Members

Project Scientist at the High Altitude Observatory of the National Center for Atmospheric Research, in Colorado (USA). Her main scientific interest lies in the field of Solar Spectropolarimetry for remote sensing of magnetic fields on the Sun.

ESA Project Scientist for SOHO, Hinode, and IRIS, based at NASA Goddard Space Flight Center near Washington, DC, USA. His research interests include wave-propagation characteristics of gravity waves and high-frequency acoustic waves in the photosphere and chromosphere of the Sun.

Researcher at Rosseland Centre for Solar Physics (RoCS), University of Oslo, Norway. His studies concern the lower-to-mid atmosphere of the Sun, regarding how magnetic fields structure dynamics of those layers. He is predominantly interested in wave activity in the lower solar atmosphere.

Solar physicist at Queen’s University Belfast, UK. His work predominantly explores the lower atmosphere of the Sun, with an emphasis placed on understanding energy flow through the turbulent and dynamic layers of the photosphere and chromosphere in the form of MHD waves.

Solar physicist at Queen’s University Belfast, UK. His work centres on the dynamics of small-scale magnetic elements that are ubiquitous across the solar disc. His work on these elements follows their evolution and formation, as well as waves that are found to propagate along them.

Research scientist at the Instituto de Astrofisica de Canarias (IAC, Spain). She has mostly been working in the field of Solar Physics, MHD wave theory, theory of partially ionized plasmas, quiet Sun magnetic fields, and spectropolarimetry.

Senior Lecturer at Northumbria University, UK. He currently leads a small research group who are motivated to understand the role magnetohydrodynamic waves play in transferring energy around the Sun’s atmosphere.

Astronomer at Stanford University, USA, researching the Sun’s magnetic fields. Her interests are observational and include both the short and long time scales of solar magnetism, i.e., MHD waves and the solar dynamo.

Lecturer at University of Newcastle, Australia. As a helioseismologist, her research includes the coupling of the photospheric magnetic field to the subsurface layers, which will provide more boundary conditions for solar dynamo and solar flux emergence models.

Researcher at ASI (Italian Space Agency). His interests are primarily the study of MHD waves, through the analysis of high spatial resolution spectropolarimetric data, and the development of new high resolution instrumentation.

Senior researcher at the Leibniz Institute for Solar Physics, KIS (DE) and at IRSOL (CH). His research includes numerical experiments of wave propagation and conversion for the interpretation and prediction of observable signals of wave activities in the solar atmosphere.

He specialises in both the theory and observational interpretation of magnetohydrodynamic waves in the solar atmosphere, in both large-scale (e.g., sunspots and pores) and small-scale (e.g., spicules and chromospheric fibrils) magnetic structures.

Postdoctoral researcher at Max Planck Institute for Solar System Research, Germany. His research particularly focuses on internal gravity waves in the lower solar atmosphere.

Postdoctoral researcher at the Rosseland Centre for Solar Physics, RoCS, at the University of Oslo, Norway. Her main interests are solar atmospheric heating, observations and simulations, plasma physics, magnetohydrodynamics, and radiative transfer.

PhD researcher at the Plasma Dynamics Group at the University of Sheffield, UK, working on observational, numerical and analytical studies of the Kelvin-Helmholtz and Rayleigh-Taylor in solar plasma.