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  • NAM 2022
    • Code of Conduct
    • COVID-19 Policy
    • Registration
    • Grants & Bursaries
    • Contacts
    • Exhibitors
    • News Archive
    • Hybrid Option
    • Conference Brochure
  • Science
    • Block Schedule
    • Parallel Sessions
    • Plenary Talks
    • Community Session
    • Special Lunches
    • Guides to NAM2022
  • Social
    • What's On?
    • Welcome Reception
    • RAS Awards Dinner
    • NAM Football
    • RAS Quilt
    • Kenilworth Castle Trip
  • Media
  • Outreach
    • SUN at NAM
    • SUN Outreach Programme
    • Art Exhibition
      • Virtual Art Exhibition
    • Art submission
    • Science Festival
    • First JWST Images
  • Warwick
    • Travel
    • Accommodation
    • Local Area
    • Campus
    • Childcare

 All attendees are expected to show respect and courtesy to other attendees and staff, and to adhere to the NAM Code of Conduct.

Parallel sessions

Sessions

id
date time
2022-03-08 11:44:00
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 IƱigo 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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