Authors: Dimitris Vassiliadis (S Tech)

Coronal imagery from the Sun-Earth line provides reference information for many other types of solar atmospheric observations and in situ measurements. A new source of for white-light coronal observations is the Compact Coronagraph 1 (CCOR-1) which was launched on board GOES-19 in June 2024 and was placed in geostationary Earth orbit (GEO). CCOR-1 has provided a large number of coronal mass ejections, helmet streamers, pseudostreamers, and other coronal structures. Instrument specifications (FOV of 3.7-17 R_Sun, angular resolution of 50 arcsec, cadence of 15 min, etc.), algorithm theoretical basis documents (ATBDs), Product User Guides (PUGs), and other information are publicly available and will be reviewed in the presentation together with open-access sites. The CCOR-1 instrument will provide a continuation of several functions of LASCO C2 and C3. It is expected to be used in synergy with other solar viewing instruments from space- and ground-based platforms. I will review the access to data at the Space Weather Prediction Center (SWPC), the National Centers for Environmental Information (NCEI), and other open-source sites.