Seminars 2018 – 2019

 

DATE SPEAKER TITLE ROOM
CANDLEMAS SEMESTER:   FEB – MAY 2019
06/02 Dr Petros Syntelis Connections between standard and blowout solar jets B
13/02 Dr Laura Hayes (Trinity College Dublin) Quasi-Periodic Pulsations in Solar Flares B
20/02 Miss Erin Goldstraw Evolution of footpoint driven coronal loops A
27/02 Dr Thomas Howson MHD Waves in a Braided Magnetic Field B
06/03 Mr Jack Reid Coronal energy release by MHD avalanches: Heating mechanisms and one-dimensional distributions C
20/03 Miss Teri Love Flare Ribbons – Detection and Feature Correlation B
27/03 Mr Daniel Chambers Magnetic reconnection at tilted 3d null points B
03/04 Mr Hendrik-Jan Van Damme Chromospheric evaporation due to phase mixing of Alfvén waves C
10/04 Dr Steph Yardley The Role of Bipole Helicity in the Solar Cycle A
17/04 Mr Alexander Prokopyszyn Phase Mixing of Partially Confined Alfvén Waves C
24/04 Miss Lianne Fyfe Establishing Observational Signatures from Coronal Braiding B
01/05 Mr Callum Fairbairn Eruptions and Flaring Activity in Quadrupolar Emerging Regions B
08/05 Mr Callan Noble The Distribution of Photospheric Magnetic Flux Features B
15/05 Dr Oliver Allanson (Reading) Electron diffusion in self-consistent numerical experiments due to whistler-mode wave-particle interactions B
MARTINMAS SEMESTER:   SEPT – DEC 2018
10/19 Dr James Threlfall Flux Rope Formation Due to Shearing and Zipper Reconnection B
17/10 Dr Craig Johnston Modelling the Transition Region & Thermal Non-Equilibrium in Coronal Loop Models A
24/10 Dr Paolo Pagano Predicting the onset of flux-rope ejections A
31/10 Dr Tom Elsden Fast Normal Modes and Field Line Resonances of a 3D Magnetospheric Waveguide A
07/11 Dr Hugh Hudson (Glasgow) The Non-Thermal Solar Corona B
14/11 Prof. Andrew Cameron (Astronomy Group, St Andrews) Three years of Sun-as-a-star radial velocities on the approach to solar minimum B
21/11 Dr David MacTaggart (Glasgow) Interpreting magnetic helicity flux in solar flux emergence B
28/11 Dr Patrick Antolin In Situ Generation of Transverse MHD Waves from Colliding Flows in the Solar Corona A