Speaker
Description
The seeing-free, multi-line, high-cadence observations delivered by Sunrise III provide a uniquely powerful new framework for studying waves and oscillations in the lower solar atmosphere. In this talk, I will present first results from our early-science investigations of active-region targets in the 327–329 nm near-UV window observed by SUSI, including line-dependent frequency structuring in a sunspot umbra, the spatial redistribution of oscillatory power across a magnetically diverse sunspot–plage–pore system, and MHD wave-mode identification and propagation in a pore. I will also discuss broader science opportunities enabled by the Sunrise III datasets, including current and future studies of wave propagation, mode conversion, magnetic structuring, and multi-height coupling in the lower solar atmosphere, particularly when the three Sunrise III science instruments are used together to provide broader coverage across atmospheric heights and diagnostics.