Members

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

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 waves in the photosphere and chromosphere of the Sun.

Professor at Queen’s University Belfast, UK, working within the Solar Physics research group. He is predominantly interested in how the Sun’s energy travels through its atmosphere, both in the form of flares and waves.

Solar physicist at Queen’s University Belfast, UK. His work centres on the dynamics of small-scale magnetic elements. 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 Astrofísica 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, providing more boundary conditions for, e.g., 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 scientist at IRSOL (CH) and KIS (DE). 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.

Scientist at the University of Sheffield. He specialises in both the theory and observational interpretation of magnetohydrodynamic waves in the solar atmosphere, in both large-scale and small-scale magnetic structures.

PhD researcher at the Astrophysics Research Centre at Queen's University Belfast, UK. His research currently focuses on the energy potentially carried by observed transverse oscillations in spicules.

José Roberto Canivete Cuissa is a PhD student at the University of Zurich and IRSOL, Switzerland. His expertise lies in analysing, modelling, and solving complex physical systems from both analytical and numerical point of view.

Postdoctoral researcher at Rosseland Centre for Solar Physics, University of Oslo, Norway. His research focuses on study of MHD waves in small chromospheric (magnetic) structures from ALMA observations.

PhD researcher at Georgia State University, USA. Her research focuses on development of a He D3 Magneto-Optical Filter which will provide wavelength standard Doppler velocity and magnetic field measurements in the upper chromosphere.

Max Mcmurdo is a PhD researcher within the Plasma Dynamics Group at the University of Sheffield, working on problems related to the MHD wave propagation in the solar atmosphere.

Postdoctoral researcher at the Rosseland Centre for Solar Physics (ROCS) Norway. Her main interests are solar atmospheric heating, observations and simulations, plasma physics, magnetohydrodynamics, and radiative transfer.

Postdoctoral researcher at KU Leuven, Belgium, working on observational, numerical and analytical studies of the Kelvin-Helmholtz and Rayleigh-Taylor in solar plasma.