Parallel sessions
Sessions
Magnetohydrodynamic Waves and Instabilities in the Solar Atmosphere in the High-Resolution Era
Vast amounts of data from high-resolution instrumentation such as the space-borne SDO/AIA or the ground-based SST have allowed the study of MHD waves in the solar atmosphere to flourish. Such waves can be both localised (e.g., oscillating coronal loops) and global (e.g. Moreton waves) and can transport significant amounts of energy across the solar atmosphere meaning they may be of crucial importance for atmospheric heating. In this session, recent advances in the field of MHD waves (both observationally and theoretically) will be discussed and future avenues of study will be put forward in light of upcoming facilities such as DKIST.
C. Nelson, J. Liu, R. Erdélyi, M. Mathioudakis
Monday PM2
Cavendish LT
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