Synergy Science with DKIST and Solar-C_EUVST

The US National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) is nearing completion on the Hawaiian island of Maui: integration of the instruments into the facility has already begun, and science operations will soon commence. With a 4 meter unobscured primary mirror, DKIST will be by far the largest solar telescope in the world, affording substantial increases in spatial and temporal resolution over current solar instrumentation. Just as important, its suite of five first-light instruments will provide highly configurable sets of precision multi-spectral, polarimetric, and imaging data, from optical to infrared wavelengths, and allow for both on-disk and off-limb (coronal) observations.

The broad range of spectroscopic UV and EUV data from Solar-C_EUVST, combined with the extensive capabilities of the DKIST instrumentation suite, will allow for very versatile scientific investigations. In this talk, I will provide an overview of DKIST capabilities and highlight some of the new science that will be made possible by combining photospheric, chromospheric, and coronal magnetometry at DKIST and multi--wavelength spectroscopic observations from EUVST.