5798 20221025153319.0 https://doi.org/10.1007/s11207-022-02063-9 DOI SCART-2022-0070 West, M. J. A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument 2022 The Sun Watcher with Active Pixels and Image Processing (SWAP) instrument on- board ESA’s PRoject for On Board Autonomy 2 (PROBA2) has provided the first un- compressed, high-cadence, continuous, large field-of-view observations of the extended extreme-ultraviolet (EUV) corona for over a complete solar cycle. It has helped shape our understanding of this previously understudied region, and pioneered research into the mid- dle corona. In this article, we present a review of all publications that have utilized these observations to explore the extended EUV corona, highlighting the unique contributions made by SWAP. The review is broadly divided into three main sections of SWAP-based studies about: i) long-lived phenomena, such as streamers, pseudo-streamers, and coronal fans; ii) dynamic phenomena, such as eruptions, jets, EUV waves, and shocks; iii) coronal EUV emission generation. We also highlight SWAP’s imaging capabilities, techniques that have been applied to observations to enhance the off-limb observations and its legacy. STCE Sun corona SWAP Coronal mass ejections Instrumentation and data management Jets Prominences Seaton, D. B. D’Huys, E. Mierla, M. Laurenza, M. Meyer, K. A. Berghmans, D. Rachmeler, L. Rodriguez, L. Stegen, K. Solar Physics 297 2022 136 luciano.rodriguez@observatoire.be https://trebuchet.public.springernature.app/get_content/06f9b883-41cd-4e19-b891-c786f02b72e8 published in REFERD