Speaker
Li Feng
Description
We summarize our science preparations for the Lyman-alpha Solar Telescope (LST) aboard the Chinese ASO-S mission. LST has the capability to simultaneously observe the Sun from the solar disk to 2.5 solar radii in both Lyman-alpha and visible light. Our particular interests are CMEs, flares, and prominences in the new Lyman-alpha waveband. We Synthesize these eruptive features in Lyman-alpha based on various numerical simulations concerning both optically thin and thick regimes. Their statistical and case studies based on Lyman-alpha measurements from GOES/EUVS, SOHO/UVCS and so on are also included to reveal flare and CME properties and develop physical diagnostic tools. The synergy with Solar Orbiter/Metis and EUI are discussed as well.
Primary authors
Li Feng
Hui Li
(Purple Mountain Observatory, CAS, China)
Ying Li
(Purple Mountain Observatory, CAS, China)
LST Team
(Purple Mountain Observatory, CAS, China)
