Waves and Oscillations in the Solar Atmosphere in the High-Resolution Era
Solar Waves
High-resolution instrumentation such as the space-borne SDO/AIA, IRIS, Parker Solar Probe, and the forthcoming Solar Orbiter missions, or the ground-based SST, GREGOR, and BBSO, along with the imminent commencing of the highest ever resolution, 4-meter-aperture solar telescope DKIST enables researchers to gain insight into MHD wave processes in the solar atmosphere with an unprecedented spatial, temporal and spectral resolution. MHD waves and oscillations are widely used for plasma diagnostics and for confirming or refuting plasma heating theories developed by modellers. Bringing together theoretical (including analytical and numerical approaches) and observational aspects, in this session, recent advances in the field of MHD waves and oscillations will be discussed, and future avenues of study will be put forward in light of the ultra-high resolution on our doorsteps. In particular, but not exclusively, the focus will be on popular wave and oscillation topics that have made major steps aided with such a superb instrumental suit in solar magneto-seismology, in areas of MHD wave coupling and wave dynamics in the solar atmosphere.
Schedule:
Session 1
09:00 Dipankar Banerjee “Wave studies from the Forthcoming Aditya L1 mission”
09:18 Dominik Utz “MBPs, waves, and the heating and structuring of the higher solar atmosphere”
09:30 Valeria Sieyra “Observational and numerical characterization of a wave-like front propagating along pseudo-open field lines above an active region”
09:42 Abhinav Prasad “Standing MHD Waves in Magnetic Annulus Flux Tube Model”
09:54 Dmitrii Kolotkov “Time signatures of fast magnetoacoustic wave trains: from tadpoles to boomerangs”
10:06 Philippa Browning “Waves and oscillations generated by magnetic reconnection in solar flares”
10:18 Krishna Prasad Sayamanthula “Compressive plasma oscillations in hot coronal loops”
Session 2
15:30 Marco Stangalini “Identification of wave modes in the lower solar atmosphere through spectropolarimetry”
15:42 Chris Nelson “Oscillations in the line-of-sight magnetic field strength in a solar pore”
15:54 Chloe Sumner “Impact of plasma inflow on magnetic twist evolution along axisymmetric flux tubes”
16:06 Matthias Waidele “Absorption of high frequency oscillations and its relation to emissivity reduction”
16:18 David Millar “The effect of a solar flare on chromospheric oscillations”
16:30 Juan Maldonado “Direct observational indications of wavelike disturbances in MBP tracks”
16:42 Piyali Chatterjee “Modeling the solar spicule forest and the coronal swirls”
Noemi Kinga Zsamberger, Anne-Marie Broomhall, David Kuridze, Robertus Erdelyi
Wednesday morning and late afternoon
All attendees are expected to show respect and courtesy to other attendees and staff, and to adhere to the NAM Code of Conduct.