Coronal Science from TRACE

Leon Golub
Harvard-Smithsonian Center for Astrophysics

The TRACE satellite is providing continuous viewing of the solar corona
with unprecedented spatial and temporal resolution. We will present an
overview of the contributions made by TRACE to the study of coronal
structure, stability and dynamics, with particular emphasis on studies
of CMEs and flares. We conclude with a discussion of the limits of the
instrumental methods and future observations