D. A. Hauglustaine
Centre national de la recherche scientifique
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Featured researches published by D. A. Hauglustaine.
Journal of Geophysical Research | 2006
David S. Stevenson; F. Dentener; Martin G. Schultz; K. Ellingsen; T. van Noije; Oliver Wild; Guang Zeng; M. Amann; C. S. Atherton; N. Bell; D. Bergmann; Isabelle Bey; T. Butler; J. Cofala; W. J. Collins; R. G. Derwent; Ruth M. Doherty; J. Drevet; Henk Eskes; Arlene M. Fiore; M. Gauss; D. A. Hauglustaine; Larry W. Horowitz; Ivar S. A. Isaksen; M. Krol; Jean-Francois Lamarque; M. G. Lawrence; V. Montanaro; Jean-François Müller; G. Pitari
Global tropospheric ozone distributions, budgets, and radiative forcings from an ensemble of 26 state-of-the-art atmospheric chemistry models have been intercompared and synthesized as part of a wider study into both the air quality and climate roles of ozone. Results from three 2030 emissions scenarios, broadly representing optimistic, likely, and pessimistic options, are compared to a base year 2000 simulation. This base case realistically represents the current global distribution of tropospheric ozone. A further set of simulations considers the influence of climate change over the same time period by forcing the central emissions scenario with a surface warming of around 0.7K. The use of a large multimodel ensemble allows us to identify key areas of uncertainty and improves the robustness of the results. Ensemble mean changes in tropospheric ozone burden between 2000 and 2030 for the 3 scenarios range from a 5% decrease, through a 6% increase, to a 15% increase. The intermodel uncertainty (±1 standard deviation) associated with these values is about ±25%. Model outliers have no significant influence on the ensemble mean results. Combining ozone and methane changes, the three scenarios produce radiative forcings of -50, 180, and 300 mW m-2, compared to a CO 2 forcing over the same time period of 800-1100 mW m-2. These values indicate the importance of air pollution emissions in short- to medium-term climate forcing and the potential for stringent/lax control measures to improve/worsen future climate forcing. The model sensitivity of ozone to imposed climate change varies between models but modulates zonal mean mixing ratios by ±5 ppbv via a variety of feedback mechanisms, in particular those involving water vapor and stratosphere-troposphere exchange. This level of climate change also reduces the methane lifetime by around 4%. The ensemble mean year 2000 tropospheric ozone budget indicates chemical production, chemical destruction, dry deposition and stratospheric input fluxes of 5100, 4650, 1000 and 550 Tg(O 3 ) yr-1, respectively. These values are significantly different to the mean budget documented by the Intergovernmental Panel on Climate Change (IPCC) Third Assessment Report (TAR). The mean ozone burden (340 Tg(O 3 )) is 10% larger than the IPCC TAR estimate, while the mean ozone lifetime (22 days) is 10% shorter. Results from individual models show a correlation between ozone burden and lifetime, and each models ozone burden and lifetime respond in similar ways across the emissions scenarios. The response to climate change is much less consistent. Models show more variability in the tropics compared to midlatitudes. Some of the most uncertain areas of the models include treatments of deep tropical convection, including lightning NO x production; isoprene emissions from vegetation and isoprenes degradation chemistry; stratosphere-troposphere exchange; biomass burning; and water vapor concentrations. Copyright 2006 by the American Geophysical Union.
Global Biogeochemical Cycles | 2006
Frank Dentener; J. Drevet; Jean-Francois Lamarque; Isabelle Bey; B. Eickhout; Arlene M. Fiore; D. A. Hauglustaine; Larry W. Horowitz; M. Krol; U. C. Kulshrestha; M. G. Lawrence; C. Galy-Lacaux; Sebastian Rast; Drew T. Shindell; David S. Stevenson; T. van Noije; C. S. Atherton; N. Bell; D. Bergman; T. Butler; J. Cofala; B. Collins; Ruth M. Doherty; K. Ellingsen; James N. Galloway; M. Gauss; V. Montanaro; J.-F. Müller; G. Pitari; Jose M. Rodriguez
We use 23 atmospheric chemistry transport models to calculate current and future (2030) deposition of reactive nitrogen (NOy, NHx) and sulfate (SOx) to land and ocean surfaces. The models are driven by three emission scenarios: (1) current air quality legislation (CLE); (2) an optimistic case of the maximum emissions reductions currently technologically feasible (MFR); and (3) the contrasting pessimistic IPCC SRES A2 scenario. An extensive evaluation of the present-day deposition using nearly all information on wet deposition available worldwide shows a good agreement with observations in Europe and North America, where 60–70% of the model-calculated wet deposition rates agree to within ±50% with quality-controlled measurements. Models systematically overestimate NHx deposition in South Asia, and underestimate NOy deposition in East Asia. We show that there are substantial differences among models for the removal mechanisms of NOy, NHx, and SOx, leading to ±1 σ variance in total deposition fluxes of about 30% in the anthropogenic emissions regions, and up to a factor of 2 outside. In all cases the mean model constructed from the ensemble calculations is among the best when comparing to measurements. Currently, 36–51% of all NOy, NHx, and SOx is deposited over the ocean, and 50–80% of the fraction of deposition on land falls on natural (nonagricultural) vegetation. Currently, 11% of the worlds natural vegetation receives nitrogen deposition in excess of the “critical load” threshold of 1000 mg(N) m−2 yr−1. The regions most affected are the United States (20% of vegetation), western Europe (30%), eastern Europe (80%), South Asia (60%), East Asia (40%), southeast Asia (30%), and Japan (50%). Future deposition fluxes are mainly driven by changes in emissions, and less importantly by changes in atmospheric chemistry and climate. The global fraction of vegetation exposed to nitrogen loads in excess of 1000 mg(N) m−2 yr−1 increases globally to 17% for CLE and 25% for A2. In MFR, the reductions in NOy are offset by further increases for NHx deposition. The regions most affected by exceedingly high nitrogen loads for CLE and A2 are Europe and Asia, but also parts of Africa.
Nature | 2006
P. Bousquet; Philippe Ciais; J. B. Miller; E. J. Dlugokencky; D. A. Hauglustaine; C. Prigent; G. R. van der Werf; P. Peylin; E.-G. Brunke; C. Carouge; R. L. Langenfelds; J. Lathière; Fabrice Papa; M. Ramonet; M. Schmidt; L. P. Steele; S. C. Tyler; James W. C. White
Methane is an important greenhouse gas, and its atmospheric concentration has nearly tripled since pre-industrial times. The growth rate of atmospheric methane is determined by the balance between surface emissions and photochemical destruction by the hydroxyl radical, the major atmospheric oxidant. Remarkably, this growth rate has decreased markedly since the early 1990s, and the level of methane has remained relatively constant since 1999, leading to a downward revision of its projected influence on global temperatures. Large fluctuations in the growth rate of atmospheric methane are also observed from one year to the next, but their causes remain uncertain. Here we quantify the processes that controlled variations in methane emissions between 1984 and 2003 using an inversion model of atmospheric transport and chemistry. Our results indicate that wetland emissions dominated the inter-annual variability of methane sources, whereas fire emissions played a smaller role, except during the 1997–1998 El Niño event. These top-down estimates of changes in wetland and fire emissions are in good agreement with independent estimates based on remote sensing information and biogeochemical models. On longer timescales, our results show that the decrease in atmospheric methane growth during the 1990s was caused by a decline in anthropogenic emissions. Since 1999, however, they indicate that anthropogenic emissions of methane have risen again. The effect of this increase on the growth rate of atmospheric methane has been masked by a coincident decrease in wetland emissions, but atmospheric methane levels may increase in the near future if wetland emissions return to their mean 1990s levels.
Journal of Geophysical Research | 2003
M. Gauss; Gunnar Myhre; G. Pitari; Michael J. Prather; Ivar S. A. Isaksen; Terje K. Berntsen; Guy P. Brasseur; F. Dentener; R. G. Derwent; D. A. Hauglustaine; Larry W. Horowitz; Daniel J. Jacob; M. Johnson; Kathy S. Law; Loretta J. Mickley; J.-F. Müller; P.-H. Plantevin; J. A. Pyle; Helen Rogers; David S. Stevenson; Jostein K. Sundet; M. van Weele; Oliver Wild
ranging from 0.40 to 0.78 W m 2 on a global and annual average. The lower stratosphere contributes an additional 7.5–9.3 DU to the calculated increase in the ozone column, increasing radiative forcing by 0.15–0.17 W m 2 . The modeled radiative forcing depends on the height distribution and geographical pattern of predicted ozone changes and shows a distinct seasonal variation. Despite the large variations between the 11 participating models, the calculated range for normalized radiative forcing is within 25%, indicating the ability to scale radiative forcing to global-mean ozone column change. INDEX TERMS: 0365 Atmospheric Composition and Structure: Troposphere—composition and chemistry; 0341 Atmospheric Composition and Structure: Middle atmosphere—constituent transport and chemistry (3334) Citation: Gauss, M., et al., Radiative forcing in the 21st century due to ozone changes in the troposphere and the lower stratosphere, J. Geophys. Res., 108(D9), 4292, doi:10.1029/2002JD002624, 2003.
Journal of Geophysical Research | 1998
D. A. Hauglustaine; Guy P. Brasseur; Stacy Walters; P. J. Rasch; Jean-François Müller; Louisa Kent Emmons; Mary Anne Carroll
In this second of two companion papers, we present results from a new global three-dimensional chemical transport model, called MOZART (model for ozone and related chemical tracers). MOZART is developed in the framework of the National Center for Atmospheric Research (NCAR) Community Climate Model (CCM) and includes a detailed representation of tropospheric chemistry. The model provides the distribution of 56 chemical species at a spatial resolution of 2.8° in both latitude and longitude, with 25 levels in the vertical (from the surface to level of 3 mbar) and a time step of 20 min. The meteorological information is supplied from a 2-year run of the NCAR Community Climate Model. The simulated distributions of ozone (O 3 ) and its precursors are evaluated by comparison with observational data. The distribution of methane, nonmethane hydrocarbons (NMHCs), and CO are generally well simulated by the model. The model evaluation in the tropics stresses the need for a better representation of biomass burning emissions in order to evaluate the budget of carbon monoxide, nitrogen species, and ozone with more accuracy in these regions. MOZART reproduces the NO observations in most parts of the troposphere. Nitric acid, however, is overestimated over the Pacific by up to a factor of 10 and over continental regions by a factor of 2-3. Discrepancies are also found in the simulation of PAN in the upper troposphere and in biomass burning regions. These results highlight shortcomings in our understanding of the nitrogen budget in the troposphere. The seasonal cycle of ozone in the troposphere is generally well reproduced by the model in comparison with ozone soundings. MOZART tends, however, to underestimate O 3 at higher latitudes, and specifically above 300 mbar. The global photochemical production and destruction of ozone in the troposphere are 3018 Tg/yr and 2511 Tg/yr, respectively (net ozone production of 507 Tg/yr). The stratospheric influx of O 3 is estimated to be 391 Tg/yr and the surface dry deposition 898 Tg/yr. The calculated global lifetime of methane is 9.9 years in the annual average.
Journal of Geophysical Research | 2005
J.-F. Lamarque; Jeffrey T. Kiehl; Guy P. Brasseur; T. Butler; Philip Cameron-Smith; W. D. Collins; W. J. Collins; Claire Granier; D. A. Hauglustaine; Peter G. Hess; Elisabeth A. Holland; Larry W. Horowitz; M. G. Lawrence; Daniel S. McKenna; P. Merilees; Michael J. Prather; P. J. Rasch; Douglas A. Rotman; Drew T. Shindell; Peter E. Thornton
n this study, we present the results of nitrogen deposition on land from a set of 29 simulations from six different tropospheric chemistry models pertaining to present-day and 2100 conditions. Nitrogen deposition refers here to the deposition (wet and dry) of all nitrogen-containing gas phase chemical species resulting from NOx (NO + NO2) emissions. We show that under the assumed IPCC SRES A2 scenario the global annual average nitrogen deposition over land is expected to increase by a factor of ∼2.5, mostly because of the increase in nitrogen emissions. This will significantly expand the areas with annual average deposition exceeding 1 gN/m2/year. Using the results from all models, we have documented the strong linear relationship between models on the fraction of the nitrogen emissions that is deposited, regardless of the emissions (present day or 2100). On average, approximately 70% of the emitted nitrogen is deposited over the landmasses. For present-day conditions the results from this study suggest that the deposition over land ranges between 25 and 40 Tg(N)/year. By 2100, under the A2 scenario, the deposition over the continents is expected to range between 60 and 100 Tg(N)/year. Over forests the deposition is expected to increase from 10 Tg(N)/year to 20 Tg(N)/year. In 2100 the nitrogen deposition changes from changes in the climate account for much less than the changes from increased nitrogen emissions.
Journal of Geophysical Research | 2006
Drew T. Shindell; G. Faluvegi; David S. Stevenson; M. Krol; Louisa Kent Emmons; Jean-Francois Lamarque; G. Pétron; F. Dentener; K. Ellingsen; Martin G. Schultz; Oliver Wild; M. Amann; C. S. Atherton; D. Bergmann; I. Bey; T. Butler; J. Cofala; W. J. Collins; R. G. Derwent; Ruth M. Doherty; J. Drevet; Henk Eskes; Arlene M. Fiore; M. Gauss; D. A. Hauglustaine; Larry W. Horowitz; Ivar S. A. Isaksen; M. G. Lawrence; V. Montanaro; Jean-François Müller
We analyze present-day and future carbon monoxide (CO) simulations in 26 state-of-the-art atmospheric chemistry models run to study future air quality and climate change. In comparison with near-global satellite observations from the MOPITT instrument and local surface measurements, the models show large underestimates of Northern Hemisphere (NH) extratropical CO, while typically performing reasonably well elsewhere. The results suggest that year-round emissions, probably from fossil fuel burning in east Asia and seasonal biomass burning emissions in south-central Africa, are greatly underestimated in current inventories such as IIASA and EDGAR3.2. Variability among models is large, likely resulting primarily from intermodel differences in representations and emissions of nonmethane volatile organic compounds (NMVOCs) and in hydrologic cycles, which affect OH and soluble hydrocarbon intermediates. Global mean projections of the 2030 CO response to emissions changes are quite robust. Global mean midtropospheric (500 hPa) CO increases by 12.6 ± 3.5 ppbv (16%) for the high-emissions (A2) scenario, by 1.7 ± 1.8 ppbv (2%) for the midrange (CLE) scenario, and decreases by 8.1 ± 2.3 ppbv (11%) for the low-emissions (MFR) scenario. Projected 2030 climate changes decrease global 500 hPa CO by 1.4 ± 1.4 ppbv. Local changes can be much larger. In response to climate change, substantial effects are seen in the tropics, but intermodel variability is quite large. The regional CO responses to emissions changes are robust across models, however. These range from decreases of 10–20 ppbv over much of the industrialized NH for the CLE scenario to CO increases worldwide and year-round under A2, with the largest changes over central Africa (20–30 ppbv), southern Brazil (20–35 ppbv) and south and east Asia (30–70 ppbv). The trajectory of future emissions thus has the potential to profoundly affect air quality over most of the worlds populated areas.
Geophysical Research Letters | 2003
Michael J. Prather; M. Gauss; Terje K. Berntsen; Ivar S. A. Isaksen; Jostein K. Sundet; Isabelle Bey; Guy P. Brasseur; Frank Dentener; R. G. Derwent; David S. Stevenson; Lee Grenfell; D. A. Hauglustaine; Larry W. Horowitz; Daniel J. Jacob; Loretta J. Mickley; Mark G. Lawrence; Rolf von Kuhlmann; Jean-François Müller; Giovanni Pitari; Helen Rogers; Matthew S. Johnson; J. A. Pyle; Kathy S. Law; Michiel van Weele; Oliver Wild
Ozone is an air quality problem today for much of the worlds population. Regions can exceed the ozone air quality standards (AQS) through a combination of local emissions, meteorology favoring pollution episodes, and the clean-air baseline levels of ozone upon which pollution builds. The IPCC 2001 assessment studied a range of global emission scenarios and found that all but one projects increases in global tropospheric ozone during the 21st century. By 2030, near-surface increases over much of the northern hemisphere are estimated to be about 5 ppb (+2 to +7 ppb over the range of scenarios). By 2100 the two more extreme scenarios project baseline ozone increases of >20 ppb, while the other four scenarios give changes of -4 to +10 ppb. Even modest increases in the background abundance of tropospheric ozone might defeat current AQS strategies. The larger increases, however, would gravely threaten both urban and rural air quality over most of the northern hemisphere.
Atmospheric Environment | 1998
Guy P. Brasseur; R.A. Cox; D. A. Hauglustaine; Ivar S. A. Isaksen; J. Lelieveld; D.H. Lister; Robert Sausen; Ulrich Schumann; Andreas Wahner; P. Wiesen
The purpose of this report prepared on behalf of the European Commission is to review the current understanding of chemical and dynamical processes in the upper troposphere and lower stratosphere, and to assess how these processes could be perturbed as a result of current and future aircraft emissions. Specifically, perturbations in the atmospheric abundance of ozone and in climate forcing, as predicted by atmospheric models, will be presented. The goal is to compile and evaluate scientific information related to the atmospheric impact of subsonic and supersonic aircraft emissions and to review the state of knowledge concerning the various aspects of this problem. In Section 2, the issues and scientific questions relevant to the problem of aircraft perturbations will be presented. The key physical and chemical processes occurring in the troposphere and stratosphere will be discussed in Section 3. Estimates of air traffic and aircraft emissions will be given in Section 4. Section 5 and 6 will review the understanding of the atmospheric impact of aircraft emissions at small and large scale, respectively. The effect of aircraft emissions on climate forcing will be discussed in Section 7. Finally, conclusions will be provided in Section 8.
Meteorologische Zeitschrift | 2005
Robert Sausen; Ivar S. A. Isaksen; Volker Grewe; D. A. Hauglustaine; David S. Lee; Gunnar Myhre; Marcus O. Köhler; Giovanni Pitari; Ulrich Schumann; Frode Stordal; C. Zerefos
New estimates of the various contributions to the radiative forcing (RF) from aviation are presented, mainly based on results from the TRADEOFF project that update those of the Intergovernmental Panel on Climate Change (IPCC, 1999). The new estimate of the total RF from aviation for 2000 is approximately the same as that of the IPCC’s estimate for 1992. This is mainly a consequence of the strongly reduced RF from contrails, which compensates the increase due to increased traffic from 1992 to 2000. The RF from other aviationinduced cirrus clouds might be as large as the present estimate of the total RF (without cirrus). However, our present knowledge on these aircraft-induced cirrus clouds is too poor to provide a reliable estimate of the associated RF. Zusammenfassung Neue Abschatzungen der einzelnen Beitrage zum Strahlungsantrieb des Luftverkehrs werden vorgestellt, die im Wesentlichen auf Ergebnissen des TRADEOFF-Projektes beruhen und die die IPCC-Abschatzungen (1999) aktualisieren. Der neue Wert fur den gesamten Strahlungsantrieb des Luftverkehrs im Jahr 2000 ist in etwa gleich gros wie die IPCC-Abschatzung fur das Jahr 1992. Das ist im Wesentlichen eine Folge des stark reduzierten Strahlungsantriebes durch Kondensstreifen, wodurch der Anstieg aufgrund der Zunahme des Verkehrs von 1992 bis 2000 kompensiert wird. Der Antrieb durch andere luftverkehrsinduzierte Wolken konnte ebenso gros sein wie die neue Abschatzung fur den gesamten Strahlungsantrieb (ohne Zirren). Jedoch ist unser heutiges Wissen uber diese luftverkehrsinduzierten Wolken nicht gut genug, um belastbare Aussagen uber den damit verbundenen Strahlungsantrieb zu machen.