PA
Patrick Antolin
Northumbria University, University of St Andrews, University of Oslo, Kyoto University, National Astronomical Observatory of Japan, Universidad de Los Andes
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Magnetic confinement fusion research
Employment
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Northumbria University Associate Professor2023 - Present
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Northumbria University Assistant Professor2022 - 2023
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Northumbria University STFC Ernest Rutherford Fellow & Proleptic Senior Lecturer2019 - 2023
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University of St Andrews STFC Ernest Rutherford Fellow2018 - 2019
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University of St Andrews Postdoctoral Researcher2016 - 2018
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National Astronomical Observatory of Japan Project Research Scientist2013 - 2015
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University of Tokyo JSPS Postdoctoral Research Fellow2013 - 2013
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KU Leuven Postdoctoral Researcher2011 - 2013
Education
- 2007 - 2012
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Kyoto University PhD2006 - 2009
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Kyoto University MSc2004 - 2006
- 1997 - 2004
- 1997 - 2003
Projects & Funding
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The Cool Alter-ego of the Hot Solar Corona Science and Technology Facilities Council2018 - 2023
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Thermodynamic Properties and Evolution of Coronal Rain Instituto de Astrofisica de Canarias2017 - 2017
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Detecting the Mechanism of Coronal Alfvénic Wave Generation in the Chromosphere Science and Technology Facilities Council2017 - 2017
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Observed Multi-Scale Variability of Coronal Loops as a Probe of Coronal Heating International Space Science Institute2017 - Present
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Unravelling the Heating of the Solar Corona Through the Cooling European Southern Observatory2017 - 2017
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Coronal Loop Magnetic Field Determination Using Coronal Rain Instituto de Astrofisica de Canarias2016 - 2016
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The Cool Alter-Ego of the Solar Corona European Southern Observatory2016 - 2016
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Forward modelling of heating - collaboration with space industry Science and Technology Facilities Council2016 - 2017
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Fine-scale structuring, braiding and heating of loops from thermal and wave instabilities Astronomical Society of Japan2015 - 2015
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Dynamics of Accretion in Magnetised Stellar Atmospheres Universitat de les Illes Balears2015 - 2015
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Kelvin-Helmholtz Instability in Coronal Loops SOLARNET2014 - 2014
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Implications for coronal heating and magnetic fields from coronal rain observations and modelling Institute Space Science Institute2014 - 2016
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Diagnostics by Forward Modelling of Magnetic Oscillations in the Solar Corona Japan Society for the Promotion of Science2013 - 2013
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IRIS & CLASP as pathfinders for Solar-C Japan Society for the Promotion of Science2013 - 2015
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The interaction between the coronal magnetic field and coronal rain through MHD waves SOLARNET2013 - 2013
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Postgraduate Studies Mombukagakusho2004 - 2009
Publications (134)
- Height-dependent thermal properties of extreme-ultraviolet campfires in the quiet Sun Save
- Multiwavelength synthesis of a flux rope-trapped mini-prominence eruption and post-flare coronal rain Save
- Fast and periodic propagating disturbances along coronal loops detected with EUI on board Solar Orbiter Save
- From simulations to observations of cool plasma: What we can learn from synthetic spectra Save
- Radiative hydrodynamic simulations of first ionization potential fractionation in solar flares Save
- Advances in the Physics of the Sun and the Solar-Heliosphere Connection – Editorial Save
- Disambiguation of Cool and Hot Emission in SDO/AIA Channels and IRIS/Slit-Jaw Imager Save
- Compression, impact, and hot rebound flows from coronal rain downflows Save
- DeepFilter: A machine learning technique for removing the hot AIA 304 Å channel component for the analysis of coronal rain Save
- Extreme-ultraviolet Synthesis of Nanojet-like Ejections due to Coalescing Flux Ropes Save
- Space-Weather Effects on Critical Infrastructure on Earth Save
- Reconnection nanojets associated with a prominence eruption observed with Solar Orbiter/EUI-HRI Save
- Do Flares Impact Neighboring Quiescent Coronal Rain? Save
- Role of magnetic shear distribution in the formation of eruptive flux ropes Save
- The solar thermostat: problems of thermal regulation in the solar atmosphere Save
- The Coronal Power Spectrum from MHD Mode Conversion above Sunspots Save
- Can we rely on EUV emission to identify coronal waveguides? Save
- Effects of coronal rain on decayless kink oscillations of coronal loops Save
- From Chromospheric Evaporation to Coronal Rain: An Investigation of the Mass and Energy Cycle of a Flare Save
- Decomposing the AIA 304 Å Channel into Its Cool and Hot Components Save