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High-resolution imaging of supermassive black holes is now possible, with newapplications to testing general relativity and horizon-scale accretion andrelativistic jet formation processes. Over the coming decade, the EHT willpropose to add new strategically placed VLBI elements operating at 1.3mm and0.87mm wavelength. In parallel, development of next-generation backendinstrumentation, coupled with high throughput correlation architectures, willboost sensitivity, allowing the new stations to be of modest collecting areawhile still improving imaging fidelity and angular resolution. The goal ofthese efforts is to move from imaging static horizon scale structure to dynamicreconstructions that capture the processes of accretion and jet launching innear real time.

Studying Black Holes on Horizon Scales with VLBI Ground Arrays