Mars open-atmosphere terraforming requires exaton-class volatile inventories and sustained multi-100 TW to PW power over centuries, whereas regional paraterraforming is plausible with near-term industry.
Because PFC warming does not directly provide buffer gas, it must be coupled to a separate pressure-building pathway to achieve E3/E4
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Terraforming Mars: Mass, Forcing, and Industrial Throughput Constraints
Mars open-atmosphere terraforming requires exaton-class volatile inventories and sustained multi-100 TW to PW power over centuries, whereas regional paraterraforming is plausible with near-term industry.