Overview of the VBI observations (both blue and red) obtained by DKIST on 24 October 2022. The top row shows a plot of the solar atmosphere observed using the photospheric TiO (a; VBI-red) and G-band (b; VBI-blue) filters. The bottom row shows a plot of the solar atmosphere observed using the chromospheric H-alpha (c; VBI-red), H-beta (d; VBI-blue), and Ca II k (e; VBI-blue) filters. The H-alpha filter was found to be off-band for that period, and this is why the chromospheric features are more visible in H-beta than in H-alpha. The white dash line presented in the VBI-Red images (a,c) highlights the VBI-Blue.