| CANDLEMAS SEMESTER: JAN – MAY 2023
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| 18/01
| No seminar
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| 25/01
| Simon Daley-Yates (Astronomy Group, St Andrews)
| Stellar Prominences and the Mass-Loss of Cool Stars
| Theatre B
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| 01/02
| Tom Howson
| How does the Sun’s atmosphere respond to heating driven by random foot point driving?
| Theatre C (1 p.m.)
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| 08/02
| David MacTaggart (Glasgow)
| Magnetic helicity in multiply connected domains and the proof of Taylor’s conjecture
| Theatre B
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| 15/02
| No seminar
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| 22/02
| No seminar
| Staff Council
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| 01/03
| No seminar
| Spring Vacation
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| 08/03
| Harry Callingham
| The effect of evaporation on Alfvén wave phase mixing in coronal loops
| Theatre C (1.15 p.m.)
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| 15/03
| Kate Mowbray
| Particle Energisation in a 3D Collapsing Magnetic Trap Model With a Braking Jet
| Theatre B
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| 22/03
| Rachel Davies
| Alfvén-Fast Wave Coupling in a 2D Non-Uniform Medium
| Theatre B
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| 25/03
| Lilli Nadol
| Asymptotic Approximation for Magnetohydrostatic Equilibrium Solutions
| Theatre B
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| 05/04
| David Dritschel (Vortex Dynamics Group)
| Recent advances in the modelling of incompressible turbulent two and three-dimensional flows
| Theatre C
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| 12/04
| George Chouliaras
| Magnetic flux emergence: Effects of partial ionization
| Theatre B
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| 19/04
| Sam Skirvin (KU Leuven)
| Alfvénic motions arising from inclined wave drivers in coronal loops
| Theatre B
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| 26/04
| Daria Sorokina (KU Leuven)
| MHD modelling of helmet streamers and streamer waves
| Theatre B
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|
28/04 (**Friday**)
| Elisabeth Enerhaug
| Identifying MHD Wave Modes in the Solar Atmosphere
| Theatre B (also Applied Mathematics Seminar)
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| 03/05
| Jonah Klowss
| Investigating the contribution of magnetic helicity to the Solar Open flux
| Theatre B
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| 10/05
| Sophie Boswell
| Force-Free Collisionless Current Sheet Equilibria
| Theatre B
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| 17/05
| No seminar
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| 24/05
| Anmol Kumar
| Investigating Solar Wind Phenomena: Models, Observations and Acceleration Processes
| Theatre B (1 p.m.)
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| 31/05
| Jack Reid
| The coronal heating problem and (partial) solutions: self-consistent nanoflare heating
| Theatre B
|
| 07/06
| Ann Vaseekar
| Quantifying the Importance of an L5 Magnetograph for Modelling the Global Solar Magnetic Field
| Theatre B
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| MARTINMAS SEMESTER: SEP – DEC 2022
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| 14/09
| No seminar
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| 21/09
| No seminar
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| 28/09
| Alan Hood
| Coronal Heating at Null Points
| Theatre C
|
| 05/10
| Cosima Breu
| Nonthermal broadening of coronal lines in a 3D MHD loop model
| Theatre B (1.15 p.m.)
|
| 12/10
| Ineke De Moortel
| (When) Can wave heating balance optically thin radiative losses in the corona?
| Theatre A
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| 19/10
| No seminar
| Independent Learning Week
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|
| 26/10
| Raheem Beg (Dundee)
| Evolution, structure and topology of self-generated turbulent reconnection layers
| Theatre C
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| 02/11
| Racquel Mäusle (TU Berlin)
|
Topology-driven three-dimensional magnetic reconnection
| Online
|
| 09/11
| Paolo Pagano (Palermo)
| Modelling asymmetric nanojets in the solar corona
| Theatre B
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| 16/11
| Tom Elsden
| Some Problems in Magnetospheric Ultra Low Frequency Waves
| Theatre B
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| 23/11
| Duncan Mackay
| A Comparison of Global Magnetofrictional Simulations of the 2015 March 20 Solar Eclipse
| Theatre B
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| 30/11
| No seminar
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| 06/12
| No seminar
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