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Parallel sessions
Sessions
UK Solar Physics Open Session
Solar5
The activity of our nearest star, the Sun, drives variability within the heliosphere in a myriad of different ways, impacting the Earth and other planets. As the only star on which we can begin to resolve physical processes at their intrinsic scales the Sun provides a unique laboratory for plasma astrophysics. In this session we welcome all contributions describing advances relating to physical processes occurring from the interior to the outer atmosphere, based on space- or ground-based observations, simulations or theory. In particular the UKSP open session seeks to promote opportunities for early career researchers to present their work.
Sarah Matthews, Natasha Jeffrey, Eamon Scullion, Anne-Marie Broomhall, Andrew Hillier, Marianna Korsos, Ryan Campbell, Jiajia Liu
Mon 09:00-10:30 / Mon 14:30-16:00
09:00-09:15 Aaron William Peat: MgII h&k Prominence Modelling and Observations
09:15-09:30 Alessandra Giunta: Abundance diagnostics in active regions with Solar Orbiter/SPICE
09:30-09:45 Iñigo Arregui: A probability distribution for the amplitude of Solar Cycle 25
09:45-10:00 Rachel Howe: How Repeatable Is the Solar Cycle? Information from Helioseismic Diagnostics
10:00-10:15 Yajie Chen: Forward Modeling of Solar Coronal Magnetic-field Measurements Based on a Magnetic-field-induced Transition in Fe X
10.15-10.30: Discussion
14:30-14:45 Tishtrya Mehta: An investigation into the prevalence of period drift in Quasi-Periodic Pulsations in solar flares over Cycle 24
14:45-15:00 Morgan Stores: X-ray Diagnostics of Spatially Extended Turbulent Electron Acceleration and Transport in Solar Flares
15:00-15:15 Timo Laitinen: Solar Energetic Particle onsets in interplanetary space: Effect of turbulent field lines
15:15-15:30 Camille Yasmina Lorfing: The transport of accelerated electron beams in the inner heliosphere
15:30-15:45 Xingyao Chen: Type III solar radio bursts observed by LOFAR and their interpretation of Radio-wave propagations
15:45-16:00 Simon Opie: Kinetic scale instabilities in small scale turbulence observed by Solar Orbiter
09:00-09:15 Aaron William Peat: MgII h&k Prominence Modelling and Observations
09:15-09:30 Alessandra Giunta: Abundance diagnostics in active regions with Solar Orbiter/SPICE
09:30-09:45 Iñigo Arregui: A probability distribution for the amplitude of Solar Cycle 25
09:45-10:00 Rachel Howe: How Repeatable Is the Solar Cycle? Information from Helioseismic Diagnostics
10:00-10:15 Yajie Chen: Forward Modeling of Solar Coronal Magnetic-field Measurements Based on a Magnetic-field-induced Transition in Fe X
10.15-10.30: Discussion
14:30-14:45 Tishtrya Mehta: An investigation into the prevalence of period drift in Quasi-Periodic Pulsations in solar flares over Cycle 24
14:45-15:00 Morgan Stores: X-ray Diagnostics of Spatially Extended Turbulent Electron Acceleration and Transport in Solar Flares
15:00-15:15 Timo Laitinen: Solar Energetic Particle onsets in interplanetary space: Effect of turbulent field lines
15:15-15:30 Camille Yasmina Lorfing: The transport of accelerated electron beams in the inner heliosphere
15:30-15:45 Xingyao Chen: Type III solar radio bursts observed by LOFAR and their interpretation of Radio-wave propagations
15:45-16:00 Simon Opie: Kinetic scale instabilities in small scale turbulence observed by Solar Orbiter
Social Sciences S0.20
Social Sciences S0.20
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