IN21A-1684
Re-processing TOMS UV Measurements to Retrieve SO2 Emissions From Volcanic Eruptions

Tuesday, 15 December 2015
Poster Hall (Moscone South)
Bradford L Fisher1, Nickolay Anatoly Krotkov2, Pawan K Bhartia2, Can Li3, David P Haffner1, Peter Leonard4, Simon A Carn5 and Jennifer W Telling5, (1)Science Systems and Applications, Inc., Lanham, MD, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)University of Maryland College Park, College Park, MD, United States, (4)ADNET Systems, Inc., Lanham, MD, United States, (5)Michigan Technological University, Houghton, MI, United States
Abstract:
The SO2 Monitoring Group at the NASA Goddard Space Flight Center is producing a new multi-satellite long term data set of volcanic SO2 column amounts and heights (MSVOLSO2L4) as part of the NASA MEaSUREs Program. Here we present re-analysis of the UV measurements (BUV) from the NASA Nimbus 7 Total Ozone Mapping Spectrometer (N7 TOMS: 1978-1993). Ozone is the dominant atmospheric absorber in the BUV spectrum, but volcanic eruptions can produce enough SO2 to be distinguished from ozone background. Quantitative retrieval of volcanic SO2 requires:
1) Separation of the O3 and SO2 absorption in BUV radiances;
2) Close to zero mean SO2 background;
3) RT forward model that accounts for the presence of volcanic ash in the plume;
4) A priori knowledge of the ozone and SO2 vertical profiles.
Our iterative retrieval algorithm returns O3 and SO2 column amounts, effective reflectivity and its spectral slope. The retrieval model also generates a 4 x 4 gain matrix for the SO2 free regions that is used to soft calibrate the measured 340 nm BUV radiance. The spectral slope implicitly accounts for the interference of volcanic ash, but more explicit ash treatment is required to better quantify SO2 errors in volcanic plumes heavily loaded with ash. This presentation will discuss the methods used to characterize the error sources and assess the quality of this unique long-term SO2 data set.