Dr Stephane Regnier

Associate Professor

School: Engineering, Physics and Mathematics

I am currently an Associate Professor in Mathematics at Northumbria University (Newcastle upon Tyne). After getting my PhD from the Universite Paris-Sud (Orsay, France), I continued to develop numerical models of magentic fields and their use to understand the physics of the Sun's atmosphere at Montana State University (Bozeman, USA), ESTEC (Noordwijk, The Netherlands), St Andrews University (Scotland), the University of Central Lancashire (Preston, UK). In 2010, I started as a lecturer at Northumbria University.

Campus Address

Pandon Building

Email Stephane

Key Publications

Please visit the Pure Research Information Portal for further information
Structure and Dynamics of Erupting Solar Prominences Using the Rolling Hough Transform: Toward a Feature-oriented Classification, Birch, H., Régnier, S. 1 Jun 2025, In: The Astrophysical Journal
Identifying Coronal Sources of L1 Solar Wind Disturbances Using the Fisk Heliospheric Magnetic Field and Potential Field Extrapolations during Three Solar Minima, Steyn, P., Johnson, D., Botha, G., Régnier, S. 1 May 2024, In: The Astrophysical Journal
Properties of magnetic null points associated with X-class flares during solar cycle 24, Edgar, R., Regnier, S. 21 Jul 2024, In: Monthly Notices of the Royal Astronomical Society
Oscillatory Reconnection as a Plasma Diagnostic in the Solar Corona, Karampelas, K., McLaughlin, J., Botha, G., Régnier, S. 1 Feb 2023, In: The Astrophysical Journal
Oscillatory Reconnection of a 2D X-point in a hot coronal plasma, Karampelas, K., McLaughlin, J., Botha, G., Regnier, S. 1 Feb 2022, In: Astrophysical Journal
The Independence of Oscillatory Reconnection Periodicity from the Initial Pulse, Karampelas, K., McLaughlin, J., Botha, G., Régnier, S. 11 Jul 2022, In: The Astrophysical Journal
Multi-Stranded Coronal Loops: Quantifying Strand Number and Heating Frequency from Simulated Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) Observations, Williams, T., Walsh, R., Regnier, S., Johnston, C. Jun 2021, In: Solar Physics
Correction to: Statistical Analysis of Solar Events Associated with Storm Sudden Commencements over One Year of Solar Maximum During Cycle 23: Propagation from the Sun to the Earth and Effects, Bocchialini, K., Grison, B., Menvielle, M., Chambodut, A., Cornilleau-Wehrlin, N., Fontaine, D., Marchaudon, A., Pick, M., Pitout, F., Schmieder, B., Régnier, S., Zouganelis, I. Apr 2019, In: Solar Physics
Damping of Propagating Kink Waves in the Solar Corona, Tiwari, A., Morton, R., Regnier, S., McLaughlin, J. 10 May 2019, In: The Astrophysical Journal
In situ generation of coronal Alfvén waves by jets, González-Avilés, J., Guzmán, F., Fedun, V., Verth, G., Sharma, R., Shelyag, S., Regnier, S. 1 Apr 2019, In: Monthly Notices of the Royal Astronomical Society

Professional Activity

Please visit the Pure Research Information Portal for further information
Invited talk: The Magnetic Universe 2023
Examination: Internal Examiner 2023
Participating in a conference, workshop, ...: National Astronomy Meeting (2023) 2023
Other: Nuffield Summer Studentship 2022
Publication Peer-review: The Astrophysical Journal (Journal) 2022
Oral presentation: Statistics of nanoflares in quiet-Sun magnetic fields: tangential discontinuities 2019
Invited talk: The Sun's magnetic fields 2019
Oral presentation: Heating coronal loops by nanoflares: testing Klimchuk's hypothesis 2019
Oral presentation: Statistics of nano- and micro-flares in active region magnetic fields 2019
Invited talk: The Solar Corona 2019

PGR Supervision

Harry Birch ??Automated Detection and Classification of Solar Prominences Using Deep Learning Techniques? Start Date: 19/09/2022
Harry Birch The Physics of Solar Prominences: an AI/ML approach Start Date: 19/09/2022 End Date: 17/10/2025
Lewis Dean Solving Partial Differential Equations with Bayesian Inference Start Date: 01/10/2024
Lewis Dean Solving Partial Differential Equations with Bayesian Inference Start Date: 01/10/2024 End Date: 17/10/2025