Authors: M. Galloy (NSF - NCAR/HAO/MLSO), G. de Toma (NSF - NCAR/HAO/MLSO), J. Burkepile (NSF - NCAR/HAO/MLSO), D. Kolinski (NSF - NCAR/HAO/MLSO), S. Tomczyk (Solar Scientific LLC)

There are new products being released for both of the Mauna Loa Solar Observatory’s currently observing instruments, COSMO K-Coronagraph (K-Cor) and Upgraded Coronal Multi-Polarimeter (UCoMP). Development for creation of density images for UCoMP is complete. Several K-Cor products including enhanced pB (unsharp mask for improved sharpness in quicklook and FITS images), synoptic maps at more heights, and difference images at a faster 30 second cadence are already available on the MLSO website. The UCoMP density product will be released for 2024 and 2025 data shortly and all products will be available for the rest of their respective missions after recalibrating both of these missions, which is scheduled for the summer/fall of 2025. Additional analysis of CME fronts from the real-time CME alerts for K-Cor will be provided when MLSO re-opens. MLSO data, starting with K-Cor and UCoMP and expanding to older instruments, will be available via a web API later this summer and fall. Clients for command line usage as well as various programming languages will be provided with plans to integrate into other data providing services. We will report on the newest developments on an expected re-opening of the road to MLSO, and continued daily observations, scheduled for this fall.