BEGIN:VCALENDAR
VERSION:2.0
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X-PUBLISHED-TTL:PT15MIN
METHOD:PUBLISH
X-WR-CALNAME:Maths & Stats: Geophysical and Astrophysical Fluid Dynamics Seminar
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11484@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251015T140000Z
DTEND:20251015T150000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Physics-based models for large-eddy simulations of (un)steady magnetohydrodynamic turbulence - Asif Nawaz (University of Edinburgh)
DESCRIPTION:Abstract: For Navier-Stokes turbulence\, contributions to the energy cascade from e.g. vortex stretching can be identified by an exact decomposition of the energy flux. This results in a quantification of the relative contributions of such effects to the kinetic energy cascade by direct numerical simulation\, and provides guidance for physics-informed LES...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11484
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11521@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251022T140000Z
DTEND:20251022T150000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Exploring 3D reconnection in the context of solar flares - Satyam Agarwal (The University of Alabama in Huntsville)
DESCRIPTION:Abstract: Solar flares are believed to be the manifestations of the magnetic reconnection process. The primary effects of reconnection are the dissipation of magnetic energy\, its conversion to kinetic energy\, and changes in the magnetic topology. We investigated various aspects of 3D reconnection in the context of solar flares. First\, we...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11521
LOCATION:Maths 311B
SEQUENCE:5
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11526@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251112T150000Z
DTEND:20251112T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: On the role of resonant absorption in the electromotive force of dynamic dynamos - Mattias Brynjell-Rahkola (University of Cambridge)
DESCRIPTION:Abstract: Large-scale dynamos refer to processes in which a magnetic field is generated and maintained on the system scale by fluid motion. The common prototype for such dynamos is the alpha-Omega dynamo\, in which a toroidal field is induced from a weak poloidal field by differential rotation\, and the electromotive force...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11526
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11520@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251119T150000Z
DTEND:20251119T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Solar Wind-Magnetosphere-Ionosphere coupling in terms of Geomagnetically Induced Currents Hazard: The MA.I.GIC. model - Mirko Piersanti (University of L&#039\\;Aquila)
DESCRIPTION:Abstract: The impact of the interplanetary shock and of the Coronal Mass Ejections (CMEs) on the Earth’s magnetosphere perturbs the geomagnetic field causing the occurrence of geomagnetic storms. Such extremely variable geomagnetic fields trigger geomagnetic effects measurable not only in the geospace but also in the ionosphere and at the...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11520
LOCATION:Maths 311B
SEQUENCE:5
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11571@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251126T150000Z
DTEND:20251126T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: A theory of magnetic field line slippage - David MacTaggart (University of Glasgow)
DESCRIPTION:Abstract: Magnetic reconnection is a fundamental property of plasmas with many applications. The theoretical treatment of magnetic reconnection in three dimensions has mainly focussed on two aspects: (1) the possible locations of reconnection via studies of magnetic topology (e.g. magnetic skeletons and quasi-separatrix layers) and (2) the rate of change...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11571
LOCATION:Maths 311B
SEQUENCE:2
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11519@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251203T150000Z
DTEND:20251203T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Theory and Modelling of Large Scale Plasmapause Surface Waves - Tom Elsden (University of St. Andrews)
DESCRIPTION:Abstract: This talk will be in the realm of MHD waves in Earth's magnetosphere. MHD waves manifest in the magnetosphere as so called ultra-low frequency (ULF) waves\, with periods in the range from a few seconds to a few minutes. They represent large scale plasma/magnetic field oscillations\, often on the scale...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11519
LOCATION:Maths 311B
SEQUENCE:2
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11551@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251210T150000Z
DTEND:20251210T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Towards a diffusion-free regime in models of stellar and planetary convection: theory and simulations - Laura Currie (University of Durham)
DESCRIPTION:Abstract: The evolution of stars and planets is governed by turbulent flows in their interiors\, which transport heat and generate magnetic fields. These flows are often convective\, and their dynamics are strongly influenced by rotation and density stratification. Modelling such convection remains a central challenge in astrophysics due to the...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11551
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11561@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20251217T150000Z
DTEND:20251217T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: From Convection Zone to the Corona: Current efforts and future plans - Valentin Aslanyan (University of Glasgow)
DESCRIPTION:More information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11561
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11609@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260121T150000Z
DTEND:20260121T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Mean field responses in disordered systems: an example from nonlinear MHD - David Hughes (University of Leeds)
DESCRIPTION:Abstract: Understanding the generation of large-scale magnetic fields and flows in MHD turbulence remains one of the most challenging problems in astrophysical fluid dynamics. The well-studied kinematic theory ignores the possibility of small-scale dynamo action\, which is prevalent at high magnetic Reynolds number. Here\, we thus examine the possibility of large-scale...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11609
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11610@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260218T150000Z
DTEND:20260218T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Rapidly Rotating Magnetohydrodynamics and the Geodynamo - Emmanuel Dormy (PSL)
DESCRIPTION:Abstract: The problem of the Geodynamo is simple to formulate (Why does the Earth possess a magnetic field?)\, yet it proves surprisingly hard to address. As with most geophysical flows\, the fluid flow of molten iron in the Earth's core is strongly influenced by the Coriolis effect. Because the liquid...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11610
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11645@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260311T150000Z
DTEND:20260311T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: On Geometric and Dynamical Relationships Between Quasi-Separatrix Layers and Field Line Slippage - Thomas Chan (University of Glasgow)
DESCRIPTION:Abstract: Magnetic reconnection is a fundamental process that underpins many dynamical processes in the solar corona. A lot of research revolves around the location of reconnection in coronal active regions\, and in 3D magnetic field configurations\, one often uses magnetic topology to determine these regions\, which require information along field...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11645
LOCATION:Maths 311B
SEQUENCE:2
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11646@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260311T150000Z
DTEND:20260311T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Dayside and Nightside Coupling in the Dungey Cycle Revealed from Slippage in an Empirical Magnetospheric Model - Matthew Brown (University of Glasgow)
DESCRIPTION:Abstract: The Dungey Cycle is a large-scale circulation of plasma and magnetic flux in the magnetosphere\, propelled by magnetic reconnection. This phenomenon occurs when interplanetary coronal mass ejections (ICMEs) enter the Earth's magnetosphere\, compressing it\, and subsequently driving the Dungey Cycle through reconnection. In this study\, an empirical magnetosphere...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11646
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11611@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260318T150000Z
DTEND:20260318T160000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Neutron star cores: normal matter and superconductivity - Andrei Igoshev (Newcastle University)
DESCRIPTION:Abstract: Neutron stars have the strongest magnetic fields in the Universe reaching 1e15 G. Magnetic field evolution in neutron star cores is not fully explored. Researchers still do not agree on whether neutron star cores are magnetised or whether the magnetic field is expelled very early from the cores.  According...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11611
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11614@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260408T140000Z
DTEND:20260408T150000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: Observing magnetised\, collisionless shocks using laser-driven platforms - Ellie Tubman (UC Berkley)
DESCRIPTION:Abstract: Magnetized\, collisionless (λmfp>> Lshock) shocks are observed throughout the universe including within supernova remnants and at Earth’s magnetopause. These shocks have the potential to accelerate particles to far greater energies than many other astrophysical processes and may provide a source of high-energy cosmic rays. One challenge\, yet to be...\N\NMore information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11614
LOCATION:Maths 311B
SEQUENCE:3
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11651@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260415T140000Z
DTEND:20260415T150000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: TBC - Francis Swan (University of Glasgow)
DESCRIPTION:More information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11651
LOCATION:Maths 311B
SEQUENCE:2
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
BEGIN:VEVENT
UID:GLW_UNI_MS_WEBEVT_11652@maths-stats.gla.ac.uk
DTSTAMP:19700101T000000Z
DTSTART:20260415T140000Z
DTEND:20260415T150000Z
SUMMARY:Geophysical and Astrophysical Fluid Dynamics Seminar: TBC - Sage Stanish (University of Glasgow)
DESCRIPTION:More information: http://www.gla.ac.uk/schools/mathematicsstatistics/events/details/?id=11652
LOCATION:Maths 311B
SEQUENCE:2
STATUS:CONFIRMED
CLASS:PUBLIC
END:VEVENT
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