Comparative Analysis of the Methane Data Products from the Tropospheric Emission Spectrometer and the Atmospheric Infrared Sounder.

Methane is the second most powerful greenhouse gas with a highly positive radiative forcing of 0.48 W/m2 (IPCC 2013). Global concentrations of methane have been steadily increasing since 2007 (Bruhwiler 2014), raising concerns about methane's impact on the future global climate. For about the last decade, the Tropospheric Emission Spectrometer (TES) on the Earth Observing System (EOS) Aura spacecraft has been detecting several trace gas species in the troposphere including methane. The goal of this study is to compare TES methane products to that of the Atmospheric Infrared Sounder (AIRS) on the EOS Aqua spacecraft so that scientific investigations may be transferred from TES to AIRS. The two instruments fly in the afternoon constellations (A-Train), providing numerous coincident measurements for comparison. In addition, they also have a similar spectral range, (3.3 to 15.4 µm) for TES (Beer, 2006) and (3.7 to 15.4 µm) for AIRS (Chahine, 2006), making both satellites sensitive to the mid and upper troposphere. This makes them ideal candidates to compare methane data products. In a previous study, total column methane was mapped and global zonal averages were compared. It was found that bias of the total column measurements between the two sounders was about constant over tropical and subtropical regions. However, because AIRS spectral resolution is lower than that of the TES, it is important to analyze the difference in vertical sensitivity. In this study, we will construct vertical profiles of methane concentration and compare them statistically through RMS difference and bias to better understand these differences. In addition, we will compare the error profile and total column errors of the TES and AIRS methane from the data to better understand error characteristics of the products.