Volatile emissions from the crater and flank

As a comparison to airborne infrared (IR) flux measurements, ground-based sampling of fumarole and soil gases was used to characterize the quiescent degassing of CO2 from Oldoinyo Lengai volcano. Aerial and ground-based measurements are in good agreement: -75% of the aerially measured CO2 flux at Lengai (0.05-0.06 x 1012 mol yr - or 6000-7200 tonnes CO2 d -1) can be attributed to seven large crater vents. In contrast to Etna and Vulcano Island, where 15-50% of the total CO2 flux emanates diffusely through the volcanic flanks, diffuse emissions were measured only within 500 m of the crater rim at Lengai, contributing < 2% of the total flux. The lack of extensive flank emissions may reflect the dimensions of the magma chamber and/or the lack of a shallow fluid flow system. Thermodynamic restoration of fumarole analyses shows that gases are the most CO2-rich and H20-poor reported for any volcano, containing 64-74% CO2, 24-34% H20, 0.88-1.0% H2, 0.1-0.4% CO and < 0.1% H2S, HC1, HF, and CH4. Volatile emissions of S, C1, and F at Oldoiyno Lengai are estimated as 4.5, 1.5, and 1.0 x 107 mol yr -, respectively. Accuracy of the airborne technique was also assessed by measuring the C emission rate from a coal-burning power plant. CO2 fluxes were measured within +10% near the plant; however, poor resolution at increased distances caused an underestimation of the flux by a factor of 2. The relatively large CO2 fluxes measured for alkaline volcanoes such as Oldoinyo Lengai or Etna may indicate that midplate volcanoes represent a large, yet relatively unknown, natural source of CO2.