1,198 publications from this institution
Abstract. Gas phase HCl was measured from the marine boundary layer (MBL) to the lower stratosphere from the NASA DC-8 during five science flights (41 h) of the Intercontinental Chemical Transport Experiment-Phase B (INTEX-B) field campaign. In the upper troposphere/lower stratosphere (UT/LS, 8–12 km) HCl was observed to range from a few tens to 100 pptv due to stratospheric influence with a background tropospheric level of less than 2 pptv. In the 8–12 km altitude range, a simple analysis of the O3/HCl correlation shows that pure stratospheric and mixed tropospheric/stratospheric air masses were encountered 30% and 15% of the time, respectively. In the mid troposphere (4–8 km) HCl levels were usually below 2 pptv except for a few cases of stratospheric influence and were much lower than reported in previous work. These data indicate that background levels of HCl in the mid and upper troposphere are very low and confirm its use in these regions as a tracer of stratospheric ozone. However, a case study suggests that HCl may be produced in the mid troposphere by the dechlorination of dust aerosols. In the remote marine boundary layer HCl levels were consistently above 20 pptv (up to 140 pptv) and strongly correlated with HNO3. Cl atom levels were estimated from the background level of HCl in the MBL. This analysis suggests a Cl concentration of ~3×103 atoms cm−3, which corresponds to the lower range of previous studies. Finally, the observed HCl levels are compared to predictions by the Real-time Air Quality Modeling System (RAQMS) to assess its ability to characterize the impact of stratospheric transport on the upper troposphere.
We use recent aircraft measurements of a comprehensive suite of anthropogenic halocarbons, carbon monoxide (CO), and related tracers to place new constraints on North American halocarbon emissions and quantify their global warming potential. Using a chemical transport model (GEOS-Chem) we find that the ensemble of observations are consistent with our prior best estimate of the U.S. anthropogenic CO source, but suggest a 30% underestimate of Mexican emissions. We develop an optimized CO emission inventory on this basis and quantify halocarbon emissions from their measured enhancements relative to CO. Emissions continue for many compounds restricted under the Montreal Protocol, and we show that halocarbons make up an important fraction of the total greenhouse gas source for both countries: our best estimate is 9% (uncertainty range 6-12%) and 32% (21-52%) of equivalent CO2 emissions for the U.S. and Mexico, respectively, on a 20 year time scale. Performance of bottom-up emission inventories is variable, with underestimates for some compounds and overestimates for others. Ongoing methylchloroform emissions are significant in the U.S. (2.8 Gg/y in 2004-2006), in contrast to bottom-up estimates (< 0.05 Gg), with implications for tropospheric OH calculations. Mexican methylchloroform emissions are minor.
Sparse monitoring of dust events in regional areas hinders a full understanding of health impacts from events such as wildfires and dust storm. Remote sensing has the potential to improve this understanding but has not been widely embraced due to temporal limitations inherent in the MODIS satellites which are unable to detect sporadic events reliably. Recently launched second-generation geostationary satellites such as Himawari-8 (July 2015, Asia and Oceania) and GOES-R (Dec 2016, North America) supply sub-hourly data which overcome earlier temporal limitations.\nThis review evaluates the ability of remote sensing to detect ground-level particulate matter concentrations particularly in light of geostationary satellites. It has concluded that there is a requirement to discard the visible portion of the wavelength spectrum and utilise thermal infrared absorption spectra in order to provide near-continuous estimates of surface concentration. This will require a better understanding of dust indices, using all available thermal infrared wavelength channels to determine the effects of moisture, particle size and composition on spectral properties.