth Analysis of the 2022 March 28 3He-rich Solar Energetic Particle Event Save
- Imaging and spectropolarimetric observations of a band-split type II solar radio burst with LOFAR Save
- Resolving spatial and temporal shock structures using LOFAR observations of type II radio bursts Save
- Magnetic connectivity of coronal loops and flare-accelerated electrons in a B-class flare Save
- Imaging a Large Coronal Loop Using Type U Solar Radio Burst Interferometry Save
- Imaging spectroscopy of a spectral bump in a type II radio burst Save
- Upgrades of the ESPERTA forecast tool for solar proton events Save
- Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations Save
- Imaging of the Quiet Sun in the Frequency Range of 20–80 MHz Save
- Lensing from small-scale travelling ionospheric disturbances observed using LOFAR Save
- Observations of Shock Propagation through Turbulent Plasma in the Solar Corona Save