A multi-year record of airborne CO2 observations in the US Southern Great Plains.

We report on 10 yr of airborne measurements of atmospheric CO₂ mole fraction from continuous and flask systems, collected between 2002 and 2012 over the Atmospheric Radiation Measurement Program Climate Research Facility in the US Southern Great Plains (SGP). These observations were designed to quantify trends and variability in atmospheric mole fraction of CO₂ and other greenhouse gases with the precision and accuracy needed to evaluate ground-based and satellite-based column CO₂ estimates, test forward and inverse models, and help with the interpretation of ground-based CO₂ mole-fraction measurements. During flights, we measured CO₂ and meteorological data continuously and collected flasks for a rich suite of additional gases: CO₂, CO, CH₄, N₂O, ¹³CO₂, carbonyl sulfide (COS), and trace hydrocarbon species. These measurements were collected approximately twice per week by small aircraft (Cessna 172 initially, then Cessna 206) on a series of horizontal legs ranging in altitude from 460m to 5500ma.m.s.l. Since the beginning of the program, more than 400 continuous CO₂ vertical profiles have been collected (2007-2012), along with about 330 profiles from NOAA/ESRL 12-flask (2006-2012) and 284 from NOAA/ESRL 2-flask (2002- 2006) packages for carbon cycle gases and isotopes. Averaged over the entire record, there were no systematic differences between the continuous and flask CO₂ observations when they were sampling the same air, i.e., over the oneminute flask-sampling time. Using multiple technologies (a flask sampler and two continuous analyzers), we documented a mean difference of <0.2 ppm between instruments. However, flask data were not equivalent in all regards; horizontal variability in CO₂ mole fraction within the 5-10 min legs sometimes resulted in significant differences between flask and continuous measurement values for those legs, and the information contained in fine-scale variability about atmospheric transport was not captured by flask-based observations. The CO₂ mole fraction trend at 3000ma.m.s.l. was 1.91 ppm yr^-1 between 2008 and 2010, very close to the concurrent trend at Mauna Loa of 1.95 ppm yr^-1. The seasonal amplitude of CO₂ mole fraction in the free troposphere (FT) was half that in the planetary boundary layer (PBL) (∼15 ppm vs. ∼30 ppm) and twice that at Mauna Loa (approximately 8 ppm). The CO₂ horizontal variability was up to 10 ppm in the PBL and less than 1 ppm at the top of the vertical profiles in the FT. [ABSTRACT FROM AUTHOR]