Parallel sessions

This cross-disciplinary session aims to bring together MHD waves experts from both solar and planetary physics. The goal is to encourage the transfer of knowledge between research fields that share areas of commonality but often remain disparate. For example, field line resonance in magnetospheres and resonant absorption in the solar corona; the Kelvin Helmholtz instability on the magnetospheric flanks and in coronal loops. We invite submissions from multiple areas of MHD wave research, from solar to planetary magnetospheres, including theoretical/numerical studies or observational studies from spacecraft or ground-based data. This session aims to bring together these research elements, including the potential of data from upcoming missions.