TRACE-P OH and HO2 measurements with the Airborne Tropospheric Hydrogen Oxides Sensor
(ATHOS) on the DC-8

 

Principal Investigator: William H. Brune, Pennsylvania State University, University Park, PA
Co-Investigators: Monica Martinez-Harder, Hartwig Harder

 

                The Airborne Tropospheric Hydrogen Oxides Sensor (ATHOS) measures OH and HO2 from the NASA DC-8. This instrument detects OH by laser induced fluorescence (LIF) in detection chambers at low pressure and detects HO2 by chemical conversion with NO followed by LIF detection. The demonstrated detection limit (S/N=2, 5 min.) for OH is about 0.005 pptv (1X105 cm-3 at 2 km altitude) and for HO2 is 0.05 pptv (1X106 cm-3 at 2 km altitude). We will use ATHOS to measure OH, HO2, and HO2/OH during TRACE-P, analyze these results by comparing them against fundamental relationships and computer models, and publish the analyses. As participants in a tower-based study this summer, we are developing an attachment to ATHOS to detect RO2+ HO2-.  It may be tested well enough to include as an attachment for TRACE-P.  TRACE-P HO, measurements will help develop a clearer picture of the atmospheric oxidation and O3 production that occur as Asian pollution spreads across the Pacific Ocean.

                We anticipate both new results and confirmation of previous results. Besides contributing to the science goals outlined in the TRACE-P NRA, HOx, measurements will be combined with simultaneous measurements of environmental factors and other chemical species to test the following hypotheses:

                  Testing these hypotheses relies heavily on the simultaneous measurements of HOx, all the chemical species that interact with HOx, and the environmental conditions, particularly the photolysis frequencies. It is important to obtain this entire measurement suite from the planetary boundary layer to the ceiling of the DC-8 at 12 km, as well as in the presence of clouds and heavy pollution nearer the Asian coast. Measurements while flying out of and into airports are important photochemical kinetics tests because of the different amounts of NO that are mixed into the continental air. In addition, measurements must be made at different times of the day and night.

                TRACE-P will add to a growing body of HO. data that we have collected with ATHOS and GTHOS, the towered-based configuration of ATHOS that we use for near-surface studies. ATHOS has participated in SUCCESS (1996), SONEX (1997), PEM Tropics B (1999), and SOLVE (1999-2000). GTHOS has participated in PROPHET, at a semi-rural heavily forested site in northern lower Michigan in summer, 1998 and in Nashville SOS, in the urban plume of Nashville in summer, 1999. These measurements are giving us a view of HO. photochemistry for a wide range of HOx sources, NOx levels, and hydrocarbon loadings. TRACE-P allows us to sample the influence of urban-level, processed pollution on a low-hydrocarbon, pristine environment, a condition that we have not previously studied extensively.

                An exciting aspect of TRACE-P is the connection between the aircraft and satellite observations. While instruments on the Terra and ENVISAT satellites cannot measure OH and HO2, they can measure chemical species that have great influence on HOx, such as CO, O3, and NO2 (a measure of NO). By comparing the satellite and aircraft measurements for a wide range of environments, we should be able to construct parameterizations of atmospheric oxidation and ozone production.