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  • 1
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 102, No. D5 ( 1997-03-20), p. 5953-5970
    Abstract: Simulations of 222 Rn and other short‐lived tracers are used to evaluate and intercompare the representations of convective and synoptic processes in 20 global atmospheric transport models. Results show that most established three‐dimensional models simulate vertical mixing in the troposphere to within the constraints offered by the observed mean 222 Rn concentrations and that subgrid parameterization of convection is essential for this purpose. However, none of the models captures the observed variability of 222 Rn concentrations in the upper troposphere, and none reproduces the high 222 Rn concentrations measured at 200 hPa over Hawaii. The established three‐dimensional models reproduce the frequency and magnitude of high‐ 222 Rn episodes observed at Crozet Island in the Indian Ocean, demonstrating that they can resolve the synoptic‐scale transport of continental plumes with no significant numerical diffusion. Large differences between models are found in the rates of meridional transport in the upper troposphere (interhemispheric exchange, exchange between tropics and high latitudes). The four two‐dimensional models which participated in the intercomparison tend to underestimate the rate of vertical transport from the lower to the upper troposphere but show concentrations of 222 Rn in the lower troposphere that are comparable to the zonal mean values in the three‐dimensional models.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1998
    In:  Journal of Geophysical Research: Atmospheres Vol. 103, No. D3 ( 1998-02-20), p. 3511-3530
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 103, No. D3 ( 1998-02-20), p. 3511-3530
    Abstract: The global distribution of ozone in the troposphere and lower stratosphere calculated with a three‐dimensional chemistry transport model driven by European Centre for Medium‐Range Weather Forecasts (ECMWF)‐analyzed meteorological fields has been compared with observed ozonesonde profiles. This comparison is presented in a new graphical format, which shows in a single panel the vertical and seasonal dependence. The modeled ozone profiles compare reasonably well with climatological ozonesonde data for various stations all over the world, especially if the variability of the ozone concentrations is taken into account. However, the ozone mixing ratios in the upper troposphere and lower stratosphere at midlatitudes are generally overestimated by the model. This is probably caused by a combination of an overestimation of the stratosphere‐troposphere exchange and the absence of heterogeneous reactions in the lower stratosphere which reduce ozone. The latitudinal dependence and seasonal dependence of the observations are reproduced by the model calculations, except for the ozone concentrations at the surface. This might be due to the neglect of nonmethane hydrocarbons, which give rise to photochemical ozone production during summer, although other factors such as emissions and deposition cannot be ruled out. The ozone column density obtained by combining calculated ozone distributions up to 50 hPa with climatological zonal mean data for ozone above 50 hPa compares reasonably well with total ozone mapping spectrometer (TOMS) observations. Particularly, the variability caused by synoptic features observable in modeled total ozone shows a high degree of correspondence to the observations. This indicates that rapid variations in the ozone column density are mainly the result of corresponding variations in ozone concentrations near the tropopause due to transport. Modeled total ozone is generally underestimated in the tropics and overestimated elsewhere compared to the TOMS observations. This overestimation, which is large in spring at northern midlatitudes and increased toward the pole, can partly be ascribed to differences between the prescribed climatological ozone concentrations above 50 hPa and the actual values in 1990. Budget calculations of tropospheric ozone showed that reducing these prescribed ozone concentrations lowers the ozone input from the stratosphere, which is largely compensated by a higher photochemical ozone production in the troposphere such that deposition, which depends on the ozone concentrations in the lower troposphere, remains almost unaffected. The reason for the overestimation needs to be investigated further using in situ measurements of several trace gases simultaneously in order to better understand the chemical processes involved. In this study a methane and carbon monoxide oxidation chemistry scheme has been employed without stratospheric chemistry. Furthermore, the comparison of TOMS total ozone observations in the tropics with model calculations seems to suggest that the treatment of ozone precursors such as the NO x emissions by lightning and biomass burning needs to be improved. The reduced correlation between observed and modeled total ozone fields at southern midlatitudes can probably be ascribed to the lower quality of the analyzed fields in that area. Because of the above mentioned discrepancies the calculated atmospheric impact of anthropogenic emissions needs to be interpreted with care.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1998
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  • 3
    In: Atmosphere, MDPI AG, Vol. 3, No. 1 ( 2012-02-09), p. 132-163
    Type of Medium: Online Resource
    ISSN: 2073-4433
    Language: English
    Publisher: MDPI AG
    Publication Date: 2012
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Atmospheres Vol. 102, No. D17 ( 1997-09-20), p. 21315-21328
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 102, No. D17 ( 1997-09-20), p. 21315-21328
    Abstract: During July 1994, submicron aerosol size distributions were measured at two sites on Tenerife, Canary Islands. One station was located in the free troposphere (FT), the other in the marine boundary layer (MBL). Transport toward these two sites was strongly decoupled: the FT was first affected by dust and sulfate‐laden air masses advecting from North Africa and later by clean air masses originating over the North Atlantic, whereas the MBL was always subject to the northeasterly trade wind circulation. In the FT the submicron aerosol distribution was predominantly monomodal with a geometric mean diameter of 120 nm and 55 nm during dusty and clean conditions, respectively. The relatively small diameter during the clean conditions indicates that the aerosol originated in the upper troposphere rather than over continental areas or in the lower stratosphere. During dusty conditions the physical and chemical properties of the submicron aerosol suggest that it has an anthropogenic origin over southern Europe and that it remains largely externally mixed with the supermicron mineral dust particles during its transport over North Africa to Tenerife. Apart from synoptic variations, a strong diurnal variation in the aerosol size distribution is observed at the FT site, characterized by a strong daytime mode of ultrafine particles. This is interpreted as being the result of photoinduced nucleation in the upslope winds, which are perturbed by anthropogenic and biogenic emissions on the island. No evidence was found for nucleation occurring in the undisturbed FT. The MBL site was not strongly affected by European pollution during the period of the measurements. The MBL aerosol size distribution was bimodal, but the relative concentration of Aitken and accumulation mode varied strongly. The accumulation mode can be related to cloud processing of the Aitken mode but also to pollution aerosol which was advected within the MBL or entrained from the FT. No bursts of nucleation were observed within the MBL.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 5
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 23, No. 16 ( 1996-08), p. 2125-2128
    Abstract: Isotope and concentration measurements are reported for CO and CH 4 in air collected in the upper troposphere and lower stratosphere between New Zealand and Antarctica in October 1993. The 13 C/ 12 C ratio of CO for the stratospheric samples, which are identified using calculated potential vorticity and coherent isotope data, like the abundance of 14 CO molecules, are much lower than all previously reported atmospheric values. The measurements manifest a very steep decrease in δ 13 C with declining CO, with one sample reaching a δ 13 C value relative to V‐PDB of −43‰ at 20 ppbv CO. This large isotope shift is caused by the local production of several ppbv of extremely depleted CO. Not only is C 4 itself a 13 C depleted precursor of CO, it is specifically the recently discovered large fractionation in Cl+CH 4 , and the availability of free Cl during ozone hole conditions, which causes the effect.
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1996
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  • 6
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Atmospheres Vol. 102, No. D23 ( 1997-12-20), p. 28219-28221
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 102, No. D23 ( 1997-12-20), p. 28219-28221
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Atmospheres Vol. 102, No. D1 ( 1997-01-20), p. 1229-1238
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 102, No. D1 ( 1997-01-20), p. 1229-1238
    Abstract: The degree of isolation of the Antarctic stratospheric vortex in late winter and spring is investigated quantitatively by using a three‐dimensional global tracer transport model, in which the transport is computed from European Centre for Medium‐Range Weather Forecasts analyzed data. The evolution of the spatial distribution of passive tracers provides information about variations in the vortex structure, as well as about the magnitude of the transport out of the Antarctic vortex. The vortex structure revealed by tracers released inside the vortex at 72.5 hPa corresponds well with the satellite‐derived distribution of total ozone. The model computations indicate that in late winter and spring of the years 1990–1993, there is a quasi‐horizontal cross‐vortex transport of about 0.24% per day of the total tracer amount, while per day, 0.83% of the vortex mass descends into the troposphere. This indicates that roughly 65% of the vortex air is flushed out during August‐September‐October, the approximate lifetime of the Antarctic vortex. This number is insensitive to changes in model resolution, although the quasi‐horizontal outflow into the midlatitude stratosphere increases at the expense of the downward outflow if a coarser resolution is used. It is concluded that during late winter and early spring (i.e., the period of major ozone depletion), the vortex is a fairly well isolated air mass.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 8
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2002
    In:  Journal of Geophysical Research: Atmospheres Vol. 107, No. D17 ( 2002-09-16), p. 3-1-3-14
    In: Journal of Geophysical Research: Atmospheres, American Geophysical Union (AGU), Vol. 107, No. D17 ( 2002-09-16), p. 3-1-3-14
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2002
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  • 9
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 38, No. 13 ( 2011-07), p. n/a-n/a
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2011
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  • 10
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 39, No. 10 ( 2012-05-28), p. n/a-n/a
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2012
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