Analysis of the Effects of Midlatitude Deep Convection on the Composition and Chemistry of the Upper Troposphere/lower Stratosphere Using Aircraft Data Collected During the Deep Convective Clouds and Chemistry (DC3) Field Campaign

Analysis of the Effects of Midlatitude Deep Convection on the Composition and Chemistry of the Upper Troposphere/lower Stratosphere Using Aircraft Data Collected During the Deep Convective Clouds and Chemistry (DC3) Field Campaign PDF Author: Jason R. Schroeder
Publisher:
ISBN: 9781339124100
Category :
Languages : en
Pages : 167

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Book Description
Measurements of trace gases were taken onboard the NASA DC-8 during the Deep Convective Clouds and Chemistry (DC3) field project with the goal of understanding the role that midlatitude deep convection plays in altering the vertical distribution of atmospherically-relevant species. Measurements of VOCs were obtained via UC Irvine’s whole air sampler (WAS) instrument, while measurements of CH4, O3, NOx [subscript], N2O, water vapor, CO, and meteorological variables were performed by a variety of other instruments operated by collaborators onboard the DC-8. Using known VOC atmospheric lifetimes and measured VOC mixing ratios in the PBL, a tracer for rapid vertical lofting of air from the planetary boundary layer (PBL) to the upper troposphere/lower stratosphere region (UT/LS) by convection was created. In this study, it was found that light hydrocarbons associated with oil and natural gas (O&NG;) and vehicular sources were widespread throughout the PBL of the DC3 study regions. In the UT/LS, enhanced levels of these light hydrocarbons were strongly correlated with water vapor, indicating a convective source. On the other hand, decreases in the measured mixing ratios of CFCs, HCFCs, and other long-lived halocarbons (LLHCs) in the UT were used as tracers for stratosphere-to-troposphere transport (STT). These two sets of tracers were used to divide the DC3 WAS merge into many subsets of data corresponding to: the PBL, convective outflow in the UT, convective outflow in the LS (i.e. overshooting tops), STT-influenced air in the troposphere, background UT air, and background LS air. Using these derived subsets of data, interactions and mixing between stratospheric intrusions and tropospheric air masses was investigated. A large number of stratospherically-influenced samples were found to have reduced levels of O3 and elevated levels of CO (both relative to background stratospheric air); indicative of mixing with anthropogenically-influenced air. Using n-butane and propane as tracers of anthropogenically-influenced air, it is shown that this type of mixing was present both at low altitudes and in the UT. At low altitudes, this mixing resulted in O3 enhancements consistent with those reported at surface sites during deep stratospheric intrusions, while in the UT, two case studies were performed to identify the process by which this mixing occurs. In the first case study, stratospheric air was found to be mixed with aged outflow from a convective storm, while in the second case study, stratospheric air was found to have mixed with outflow from an active storm occurring in the vicinity of a stratospheric intrusion. From these analyses, it was concluded that deep convective events may facilitate the mixing between stratospheric air and polluted boundary layer air in the UT. Throughout the entire DC3 study region, this mixing was found to be prevalent: 72% of all samples that involve stratosphere-troposphere mixing show influence of polluted air. Applying a simple chemical kinetics analysis to these data, it is shown that the instantaneous production of OH in these mixed stratospheric-polluted air masses was 11 ± 8 (± 1?) times higher than that of stratospheric air, and 4.2 ± 1.8 times higher than that of background upper tropospheric air, which could result in a quick, high magnitude pulse of O3 production and reduced lifetimes of OH-controlled species in the UT. These derived subsets of data were used to investigate the effects of deep convection on mixing ratios of organic chlorine and organic bromine in the UT and LS over the DC3 study region. In the LS, it was found that mixing ratios of organic chlorine in overshooting tops were higher than mixing ratios of organic chlorine in the background LS by an average of 217 ± 179 pptv (6.3 ± 5.2% enhancement), while the total organic bromine mixing ratio in overshooting tops was higher than that of the background LS by an average of 2.8 ± 3.2 pptv (17.4 ± 19.9% enhancement). In both cases, short-lived halocarbons made up a large portion of this enhancement. In the UT, convection was found to play a much more complicated role on the organic halogen content of the region. Model back trajectories and analysis of the chemical composition of the background UT revealed that long-range transport of outflow from East Asia and from the central Pacific affected the background UT of the DC3 study region to varying degrees on different days. When the background UT was affected by East Asian outflow, mixing ratios of organic chlorine in convective outflow were lower than those of the local background UT by up to 150 ± 115 pptv (3.7 ± 2.9% enhancement). On the other hand, when the background UT was affected by clean outflow from the central Pacific, mixing ratios of organic chlorine in convective outflow were higher than the local background UT by up to 115 ± 98 pptv (3.2 ± 2.6% enhancement). Mixing ratios of organic bromine in the background UT were unaffected by these long-range transport processes. However, mixing ratios of organic bromine in convective outflow were highly variable and were affected by the transport of brominated very short-lived halocarbons (VSLH) from the Gulf of Mexico to the surface of the DC3 study region. When organic bromine enhancements in convective outflow were calculated on a flight-by-flight basis, organic bromine mixing ratios in convective outflow were higher than those in the background UT by an average of 1.7 ± 1.6 pptv (8.5 ± 8.1%). Based on these results, it is speculated that deep convection may play an indirect role in climate change by introducing pulses of short-lived halocarbons into the UT/LS, which in turn result in relatively quick (on the order of a few months) pulses of O3 loss in the region.

Analysis of the Effects of Midlatitude Deep Convection on the Composition and Chemistry of the Upper Troposphere/lower Stratosphere Using Aircraft Data Collected During the Deep Convective Clouds and Chemistry (DC3) Field Campaign

Analysis of the Effects of Midlatitude Deep Convection on the Composition and Chemistry of the Upper Troposphere/lower Stratosphere Using Aircraft Data Collected During the Deep Convective Clouds and Chemistry (DC3) Field Campaign PDF Author: Jason R. Schroeder
Publisher:
ISBN: 9781339124100
Category :
Languages : en
Pages : 167

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Book Description
Measurements of trace gases were taken onboard the NASA DC-8 during the Deep Convective Clouds and Chemistry (DC3) field project with the goal of understanding the role that midlatitude deep convection plays in altering the vertical distribution of atmospherically-relevant species. Measurements of VOCs were obtained via UC Irvine’s whole air sampler (WAS) instrument, while measurements of CH4, O3, NOx [subscript], N2O, water vapor, CO, and meteorological variables were performed by a variety of other instruments operated by collaborators onboard the DC-8. Using known VOC atmospheric lifetimes and measured VOC mixing ratios in the PBL, a tracer for rapid vertical lofting of air from the planetary boundary layer (PBL) to the upper troposphere/lower stratosphere region (UT/LS) by convection was created. In this study, it was found that light hydrocarbons associated with oil and natural gas (O&NG;) and vehicular sources were widespread throughout the PBL of the DC3 study regions. In the UT/LS, enhanced levels of these light hydrocarbons were strongly correlated with water vapor, indicating a convective source. On the other hand, decreases in the measured mixing ratios of CFCs, HCFCs, and other long-lived halocarbons (LLHCs) in the UT were used as tracers for stratosphere-to-troposphere transport (STT). These two sets of tracers were used to divide the DC3 WAS merge into many subsets of data corresponding to: the PBL, convective outflow in the UT, convective outflow in the LS (i.e. overshooting tops), STT-influenced air in the troposphere, background UT air, and background LS air. Using these derived subsets of data, interactions and mixing between stratospheric intrusions and tropospheric air masses was investigated. A large number of stratospherically-influenced samples were found to have reduced levels of O3 and elevated levels of CO (both relative to background stratospheric air); indicative of mixing with anthropogenically-influenced air. Using n-butane and propane as tracers of anthropogenically-influenced air, it is shown that this type of mixing was present both at low altitudes and in the UT. At low altitudes, this mixing resulted in O3 enhancements consistent with those reported at surface sites during deep stratospheric intrusions, while in the UT, two case studies were performed to identify the process by which this mixing occurs. In the first case study, stratospheric air was found to be mixed with aged outflow from a convective storm, while in the second case study, stratospheric air was found to have mixed with outflow from an active storm occurring in the vicinity of a stratospheric intrusion. From these analyses, it was concluded that deep convective events may facilitate the mixing between stratospheric air and polluted boundary layer air in the UT. Throughout the entire DC3 study region, this mixing was found to be prevalent: 72% of all samples that involve stratosphere-troposphere mixing show influence of polluted air. Applying a simple chemical kinetics analysis to these data, it is shown that the instantaneous production of OH in these mixed stratospheric-polluted air masses was 11 ± 8 (± 1?) times higher than that of stratospheric air, and 4.2 ± 1.8 times higher than that of background upper tropospheric air, which could result in a quick, high magnitude pulse of O3 production and reduced lifetimes of OH-controlled species in the UT. These derived subsets of data were used to investigate the effects of deep convection on mixing ratios of organic chlorine and organic bromine in the UT and LS over the DC3 study region. In the LS, it was found that mixing ratios of organic chlorine in overshooting tops were higher than mixing ratios of organic chlorine in the background LS by an average of 217 ± 179 pptv (6.3 ± 5.2% enhancement), while the total organic bromine mixing ratio in overshooting tops was higher than that of the background LS by an average of 2.8 ± 3.2 pptv (17.4 ± 19.9% enhancement). In both cases, short-lived halocarbons made up a large portion of this enhancement. In the UT, convection was found to play a much more complicated role on the organic halogen content of the region. Model back trajectories and analysis of the chemical composition of the background UT revealed that long-range transport of outflow from East Asia and from the central Pacific affected the background UT of the DC3 study region to varying degrees on different days. When the background UT was affected by East Asian outflow, mixing ratios of organic chlorine in convective outflow were lower than those of the local background UT by up to 150 ± 115 pptv (3.7 ± 2.9% enhancement). On the other hand, when the background UT was affected by clean outflow from the central Pacific, mixing ratios of organic chlorine in convective outflow were higher than the local background UT by up to 115 ± 98 pptv (3.2 ± 2.6% enhancement). Mixing ratios of organic bromine in the background UT were unaffected by these long-range transport processes. However, mixing ratios of organic bromine in convective outflow were highly variable and were affected by the transport of brominated very short-lived halocarbons (VSLH) from the Gulf of Mexico to the surface of the DC3 study region. When organic bromine enhancements in convective outflow were calculated on a flight-by-flight basis, organic bromine mixing ratios in convective outflow were higher than those in the background UT by an average of 1.7 ± 1.6 pptv (8.5 ± 8.1%). Based on these results, it is speculated that deep convection may play an indirect role in climate change by introducing pulses of short-lived halocarbons into the UT/LS, which in turn result in relatively quick (on the order of a few months) pulses of O3 loss in the region.

Diagnostic Tools in Atmospheric Physics

Diagnostic Tools in Atmospheric Physics PDF Author: Società italiana di fisica
Publisher: IOS Press
ISBN: 161499210X
Category : Science
Languages : en
Pages : 365

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Book Description
This volume addresses a number of experimental techniques and methods for the treatment of data introduced in the last ten years or so in different fields of the atmospheric sciences. Considerable emphasis has been given since their introduction to the use of satellites or spaceborne measurements with a recent example being the important results obtained with UARS. Of particular interest are the airborne instruments developed for the stratospheric measurement campaign organized by the NASA since 1976 to study the ozone hole and followed later by similar experiments to study the high-latitude ozone depletion in the northern hemisphere. The results of these experiments have helped clarify the role of chlorine-bearing compounds in the ozone depletion and the effect of the heterogeneous processes. The book is organized in 4 chapters: the first 3 divide the different techniques according to the location of the measuring instrumentation (ground, air and space) with the 4th chapter dealing with theory and analysis.

A Review of NASA's 'Atmospheric Effects of Stratospheric Aircraft' Project

A Review of NASA's 'Atmospheric Effects of Stratospheric Aircraft' Project PDF Author: National Research Council
Publisher: National Academies Press
ISBN: 0309065895
Category : Technology & Engineering
Languages : en
Pages : 60

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Book Description
The NRC Panel on the Atmospheric Effects of Aviation (PAEAN) was established to provide guidance to NASA's Atmospheric Effects of Aviation Program (AEAP) by evaluating the appropriateness of the program's research plan, appraising the project-sponsored results relative to the current state of scientific knowledge, identifying key scientific uncertainties, and suggesting research activities likely to reduce those uncertainties. Over the last few years, the panel has written periodic reviews of both the subsonic aviation (Subsonic Assessment-SASS) and the supersonic aviation (Atmospheric Effects of Stratospheric Aircraft-AESA) components of AEAP, including: An Interim Review of the Subsonic Assessment Project (1997); An Interim Assessment of AEAP's Emissions Characterization and Near-Field Interactions Elements (1997); An Interim Review of the AESA Project: Science and Progress (1998); Atmospheric Effects of Aviation: A Review of NASA's Subsonic Assessment Project (1998). This report constitutes the final review of AESA and will be the last report written by this panel. The primary audience for these reports is the program managers and scientists affiliated with AEAP, although in some cases the topics discussed are of interest to a wider audience.

Environmental Catalysis

Environmental Catalysis PDF Author: Vicki H. Grassian
Publisher: CRC Press
ISBN: 1420027670
Category : Science
Languages : en
Pages : 723

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Book Description
The study of environmental interfaces and environmental catalysis is central to finding more effective solutions to air pollution and in understanding of how pollution impacts the natural environment. Encompassing concepts, techniques, and methods, Environmental Catalysis provides a mix of theory, computation, analysis, and synthesis to support the

The Atmospheric Effects of Stratospheric Aircraft Project

The Atmospheric Effects of Stratospheric Aircraft Project PDF Author: National Research Council
Publisher: National Academies Press
ISBN: 0309173760
Category : Technology & Engineering
Languages : en
Pages : 68

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Book Description
Scientists and policy-makers alike are concerned that operation of a fleet of high-speed civil transport (HSCT) aircraft could significantly affect the global atmosphere. HSCT emissions may have a direct effect on the chemistry of the atmosphere, leading to changes in the distribution of ozone; they may also have indirect effects on ozone and on global climate through coupling with radiative and dynamical processes in the atmosphere. An assessment of the atmospheric impact of a fleet of HSCTs thus requires not only an understanding of the chemistry of the natural stratosphere and its possible perturbations by HSCT emissions, but also an understanding of the pathways for transport of HSCT emissions within the atmosphere, and the resulting temporal and spatial distribution of HSCT emissions. The results of NASA's Atmospheric Effects of Stratospheric Aircraft (AESA) project were summarized in a 1995 NASA assessment. The present report looks at that summary and at more recent work to evaluate the state of the science. AESA has made good progress in the past few years. Satellite and aircraft observations have elucidated important aspects of large-scale transport processes. Field campaigns have provided a much better picture of the relative importance, below 20 km altitude, of the major catalytic cycles for ozone destruction. Careful intercomparisons of assessment models have led to reduction of some of the differences among the models. However, a number of uncertainties and inconsistencies still remain.

A 13-year Trajectory-based Analysis of Convection-driven Changes in Upper Troposphere Lower Stratosphere Composition Over the United States

A 13-year Trajectory-based Analysis of Convection-driven Changes in Upper Troposphere Lower Stratosphere Composition Over the United States PDF Author: Emily Nicole Tinney
Publisher:
ISBN:
Category : Convection (Meteorology)
Languages : en
Pages : 63

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The Atmospheric Effects of Stratospheric Aircraft: A First Program Report

The Atmospheric Effects of Stratospheric Aircraft: A First Program Report PDF Author: Michael J. Prather
Publisher:
ISBN:
Category : Aeronautics, Commercial
Languages : en
Pages : 246

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Geophysik II / Geophysics II

Geophysik II / Geophysics II PDF Author:
Publisher: Springer Science & Business Media
ISBN: 3642458815
Category : Science
Languages : de
Pages : 1054

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Book Description
45 downwards because (j on the average increases with height; but this conclusion does not follow from (18.3) when the dependency of Kc upon ~o is taken into consideration. s 2 ERTELl and PRIESTLEY and SWINBANK have shown that the upward eddy flux of sensible heat must be larger than indicated by (18.3), because this formula does not account for the fact that rising eddies are systematically warmer than sinking eddies because of the effect of buoyancy. The reader is referred to the reviews by SUTTON [22], [23] and PRIESTLEY and SHEP PARD [15) for further details concerning eddy-flux of heat and turbulent diffusion. 19. RICHARDSON'S criterion. The right-hand side of (15.10) represents the rate of production of eddy energy. The last term represents energy loss by dissipation; in order that the eddy energy shall be maintained, it is therefore necessary that P div V" - (! V" v" . grad. v > O.

Understanding Stratospheric Water Vapor Variability and Model-simulated Rainfall Biases from the Perspective of Convection

Understanding Stratospheric Water Vapor Variability and Model-simulated Rainfall Biases from the Perspective of Convection PDF Author: Kai (M.S. in statistics) Zhang
Publisher:
ISBN:
Category :
Languages : en
Pages : 350

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Book Description
Convection and its interactions with transport of heat, water and momentum are essential in understanding many aspects of the climate system, for example, tracer transport in both the troposphere and lower stratosphere, the modelling of rainfall and prediction of climate change. The goal of this dissertation is to examine the role of convection variability in the related atmospheric composition transport and rainfall processes using both observations and climate models. The relationships between deep convection and the global diabatic heat budget are studied to understand the coupling between convection, temperature and general circulation. By examining the influence of convection on diabatic heating in the troposphere and stratosphere, we can gain a comprehensive understanding of the tropical convection and its influence on large-scale atmospheric circulation and stratosphere composition, especially on the cross-tropospuase transport of water vapor. We show that transient variability in deep convection is highly correlated with diabatic heating throughout the troposphere and stratosphere. Enhanced deep convection is linked to amplified heating in the tropical troposphere and in the mid-latitude storm tracks, tied to latent heat release. Enhanced convection is also linked to radiative cooling in the lower stratosphere, due to weaker upwelling longwave (LW) from lower altitudes. Transient deep convection modulates LW and shortwave (SW) radiation in the troposphere, with compensating effects that are linked to variations in cloud fraction and liquid and ice water content. Then we explore the variability of lower stratospheric (LS) water vapor in the Northern Hemisphere (NH) monsoon regions based on satellite observations and trajectory model simulations driven by diabatic heating in reanalyses. The links between stratospheric water vapor, fluctuations in deep convection and large-scale circulation and temperature are quantified. Results suggest that temperature plays a dominant role on water vapor variations with stronger convection leads to cold dehydration temperatures and a relatively dry stratosphere. Besides, the seasonal increase of stratospheric water vapor can be attributed to the geographic variations of convection and resultant variations of the dehydration center, of which the influence is comparable to the influence of the local dehydration temperature increase. Specifically, the seasonal geographic shift of the dehydration center from the east to the west Asian monsoon region with warmer tropopause temperatures could increase water vapor significantly. Dry biases over Southern Amazonia are observed in Community Atmosphere Model version 5 (CAM5). We use hindcast simulations to track the root causes for the biases. Results suggest that the dry bias is present by day 2 (24 to 48 hours) of model integrations and is very robust for all the seasons with largest bias magnitude during the southern summer (Dec-Feb, wet season). The near-surface-warm biases and low biases of humidity in the lower troposphere that exist since day 2 may be significant factors influencing the dry biases. The low biases of humidity are contributed by both physical components (shallow convective scheme and Zhang-McFarlane convective scheme, and maybe weak turbulence term), and dynamics (weak moisture convergence). We further evaluate the CAM5 with a higher-order turbulence closure scheme, named Cloud Layers Unified By Binomials (CLUBB), and a Multiscale Modeling Framework, referred as the "super-parameterization" (SP) with two different microphysics configurations to investigate their influences on rainfall simulations over Southern Amazonia. The two different microphysics configurations in SP are the one-moment cloud microphysics without aerosol treatment (SP1) and two-moment cloud microphysics coupled with aerosol treatment (SP2). Results show that both SP2 and CLUBB effectively reduce the low biases of rainfall, mainly during the wet season, and reduce low biases of humidity in the lower troposphere with further reduced shallow clouds and increased surface solar flux. These changes increase moist static energy, contribute to stronger convection and more rainfall. SP2 appears to realistically capture the observed increase of relative humidity prior to deep convection and it significantly increases rainfall in the afternoon; CLUBB significantly delays the afternoon peak time and produces more precipitation in the early morning, due to more gradual transition between shallow and deep convection. In CAM5 and CAM5 with CLUBB, occurrence of deep convection appears to be a result of stronger heating rather than higher relative humidity.

The Effects of Stratospheric Pollution by Aircraft, Report of Findings--final Report

The Effects of Stratospheric Pollution by Aircraft, Report of Findings--final Report PDF Author: United States. Department of Transportation. Climatic Impact Assessment Program Office
Publisher:
ISBN:
Category : Air
Languages : en
Pages : 870

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