Routine gas flaring wastes an estimated 140 billion cubic metres of natural gas per year and emits hundreds of millions of tonnes of CO₂ and methane equivalents globally. National regulators and finance ministries rarely have an independent view of what is actually burning at remote upstream sites—they depend entirely on operator self-reporting, which carries obvious incentive to understate. Without sovereign satellite coverage, a government cannot distinguish a brief, legally sanctioned pressure-relief flare from weeks of continuous unreported combustion.
Shortwave-infrared (SWIR) sensors in the 1.6 µm and 2.2 µm bands cut through daytime solar glare and night-time darkness to resolve individual flare stacks and quantify radiant heat flux. Paired with a thermal infrared (TIR) channel at 3.9 µm, the constellation can estimate flame temperature and combustion efficiency, separating clean burns from smoky, methane-rich incomplete combustion events. A 16-satellite walker constellation at 550 km revisits any point on the equator every 2–3 hours—sufficient to catch episodic flares that disappear before the next Landsat or Sentinel overpass.
The operational output is a continuously updated national flare registry: every detected event geo-tagged, timed and attributed to a licensed block or operator, with radiant power converted to estimated gas volume via published combustion models. Regulators can issue penalty notices backed by independent satellite evidence; the ministry of finance gains a cross-check on royalty declarations; and international climate negotiators arrive at COP with audited national flaring totals rather than contested estimates. Renting this from a commercial provider means the evidence chain is controlled offshore—inadmissible in some jurisdictions and subject to vendor data-access policies the sovereign has no power to alter.