Deadline: 8th April
Session: MHD Wave Coupling From Photosphere To Corona
MHD waves have been a staple topic of UK solar physics research over the
past few decades. The main reason for this sustained interest is their almost
constant and ubiquitous presence throughout the solar atmosphere, having now been observed in structures ranging from resolution-limited, small-scale spicules to large-scale sunspots. This abundance of MHD waves suggests that they could play a key role in providing non-thermal energy from the relatively cool solar photosphere (~6000 K) to the hot corona. This session aims to highlight the breadth of research being undertaken into solar MHD waves from across the country.
Abstract submission, with no registration required, can be found at: https://nam2016.org
Chris Nelson, Rick Morton, James McLaughlin, Mihalis Mathioudakis