Seminars 2023–2024

DATESPEAKERTITLEROOM
CANDLEMAS SEMESTER:   JAN – JUN 2024
17/01 Biswajit Mondal (NASA Marshall Space Flight Centre) Heating of coronal X-ray bright points (XBP) Teams (Theatre B) (3 p.m.)
24/01 Tony Arber (Warwick) Improved thermal conduction models for the solar corona Theatre B
31/01 Cosima Breu A Comprehensive Simulation of Solar Wind Formation from the Solar Interior: Significant Cross-field Energy Transport by Interchange Reconnection near the Sun by Haruhisa Iijima et al. Theatre B
07/02 Thomas Williams (Durham) Automated Detection of coronaL MAss Ejecta origiNs for Space Weather AppliCations (ALMANAC) Theatre B
14/02 Georgios Chouliaris Effects of partially ionized plasma to the magnetic flux emergence process Theatre B
21/02   Staff Council  
28/02 Kate Mowbray Estimating particle energisation in collapsing magnetic trap (CMT) models for solar flares Theatre B
06/03   Postponed  
13/03 Takayoshi Oba (Max Planck Institute for Solar System Research) Three-dimensional convective velocity fields in the solar photosphere Teams (Theatre B)
20/03 Daniel Johnson The Properties and Consequences of Thermal Conduction at X-Points Theatre B
27/03 Ross Pallister (Northumbria) Constraining the Properties of the Acceleration Region Plasma Environment with Solar Energetic Electrons Theatre B
03/04 Craig Stark (Glasgow) Substellar atmospheres: a laboratory for non-equilibrium plasmas Physics Theatre C
10/04 Mathew Owens (Reading) Space-weather forecasting: When less is more Theatre B
17/04 Lilli Nadol Analytical 3D MHS magnetic field line modelling Theatre B
24/04 Jonah Klowss The contribution of magnetic helicity condensation to ambient increase in the Solar Open Flux Theatre B
01/05 Thomas Neukirch Accelerated particle beams in a 3D simulation of the quiet Sun. Effects of advanced beam propagation modelling by Lars Frogner et al. Theatre B
08/05 Andy Wright Observations and Simulations of Resonant Alfven waves in 3D Theatre B
10/05 Harry Callingham The evolution of the coronal loop structure due to the phase mixing of Alfvén waves Theatre B
15/05 Sophie Boswell Kinetic Models of Solar Wind Current Sheets Theatre B
23/05 Ann Vaseekar Quantifying the Importance of an L4 or L5 Magnetograph for Modelling the Global Solar Magnetic Field Booth Lecture Theatre
(2 p.m.)
24/05 Anmol Kumar Behaviour of Alfvén Waves in a Solar Wind Background Theatre B
(2 p.m.)
19/06 Jordan Talbot (Northumbria)   Theatre B
MARTINMAS SEMESTER:   SEP – DEC 2023
07/09 Alexander Degeling
(Shandong University)
Chaos in Space! Surfing Electrons Wreak Havoc! Theatre B
13/09 Ruhann Steyn (Northumbria University) The connection between L1 solar wind observations and their solar sources during the 2008/2009 and 2019/2020 solar minima using the Fisk heliospheric magnetic field Theatre B
20/09 Mariana Andrea Cécere (Córdoba, Argentina) Numerical Study of Coronal Loop Oscillations: Triggers and Emission Theatre B
27/09 Valentin Aslanyan (Dundee) Interchange reconnection in the solar corona and how to observe it Theatre B
04/10   No seminar  
11/10   Staff Council  
18/10 Sargam Mulay (Glasgow) A detailed investigation of molecular hydrogen at three flare ribbons Theatre B
25/10 Oliver Rice (Durham) Solar Coronal Models and the Potential Prediction of Solar Eruptions Theatre B
01/11 Clare Parnell 3D Magnetic Reconnection: On the creation and significance of Cluster and Intercluster Separators Theatre B
08/11   No seminar  
15/11 Jack Reid Quantifying when and where strong magnetic skew forms in a data-driven global, non-potential model of the solar corona: the importance of when and where flux is observed to emerge and the limitations imposed by an Earth-bound field of view Theatre B
22/11 Jordi De Jonghe The Legolas code: features and applications Theatre B
29/11   Graduation  
06/12 Ravindra Desai (Warwick) Modelling extreme space weather events Theatre B
13/12 Alex Russell 3D vs. 2.5D Plasmoid-Mediated Reconnection: Reconnection Rates, Mean Fields and Wings Theatre B
14/12 Jaume Terradas (University of the Balearic Islands) 3D magnetohydrostatic models of coronal structures and their stability using Euler potentials Theatre B